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{{Short description|State of matter}}
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[[File:Bose-Einstein Condensation.ogv|thumb|upright=1.5|Illustration of Bose-Einstein condensation: as the temperature of the ensemble of bosons is reduced, the overlap between the particles' wavefunctions increases as the thermal de Broglie wavelength increases. At one point, when the overlap becomes significant, a macroscopic number of particles condense into the ground state.]]

In [[condensed matter physics]], a '''Bose–Einstein condensate''' ('''BEC''') is a [[state of matter]] that is typically formed when a [[gas]] of [[boson]]s at very low [[Density|densities]] is cooled to [[temperature]]s very close to [[absolute zero#Relation with Bose–Einstein condensate|absolute zero]], i.e., {{convert|0|K|C F}}. Under such conditions, a large fraction of bosons occupy the lowest [[quantum state]], at which microscopic [[Quantum mechanics|quantum-mechanical]] phenomena, particularly [[wave interference#Quantum interference|wavefunction interference]], become apparent [[Macroscopic quantum phenomena|macroscopically]]. 
More generally, condensation refers to the appearance of macroscopic occupation of one or several states: for example, in [[BCS theory]], a superconductor is a condensate of [[Cooper pair]]s.<ref>{{cite book |last1=Leggett |first1=Anthony J. |title=Quantum liquids: Bose condensation and Cooper pairing in condensed-matter systems |date=2022 |publisher=Oxford University Press |location=Oxford |isbn=9780192856944 |edition=First published in paperback}}</ref> As such, condensation can be associated with [[phase transition]], and the macroscopic occupation of the state is the [[order parameter]].

Bose–Einstein condensate was first predicted, generally, in 1924–1925 by [[Albert Einstein]],<ref>{{cite journal |last1=Einstein |first1=Albert |date=10 July 1924 |title=Quantentheorie des einatomigen idealen Gases |language=de |url=https://www.uni-muenster.de/imperia/md/content/physik_ap/demokritov/mbecfornonphysicists/einstein_1924_1925.pdf |url-status=live |journal=Königliche Preußische Akademie der Wissenschaften. Sitzungsberichte |pages=261–267 |archive-url=https://ghostarchive.org/archive/20221009/https://www.uni-muenster.de/imperia/md/content/physik_ap/demokritov/mbecfornonphysicists/einstein_1924_1925.pdf |archive-date=2022-10-09}}</ref> crediting a pioneering paper by [[Satyendra Nath Bose]] on the new field now known as [[quantum statistics]].<ref>A. Douglas Stone, Chapter 24, ''The Indian Comet'', in the book ''Einstein and the Quantum'', Princeton University Press, Princeton, New Jersey, 2013.</ref> In 1995, the Bose–Einstein condensate was created by [[Eric Allin Cornell|Eric Cornell]] and [[Carl Wieman]] of the [[University of Colorado Boulder]] using [[rubidium]] atoms; later that year, [[Wolfgang Ketterle]] of [[Massachusetts Institute of Technology|MIT]] produced a BEC using [[sodium]] atoms. In 2001 Cornell, Wieman, and Ketterle shared the [[Nobel Prize in Physics]] "for the achievement of Bose–Einstein condensation in dilute gases of alkali atoms, and for early fundamental studies of the properties of the condensates".<ref>{{Cite web |date=October 9, 2001 |title=The Nobel Prize in Physics 2001 |url=https://www.nobelprize.org/prizes/physics/2001/summary/}}</ref>

== History ==
[[File:Bose Einstein condensate.png|right|thumb|238px|Velocity-distribution data (3 views) for gas of [[rubidium]] atoms, confirming the discovery of a new phase of matter, the Bose–Einstein condensate. {{nowrap|Left: just}} before the appearance of a Bose–Einstein condensate. {{nowrap|Center: just}} after the appearance of the condensate. {{nowrap|Right: after}} further evaporation, leaving a sample of nearly pure condensate.]]

