Chemistry:Hydrogen

From HandWiki
Hydrogen, 1H
Hydrogen discharge tube.jpg
Purple glow in its plasma state
Hydrogen
Appearancecolorless gas
Standard atomic weight Ar, std(H)[1.007841.00811] conventional: 1.008
Hydrogen in the periodic table
Hydrogen Helium
Lithium Beryllium Boron Carbon Nitrogen Oxygen Fluorine Neon
Sodium Magnesium Aluminium Silicon Phosphorus Sulfur Chlorine Argon
Potassium Calcium Scandium Titanium Vanadium Chromium Manganese Iron Cobalt Nickel Copper Zinc Gallium Germanium Arsenic Selenium Bromine Krypton
Rubidium Strontium Yttrium Zirconium Niobium Molybdenum Technetium Ruthenium Rhodium Palladium Silver Cadmium Indium Tin Antimony Tellurium Iodine Xenon
Caesium Barium Lanthanum Cerium Praseodymium Neodymium Promethium Samarium Europium Gadolinium Terbium Dysprosium Holmium Erbium Thulium Ytterbium Lutetium Hafnium Tantalum Tungsten Rhenium Osmium Iridium Platinum Gold Mercury (element) Thallium Lead Bismuth Polonium Astatine Radon
Francium Radium Actinium Thorium Protactinium Uranium Neptunium Plutonium Americium Curium Berkelium Californium Einsteinium Fermium Mendelevium Nobelium Lawrencium Rutherfordium Dubnium Seaborgium Bohrium Hassium Meitnerium Darmstadtium Roentgenium Copernicium Nihonium Flerovium Moscovium Livermorium Tennessine Oganesson


H

Li
– ← hydrogenhelium
Atomic number (Z)1
Groupgroup 1: hydrogen and alkali metals
Periodperiod 1
Block  s-block
Element category  s-block
Electron configuration1s1
Electrons per shell1
Physical properties
Phase at STPgas
Melting point(H2) 13.99 K ​(−259.16 °C, ​−434.49 °F)
Boiling point(H2) 20.271 K ​(−252.879 °C, ​−423.182 °F)
Density (at STP)0.08988 g/L
when liquid (at m.p.)0.07 g/cm3 (solid: 0.0763 g/cm3)[1]
when liquid (at b.p.)0.07099 g/cm3
Triple point13.8033 K, ​7.041 kPa
Critical point32.938 K, 1.2858 MPa
Heat of fusion(H2) 0.117 kJ/mol
Heat of vaporization(H2) 0.904 kJ/mol
Molar heat capacity(H2) 28.836 J/(mol·K)
Vapor pressure
P (Pa) 1 10 100 1 k 10 k 100 k
at T (K) 15 20
Atomic properties
Oxidation states−1, +1 (an amphoteric oxide)
ElectronegativityPauling scale: 2.20
Ionization energies
  • 1st: 1312.0 kJ/mol
Covalent radius31±5 pm
Van der Waals radius120 pm
Color lines in a spectral range
Spectral lines of hydrogen
Other properties
Natural occurrenceprimordial
Crystal structurehexagonal
Hexagonal crystal structure for hydrogen
Speed of sound1310 m/s (gas, 27 °C)
Thermal conductivity0.1805 W/(m·K)
Magnetic orderingdiamagnetic[2]
Magnetic susceptibility−3.98·10−6 cm3/mol (298 K)[3]
CAS Number12385-13-6
1333-74-0 (H2)
History
DiscoveryHenry Cavendish[4][5] (1766)
Named byAntoine Lavoisier[6] (1783)
Main isotopes of hydrogen
Iso­tope Abun­dance Physics:Half-life (t1/2) Decay mode Pro­duct
1H 99.98% stable
2H 0.02% stable
3H trace 12.32 y β 3He
Category Category: Hydrogen
view · talk · edit | references
H
data m.p. cat
in calc from C diff report ref
C −259.16
K 13.99 13.99 0
F −434.49 −434.49 0
max precision 2
WD


input C: −259.16, K: 13.99, F: −434.49
comment
H
data b.p. cat
in calc from C diff report ref
C −252.879
K 20.271 20.271 0
F −423.182 −423.182 0
max precision 3
WD


input C: −252.879, K: 20.271, F: −423.182
comment

Hydrogen is a chemical element; it has symbol H and atomic number 1. It is the lightest element and, at standard conditions, is a gas of diatomic molecules with the formula H
2
. It is colorless, odorless, tasteless,[7] non-toxic, and highly combustible. Hydrogen is the most abundant chemical substance in the universe, constituting roughly 75% of all normal matter.[8][note 1] Stars such as the Sun are mainly composed of hydrogen in the plasma state. Most of the hydrogen on Earth exists in molecular forms such as water and organic compounds. For the most common isotope of hydrogen (symbol 1H) each atom has one proton, one electron, and no neutrons.

In the early universe, the formation of protons, the nuclei of hydrogen, occurred during the first second after the Big Bang. The emergence of neutral hydrogen atoms throughout the universe occurred about 370,000 years later during the recombination epoch, when the plasma had cooled enough for electrons to remain bound to protons.[9]

Hydrogen is nonmetallic (except when it becomes metallic at extremely high pressures) and readily forms a single covalent bond with most nonmetallic elements, forming compounds such as water and nearly all organic compounds. Hydrogen plays a particularly important role in acid–base reactions because these reactions usually involve the exchange of protons between soluble molecules. In ionic compounds, hydrogen can take the form of a negative charge (i.e., anion) where it is known as a hydride, or as a positively charged (i.e., cation) species denoted by the symbol H+
. The H+
cation is simply a proton (symbol p) but its behavior in aqueous solutions and in ionic compounds involves screening of its electric charge by nearby polar molecules or anions. Because hydrogen is the only neutral atom for which the Schrödinger equation can be solved analytically,[10] the study of its energetics and chemical bonding has played a key role in the development of quantum mechanics.

Hydrogen gas was first artificially produced in the early 16th century by the reaction of acids on metals. In 1766–1781, Henry Cavendish was the first to recognize that hydrogen gas was a discrete substance[11] and that it produces water when burned, the property for which it was later named: in Greek, hydrogen means "water-former".

Industrial production is mainly from steam reforming of natural gas. A small percentage is also produced using more energy-intensive methods such as the electrolysis of water.[12][13] Most hydrogen is used near the site of its production, the two largest uses being fossil fuel processing (e.g., hydrocracking) and ammonia production. Hydrogen can be deployed as an energy source in fuel cells to produce electricity, or via combustion to generate heat.[14] When hydrogen is consumed in fuel cells, the only emission at the point of use is water vapour.[14] Combustion of hydrogen can lead to the thermal formation of nitrogen oxides.[14] Hydrogen atoms may embrittle metals.[15]

Properties

Combustion

File:19. Експлозија на смеса од водород и воздух.webm

A black cup-like object hanging by its bottom with blue glow coming out of its opening.
The Space Shuttle Main Engine burnt hydrogen with oxygen, producing a nearly invisible flame at full thrust.

Hydrogen gas (dihydrogen or molecular hydrogen)[16] is highly flammable:

2 H
2
(g) + O
2
(g) → 2 H
2
O(l)
(572 kJ/2 mol = 286 kJ/mol = 141.865 MJ/kg)[note 2]

The enthalpy of combustion is −286 kJ/mol.[17]

Hydrogen gas forms explosive mixtures with air in concentrations from 4–74%[18] and with chlorine at 5–95%. The hydrogen autoignition temperature, the temperature of spontaneous ignition in air, is 500 °C (932 °F).[19]

Flame

Pure hydrogen-oxygen flames emit ultraviolet light and with high oxygen mix are nearly invisible to the naked eye, as illustrated by the faint plume of the Space Shuttle Main Engine, compared to the highly visible plume of a Space Shuttle Solid Rocket Booster, which uses an ammonium perchlorate composite. The detection of a burning hydrogen leak may require a flame detector; such leaks can be very dangerous. Hydrogen flames in other conditions are blue, resembling blue natural gas flames.[20] The destruction of the Hindenburg airship was a notorious example of hydrogen combustion and the cause is still debated. The visible flames in the photographs were the result of carbon compounds in the airship skin burning.[21]

Reactants

H
2
is unreactive compared to diatomic elements such as halogens or oxygen. The thermodynamic basis of this low reactivity is the very strong H–H bond, with a bond dissociation energy of 435.7 kJ/mol.[22] The kinetic basis of the low reactivity is the nonpolar nature of H
2
and its weak polarizability. It spontaneously reacts with chlorine and fluorine to form hydrogen chloride and hydrogen fluoride, respectively.[23] The reactivity of H
2
is strongly affected by the presence of metal catalysts. Thus, while mixtures of H
2
with O
2
or air combust readily when heated to at least 500 °C by a spark or flame, they do not react at room temperature in the absence of a catalyst.

Electron energy levels

Main page: Physics:Hydrogen atom
Drawing of a light-gray large sphere with a cut off quarter and a black small sphere and numbers 1.7x10−5 illustrating their relative diameters.
A depiction of a hydrogen atom with size of central proton shown, and the atomic diameter shown as about twice the Bohr model radius (image not to scale)

The ground state energy level of the electron in a hydrogen atom is −13.6 eV,[24] which is equivalent to an ultraviolet photon of roughly 91 nm wavelength.[25]

The energy levels of hydrogen can be calculated fairly accurately using the Bohr model of the atom, which conceptualizes the electron as "orbiting" the proton in analogy to the Earth's orbit of the Sun. However, the atomic electron and proton are held together by electromagnetic force, while planets and celestial objects are held by gravity. Because of the discretization of angular momentum postulated in early quantum mechanics by Bohr, the electron in the Bohr model can only occupy certain allowed distances from the proton, and therefore only certain allowed energies.[26]

A more accurate description of the hydrogen atom comes from a purely quantum mechanical treatment that uses the Schrödinger equation, Dirac equation or Feynman path integral formulation to calculate the probability density of the electron around the proton.[27] The most complicated treatments allow for the small effects of special relativity and vacuum polarization. In the quantum mechanical treatment, the electron in a ground state hydrogen atom has no angular momentum at all—illustrating how the "planetary orbit" differs from electron motion.

