Physics:Hartree

From HandWiki

The hartree (symbol: Eh), also known as the Hartree energy, is the unit of energy in the atomic units system, named after the British physicist Douglas Hartree. Its CODATA recommended value is Eh = 4.3597447222071(85)×10−18 J[1] = . The name "hartree" was suggested for this unit of energy.[2][3]

The hartree is approximately the negative electric potential energy of the electron in a hydrogen atom in its ground state and, by the virial theorem, approximately twice its ionization energy; the relationships are not exact because of the finite mass of the nucleus of the hydrogen atom and relativistic corrections.

The hartree is usually used as a unit of energy in atomic physics and computational chemistry: for experimental measurements at the atomic scale, the electronvolt (eV) or the reciprocal centimetre (cm−1) are much more widely used.

Other relationships

Eh=2mea02=me(e24πε0)2=mec2α2=cαa0
= 2 Ry = 2 Rhc
=
= 4.3597447222071(85)×10−18 J[1]
= 4.3597447222060(48)×10−11 erg
2625.4996394799(50) kJ/mol
627.5094740631(12) kcal/mol
219474.63136320(43) cm−1
6579.683920502(13) THz

where:

Effective hartree units are used in semiconductor physics where e2 is replaced by e2/ε and ε is the static dielectric constant. Also, the electron mass is replaced by the effective band mass m*. The effective hartree in semiconductors becomes small enough to be measured in millielectronvolts (meV).[4]

References

  1. 1.0 1.1 "2018 CODATA Value: Hartree energy". The NIST Reference on Constants, Units, and Uncertainty. NIST. 20 May 2019. http://physics.nist.gov/cgi-bin/cuu/Value?hr. Retrieved 2019-05-20. 
  2. Shull, H.; Hall, G.G. (1959). "Atomic Units". Nature (Nature Publishing Group) 184 (4698): 1559–1560. doi:10.1038/1841559a0. Bibcode1959Natur.184.1559S. 
  3. McWeeny, R. (May 1973). "Natural Units in Atomic and Molecular Physics" (in en). Nature 243 (5404): 196–198. doi:10.1038/243196a0. ISSN 0028-0836. Bibcode1973Natur.243..196M. https://www.nature.com/articles/243196a0. 
  4. Tsuneya Ando, Alan B. Fowler, and Frank Stern Rev. Mod. Phys. 54, 437 (1982)