Bose first sent a paper to Einstein on the [[quantum statistics]] of light quanta (now called [[photon]]s), in which he derived [[Planck's law|Planck's quantum radiation law]] without any reference to classical physics. Einstein was impressed, translated the paper himself from English to German and submitted it for Bose to the ''[[Zeitschrift für Physik]]'', which published it in 1924.<ref>{{cite journal |author=S. N. Bose |year=1924 |title=Plancks Gesetz und Lichtquantenhypothese |language=de |journal=Zeitschrift für Physik |volume=26 |issue=1 |pages=178–181 |bibcode=1924ZPhy...26..178B |doi=10.1007/BF01327326 |s2cid=186235974 }}</ref> (The Einstein manuscript, once believed to be lost, was found in a library at [[Leiden University]] in 2005.<ref>{{cite web |url=http://www.lorentz.leidenuniv.nl/history/Einstein_archive/ |title=Leiden University Einstein archive |publisher=Lorentz.leidenuniv.nl |date=27 October 1920 |access-date=23 March 2011}}</ref>) Einstein then extended Bose's ideas to matter in two other papers.<ref>{{cite journal |author=A. Einstein |year=1925 |title=Quantentheorie des einatomigen idealen Gases |language=de |journal=Sitzungsberichte der Preussischen Akademie der Wissenschaften |volume=1 |page=3}}</ref><ref>{{cite book |first=Ronald W. |last=Clark |title=Einstein: The Life and Times |publisher=Avon Books |year=1971 |pages=[https://archive.org/details/einstein00rona/page/408 408–409] |isbn=978-0-380-01159-9 |url-access=registration |url=https://archive.org/details/einstein00rona/page/408 }}</ref> The result of their efforts is the concept of a [[Bose gas]], governed by [[Bose–Einstein statistics]], which describes the statistical distribution of [[identical particles]] with [[integer]] [[Spin (physics)|spin]], now called [[boson]]s. Bosons are allowed to share a quantum state. Einstein proposed that cooling bosonic atoms to a very low temperature would cause them to fall (or "condense") into the lowest accessible [[quantum state]], resulting in a new form of matter. Bosons include the [[photon]], [[polariton]]s, [[magnon]]s, some [[atom]]s and [[molecule]]s (depending on the number of [[nucleon]]s, see [[#Isotopes]]) such as atomic hydrogen, [[helium-4]], lithium-7, rubidium-87 or strontium-84.

In 1938, [[Fritz London]] proposed the BEC as a mechanism for [[superfluidity]] in {{SimpleNuclide|Helium|4}} and [[superconductivity]].<ref name=London:1938/><ref>London, F. ''Superfluids'', Vol. I and II, (reprinted New York: Dover 1964).</ref>