Spin isomers

Main page: Physics:Spin isomers of hydrogen

Molecular H
2
exists as two spin isomers, i.e. compounds that differ only in the spin states of their nuclei.[28] In the orthohydrogen form, the spins of the two nuclei are parallel, forming a spin triplet state having a total molecular spin [math]\displaystyle{ S = 1 }[/math]; in the parahydrogen form the spins are antiparallel and form a spin singlet state having spin [math]\displaystyle{ S = 0 }[/math]. The equilibrium ratio of ortho- to para-hydrogen depends on temperature. At room temperature or warmer, equilibrium hydrogen gas contains about 25% of the para form and 75% of the ortho form.[29] The ortho form is an excited state, having higher energy than the para form by 1.455 kJ/mol,[30] and it converts to the para form over the course of several minutes when cooled to low temperature.[31] The thermal properties of the forms differ because they differ in their allowed rotational quantum states, resulting in different thermal properties such as the heat capacity.[32]

The ortho-to-para ratio in H
2
is an important consideration in the liquefaction and storage of liquid hydrogen: the conversion from ortho to para is exothermic and produces enough heat to evaporate most of the liquid if not converted first to parahydrogen during the cooling process.[33] Catalysts for the ortho-para interconversion, such as ferric oxide and activated carbon compounds, are used during hydrogen cooling to avoid this loss of liquid.[34]

Phases

Hydrogen gas is colorless and transparent, here contained in a glass ampoule.
Phase diagram of hydrogen on logarithmic scales. Lines show boundaries between phases, with the end of the liquid-gas line indicating the critical point. The triple point of hydrogen is just off-scale to the left.
Phase diagram of hydrogen. The temperature and pressure scales are logarithmic, so one unit corresponds to a 10× change. The left edge corresponds to 105 Pa, which is about atmospheric pressure.[image reference needed]

Compounds

Covalent and organic compounds

While H
2
is not very reactive under standard conditions, it does form compounds with most elements. Hydrogen can form compounds with elements that are more electronegative, such as halogens (F, Cl, Br, I), or oxygen; in these compounds hydrogen takes on a partial positive charge.[35] When bonded to a more electronegative element, particularly fluorine, oxygen, or nitrogen, hydrogen can participate in a form of medium-strength noncovalent bonding with another electronegative element with a lone pair, a phenomenon called hydrogen bonding that is critical to the stability of many biological molecules.[36][37] Hydrogen also forms compounds with less electronegative elements, such as metals and metalloids, where it takes on a partial negative charge. These compounds are often known as hydrides.[38]

Hydrogen forms a vast array of compounds with carbon called the hydrocarbons, and an even vaster array with heteroatoms that, because of their general association with living things, are called organic compounds.[39] The study of their properties is known as organic chemistry[40] and their study in the context of living organisms is known as biochemistry.[41] By some definitions, "organic" compounds are only required to contain carbon. However, most of them also contain hydrogen, and because it is the carbon-hydrogen bond that gives this class of compounds most of its particular chemical characteristics, carbon-hydrogen bonds are required in some definitions of the word "organic" in chemistry.[39] Millions of hydrocarbons are known, and they are usually formed by complicated pathways that seldom involve elemental hydrogen.

Hydrogen is highly soluble in many rare earth and transition metals[42] and is soluble in both nanocrystalline and amorphous metals.[43] Hydrogen solubility in metals is influenced by local distortions or impurities in the crystal lattice.[44] These properties may be useful when hydrogen is purified by passage through hot palladium disks, but the gas's high solubility is a metallurgical problem, contributing to the embrittlement of many metals,[15] complicating the design of pipelines and storage tanks.[45]

Hydrides

Main page: Physics:Hydride
A sample of sodium hydride

Compounds of hydrogen are often called hydrides, a term that is used fairly loosely. The term "hydride" suggests that the H atom has acquired a negative or anionic character, denoted H
, and is used when hydrogen forms a compound with a more electropositive element. The existence of the hydride anion, suggested by Gilbert N. Lewis in 1916 for group 1 and 2 salt-like hydrides, was demonstrated by Moers in 1920 by the electrolysis of molten lithium hydride (LiH), producing a stoichiometric quantity of hydrogen at the anode.[46] For hydrides other than group 1 and 2 metals, the term is quite misleading, considering the low electronegativity of hydrogen. An exception in group 2 hydrides is BeH
2
, which is polymeric. In lithium aluminium hydride, the [AlH
4
]
anion carries hydridic centers firmly attached to the Al(III).

Although hydrides can be formed with almost all main-group elements, the number and combination of possible compounds varies widely; for example, more than 100 binary borane hydrides are known, but only one binary aluminium hydride.[47] Binary indium hydride has not yet been identified, although larger complexes exist.[48]

In inorganic chemistry, hydrides can also serve as bridging ligands that link two metal centers in a coordination complex. This function is particularly common in group 13 elements, especially in boranes (boron hydrides) and aluminium complexes, as well as in clustered carboranes.[49]

Protons and acids

Oxidation of hydrogen removes its electron and gives H+
, which contains no electrons and a nucleus which is usually composed of one proton. That is why H+
is often called a proton. This species is central to discussion of acids. Under the Brønsted–Lowry acid–base theory, acids are proton donors, while bases are proton acceptors.

A bare proton, H+
, cannot exist in solution or in ionic crystals because of its unstoppable attraction to other atoms or molecules with electrons. Except at the high temperatures associated with plasmas, such protons cannot be removed from the electron clouds of atoms and molecules, and will remain attached to them. However, the term 'proton' is sometimes used loosely and metaphorically to refer to positively charged or cationic hydrogen attached to other species in this fashion, and as such is denoted "H+
" without any implication that any single protons exist freely as a species.

To avoid the implication of the naked "solvated proton" in solution, acidic aqueous solutions are sometimes considered to contain a less unlikely fictitious species, termed the "hydronium ion" ([H
3
O]+
). However, even in this case, such solvated hydrogen cations are more realistically conceived as being organized into clusters that form species closer to [H
9
O
4
]+
.[50] Other oxonium ions are found when water is in acidic solution with other solvents.[51]

Although exotic on Earth, one of the most common ions in the universe is the H+
3
ion, known as protonated molecular hydrogen or the trihydrogen cation.[52]

Isotopes

Main page: Physics:Isotopes of hydrogen
Blausen 0530 HydrogenIsotopes.png
Hydrogen discharge (spectrum) tube
Deuterium discharge (spectrum) tube

Hydrogen has three naturally occurring isotopes, denoted 1H, 2H and 3H. Other, highly unstable nuclei (4H to 7H) have been synthesized in the laboratory but not observed in nature.[53][54]

  • 1H is the most common hydrogen isotope, with an abundance of more than 99.98%. Because the nucleus of this isotope consists of only a single proton, it is given the descriptive but rarely used formal name protium.[55] It is unique among all stable isotopes in having no neutrons; see diproton for a discussion of why others do not exist.
  • 2H, the other stable hydrogen isotope, is known as deuterium and contains one proton and one neutron in the nucleus. Nearly all deuterium in the universe is thought to have been produced at the time of the Big Bang, and has endured since that time. Deuterium is not radioactive, and does not represent a significant toxicity hazard. Water enriched in molecules that include deuterium instead of normal hydrogen is called heavy water. Deuterium and its compounds are used as a non-radioactive label in chemical experiments and in solvents for 1H-NMR spectroscopy.[56] Heavy water is used as a neutron moderator and coolant for nuclear reactors. Deuterium is also a potential fuel for commercial nuclear fusion.[57]
  • 3H is known as tritium and contains one proton and two neutrons in its nucleus. It is radioactive, decaying into helium-3 through beta decay with a half-life of 12.32 years.[49] It is radioactive enough to be used in luminous paint to enhance the visibility of data displays, such as for painting the hands and dial-markers of watches. The watch glass prevents the small amount of radiation involved from escaping the case.[58] Small amounts of tritium are produced naturally by the interaction of cosmic rays with atmospheric gases; tritium has also been released during nuclear weapons tests.[59] It is used in nuclear fusion reactions,[60] as a tracer in isotope geochemistry,[61] and in specialized self-powered lighting devices.[62] Tritium has also been used in chemical and biological labeling experiments as a radiolabel.[63]

Unique among the elements, distinct names are assigned to its isotopes in common use today. During the early study of radioactivity, various heavy radioactive isotopes were given their own names, but such names are no longer used, except for deuterium and tritium. The symbols D and T (instead of 2H and 3H) are sometimes used for deuterium and tritium, but the symbol P is already in use for phosphorus and thus is not available for protium.[64] In its nomenclatural guidelines, the International Union of Pure and Applied Chemistry (IUPAC) allows any of D, T, 2H, and 3H to be used, although 2H and 3H are preferred.[65]

The exotic atom muonium (symbol Mu), composed of an antimuon and an electron, can also be considered a light radioisotope of hydrogen.[66] Because muons decay with lifetime 2.2 µs, muonium is too unstable to exhibit observable chemistry.[67] Nevertheless, muonium compounds are important test cases for quantum simulation, due to the mass difference between the antimuon and the proton,[68] and IUPAC nomenclature incorporates such hypothetical compounds as muonium chloride (MuCl) and sodium muonide (NaMu), analogous to hydrogen chloride and sodium hydride respectively.[69]

Thermal and physical properties

Table of thermal and physical properties of hydrogen (H2) at atmospheric pressure:[70][71]

Temperature (K) Density (kg/m^3) Specific heat (kJ/kg °C) Dynamic viscosity (kg/m s) Kinematic viscosity (m^2/s) Thermal conductivity (W/m °C) Thermal diffusivity (m^2/s) Prandtl Number
100 0.24255 11.23 4.21E-06 1.74E-05 6.70E-02 2.46E-05 0.707
150 0.16371 12.602 5.60E-06 3.42E-05 0.0981 4.75E-05 0.718
200 0.1227 13.54 6.81E-06 5.55E-05 0.1282 7.72E-05 0.719
250 0.09819 14.059 7.92E-06 8.06E-05 0.1561 1.13E-04 0.713
300 0.08185 14.314 8.96E-06 1.10E-04 0.182 1.55E-04 0.706
350 0.07016 14.436 9.95E-06 1.42E-04 0.206 2.03E-04 0.697
400 0.06135 14.491 1.09E-05 1.77E-04 0.228 2.57E-04 0.69
450 0.05462 14.499 1.18E-05 2.16E-04 0.251 3.16E-04 0.682
500 0.04918 14.507 1.26E-05 2.57E-04 0.272 3.82E-04 0.675
550 0.04469 14.532 1.35E-05 3.02E-04 0.292 4.52E-04 0.668
600 0.04085 14.537 1.43E-05 3.50E-04 0.315 5.31E-04 0.664
700 0.03492 14.574 1.59E-05 4.55E-04 0.351 6.90E-04 0.659
800 0.0306 14.675 1.74E-05 5.69E-04 0.384 8.56E-04 0.664
900 0.02723 14.821 1.88E-05 6.90E-04 0.412 1.02E-03 0.676
1000 0.02424 14.99 2.01E-05 8.30E-04 0.448 1.23E-03 0.673
1100 0.02204 15.17 2.13E-05 9.66E-04 0.488 1.46E-03 0.662
1200 0.0202 15.37 2.26E-05 1.12E-03 0.528 1.70E-03 0.659
1300 0.01865 15.59 2.39E-05 1.28E-03 0.568 1.96E-03 0.655
1400 0.01732 15.81 2.51E-05 1.45E-03 0.61 2.23E-03 0.65
1500 0.01616 16.02 2.63E-05 1.63E-03 0.655 2.53E-03 0.643
1600 0.0152 16.28 2.74E-05 1.80E-03 0.697 2.82E-03 0.639
1700 0.0143 16.58 2.85E-05 1.99E-03 0.742 3.13E-03 0.637
1800 0.0135 16.96 2.96E-05 2.19E-03 0.786 3.44E-03 0.639
1900 0.0128 17.49 3.07E-05 2.40E-03 0.835 3.73E-03 0.643
2000 0.0121 18.25 3.18E-05 2.63E-03 0.878 3.98E-03 0.661

History

Discovery and use

Main page: Physics:Timeline of hydrogen technologies

Robert Boyle

Robert Boyle, who discovered the reaction between iron filings and dilute acids

In 1671, the Irish scientist Robert Boyle discovered and described the reaction between iron filings and dilute acids, which results in the production of hydrogen gas.[72][73]

Having provided a saline spirit [hydrochloric acid], which by an uncommon way of preparation was made exceeding sharp and piercing, we put into a vial, capable of containing three or four ounces of water, a convenient quantity of filings of steel, which were not such as are commonly sold in shops to Chymists and Apothecaries, (those being usually not free enough from rust) but such as I had a while before caus'd to be purposely fil'd off from a piece of good steel. This metalline powder being moistn'd in the viol with a little of the menstruum, was afterwards drench'd with more; whereupon the mixture grew very hot, and belch'd up copious and stinking fumes; which whether they consisted altogether of the volatile sulfur of the Mars [iron], or of metalline steams participating of a sulfureous nature, and join'd with the saline exhalations of the menstruum, is not necessary to be here discuss'd. But whencesoever this stinking smoak proceeded, so inflammable it was, that upon the approach of a lighted candle to it, it would readily enough take fire, and burn with a blewish and somewhat greenish flame at the mouth of the viol for a good while together; and that, though with little light, yet with more strength than one would easily suspect.

