Physics:Bose–Einstein condensation of quasiparticles

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Short description: Occurrence in collective excitations

Bose–Einstein condensation can occur in quasiparticles, particles that are effective descriptions of collective excitations in materials. Some have integer spins and can be expected to obey Bose–Einstein statistics like traditional particles. Conditions for condensation of various quasiparticles have been predicted and observed. The topic continues to be an active field of study.

Properties

BECs form when low temperatures cause nearly all particles to occupy the lowest quantum state. Condensation of quasiparticles occurs in ultracold gases and materials. The lower masses of material quasiparticles relative to atoms lead to higher BEC temperatures. An ideal Bose gas has a phase transitions when inter-particle spacing approaches the thermal De-Broglie wavelength: [math]\displaystyle{ k_B T =~ \hbar^2 n^{2/3}/M }[/math]. The critical concentration is then [math]\displaystyle{ N \propto (T/2 \pi)^3 u^{1/2} P / v \hbar^3 }[/math], leading to a critical temperature: [math]\displaystyle{ T_c \lt 32\pi^3 \hbar^6 V^2u_0P^2 }[/math]. The particles obey the Bose–Einstein distribution and all occupy the ground state:

The Bose gas can be considered in a harmonic trap, [math]\displaystyle{ V(r) = M \omega^2 /2 }[/math], with the ground state occupancy fraction as a function of temperature:

[math]\displaystyle{ f(0) = \frac{N_0(t)} N = 1 - \left( \frac T {T_c} \right)^3 }[/math]

This can be achieved by cooling and magnetic or optical control of the system. Spectroscopy can detect shifts in peaks indicating thermodynamic phases with condensation. Quasiparticle BEC can be superfluids. Signs of such states include spatial and temporal coherence and polarization changes. Observation for excitons in solids was seen in 2005 and for magnons in materials and polaritons in microcavities in 2006. Graphene is another important solid state system for studies of condensed matter including quasi particles; It's a 2D electron gas, similar to other thin films.[1][2]

Excitons

Excitons are electron-hole pairs. Similar to helium-4 superfluidity[3] at the [math]\displaystyle{ \lambda }[/math]-point (2.17K);[4][5] a condensate was proposed by Böer et al. in 1961.[6] Experimental phenomenon were predicted leading to various pulsed laser searches that failed to produce evidence. Signs were first seen by Fuzukawa et al. in 1990, but definite detection was published later in the 2000s. Condensed excitons are a superfluid and will not interact with phonons. While the normal exciton absorption is broadened by phonons, in the superfluid absorption degenerates to a line.

Theory

Excitons results from photons exciting electrons creating holes, which are then attracted and can form bound states. The 1s paraexciton and orthoexciton are possible. The 1s triplet spin state, 12.1meV below the degenerate orthoexciton states(lifetime ~ns), is decoupled and has a long lifetime to an optical decay. Dilute gas densities (n~1014cm−3) are possible, but paraexciton generation scales poorly, so significant heating occurs in creating high densities(1017cm−3) preventing BECs. Assuming a thermodynamic phase occurs when separation reaches the de Broglie wavelength([math]\displaystyle{ \lambda_{dB} }[/math]) gives:

[math]\displaystyle{ n^{1/3} = \hbar^{-1}(m_\text{eff} kT_{cr})^{1/2} \longrightarrow T_c = \frac{n^{2/3} \hbar^2}{k m_\text{eff}} }[/math]

 

 

 

 

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Where, [math]\displaystyle{ n }[/math] is the exciton density, effective mass(of electron mass order) [math]\displaystyle{ m_\text{eff} }[/math], and [math]\displaystyle{ \hbar }[/math],[math]\displaystyle{ k }[/math] are the Planck and Boltzmann constants. Density depends on the optical generation [math]\displaystyle{ g }[/math] and lifetime as: [math]\displaystyle{ n = g\tau }[/math]. Tuned lasers create excitons which efficiently self-annihilate at a rate: [math]\displaystyle{ dn/dt = -an^2 }[/math], preventing a high density paraexciton BEC.[7] A potential well limits diffusion, damps exciton decay, and lowers the critical number, yielding an improved critical temperature versus the T3/2 scaling of free particles:

[math]\displaystyle{ N_c = \zeta(3) \left( \frac{kT}{\hbar \omega} \right)^3 }[/math]

Experiments

In an ultrapure Cu2O crystal: [math]\displaystyle{ \tau }[/math] = 10s. For an achievable T = 0.01K, a manageable optical pumping rate of 105/s should produce a condensate.[8] More detailed calculations by J. Keldysh[9] and later by D. Snoke et al.[10] started a large number of experimental searches into the 1990s that failed to detect signs.[11][12][13] Pulse methods led to overheating, preventing condensate states. Helium cooling allows mili-kelvin setups and continuous wave optics improves on pulsed searches. Relaxation explosion of a condensate at lattice temperature 354 mK was seen by Yoshioka et al. in 2011.[14] Recent experiments by Stolz et al. using a potential trap have given more evidence at ultralow temperature 37 mK.[7] In a parabolic trap with exciton temperature 200 mK and lifetime broadened to 650ns, the dependence of luminescence on laser intensity has a kink which indicates condensation. The theory of a Bose gas is extended to a mean field interacting gas by a Bogoliubov approach to predict the exciton spectrum; The kink is considered a sign of transition to BEC. Signs were seen for a dense gas BEC in a GaAs quantum well.[15]

Magnons

Magnons, electron spin waves, can be controlled by a magnetic field. Densities from the limit of a dilute gas to a strongly interacting Bose liquid are possible. Magnetic ordering is the analog of superfluidity. The condensate appears as the emission of monochromatic microwaves, which are tunable with the applied magnetic field.

In 1999 condensation was demonstrated in antiferromagnetic TlCuCl3,[16] at temperatures as large as 14 K. The high transition temperature (relative to atomic gases) is due to the small mass (near an electron) and greater density. In 2006, condensation in a ferromagnetic Yttrium-iron-garnet thin film was seen even at room temperature[17][18] with optical pumping. Condensation was reported in gadolinium in 2011.[19] Magnon BECs have been considered as qubits for quantum computing.[20]

Polaritons

Polaritons, caused by light coupling to excitons, occur in optical cavities and condensation of exciton-polaritons in an optical microcavity was first published in Nature in 2006.[21] Semiconductor cavity polariton gases transition to ground state occupation at 19K.[21] Bogoliubov excitations were seen polariton BECs in 2008.[22] The signatures of BEC were observed at room temperature for the first time in 2013, in a large exciton energy semiconductor device [23][24] and in a polymer microcavity.[25]

Other quasiparticles

Rotons, an elementary excitation in superfluid 4He introduced by Landau,[26] were discussed by Feynman[27] and others.[28] Rotons condense at low temperature. Experiments have been proposed and the expected spectrum has been studied,[29][30][31] but roton condensates have not been detected. Phonons were first observed in a condensate in 2004 by ultrashort pulses in a bismuth crystal at 7K.[32]