The quest to produce a Bose–Einstein condensate in the laboratory was stimulated by a paper published in 1976 by two program directors at the [[National Science Foundation]] (William Stwalley and Lewis Nosanow), proposing to use spin-polarized atomic [[hydrogen]] to produce a gaseous BEC.<ref>{{cite journal |last1=Stwalley |first1=W. |date=12 April 1976 |title=Possible "New" Quantum Systems |journal=Physical Review Letters |volume=36 |issue=15 |pages=910–913 |bibcode=1976PhRvL..36..910S |doi=10.1103/PhysRevLett.36.910}}</ref> This led to the immediate pursuit of the idea by four independent research groups; these were led by Isaac Silvera ([[University of Amsterdam]]), Walter Hardy ([[University of British Columbia]]), Thomas Greytak ([[Massachusetts Institute of Technology]]) and David Lee ([[Cornell University]]).<ref>{{cite arXiv |last1=Cornell |first1=E. |title=Experiments in Dilute Atomic Bose–Einstein Condensation |date=1999 |eprint=cond-mat/9903109}}</ref> However, cooling atomic hydrogen turned out to be technically difficult, and Bose-Einstein condensation of atomic hydrogen was only realized in 1998.<ref name="v594">{{cite journal | last1=Fried | first1=Dale G. | last2=Killian | first2=Thomas C. | last3=Willmann | first3=Lorenz | last4=Landhuis | first4=David | last5=Moss | first5=Stephen C. | last6=Kleppner | first6=Daniel | last7=Greytak | first7=Thomas J. | title=Bose-Einstein Condensation of Atomic Hydrogen | journal=Physical Review Letters | volume=81 | issue=18 | date=1998-11-02 | issn=0031-9007 | doi=10.1103/PhysRevLett.81.3811 | pages=3811–3814| arxiv=physics/9908044 }}</ref><ref name="m380">{{cite journal | last1=Greytak | first1=T.J | last2=Kleppner | first2=D | last3=Fried | first3=D.G | last4=Killian | first4=T.C | last5=Willmann | first5=L | last6=Landhuis | first6=D | last7=Moss | first7=S.C | title=Bose–Einstein condensation in atomic hydrogen | journal=Physica B: Condensed Matter | volume=280 | issue=1–4 | date=2000 | doi=10.1016/S0921-4526(99)01415-5 | pages=20–26 | url=http://web.mit.edu/physics/greytak-kleppner/publications/LT22_Talk.pdf}}</ref>

On 5 June 1995, the first gaseous condensate was produced by [[Eric Allin Cornell|Eric Cornell]] and [[Carl Wieman]] at the [[University of Colorado at Boulder]] [[National Institute of Standards and Technology|NIST]]–[[JILA]] lab, in a gas of [[rubidium]] atoms cooled to 170&nbsp;[[kelvin|nanokelvins]] (nK).<ref name=":0">{{Cite journal |last1=Anderson |first1=M. H. |last2=Ensher |first2=J. R. |last3=Matthews |first3=M. R. |last4=Wieman |first4=C. E. |last5=Cornell |first5=E. A. |date=1995-07-14 |title=Observation of Bose-Einstein Condensation in a Dilute Atomic Vapor |journal=Science |language=en |volume=269 |issue=5221 |pages=198–201 |doi=10.1126/science.269.5221.198 |issn=0036-8075 |pmid=17789847 |bibcode=1995Sci...269..198A |doi-access=free}}</ref> Shortly thereafter, [[Wolfgang Ketterle]] at MIT produced a Bose–Einstein Condensate in a gas of [[sodium]] atoms. For their achievements Cornell, Wieman, and Ketterle received the 2001 [[Nobel Prize in Physics]].<ref>{{cite web |last = Levi |first = Barbara Goss |author-link=Barbara Goss Levi |title = Cornell, Ketterle, and Wieman Share Nobel Prize for Bose–Einstein Condensates |work = Search & Discovery |publisher = Physics Today online |year = 2001 |url = http://www.physicstoday.org/pt/vol-54/iss-12/p14.html |access-date = 26 January 2008 |archive-url = https://archive.today/20071024134547/http://www.physicstoday.org/pt/vol-54/iss-12/p14.html |archive-date = 24 October 2007}}</ref> Bose-Einstein condensation of alkali gases is easier because they can be pre-cooled with [[laser cooling]] techniques, unlike atomic hydrogen at the time, which give a significant head start when performing the final forced evaporative cooling to cross the condensation threshold.<ref name="m380" /> These early studies founded the field of [[ultracold atom]]s, and hundreds of research groups around the world now routinely produce BECs of dilute atomic vapors in their labs.