The word "sulfureous" may be somewhat confusing, especially since Boyle did a similar experiment with iron and sulfuric acid.[74] However, in all likelihood, "sulfureous" should here be understood to mean combustible.[75]

Henry Cavendish

In 1766, Henry Cavendish was the first to recognize hydrogen gas as a discrete substance, by naming the gas from a metal-acid reaction "inflammable air". He speculated that "inflammable air" was in fact identical to the hypothetical substance called "phlogiston"[76][77] and further finding in 1781 that the gas produces water when burned. He is usually given credit for the discovery of hydrogen as an element.[4][5]

Antoine Lavoisier

Antoine Lavoisier, who identified the element that came to be known as hydrogen

In 1783, Antoine Lavoisier identified the element that came to be known as hydrogen[78] when he and Laplace reproduced Cavendish's finding that water is produced when hydrogen is burned.[5] Lavoisier produced hydrogen for his experiments on mass conservation by reacting a flux of steam with metallic iron through an incandescent iron tube heated in a fire. Anaerobic oxidation of iron by the protons of water at high temperature can be schematically represented by the set of following reactions:

1) Fe + H
2
O → FeO + H
2
2) Fe + 3 H
2
O → Fe
2
O
3
+ 3 H
2
3) Fe + 4 H
2
O → Fe
3
O
4
+ 4 H
2

Many metals such as zirconium undergo a similar reaction with water leading to the production of hydrogen.

19th century

François Isaac de Rivaz built the first de Rivaz engine, an internal combustion engine powered by a mixture of hydrogen and oxygen in 1806. Edward Daniel Clarke invented the hydrogen gas blowpipe in 1819. The Döbereiner's lamp and limelight were invented in 1823.[5]

Hydrogen was liquefied for the first time by James Dewar in 1898 by using regenerative cooling and his invention, the vacuum flask.[5] He produced solid hydrogen the next year.[5]

Hydrogen-lifted airship

Airship Hindenburg over New York
The Hindenburg over New York City in 1937

The first hydrogen-filled balloon was invented by Jacques Charles in 1783.[5] Hydrogen provided the lift for the first reliable form of air-travel following the 1852 invention of the first hydrogen-lifted airship by Henri Giffard.[5] German count Ferdinand von Zeppelin promoted the idea of rigid airships lifted by hydrogen that later were called Zeppelins; the first of which had its maiden flight in 1900.[5] Regularly scheduled flights started in 1910 and by the outbreak of World War I in August 1914, they had carried 35,000 passengers without a serious incident. Hydrogen-lifted airships were used as observation platforms and bombers during the war.

The first non-stop transatlantic crossing was made by the British airship R34 in 1919. Regular passenger service resumed in the 1920s and the discovery of helium reserves in the United States promised increased safety, but the U.S. government refused to sell the gas for this purpose. Therefore, H
2
was used in the Hindenburg airship, which was destroyed in a midair fire over New Jersey on 6 May 1937.[5] The incident was broadcast live on radio and filmed. Ignition of leaking hydrogen is widely assumed to be the cause, but later investigations pointed to the ignition of the aluminized fabric coating by static electricity. But the damage to hydrogen's reputation as a lifting gas was already done and commercial hydrogen airship travel ceased. Hydrogen is still used, in preference to non-flammable but more expensive helium, as a lifting gas for weather balloons.

Deuterium and tritium

Deuterium was discovered in December 1931 by Harold Urey, and tritium was prepared in 1934 by Ernest Rutherford, Mark Oliphant, and Paul Harteck.[4] Heavy water, which consists of deuterium in the place of regular hydrogen, was discovered by Urey's group in 1932.[5]

Hydrogen-cooled turbogenerator

The first hydrogen-cooled turbogenerator went into service with gaseous hydrogen as a coolant in the rotor and the stator in 1937 at Dayton, Ohio, by the Dayton Power & Light Co.;[79] because of the thermal conductivity and very low viscosity of hydrogen gas, thus lower drag than air, this is the most common type in its field today for large generators (typically 60 MW and bigger; smaller generators are usually air-cooled).

Nickel–hydrogen battery

The nickel–hydrogen battery was used for the first time in 1977 aboard the U.S. Navy's Navigation technology satellite-2 (NTS-2).[80] The International Space Station,[81] Mars Odyssey[82] and the Mars Global Surveyor[83] are equipped with nickel-hydrogen batteries. In the dark part of its orbit, the Hubble Space Telescope is also powered by nickel-hydrogen batteries, which were finally replaced in May 2009,[84] more than 19 years after launch and 13 years beyond their design life.[85]

Role in quantum theory

A line spectrum showing black background with narrow lines superimposed on it: one violet, one blue, one cyan, and one red.
Hydrogen emission spectrum lines in the four visible lines of the Balmer series

Because of its simple atomic structure, consisting only of a proton and an electron, the hydrogen atom, together with the spectrum of light produced from it or absorbed by it, has been central to the development of the theory of atomic structure.[86] Furthermore, study of the corresponding simplicity of the hydrogen molecule and the corresponding cation H+
2
brought understanding of the nature of the chemical bond, which followed shortly after the quantum mechanical treatment of the hydrogen atom had been developed in the mid-1920s.

One of the first quantum effects to be explicitly noticed (but not understood at the time) was a Maxwell observation involving hydrogen, half a century before full quantum mechanical theory arrived. Maxwell observed that the specific heat capacity of H
2
unaccountably departs from that of a diatomic gas below room temperature and begins to increasingly resemble that of a monatomic gas at cryogenic temperatures. According to quantum theory, this behavior arises from the spacing of the (quantized) rotational energy levels, which are particularly wide-spaced in H
2
because of its low mass. These widely spaced levels inhibit equal partition of heat energy into rotational motion in hydrogen at low temperatures. Diatomic gases composed of heavier atoms do not have such widely spaced levels and do not exhibit the same effect.[87]

Antihydrogen (H) is the antimatter counterpart to hydrogen. It consists of an antiproton with a positron. Antihydrogen is the only type of antimatter atom to have been produced (As of 2015).[88][89]

Cosmic prevalence and distribution

A white-green cotton-like clog on black background.
NGC 604, a giant region of ionized hydrogen in the Triangulum Galaxy

Hydrogen, as atomic H, is the most abundant chemical element in the universe, making up 75 percent of normal matter by mass and more than 90 percent by number of atoms. (Most of the mass of the universe, however, is not in the form of chemical-element type matter, but rather is postulated to occur as yet-undetected forms of mass such as dark matter and dark energy.[90])

Hydrogen is found in great abundance in stars and gas giant planets. Molecular clouds of H
2
are associated with star formation. Hydrogen plays a vital role in powering stars through the proton-proton reaction in case of stars with very low to approximately 1 mass of the Sun and the CNO cycle of nuclear fusion in case of stars more massive than the Sun.[91]

States

Throughout the universe, hydrogen is mostly found in the atomic and plasma states, with properties quite distinct from those of molecular hydrogen. As a plasma, hydrogen's electron and proton are not bound together, resulting in very high electrical conductivity and high emissivity (producing the light from the Sun and other stars). The charged particles are highly influenced by magnetic and electric fields. For example, in the solar wind they interact with the Earth's magnetosphere giving rise to Birkeland currents and the aurora.

Hydrogen is found in the neutral atomic state in the interstellar medium because the atoms seldom collide and combine. They are the source of the 21-cm hydrogen line at 1420 MHz that is detected in order to probe primordial hydrogen.[92] The large amount of neutral hydrogen found in the damped Lyman-alpha systems is thought to dominate the cosmological baryonic density of the universe up to a redshift of z = 4.[93]

Under ordinary conditions on Earth, elemental hydrogen exists as the diatomic gas, H
2
. Hydrogen gas is very rare in the Earth's atmosphere (around 0.53 ppm on a molar basis[94]) because of its light weight, which enables it to escape from the atmosphere more rapidly than heavier gases. However, hydrogen is the third most abundant element on the Earth's surface,[95] mostly in the form of chemical compounds such as hydrocarbons and water.[49]

A molecular form called protonated molecular hydrogen (H+
3
) is found in the interstellar medium, where it is generated by ionization of molecular hydrogen from cosmic rays. This ion has also been observed in the upper atmosphere of the planet Jupiter. The ion is relatively stable in the environment of outer space due to the low temperature and density. H+
3
is one of the most abundant ions in the universe, and it plays a notable role in the chemistry of the interstellar medium.[96] Neutral triatomic hydrogen H
3
can exist only in an excited form and is unstable.[97] By contrast, the positive hydrogen molecular ion (H+
2
) is a rare molecule in the universe.

Production

Main page: Chemistry:Hydrogen production

Many methods exist for producing H2, but three dominate commercially: steam reforming often coupled to water-gas shift, partial oxidation of hydrocarbons, and water electrolysis.[98]

Steam reforming

Inputs and outputs of steam reforming of natural gas, a process used in hydrogen production

Hydrogen is mainly produced by steam reforming, the reaction of water and methane.[99][100] [101] Thus, at high temperatures (1000–1400 K, 700–1100 °C or 1300–2000 °F), steam (water vapor) reacts with methane to yield carbon monoxide and H
2
.

CH
4
+ H
2
O → CO + 3 H
2

Steam reforming is also used for the industrial preparation of ammonia.

This reaction is favored at low pressures, Nonetheless, conducted at high pressures (2.0 MPa, 20 atm or 600 inHg) because high-pressure H
2
is the most marketable product, and pressure swing adsorption (PSA) purification systems work better at higher pressures. The product mixture is known as "synthesis gas" because it is often used directly for the production of methanol and many other compounds. Hydrocarbons other than methane can be used to produce synthesis gas with varying product ratios. One of the many complications to this highly optimized technology is the formation of coke or carbon:

CH
4
→ C + 2 H
2

Consequently, steam reforming typically employs an excess of H
2
O
. Additional hydrogen can be recovered from the steam by use of carbon monoxide through the water gas shift reaction. This process requires an iron oxide catalyst:[101]

CO + H
2
O → CO
2
+ H
2

Hydrogen is sometimes produced and consumed in the same industrial process, without being separated. In the Haber process for the production of ammonia, hydrogen is generated from natural gas.[102]

Partial oxidation of hydrocarbons

Other methods for CO and H
2
production include partial oxidation of hydrocarbons:[103]

2 CH
4
+ O
2
→ 2 CO + 4 H
2

Although less important commercially, coal can serve as a prelude to the shift reaction above:[101]

C + H
2
O → CO + H
2

Olefin production units may produce substantial quantities of byproduct hydrogen particularly from cracking light feedstocks like ethane or propane.[104]

Water electrolysis

Inputs and outputs of the electrolysis of water production of hydrogen

The electrolysis of water is a conceptually simple method of producing hydrogen.