See also

Important publications

References

  1. ↑ Eisenstein, JP; Macdonald, AH (9 December 2004). "Bose–Einstein condensation of excitons in bilayer electron systems". Nature 432 (7018): 691–694. doi:10.1038/nature03081. PMID 15592403. Bibcode: 2004Natur.432..691E. 
  2. ↑ Berman, OL; Kezerashvili, RY; Lozovik, YE; Snoke, DW (1 November 2010). "Bose–Einstein condensation and superfluidity of trapped polaritons in graphene and quantum wells embedded in a microcavity". Philosophical Transactions of the Royal Society A 368 (1932): 5459–82. doi:10.1098/rsta.2010.0208. PMID 21041225. Bibcode: 2010RSPTA.368.5459B. 
  3. ↑ London, F (1938). "The [math]\displaystyle{ \lambda }[/math]-Point of Liquid Helium and the Bose–Einstein Condensation". Nature 141 (3571): 643–644. doi:10.1038/141643a0. Bibcode: 1938Natur.141..643L. 
  4. ↑ Einstein, A. (1920) Proc. Berlin Acad. Science
  5. ↑ Kapiza, P (1938). "Viscosity of Liquid Helium below the λ-Point". Nature 141 (3558): 74. doi:10.1038/141074a0. Bibcode: 1938Natur.141...74K. 
  6. ↑ Blatt, J.M., K.W. Boer, and W. Brandt, (1962) Bose–Einstein Condensation of excitons, Phys. Rev. 126.5, 1691
  7. ↑ 7.0 7.1 Heinrich Stolz (2012). "Condensation of excitons in Cu2O at ultracold temperatures: Experiment and theory". New Journal of Physics 14 (10): 105007. doi:10.1088/1367-2630/14/10/105007. Bibcode: 2012NJPh...14j5007S. 
  8. ↑ Aurora, C.P. (2001) Thermodynamics, McGraw-Hill
  9. ↑ Keldysh, L.V. (1965). "Diagram Technique for Nonequilibrium Processes". Sov. Phys. JETP 20: 1018. http://www.jetp.ac.ru/cgi-bin/dn/e_020_04_1018.pdf. 
  10. ↑ Snoke, D.W.; Wolfe, J.P.; Mysyrovicz, A. (1990). "Evidence for Bose-Einstein condensation of excitons inCu2O". Phys. Rev. B 41 (16): 11171–11184. doi:10.1103/physrevb.41.11171. PMID 9993538. Bibcode: 1990PhRvB..4111171S. 
  11. ↑ Naka, N.; Nagasawa, N. (2005). "Bosonic stimulation of cold excitons in a harmonic potential trap in CuO". Journal of Luminescence 112 (1–4): 11–16. doi:10.1016/j.jlumin.2004.09.035. Bibcode: 2005JLum..112...11N. 
  12. ↑ Joshioka, K.; Ideguchi, T.; Mysyrovicz, A; Kuwata-Gonokami, M. (2010). "Quantum inelastic collisions between paraexcitons inCu2O". Phys. Rev. B 82 (4): 041201. doi:10.1103/physrevb.82.041201. Bibcode: 2010PhRvB..82d1201Y. 
  13. ↑ Stolz, H.; Semkat, D. (2010). "Unique signatures for Bose-Einstein condensation in the decay luminescence lineshape of weakly interacting excitons in a potential trap". Phys. Rev. B 81 (8): 081302. doi:10.1103/physrevb.81.081302. Bibcode: 2010PhRvB..81h1302S. 
  14. ↑ Yoshioka, Kosuke; Chae, Eunmi; Kuwata-Gonokami, Makoto (May 31, 2011). "Transition to a Bose–Einstein condensate and relaxation explosion of excitons at sub-Kelvin temperatures". Nature Communications 2 (328): 328–. doi:10.1038/ncomms1335. Bibcode: 2011NatCo...2..328Y. 
  15. ↑ Alloing, Mathieu; Beian, Mussie; Lewenstein, Maciej; Fuster, David; González, Yolanda; González, Luisa; Combescot, Roland; Combescot, Monique et al. (July 2014). "Evidence for a Bose–Einstein condensate of excitons". EPL 107 (1): 10012. doi:10.1209/0295-5075/107/10012. Bibcode: 2014EL....10710012A. 
  16. ↑ Nikuni, T.; Oshikawa, M.; Oosawa, A.; Tanaka, H. (1999). "Bose–Einstein Condensation of Dilute Magnons in TlCuCl3". Physical Review Letters 84 (25): 5868–71. doi:10.1103/PhysRevLett.84.5868. PMID 10991075. Bibcode: 2000PhRvL..84.5868N. 
  17. ↑ Demokritov, S.O.; Demidov, VE; Dzyapko, O; Melkov, GA; Serga, AA; Hillebrands, B; Slavin, AN (2006). "Bose–Einstein condensation of quasi-equilibrium magnons at room temperature under pumping". Nature 443 (7110): 430–433. doi:10.1038/nature05117. PMID 17006509. Bibcode: 2006Natur.443..430D. 