2 H
2
O(l) → 2 H
2
(g) + O
2
(g)

Commercial electrolyzers use nickel-based catalysts in strongly alkaline solution. Platinum is a superior catalyst but is expensive.[105]

Electrolysis of brine to yield chlorine also produces hydrogen as a co-product.[106]

Methane pyrolysis

Hydrogen can be produced by pyrolysis of natural gas (methane).

This route has a lower carbon footprint than commercial hydrogen production processes.[107][108][109][110] Developing a commercial methane pyrolysis process could expedite the expanded use of hydrogen in industrial and transportation applications. Methane pyrolysis is accomplished by passing methane through a molten metal catalyst containing dissolved nickel. Methane is converted to hydrogen gas and solid carbon.[111][112]

CH
4
(g) → C(s) + 2 H
2
(g)
(ΔH° = 74 kJ/mol)

The carbon may be sold as a manufacturing feedstock or fuel, or landfilled.

Further research continues in several laboratories, including at Karlsruhe Liquid-metal Laboratory [113] and at University of California – Santa Barbara.[114] BASF built a methane pyrolysis pilot plant.[115]

Thermochemical

More than 200 thermochemical cycles can be used for water splitting. Many of these cycles such as the iron oxide cycle, cerium(IV) oxide–cerium(III) oxide cycle, zinc zinc-oxide cycle, sulfur-iodine cycle, copper-chlorine cycle and hybrid sulfur cycle have been evaluated for their commercial potential to produce hydrogen and oxygen from water and heat without using electricity.[116] A number of laboratories (including in France , Germany , Greece, Japan , and the United States ) are developing thermochemical methods to produce hydrogen from solar energy and water.[117]

Laboratory methods

H
2
is produced in laboratories, often as a by-product of other reactions. Many metals react with water to produce H
2
, but the rate of hydrogen evolution depends on the metal, the pH, and the presence of alloying agents. Most commonly, hydrogen evolution is induced by acids. The alkali and alkaline earth metals, aluminium, zinc, manganese, and iron react readily with aqueous acids. This reaction is the basis of the Kipp's apparatus, which once was used as a laboratory gas source:

Zn + 2 H+
→ Zn2+ + H
2

In the absence of acid, the evolution of H
2
is slower. Because iron is widely used structural material, its anaerobic corrosion is of technological significance:

Fe + 2 H
2
O → Fe(OH)
2
+ H
2

Many metals, such as aluminium, are slow to react with water because they form passivated coatings of oxides. An alloy of aluminium and gallium, however, does react with water.[118] At high pH, aluminium can produce H
2
:

2 Al + 6 H
2
O + 2 OH
→ 2 [Al(OH)
4
]
+ 3 H
2

Some metal-containing compounds react with acids to evolve H
2
. Under anaerobic conditions, ferrous hydroxide (Fe(OH)2) can be oxidized by the protons of water to form magnetite and H
2
. This process is described by the Schikorr reaction:

3 Fe(OH)
2
→ Fe
3
O
4
+ 2 H
2
O + H
2

This process occurs during the anaerobic corrosion of iron and steel in oxygen-free groundwater and in reducing soils below the water table.

Biohydrogen

H
2
is produced by hydrogenase enzymes in some fermentation.[119]

Wells

There is a well in Mali and deposits in several other countries, such as France.[120]

Applications

Petrochemical industry

Large quantities of H
2
are used in the "upgrading" of fossil fuels. Key consumers of H
2
include hydrodealkylation, hydrodesulfurization, and hydrocracking. Many of these reactions can be classified as hydrogenolysis, i.e., the cleavage of bonds by hydrogen. Illustrative is the separation of sulfur from liquid fossil fuels:[98]

R
2
S + 2 H
2
→ H
2
S + 2 RH

Hydrogenation

Hydrogenation, the addition of H
2
to various substrates is conducted on a large scale. The hydrogenation of N
2
to produce ammonia by the Haber–Bosch process consumes a few percent of the energy budget in the entire industry. The resulting ammonia is used to supply the majority of the protein consumed by humans.[121] Hydrogenation is used to convert unsaturated fats and oils to saturated (trans) fats and oils. The major application is the production of margarine. Methanol is produced by hydrogenation of carbon dioxide. It is similarly the source of hydrogen in the manufacture of hydrochloric acid. H
2
is also used as a reducing agent for the conversion of some ores to the metals.[122]

Coolant

Main page: Physics:Hydrogen-cooled turbo generator

Hydrogen is commonly used in power stations as a coolant in generators due to a number of favorable properties that are a direct result of its light diatomic molecules. These include low density, low viscosity, and the highest specific heat and thermal conductivity of all gases.

Energy carrier

Elemental hydrogen is widely discussed in the context of energy, as an energy carrier with potential to help the decarbonisation of economies to mitigate greenhouse gas emissions.[123][124] This therefore requires hydrogen to be produced cleanly, in quantities to supply in sectors and applications where cheaper and more energy efficient mitigation alternatives are limited. These include heavy industry and long-distance transport.[123] Hydrogen is a ''carrier'' of energy rather than an energy resource, because there is no naturally occurring source of hydrogen in useful quantities.[125]

Hydrogen can be deployed as an energy source in fuel cells to produce electricity, or via combustion to generate heat.[14] When hydrogen is consumed in fuel cells, the only emission at the point of use is water vapour.[14] Combustion of hydrogen can lead to the thermal formation of harmful nitrogen oxides.[14] The overall lifecycle emissions of hydrogen depend on how it is produced. Nearly all of the world's current supply of hydrogen is created from fossil fuels.[126][127] The main method is steam methane reforming, in which hydrogen is produced from a chemical reaction between steam and methane, the main component of natural gas. Producing one tonne of hydrogen through this process emits 6.6–9.3 tonnes of carbon dioxide.[128] While carbon capture and storage (CCS) could remove a large fraction of these emissions, the overall carbon footprint of hydrogen from natural gas is difficult to assess (As of 2021), in part because of emissions (including vented and fugitive methane) created in the production of the natural gas itself.[129]

Electricity can be used to split water molecules, producing sustainable hydrogen provided the electricity was generated sustainably. However, this electrolysis process is currently more expensive than creating hydrogen from methane without CCS and the efficiency of energy conversion is inherently low.[124] Hydrogen can be produced when there is a surplus of variable renewable electricity, then stored and used to generate heat or to re-generate electricity.[130] Hydrogen created through electrolysis using renewable energy is commonly referred to as "green hydrogen."[131] It can be further transformed into synthetic fuels such as ammonia and methanol.[132]

Innovation in hydrogen electrolysers could make large-scale production of hydrogen from electricity more cost-competitive.[133] There is potential for hydrogen produced this way to play a significant role in decarbonising energy systems where there are challenges and limitations to replacing fossil fuels with direct use of electricity.[123]

Hydrogen fuel can produce the intense heat required for industrial production of steel, cement, glass, and chemicals, thus contributing to the decarbonisation of industry alongside other technologies, such as electric arc furnaces for steelmaking.[134] However, it is likely to play a larger role in providing industrial feedstock for cleaner production of ammonia and organic chemicals.[123] For example, in steelmaking, hydrogen could function as a clean energy carrier and also as a low-carbon catalyst replacing coal-derived coke.[135] Hydrogen used to decarbonise transportation is likely to find its largest applications in shipping, aviation and to a lesser extent heavy goods vehicles, through the use of hydrogen-derived synthetic fuels such as ammonia and methanol, and fuel cell technology.[123] For light duty vehicles including passenger cars, hydrogen is far behind other alternative fuel vehicles, especially compared with the rate of adoption of battery electric vehicles, and may not play a significant role in future.[136]

Disadvantages of hydrogen as an energy carrier include high costs of storage and distribution due to hydrogen's explosivity, its large volume compared to other fuels, and its tendency to make pipes brittle.[129]

Semiconductor industry

Hydrogen is employed to saturate broken ("dangling") bonds of amorphous silicon and amorphous carbon that helps stabilizing material properties.[137] It is also a potential electron donor in various oxide materials, including ZnO,[138][139] SnO
2
, CdO, MgO,[140] ZrO
2
, HfO
2
, La
2
O
3
, Y
2
O
3
, TiO
2
, SrTiO
3
, LaAlO
3
, SiO
2
, Al
2
O
3
, ZrSiO
4
, HfSiO
4
, and SrZrO
3
.[141]

Niche and evolving uses

  • Buoyant lifting: Because H
    2
    is lighter than air, having only 7% of the density of air, it was once widely used as a lifting gas in balloons and airships.[145]
  • Leak detection: Pure or mixed with nitrogen (sometimes called forming gas), hydrogen is a tracer gas for detection of minute leaks. Applications can be found in the automotive, chemical, power generation, aerospace, and telecommunications industries.[146] Hydrogen is an authorized food additive (E 949) that allows food package leak testing, as well as having anti-oxidizing properties.[147]

Biological reactions

H
2
is a product of some types of anaerobic metabolism and is produced by several microorganisms, usually via reactions catalyzed by iron- or nickel-containing enzymes called hydrogenases. These enzymes catalyze the reversible redox reaction between H
2
and its component two protons and two electrons. Creation of hydrogen gas occurs in the transfer of reducing equivalents, produced during pyruvate fermentation, to water.[151] The natural cycle of hydrogen production and consumption by organisms is called the hydrogen cycle.[152] Bacteria such as Mycobacterium smegmatis can utilize the small amount of hydrogen in the atmosphere as a source of energy when other sources are lacking, using a hydrogenase with small channels that exclude oxygen and so permits the reaction to occur even though the hydrogen concentration is very low and the oxygen concentration is as in normal air.[94][153]

Hydrogen is the most abundant element in the human body in terms of numbers of atoms of the element but the third most abundant element by mass. H
2
occurs in the breath of humans due to the metabolic activity of hydrogenase-containing microorganisms in the large intestine and is a natural component of flatus. The concentration in the breath of fasting people at rest is typically less than 5 parts per million (ppm) but can be 50 ppm when people with intestinal disorders consume molecules they cannot absorb during diagnostic hydrogen breath tests.[154]

Water splitting, in which water is decomposed into its component protons, electrons, and oxygen, occurs in the light reactions in all photosynthetic organisms. Some such organisms, including the alga Chlamydomonas reinhardtii and cyanobacteria, have evolved a second step in the dark reactions in which protons and electrons are reduced to form H
2
gas by specialized hydrogenases in the chloroplast.[155] Efforts have been undertaken to genetically modify cyanobacterial hydrogenases to efficiently synthesize H
2
gas even in the presence of oxygen.[156] Efforts have also been undertaken with genetically modified alga in a bioreactor.[157]

Safety and precautions

Main page: Chemistry:Hydrogen safety
Hydrogen
Hazards
GHS pictograms GHS02: Flammable
GHS Signal word Danger
H220
P202, P210, P271, P403, P377, P381[158]
NFPA 704 (fire diamond)
Flammability code 4: Will rapidly or completely vaporize at normal atmospheric pressure and temperature, or is readily dispersed in air and will burn readily. Flash point below 23 °C (73 °F). E.g. propaneHealth code 0: Exposure under fire conditions would offer no hazard beyond that of ordinary combustible material. E.g. sodium chlorideReactivity code 0: Normally stable, even under fire exposure conditions, and is not reactive with water. E.g. liquid nitrogenSpecial hazards (white): no codeNFPA 704 four-colored diamond
4
0
0
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
Infobox references

Hydrogen poses a number of hazards to human safety, from potential detonations and fires when mixed with air to being an asphyxiant in its pure, oxygen-free form.[159] In addition, liquid hydrogen is a cryogen and presents dangers (such as frostbite) associated with very cold liquids.[160] Hydrogen dissolves in many metals and in addition to leaking out, may have adverse effects on them, such as hydrogen embrittlement,[161] leading to cracks and explosions.[162] Hydrogen gas leaking into external air may spontaneously ignite. Moreover, hydrogen fire, while being extremely hot, is almost invisible, and thus can lead to accidental burns.[163]

Even interpreting the hydrogen data (including safety data) is confounded by a number of phenomena. Many physical and chemical properties of hydrogen depend on the parahydrogen/orthohydrogen ratio (it often takes days or weeks at a given temperature to reach the equilibrium ratio, for which the data is usually given). Hydrogen detonation parameters, such as critical detonation pressure and temperature, strongly depend on the container geometry.[159]

See also


Notes

  1. However, most of the universe's mass is not in the form of baryons or chemical elements. See dark matter and dark energy.
  2. 286 kJ/mol: energy per mole of the combustible material (molecular hydrogen).

References

  1. Wiberg, Egon; Wiberg, Nils; Holleman, Arnold Frederick (2001). Inorganic chemistry. Academic Press. p. 240. ISBN 978-0123526519. https://books.google.com/books?id=vEwj1WZKThEC&pg=PA240. 
  2. Lide, D. R., ed (2005). "Magnetic susceptibility of the elements and inorganic compounds". CRC Handbook of Chemistry and Physics (86th ed.). Boca Raton (FL): CRC Press. ISBN 978-0-8493-0486-6. https://web.archive.org/web/20110303222309/http://www-d0.fnal.gov/hardware/cal/lvps_info/engineering/elementmagn.pdf. 
  3. Weast, Robert (1984). CRC, Handbook of Chemistry and Physics. Boca Raton, Florida: Chemical Rubber Company Publishing. pp. E110. ISBN 978-0-8493-0464-4. 
  4. 4.0 4.1 4.2 "Hydrogen". Van Nostrand's Encyclopedia of Chemistry. Wylie-Interscience. 2005. pp. 797–799. ISBN 978-0-471-61525-5. 
  5. 5.00 5.01 5.02 5.03 5.04 5.05 5.06 5.07 5.08 5.09 5.10 5.11 Emsley, John (2001). Nature's Building Blocks. Oxford: Oxford University Press. pp. 183–191. ISBN 978-0-19-850341-5. 
  6. Stwertka, Albert (1996). A Guide to the Elements. Oxford University Press. pp. 16–21. ISBN 978-0-19-508083-4. 
  7. "Hydrogen" (in en). https://www.britannica.com/science/hydrogen. 
  8. Boyd, Padi (19 July 2014). "What is the chemical composition of stars?". NASA. https://imagine.gsfc.nasa.gov/ask_astro/stars.html#961112a. 
  9. Tanabashi et al. (2018) p. 358. Chpt. 21.4.1: "Big-Bang Cosmology" (Revised September 2017) by K.A. Olive and J.A. Peacock.[full citation needed]
  10. Laursen, S.; Chang, J.; Medlin, W.; Gürmen, N.; Fogler, H. S. (27 July 2004). "An extremely brief introduction to computational quantum chemistry". University of Michigan. http://www.umich.edu/~elements/5e/web_mod/quantum/introduction_3.htm. 
  11. Presenter: Professor Jim Al-Khalili (21 January 2010). "Discovering the Elements". Chemistry: A Volatile History. 25:40 minutes in. BBC. BBC Four. Archived from the original on 25 January 2010. Retrieved 9 February 2010.
  12. Dincer, Ibrahim; Acar, Canan (14 September 2015). "Review and evaluation of hydrogen production methods for better sustainability" (in en). International Journal of Hydrogen Energy 40 (34): 11094–11111. doi:10.1016/j.ijhydene.2014.12.035. ISSN 0360-3199. https://www.sciencedirect.com/science/article/pii/S0360319914034119. Retrieved 4 February 2022. 
  13. "Hydrogen Basics – Production". Florida Solar Energy Center. 2007. http://www.fsec.ucf.edu/en/consumer/hydrogen/basics/production.htm. 
  14. 14.0 14.1 14.2 14.3 14.4 14.5 Lewis, Alastair C. (10 June 2021). "Optimising air quality co-benefits in a hydrogen economy: a case for hydrogen-specific standards for NO x emissions" (in en). Environmental Science: Atmospheres 1 (5): 201–207. doi:10.1039/D1EA00037C.  This article incorporates text from this source, which is available under the CC BY 3.0 license.
  15. 15.0 15.1 Rogers, H. C. (1999). "Hydrogen Embrittlement of Metals". Science 159 (3819): 1057–1064. doi:10.1126/science.159.3819.1057. PMID 17775040. Bibcode1968Sci...159.1057R. 
  16. "Dihydrogen". O=CHem Directory. University of Southern Maine. http://www.usm.maine.edu/~newton/Chy251_253/Lectures/LewisStructures/Dihydrogen.html. 
  17. Committee on Alternatives and Strategies for Future Hydrogen Production and Use (2004). The Hydrogen Economy: Opportunities, Costs, Barriers, and R&D Needs. National Academies Press. p. 240. ISBN 978-0-309-09163-3. https://books.google.com/books?id=ugniowznToAC&pg=PA240. Retrieved 3 September 2020. 
  18. Carcassi, M. N.; Fineschi, F. (2005). "Deflagrations of H2–air and CH4–air lean mixtures in a vented multi-compartment environment". Energy 30 (8): 1439–1451. doi:10.1016/j.energy.2004.02.012. 
  19. Patnaik, P. (2007). A Comprehensive Guide to the Hazardous Properties of Chemical Substances. Wiley-Interscience. p. 402. ISBN 978-0-471-71458-3. https://books.google.com/books?id=-CRRJBVv5d0C&pg=PA402. Retrieved 3 September 2020. 
  20. Schefer, E. W.; Kulatilaka, W. D.; Patterson, B. D.; Settersten, T. B. (June 2009). "Visible emission of hydrogen flames". Combustion and Flame 156 (6): 1234–1241. doi:10.1016/j.combustflame.2009.01.011. https://zenodo.org/record/1258847. Retrieved 30 June 2019. 
  21. "Myths about the Hindenburg Crash" (in en-US). https://www.airships.net/hindenburg/disaster/myths/. 
  22. Lide, David R., ed (2006). CRC Handbook of Chemistry and Physics (87th ed.). Boca Raton, FL: CRC Press. ISBN 0-8493-0487-3. 
  23. Clayton, D. D. (2003). Handbook of Isotopes in the Cosmos: Hydrogen to Gallium. Cambridge University Press. ISBN 978-0-521-82381-4. 
  24. "Energy Levels". University of Nebraska Lincoln. 2009. http://astro.unl.edu/naap/hydrogen/levels.html. 
  25. "photon wavelength 13.6 eV". Wolfram Alpha. 20 May 2015. http://www.wolframalpha.com/input/?i=photon+wavelength+13.6+ev. 
  26. Stern, D. P. (16 May 2005). "The Atomic Nucleus and Bohr's Early Model of the Atom". NASA Goddard Space Flight Center (mirror). http://www.iki.rssi.ru/mirrors/stern/stargaze/Q5.htm. 
  27. Stern, D. P. (13 February 2005). "Wave Mechanics". NASA Goddard Space Flight Center. http://www-spof.gsfc.nasa.gov/stargaze/Q7.htm. 
  28. Staff (2003). "Hydrogen (H2) Properties, Uses, Applications: Hydrogen Gas and Liquid Hydrogen". Universal Industrial Gases, Inc.. http://www.uigi.com/hydrogen.html. 
  29. Green, Richard A. (2012). "The theory and practice of hyperpolarization in magnetic resonance using parahydrogen". Prog. Nucl. Magn. Reson. Spectrosc. 67: 1–48. doi:10.1016/j.pnmrs.2012.03.001. PMID 23101588. https://www.sciencedirect.com/science/article/abs/pii/S0079656512000477. Retrieved 28 August 2021. 
  30. "Die Entdeckung des para-Wasserstoffs (The discovery of para-hydrogen)" (in de). https://www.mpibpc.mpg.de/146336/para-Wasserstoff. 
  31. Milenko, Yu. Ya.; Sibileva, R. M.; Strzhemechny, M. A. (1997). "Natural ortho-para conversion rate in liquid and gaseous hydrogen". Journal of Low Temperature Physics 107 (1–2): 77–92. doi:10.1007/BF02396837. Bibcode1997JLTP..107...77M. 
  32. Hritz, J. (March 2006). "CH. 6 – Hydrogen". NASA Glenn Research Center Glenn Safety Manual, Document GRC-MQSA.001. NASA. http://smad-ext.grc.nasa.gov/gso/manual/chapter_06.pdf. 
  33. Amos, Wade A. (1 November 1998). "Costs of Storing and Transporting Hydrogen". National Renewable Energy Laboratory. pp. 6–9. http://www.nrel.gov/docs/fy99osti/25106.pdf. 
  34. Svadlenak, R. E.; Scott, A. B. (1957). "The Conversion of Ortho- to Parahydrogen on Iron Oxide-Zinc Oxide Catalysts". Journal of the American Chemical Society 79 (20): 5385–5388. doi:10.1021/ja01577a013. 
  35. Clark, J. (2002). "The Acidity of the Hydrogen Halides". Chemguide. http://www.chemguide.co.uk/inorganic/group7/acidityhx.html#top. 
  36. Kimball, J. W. (7 August 2003). "Hydrogen". Kimball's Biology Pages. http://users.rcn.com/jkimball.ma.ultranet/BiologyPages/H/HydrogenBonds.html. 
  37. IUPAC Compendium of Chemical Terminology, Electronic version, Hydrogen Bond
  38. Sandrock, G. (2 May 2002). "Metal-Hydrogen Systems". Sandia National Laboratories. http://hydpark.ca.sandia.gov/DBFrame.html. 
  39. 39.0 39.1 "Structure and Nomenclature of Hydrocarbons". Purdue University. http://chemed.chem.purdue.edu/genchem/topicreview/bp/1organic/organic.html. 
  40. "Organic Chemistry". Dictionary.com. Lexico Publishing Group. 2008. http://dictionary.reference.com/browse/organic%20chemistry. 
  41. "Biochemistry". Dictionary.com. Lexico Publishing Group. 2008. http://dictionary.reference.com/browse/biochemistry. 
  42. Takeshita, T.; Wallace, W. E.; Craig, R. S. (1974). "Hydrogen solubility in 1:5 compounds between yttrium or thorium and nickel or cobalt". Inorganic Chemistry 13 (9): 2282–2283. doi:10.1021/ic50139a050. 
  43. Kirchheim, R.; Mutschele, T.; Kieninger, W.; Gleiter, H.; Birringer, R.; Koble, T. (1988). "Hydrogen in amorphous and nanocrystalline metals". Materials Science and Engineering 99 (1–2): 457–462. doi:10.1016/0025-5416(88)90377-1. 
  44. Kirchheim, R. (1988). "Hydrogen solubility and diffusivity in defective and amorphous metals". Progress in Materials Science 32 (4): 262–325. doi:10.1016/0079-6425(88)90010-2. 
  45. Christensen, C. H.; Nørskov, J. K.; Johannessen, T. (9 July 2005). "Making society independent of fossil fuels – Danish researchers reveal new technology". Technical University of Denmark. http://news.mongabay.com/2005/0921-hydrogen_tablet.html. 
  46. Moers, K. (1920). "Investigations on the Salt Character of Lithium Hydride". Zeitschrift für Anorganische und Allgemeine Chemie 113 (191): 179–228. doi:10.1002/zaac.19201130116. https://zenodo.org/record/1428170. Retrieved 24 August 2019. 
  47. Downs, A. J.; Pulham, C. R. (1994). "The hydrides of aluminium, gallium, indium, and thallium: a re-evaluation". Chemical Society Reviews 23 (3): 175–184. doi:10.1039/CS9942300175. 