  18. ↑ Magnon Bose Einstein Condensation made simple. Website of the "Westfählische Wilhelms Universität Münster" Prof.Demokritov. Retrieved 25 June 2012.
  19. ↑ Mathew, SP; Kaul, SN (Jul 6, 2011). "Bose–Einstein condensation of magnons in polycrystalline gadolinium with nano-size grains". J Phys Condens Matter 23 (26): 266003. doi:10.1088/0953-8984/23/26/266003. PMID 21673396. Bibcode: 2011JPCM...23z6003M. 
  20. ↑ Andrianov, S. N; Moiseev, S. A (2 October 2014). "Magnon qubit and quantum computing on magnon Bose–Einstein condensates". Phys. Rev. A 90 (4): 042303. doi:10.1103/PhysRevA.90.042303. Bibcode: 2014PhRvA..90d2303A. 
  21. ↑ 21.0 21.1 Kasprzak, J; Richard, M; Kundermann, S; Baas, A; Jeambrun, P; Keeling, JM; Marchetti, FM; Szymańska, MH et al. (28 September 2006). "Bose–Einstein condensation of exciton polaritons". Nature 443 (7110): 409–414. doi:10.1038/nature05131. PMID 17006506. Bibcode: 2006Natur.443..409K. 
  22. ↑ Utsunomiya, S; Tian, L; Roumpos, G; Lai, C. W; Kumada, N; Fujisawa, T; Kuwata-Gonokami, M; Löffler, A et al. (2008). "Observation of Bogoliubov excitations in exciton-polariton condensates". Nature Physics 4 (9): 700–705. doi:10.1038/nphys1034. Bibcode: 2008NatPh...4..673U. 
  23. ↑ Das, A; Bhattacharya, P; Heo, J; Banerjee, A; Guo, W (February 19, 2013). "Polariton Bose–Einstein condensate at room temperature in an Al(Ga)N nanowire–dielectric microcavity with a spatial potential trap". Proceedings of the National Academy of Sciences 110 (8): 2735–2740. doi:10.1073/pnas.1210842110. PMID 23382183. Bibcode: 2013PNAS..110.2735D. 
  24. ↑ Francis, Matthew (Feb 6, 2013). "SCIENTIFIC METHOD / SCIENCE & EXPLORATION Bose–Einstein condensate created at room temperature". Ars Technica. https://arstechnica.com/science/2013/02/bose-einstein-condensate-created-at-room-temperature/. 
  25. ↑ Plumhof, JD; Stöferle, T; Mai, L; Scherf, U; Mahrt, RF (8 December 2013). "Room-temperature Bose–Einstein condensation of cavity exciton–polaritons in a polymer". Nature Materials 13 (3): 247–252. doi:10.1038/nmat3825. PMID 24317189. Bibcode: 2014NatMa..13..247P. 
  26. ↑ L. Landau (1941). J. Phys. USSR 5: 71. 
  27. ↑ Feynman, R. P (1954). "R. P. Feynman". Phys. Rev. 94 (2): 262–277. doi:10.1103/PhysRev.94.262. Bibcode: 1954PhRv...94..262F. https://authors.library.caltech.edu/3539/1/FEYpr54a.pdf. 
  28. ↑ Iordanskiĭ, S. V; Pitaevskiĭ, Lev P (1980). "Bose condensation of moving rotons". Soviet Physics Uspekhi 23 (6): 317–318. doi:10.1070/PU1980v023n06ABEH004937. Bibcode: 1980SvPhU..23..317I. 
  29. ↑ L. A. Melnikovsky (22 July 2011). "Bose–Einstein condensation of rotons". Phys. Rev. B 84 (2): 024525. doi:10.1103/PhysRevB.84.024525. Bibcode: 2011PhRvB..84b4525M. 
  30. ↑ Blakie, P. B; Baillie, D; Bisset, R. N (15 August 2012). "Roton spectroscopy in a harmonically trapped dipolar Bose–Einstein condensate". Phys. Rev. A 86 (2): 021604. doi:10.1103/PhysRevA.86.021604. Bibcode: 2012PhRvA..86b1604B. 
  31. ↑ Galli, D. E; Reatto, L; Rossi, M (2014). "Quantum Monte Carlo study of a vortex in superfluid He4 and search for a vortex state in the solid". Phys. Rev. B 89 (22): 224516. doi:10.1103/PhysRevB.89.224516. Bibcode: 2014PhRvB..89v4516G. 
  32. ↑ Misochko, O. V; Hase, Muneaki; Ishioka, K; Kitajima, M (16 February 2004). "Transient Bose–Einstein condensation of phonons". Physics Letters A 321 (5–6): 381–387. doi:10.1016/j.physleta.2003.11.063. Bibcode: 2004PhLA..321..381M. 



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