  48. Hibbs, D. E.; Jones, C.; Smithies, N. A. (1999). "A remarkably stable indium trihydride complex: synthesis and characterisation of [InH3P(C6H11)3]". Chemical Communications (2): 185–186. doi:10.1039/a809279f. 
  49. 49.0 49.1 49.2 Miessler, G. L.; Tarr, D. A. (2003). Inorganic Chemistry (3rd ed.). Prentice Hall. ISBN 978-0-13-035471-6. https://archive.org/details/inorganicchemist03edmies. 
  50. Okumura, A. M.; Yeh, L. I.; Myers, J. D.; Lee, Y. T. (1990). "Infrared spectra of the solvated hydronium ion: vibrational predissociation spectroscopy of mass-selected H3O+•(H2O)n•(H2)m". Journal of Physical Chemistry 94 (9): 3416–3427. doi:10.1021/j100372a014. 
  51. Perdoncin, G.; Scorrano, G. (1977). "Protonation Equilibria in Water at Several Temperatures of Alcohols, Ethers, Acetone, Dimethyl Sulfide, and Dimethyl Sulfoxide". Journal of the American Chemical Society 99 (21): 6983–6986. doi:10.1021/ja00463a035. 
  52. Carrington, A.; McNab, I. R. (1989). "The infrared predissociation spectrum of triatomic hydrogen cation (H3+)". Accounts of Chemical Research 22 (6): 218–222. doi:10.1021/ar00162a004. 
  53. Gurov, Y. B.; Aleshkin, D. V.; Behr, M. N.; Lapushkin, S. V.; Morokhov, P. V.; Pechkurov, V. A.; Poroshin, N. O.; Sandukovsky, V. G. et al. (2004). "Spectroscopy of superheavy hydrogen isotopes in stopped-pion absorption by nuclei". Physics of Atomic Nuclei 68 (3): 491–97. doi:10.1134/1.1891200. Bibcode2005PAN....68..491G. 
  54. Korsheninnikov, A.; Nikolskii, E.; Kuzmin, E.; Ozawa, A.; Morimoto, K.; Tokanai, F.; Kanungo, R.; Tanihata, I. et al. (2003). "Experimental Evidence for the Existence of 7H and for a Specific Structure of 8He". Physical Review Letters 90 (8): 082501. doi:10.1103/PhysRevLett.90.082501. PMID 12633420. Bibcode2003PhRvL..90h2501K. 
  55. Urey, H. C.; Brickwedde, F. G.; Murphy, G. M. (1933). "Names for the Hydrogen Isotopes". Science 78 (2035): 602–603. doi:10.1126/science.78.2035.602. PMID 17797765. Bibcode1933Sci....78..602U. 
  56. Oda, Y.; Nakamura, H.; Yamazaki, T.; Nagayama, K.; Yoshida, M.; Kanaya, S.; Ikehara, M. (1992). "1H NMR studies of deuterated ribonuclease HI selectively labeled with protonated amino acids". Journal of Biomolecular NMR 2 (2): 137–47. doi:10.1007/BF01875525. PMID 1330130. 
  57. Broad, W. J. (11 November 1991). "Breakthrough in Nuclear Fusion Offers Hope for Power of Future". The New York Times. https://query.nytimes.com/gst/fullpage.html?res=9D0CE4D81030F932A25752C1A967958260. 
  58. 58.0 58.1 Traub, R. J.; Jensen, J. A. (June 1995). "Tritium radioluminescent devices, Health and Safety Manual". International Atomic Energy Agency. p. 2.4. http://www.iaea.org/inis/collection/NCLCollectionStore/_Public/27/001/27001618.pdf. 
  59. Staff (15 November 2007). "Tritium". U.S. Environmental Protection Agency. http://www.epa.gov/rpdweb00/radionuclides/tritium.html. 
  60. Nave, C. R. (2006). "Deuterium-Tritium Fusion". HyperPhysics. Georgia State University. http://hyperphysics.phy-astr.gsu.edu/Hbase/nucene/fusion.html. 
  61. Kendall, C.; Caldwell, E. (1998). "Chapter 2: Fundamentals of Isotope Geochemistry". Isotope Tracers in Catchment Hydrology (US Geological Survey): 51–86. doi:10.1016/B978-0-444-81546-0.50009-4. http://wwwrcamnl.wr.usgs.gov/isoig/isopubs/itchch2.html#2.5.1. Retrieved 8 March 2008. 
  62. "The Tritium Laboratory". University of Miami. 2008. http://www.rsmas.miami.edu/groups/tritium/. 
  63. 63.0 63.1 Holte, A. E.; Houck, M. A.; Collie, N. L. (2004). "Potential Role of Parasitism in the Evolution of Mutualism in Astigmatid Mites". Experimental and Applied Acarology 25 (2): 97–107. doi:10.1023/A:1010655610575. PMID 11513367. 
  64. van der Krogt, P. (5 May 2005). "Hydrogen". Elementymology & Elements Multidict. http://elements.vanderkrogt.net/element.php?sym=H. 
  65. § IR-3.3.2, Provisional Recommendations , Nomenclature of Inorganic Chemistry, Chemical Nomenclature and Structure Representation Division, IUPAC. Accessed on line 3 October 2007.
  66. IUPAC (1997). "Muonium". in A.D. McNaught, A. Wilkinson. Compendium of Chemical Terminology (2nd ed.). Blackwell Scientific Publications. doi:10.1351/goldbook.M04069. ISBN 978-0-86542-684-9. http://goldbook.iupac.org/M04069.html. Retrieved 15 November 2016. 
  67. V.W. Hughes (1960). "Formation of Muonium and Observation of its Larmor Precession". Physical Review Letters 5 (2): 63–65. doi:10.1103/PhysRevLett.5.63. Bibcode1960PhRvL...5...63H. 
  68. Bondi, D.K.; Connor, J.N.L.; Manz, J.; Römelt, J. (20 October 1983). "Exact quantum and vibrationally adiabatic quantum, semiclassical and quasiclassical study of the collinear reactions Cl + MuCl, Cl + HCl, Cl + DCl". Molecular Physics 50 (3): 467–488. doi:10.1080/00268978300102491. ISSN 0026-8976. Bibcode1983MolPh..50..467B. 
  69. W.H. Koppenol; IUPAC (2001). "Names for muonium and hydrogen atoms and their ions". Pure and Applied Chemistry 73 (2): 377–380. doi:10.1351/pac200173020377. http://www.iupac.org/publications/pac/2001/pdf/7302x0377.pdf. Retrieved 15 November 2016. 
  70. Holman, Jack P. (2002) (in English). Heat transfer (9th ed.). New York, NY: McGraw-Hill. pp. 600–606. ISBN 0-07-240655-0. OCLC 46959719. https://www.worldcat.org/oclc/46959719. 
  71. Incropera 1 Dewitt 2 Bergman 3 Lavigne 4, Frank P. 1 David P. 2 Theodore L. 3 Adrienne S. 4 (2007) (in English). Fundamentals of heat and mass transfer. (6th ed.). Hoboken, NJ: John Wiley and Sons, Inc.. pp. 941–950. ISBN 978-0-471-45728-2. OCLC 62532755. https://www.worldcat.org/oclc/62532755. 
  72. Boyle, R. (1672). Tracts written by the Honourable Robert Boyle containing new experiments, touching the relation betwixt flame and air, and about explosions, an hydrostatical discourse occasion'd by some objections of Dr. Henry More against some explications of new experiments made by the author of these tracts: To which is annex't, an hydrostatical letter, dilucidating an experiment about a way of weighing water in water, new experiments, of the positive or relative levity of bodies under water, of the air's spring on bodies under water, about the differing pressure of heavy solids and fluids. Printed for Richard Davis. pp. 64–65. https://quod.lib.umich.edu/e/eebo2/A29057.0001.001?rgn=main;view=fulltext. 
  73. Winter, M. (2007). "Hydrogen: historical information". WebElements Ltd. http://education.jlab.org/itselemental/ele001.html. 
  74. Szydło, Z. A. (2020). "Hydrogen - Some Historical Highlights". Chemistry-Didactics-Ecology-Metrology 25 (1–2): 5–34. doi:10.2478/cdem-2020-0001. 
  75. Ramsay, W. (1896). The gases of the atmosphere: The history of their discovery. Macmillan. pp. 19. https://www.gutenberg.org/files/52778/52778-h/52778-h.htm. 
  76. Musgrave, A. (1976). "Why did oxygen supplant phlogiston? Research programmes in the Chemical Revolution". in Howson, C.. Method and appraisal in the physical sciences. The Critical Background to Modern Science, 1800–1905. Cambridge University Press. doi:10.1017/CBO9780511760013. ISBN 978-0-521-21110-9. http://ebooks.cambridge.org/chapter.jsf?bid=CBO9780511760013&cid=CBO9780511760013A009. Retrieved 22 October 2011. 
  77. Cavendish, Henry (12 May 1766). "Three Papers, Containing Experiments on Factitious Air, by the Hon. Henry Cavendish, F. R. S.". Philosophical Transactions 56: 141–184. doi:10.1098/rstl.1766.0019. Bibcode1766RSPT...56..141C. 
  78. Stwertka, Albert (1996). A Guide to the Elements. Oxford University Press. pp. 16–21. ISBN 978-0-19-508083-4. https://archive.org/details/guidetoelements00stwe. 
  79. National Electrical Manufacturers Association (1946). A chronological history of electrical development from 600 B.C. New York, N.Y., National Electrical Manufacturers Association. p. 102. https://archive.org/stream/chronologicalhis00natirich/chronologicalhis00natirich_djvu.txt. Retrieved 9 February 2016. 
  80. Stockel, J.F; j.d. Dunlop; Betz, F (1980). "NTS-2 Nickel-Hydrogen Battery Performance 31". Journal of Spacecraft and Rockets 17: 31–34. doi:10.2514/3.57704. Bibcode1980JSpRo..17...31S. 
  81. Jannette, A. G.; Hojnicki, J. S.; McKissock, D. B.; Fincannon, J.; Kerslake, T. W.; Rodriguez, C. D. (July 2002). "Validation of international space station electrical performance model via on-orbit telemetry". pp. 45–50. doi:10.1109/IECEC.2002.1391972. ISBN 0-7803-7296-4. https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/20020070612_2002115777.pdf. Retrieved 11 November 2011. 
  82. Anderson, P. M.; Coyne, J. W. (2002). "A lightweight, high reliability, single battery power system for interplanetary spacecraft". Proceedings, IEEE Aerospace Conference. 5. pp. 5–2433. doi:10.1109/AERO.2002.1035418. ISBN 978-0-7803-7231-3. 
  83. "Mars Global Surveyor". Astronautix.com. http://www.astronautix.com/craft/marveyor.htm. 
  84. Lori Tyahla, ed (7 May 2009). "Hubble servicing mission 4 essentials". NASA. http://www.nasa.gov/mission_pages/hubble/servicing/SM4/main/SM4_Essentials.html. 
  85. Hendrix, Susan (25 November 2008). "Extending Hubble's mission life with new batteries". in Lori Tyahla. NASA. http://www.nasa.gov/mission_pages/hubble/servicing/series/battery_story.html. 
  86. Crepeau, R. (1 January 2006). Niels Bohr: The Atomic Model. ISBN 978-1-4298-0723-4. 
  87. Berman, R.; Cooke, A. H.; Hill, R. W. (1956). "Cryogenics". Annual Review of Physical Chemistry 7: 1–20. doi:10.1146/annurev.pc.07.100156.000245. Bibcode1956ARPC....7....1B. 
  88. Charlton, Mike; Van Der Werf, Dirk Peter (1 March 2015). "Advances in antihydrogen physics". Science Progress 98 (1): 34–62. doi:10.3184/003685015X14234978376369. PMID 25942774. 
  89. Kellerbauer, Alban (29 January 2015). "Why Antimatter Matters". European Review 23 (1): 45–56. doi:10.1017/S1062798714000532. 
  90. Gagnon, S.. "Hydrogen". Jefferson Lab. http://education.jlab.org/itselemental/ele001.html. 
  91. Haubold, H.; Mathai, A. M. (15 November 2007). "Solar Thermonuclear Energy Generation". Columbia University. http://neutrino.aquaphoenix.com/un-esa/sun/sun-chapter4.html. 
  92. "Hydrogen". http://mysite.du.edu/~jcalvert/phys/hydrogen.htm. 
  93. Storrie-Lombardi, L. J.; Wolfe, A. M. (2000). "Surveys for z > 3 Damped Lyman-alpha Absorption Systems: the Evolution of Neutral Gas". Astrophysical Journal 543 (2): 552–576. doi:10.1086/317138. Bibcode2000ApJ...543..552S. 
  94. 94.0 94.1 Rhys Grinter et al. (2023). "Structural basis for bacterial energy extraction from atmospheric hydrogen". Nature 615 (7952): 541–547. doi:10.1038/s41586-023-05781-7. PMID 36890228. Bibcode2023Natur.615..541G. 
  95. Dresselhaus, M. (15 May 2003). "Basic Research Needs for the Hydrogen Economy". APS March Meeting Abstracts (Argonne National Laboratory, U.S. Department of Energy, Office of Science Laboratory) 2004: m1.001. Bibcode2004APS..MAR.m1001D. http://www.sc.doe.gov/bes/hydrogen.pdf. Retrieved 5 February 2008. 
  96. McCall Group; Oka Group (22 April 2005). "H3+ Resource Center". Universities of Illinois and Chicago. http://h3plus.uiuc.edu/. 
  97. Helm, H. (2003), "Coupling of Bound States to Continuum States in Neutral Triatomic Hydrogen", Dissociative Recombination of Molecular Ions with Electrons, Department of Molecular and Optical Physics, University of Freiburg, Germany, pp. 275–288, doi:10.1007/978-1-4615-0083-4_27, ISBN 978-1-4613-4915-0 
  98. 98.0 98.1 Baade, William F.; Parekh, Uday N.; Raman, Venkat S. (2001). "Hydrogen". Kirk-Othmer Encyclopedia of Chemical Technology. doi:10.1002/0471238961.0825041803262116.a01.pub2. ISBN 9780471484943. 
  99. Freyermuth, George H. "1934 Patent: "The manufacture of hydrogen from methane hydrocarbons by the action of steam at elevated temperature"". United States Patent and Trademark Office. http://patft.uspto.gov/netacgi/nph-Parser?Sect1=PTO1&Sect2=HITOFF&p=1&u=/netahtml/PTO/srchnum.html&r=1&f=G&l=50&d=PALL&s1=1970695.PN.. 
  100. Press, Roman J.; Santhanam, K. S. V.; Miri, Massoud J.; Bailey, Alla V.; Takacs, Gerald A. (2008). Introduction to Hydrogen Technology. John Wiley & Sons. pp. 249. ISBN 978-0-471-77985-8. https://archive.org/details/introductiontohy0000unse/page/249/mode/2up. 
  101. 101.0 101.1 101.2 Oxtoby, D. W. (2002). Principles of Modern Chemistry (5th ed.). Thomson Brooks/Cole. ISBN 978-0-03-035373-4. 
  102. Funderburg, E. (2008). "Why Are Nitrogen Prices So High?". The Samuel Roberts Noble Foundation. http://www.noble.org/Ag/Soils/NitrogenPrices/Index.htm. 
  103. "Hydrogen Properties, Uses, Applications". Universal Industrial Gases, Inc.. 2007. http://www.uigi.com/hydrogen.html. 
  104. Hannula, Ilkka (2015). "Co-production of synthetic fuels and district heat from biomass residues, carbon dioxide and electricity: Performance and cost analysis". Biomass and Bioenergy 74: 26–46. doi:10.1016/j.biombioe.2015.01.006. ISSN 0961-9534. http://dx.doi.org/10.1016/j.biombioe.2015.01.006. 
  105. Gong, Ming; Zhou, Wu; Tsai, Mon-Che; Zhou, Jigang; Guan, Mingyun; Lin, Meng-Chang; Zhang, Bo; Hu, Yongfeng et al. (2014). "Nanoscale nickel oxide/Nickel heterostructures for active hydrogen evolution electrocatalysis". Nature Communications 5: 4695. doi:10.1038/ncomms5695. PMID 25146255. Bibcode2014NatCo...5.4695G. 
  106. Lees, A. (2007). "Chemicals from salt". BBC. http://www.bbc.co.uk/schools/gcsebitesize/chemistry/usefulproductsrocks/chemicals_saltrev3.shtml. 
  107. Von Wald, Gregory A. (2020). "Optimization-based technoeconomic analysis of molten-media methane pyrolysis for reducing industrial sector CO2 emissions". Sustainable Energy & Fuels (Royal Society of Chemistry) 4 (9): 4598–4613. doi:10.1039/D0SE00427H. https://pubs.rsc.org/en/content/articlelanding/2020/SE/D0SE00427H. Retrieved 31 October 2020. 
  108. Schneider, Stefan (2020). "State of the Art of Hydrogen Production via Pyrolysis of Natural Gas". ChemBioEng Reviews (Wiley Online Library) 7 (5): 150–158. doi:10.1002/cben.202000014. 
  109. Cartwright, Jon. "The reaction that would give us clean fossil fuels forever". https://www.newscientist.com/article/mg23230940-200-crack-methane-for-fossil-fuels-without-tears/. 
  110. Karlsruhe Institute of Technology. "Hydrogen from methane without CO2 emissions". https://phys.org/news/2013-04-hydrogen-methane-co2-emissions.html. 
  111. Upham, D. Chester (2017). "Catalytic molten metals for the direct conversion of methane to hydrogen and separable carbon". Science (American Association for Advancement of Science) 358 (6365): 917–921. doi:10.1126/science.aao5023. PMID 29146810. Bibcode2017Sci...358..917U. 
  112. Clarke, Palmer (2020). "Dry reforming of methane catalyzed by molten metal alloys". Nature Catalysis 3: 83–89. doi:10.1038/s41929-019-0416-2. https://www.nature.com/articles/s41929-019-0416-2. Retrieved 31 October 2020. 
  113. Gusev, Alexander. "KITT/IASS – Producing CO2 Free Hydrogen From Natural Gas For Energy Usage". Institute for Advanced Sustainability Studies. http://www.europeanenergyinnovation.eu/Latest-Research/Spring-2019/KITT-IASS-Producing-CO2-free-hydrogen-from-natural-gas-for-energy-usage. 
  114. Fernandez, Sonia. "Researchers develop potentially low-cost, low-emissions technology that can convert methane without forming CO2". American Institute of Physics. https://phys.org/news/2017-11-potentially-low-cost-low-emissions-technology-methane.html. 
  115. BASF. "BASF researchers working on fundamentally new, low-carbon production processes, Methane Pyrolysis". BASF. https://www.basf.com/us/en/who-we-are/sustainability/we-produce-safely-and-efficiently/energy-and-climate-protection/carbon-management/interview-methane-pyrolysis.html. 
  116. Weimer, Al (25 May 2005). "Development of solar-powered thermochemical production of hydrogen from water". Solar Thermochemical Hydrogen Generation Project. http://www.hydrogen.energy.gov/pdfs/review05/pd28_weimer.pdf. 
  117. Perret, R.. "Development of Solar-Powered Thermochemical Production of Hydrogen from Water, DOE Hydrogen Program, 2007". http://www.hydrogen.energy.gov/pdfs/progress07/ii_f_1_perret.pdf. 
  118. Parmuzina, A.V.; Kravchenko, O.V. (2008). "Activation of aluminium metal to evolve hydrogen from water". International Journal of Hydrogen Energy 33 (12): 3073–3076. doi:10.1016/j.ijhydene.2008.02.025. 
  119. Lubitz, Wolfgang; Reijerse, Eduard; Van Gastel, Maurice (2007). "[NiFe] and [FeFe] Hydrogenases Studied by Advanced Magnetic Resonance Techniques". Chemical Reviews 107 (10): 4331–4365. doi:10.1021/cr050186q. PMID 17845059. 
  120. "Natural Hydrogen: A Potential Clean Energy Source Beneath Our Feet" (in en-US). https://e360.yale.edu/features/natural-geologic-hydrogen-climate-change. 
  121. Smil, Vaclav (2004). Enriching the Earth: Fritz Haber, Carl Bosch, and the Transformation of World Food Production (1st ed.). Cambridge, MA: MIT. ISBN 978-0-262-69313-4. 
  122. Chemistry Operations (15 December 2003). "Hydrogen". Los Alamos National Laboratory. http://periodic.lanl.gov/1.shtml. 
  123. 123.0 123.1 123.2 123.3 123.4 IPCC (2022). Shukla, P.R.; Skea, J.; Slade, R. et al.. eds. Climate Change 2022: Mitigation of Climate Change. Contribution of Working Group III to the Sixth Assessment Report of the Intergovernmental Panel on Climate Change. Cambridge, UK and New York, NY, US: Cambridge University Press (In Press). pp. 91–92. doi:10.1017/9781009157926. ISBN 9781009157926. https://ipcc.ch/report/ar6/wg3/downloads/report/IPCC_AR6_WGIII_FullReport.pdf. 
  124. 124.0 124.1 Evans, Simon; Gabbatiss, Josh (30 November 2020). "In-depth Q&A: Does the world need hydrogen to solve climate change?". https://www.carbonbrief.org/in-depth-qa-does-the-world-need-hydrogen-to-solve-climate-change. 
  125. McCarthy, J. (31 December 1995). "Hydrogen". Stanford University. http://www-formal.stanford.edu/jmc/progress/hydrogen.html. 
  126. Reed, Stanley; Ewing, Jack (2021-07-13). "Hydrogen Is One Answer to Climate Change. Getting It Is the Hard Part.". The New York Times. ISSN 0362-4331. https://www.nytimes.com/2021/07/13/business/hydrogen-climate-change.html. 
  127. IRENA (2019). Hydrogen: A renewable energy perspective. p. 9. ISBN 978-92-9260-151-5. https://www.irena.org/-/media/Files/IRENA/Agency/Publication/2019/Sep/IRENA_Hydrogen_2019.pdf. Retrieved 17 October 2021. .
  128. Bonheure, Mike; Vandewalle, Laurien A.; Marin, Guy B.; Van Geem, Kevin M. (March 2021). "Dream or Reality? Electrification of the Chemical Process Industries". American Institute of Chemical Engineers. https://www.aiche-cep.com/cepmagazine/march_2021/MobilePagedArticle.action?articleId=1663852. 
  129. 129.0 129.1 Griffiths, Steve; Sovacool, Benjamin K.; Kim, Jinsoo; Bazilian, Morgan et al. (2021). "Industrial decarbonization via hydrogen: A critical and systematic review of developments, socio-technical systems and policy options". Energy Research & Social Science 80: 39. doi:10.1016/j.erss.2021.102208. ISSN 2214-6296. https://www.sciencedirect.com/science/article/pii/S2214629621003017?dgcid=coauthor. Retrieved 11 September 2021. 
  130. Palys, Matthew J.; Daoutidis, Prodromos (2020). "Using hydrogen and ammonia for renewable energy storage: A geographically comprehensive techno-economic study". Computers & Chemical Engineering 136: 106785. doi:10.1016/j.compchemeng.2020.106785. ISSN 0098-1354. 
  131. "Hydrogen industry must clean itself up before expanding into new…" (in en). 31 August 2021. https://www.canarymedia.com/articles/hydrogen/hydrogen-industry-must-clean-itself-up-before-expanding-into-new-uses-report-finds. 
  132. IRENA (2021). World Energy Transitions Outlook: 1.5°C Pathway. pp. 12, 22. ISBN 978-92-9260-334-2. https://www.irena.org/-/media/Files/IRENA/Agency/Publication/2021/March/IRENA_World_Energy_Transitions_Outlook_2021.pdf. 
  133. IEA (2021). Net Zero by 2050: A Roadmap for the Global Energy Sector. pp. 15, 75–76. https://iea.blob.core.windows.net/assets/ad0d4830-bd7e-47b6-838c-40d115733c13/NetZeroby2050-ARoadmapfortheGlobalEnergySector.pdf. 
  134. Kjellberg-Motton, Brendan (2022-02-07). "Steel decarbonisation gathers speed | Argus Media" (in en). https://www.argusmedia.com/en//news/2299399-steel-decarbonisation-gathers-speed. 
  135. Blank, Thomas; Molly, Patrick (January 2020). "Hydrogen's Decarbonization Impact for Industry". Rocky Mountain Institute. pp. 2, 7, 8. https://rmi.org/wp-content/uploads/2020/01/hydrogen_insight_brief.pdf. 
  136. Plötz, Patrick (2022-01-31). "Hydrogen technology is unlikely to play a major role in sustainable road transport" (in en). Nature Electronics 5 (1): 8–10. doi:10.1038/s41928-021-00706-6. ISSN 2520-1131. https://www.nature.com/articles/s41928-021-00706-6. 
  137. Le Comber, P. G.; Jones, D. I.; Spear, W. E. (1977). "Hall effect and impurity conduction in substitutionally doped amorphous silicon". Philosophical Magazine 35 (5): 1173–1187. doi:10.1080/14786437708232943. Bibcode1977PMag...35.1173C. 
  138. Van de Walle, C. G. (2000). "Hydrogen as a cause of doping in zinc oxide". Physical Review Letters 85 (5): 1012–1015. doi:10.1103/PhysRevLett.85.1012. PMID 10991462. Bibcode2000PhRvL..85.1012V. http://pubman.mpdl.mpg.de/pubman/item/escidoc:741885/component/escidoc:932688/PRL-85-1012-2000.pdf. Retrieved 1 August 2018. 
  139. Janotti, A.; Van De Walle, C. G. (2007). "Hydrogen multicentre bonds". Nature Materials 6 (1): 44–47. doi:10.1038/nmat1795. PMID 17143265. Bibcode2007NatMa...6...44J. 
  140. Kilic, C.; Zunger, Alex (2002). "n-type doping of oxides by hydrogen". Applied Physics Letters 81 (1): 73–75. doi:10.1063/1.1482783. Bibcode2002ApPhL..81...73K. 
  141. Peacock, P. W.; Robertson, J. (2003). "Behavior of hydrogen in high dielectric constant oxide gate insulators". Applied Physics Letters 83 (10): 2025–2027. doi:10.1063/1.1609245. Bibcode2003ApPhL..83.2025P. 
  142. Durgutlu, A. (2003). "Experimental investigation of the effect of hydrogen in argon as a shielding gas on TIG welding of austenitic stainless steel". Materials & Design 25 (1): 19–23. doi:10.1016/j.matdes.2003.07.004. 
  143. "Atomic Hydrogen Welding". Specialty Welds. 2007. http://www.specialwelds.com/underwater-welding/atomic-hydrogen-welding.htm. 
  144. Hardy, W. N. (2003). "From H2 to cryogenic H masers to HiTc superconductors: An unlikely but rewarding path". Physica C: Superconductivity 388–389: 1–6. doi:10.1016/S0921-4534(02)02591-1. Bibcode2003PhyC..388....1H. 
  145. Almqvist, Ebbe (2003). History of industrial gases. New York, N.Y.: Kluwer Academic/Plenum Publishers. pp. 47–56. ISBN 978-0-306-47277-0. https://books.google.com/books?id=OI0fTJhydh4C. Retrieved 20 May 2015. 
  146. Block, M. (3 September 2004). "Hydrogen as Tracer Gas for Leak Detection". Montreal, Canada: Sensistor Technologies. http://www.ndt.net/abstract/wcndt2004/523.htm. Retrieved 25 March 2008. 
  147. "Report from the Commission on Dietary Food Additive Intake". European Union. http://ec.europa.eu/food/fs/sfp/addit_flavor/flav15_en.pdf. 
  148. Reinsch, J.; Katz, A.; Wean, J.; Aprahamian, G.; MacFarland, J. T. (1980). "The deuterium isotope effect upon the reaction of fatty acyl-CoA dehydrogenase and butyryl-CoA". J. Biol. Chem. 255 (19): 9093–97. doi:10.1016/S0021-9258(19)70531-6. PMID 7410413. 
  149. "NASA/TM—2002-211915: Solid Hydrogen Experiments for Atomic Propellants". https://ntrs.nasa.gov/api/citations/20030005922/downloads/20030005922.pdf. 
  150. Bergeron, K. D. (2004). "The Death of no-dual-use". Bulletin of the Atomic Scientists 60 (1): 15–17. doi:10.2968/060001004. Bibcode2004BuAtS..60a..15B. http://find.galegroup.com/itx/start.do?prodId=SPJ.SP06. Retrieved 13 April 2008. 
  151. Cammack, R.; Robson, R. L. (2001). Hydrogen as a Fuel: Learning from Nature. Taylor & Francis Ltd. pp. 202–203. ISBN 978-0-415-24242-4. https://books.google.com/books?id=GTzajKoBoNwC&pg=PA202. Retrieved 3 September 2020. 
  152. Rhee, T. S.; Brenninkmeijer, C. A. M.; Röckmann, T. (19 May 2006). "The overwhelming role of soils in the global atmospheric hydrogen cycle". Atmospheric Chemistry and Physics 6 (6): 1611–1625. doi:10.5194/acp-6-1611-2006. Bibcode2006ACP.....6.1611R. https://hal.archives-ouvertes.fr/hal-00301903/file/acpd-5-11215-2005.pdf. Retrieved 24 August 2019. 
  153. Alex Wilkins (Mar 8, 2023). "Soil bacteria enzyme generates electricity from hydrogen in the air". New Scientist 257 (3430): 13. doi:10.1016/S0262-4079(23)00459-1. Bibcode2023NewSc.257...13W. https://www.newscientist.com/article/2363552-soil-bacteria-enzyme-generates-electricity-from-hydrogen-in-the-air/. 
  154. Eisenmann, Alexander; Amann, Anton; Said, Michael; Datta, Bettina; Ledochowski, Maximilian (2008). "Implementation and interpretation of hydrogen breath tests". Journal of Breath Research 2 (4): 046002. doi:10.1088/1752-7155/2/4/046002. PMID 21386189. Bibcode2008JBR.....2d6002E. http://pdfs.semanticscholar.org/2f16/5a981d54c41da92c1ae81af44021a88f1b95.pdf. Retrieved 26 December 2020. 
  155. Kruse, O.; Rupprecht, J.; Bader, K.; Thomas-Hall, S.; Schenk, P. M.; Finazzi, G.; Hankamer, B. (2005). "Improved photobiological H2 production in engineered green algal cells". The Journal of Biological Chemistry 280 (40): 34170–7. doi:10.1074/jbc.M503840200. PMID 16100118. http://espace.library.uq.edu.au/view/UQ:75490/UQ75490_OA.pdf. Retrieved 24 August 2019. 
  156. Smith, Hamilton O.; Xu, Qing (2005). "IV.E.6 Hydrogen from Water in a Novel Recombinant Oxygen-Tolerant Cyanobacteria System". FY2005 Progress Report. United States Department of Energy. http://www.hydrogen.energy.gov/pdfs/progress05/iv_e_6_smith.pdf. 
  157. Williams, C. (24 February 2006). "Pond life: the future of energy". Science (The Register). https://www.theregister.co.uk/2006/02/24/pond_scum_breakthrough/. 
  158. "MyChem: Chemical". http://isolab.ess.washington.edu/isolab/images/documents/msds_sds/hydrogen.pdf. 
  159. 159.0 159.1 Brown, W. J. (1997). "Safety Standard for Hydrogen and Hydrogen Systems". https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19970033338.pdf. 
  160. "Liquid Hydrogen MSDS". Praxair, Inc.. September 2004. http://www.hydrogenandfuelcellsafety.info/resources/mdss/Praxair-LH2.pdf. 
  161. "'Bugs' and hydrogen embrittlement". Science News 128 (3): 41. 20 July 1985. doi:10.2307/3970088. 
  162. Hayes, B.. "Union Oil Amine Absorber Tower". TWI. http://www.twi.co.uk/content/oilgas_casedown29.html. 
  163. Walker, James L.; Waltrip, John S.; Zanker, Adam (1988). "Lactic acid to magnesium supply-demand relationships". Encyclopedia of Chemical Processing and Design. 28. New York: Dekker. p. 186. ISBN 978-0-8247-2478-8. https://books.google.com/books?id=8erDL_DnsgAC&pg=PAPA186. Retrieved 20 May 2015. 

Further reading

External links