Since 1995, many other atomic species have been condensed (see [[#Isotopes]]), and BECs have also been realized using molecules, [[polariton]]s, and other quasi-particles. BECs of photons can be made, for example, in dye microcavites with wavelength-scale mirror separation, forming a two-dimensional harmonically confined photon gas with tunable chemical potential.<ref name=Klaers:2010/> BEC of plasmonic quasiparticles (plasmon-exciton polaritons) has been realized in periodic arrays of metal nanoparticles overlaid with dye molecules,<ref name=Hakala:2018/> exhibiting ultrafast sub-picosecond dynamics<ref name=Väkeväinen:2020/> and long-range correlations.<ref name=Moilanen:2021/>

== Critical temperature ==
This transition to BEC occurs below a critical temperature, which for a uniform [[Three-dimensional space|three-dimensional]] gas consisting of non-interacting particles with no apparent internal degrees of freedom is given by
: <math>
 T_\text{c} = \left(\frac{n}{\zeta(3/2)}\right)^{2/3} \frac{2\pi\hbar^2}{m k_\text{B}} \approx 3.3125\,\frac{\hbar^2 n^{2/3}}{m k_\text{B}},
</math>
where:
: <math>T_\text{c}</math> is the critical temperature,
: <math>n</math> is the [[Number density|particle density]],
: <math>m</math> is the mass per boson,
: <math>\hbar</math> is the reduced [[Planck constant]],
: <math>k_\text{B}</math> is the [[Boltzmann constant]],
: <math>\zeta</math> is the [[Riemann zeta function]] (<math>\zeta(3/2) \approx 2.6124</math><ref>{{OEIS|id=A078434}}</ref>).

Interactions shift the value, and the corrections can be calculated by [[mean-field theory]].
This formula is derived from finding the gas degeneracy in the [[Bose gas]] using [[Bose–Einstein statistics]].

The critical temperature depends on the density. A more concise and experimentally relevant<ref>Producing Bose-Einstein condensates experimentally often involves a change in both density and temperature. This is the case with evaporative cooling of dilute gases, for which the temperature is decreased by loosing particles. The goal is then to reduce the temperature faster than particles are lost, so that the phase-space density increases overall.</ref> condition involves the phase-space density <math>\mathcal{D}=n \lambda_T^3</math>, where
: <math>\lambda_T=\hbar \sqrt{\frac{2\pi}{m k_\text{B} T}}</math>
is the [[thermal de Broglie wavelength]]. It is a dimensionless quantity. The transition to BEC occurs when the phase-space density is greater than critical value:
: <math>\mathcal{D}_\text{c}=\zeta(3/2)</math>
in 3D uniform space. This is equivalent to the above condition on the temperature. In a 3D harmonic potential, the critical value is instead
: <math>\mathcal{D}_\text{c}=\zeta(3)\approx 1.202</math><ref>{{OEIS|id=A002117}}</ref>
where <math>n</math> has to be understood as the peak density.

== Derivation ==

=== Ideal Bose gas ===
For an ideal [[Bose gas]] we have the equation of state

: <math>\frac{1}{v} = \frac{1}{\lambda^3} g_{3/2}(f) + \frac{1}{V}\frac{f}{1 - f},</math>

where <math>v = V/N</math> is the per-particle volume, <math>\lambda</math> is the [[Thermal de Broglie wavelength|thermal wavelength]], <math>f</math> is the [[fugacity]], and
: <math>g_\alpha(f) = \sum\limits_{n=1}^\infty \frac{f^n}{n^\alpha}.</math>

It is noticeable that <math>g_{3/2}</math> is a monotonically growing function of <math>f</math> in <math>f \in [0, 1]</math>, which are the only values for which the series converge.
Recognizing that the second term on the right-hand side contains the expression for the average occupation number of the fundamental state <math>\langle n_0 \rangle</math>, the equation of state can be rewritten as

: <math>\frac{1}{v} = \frac{1}{\lambda^3} g_{3/2}(f) + \frac{\langle n_0\rangle}{V} \Leftrightarrow \frac{\langle n_0\rangle}{V} \lambda^3 = \frac{\lambda^3}{v} - g_{3/2}(f).</math>

Because the left term on the second equation must always be positive, <math>\frac{\lambda^3}{v} > g_{3/2}(f)</math>, and because <math>g_{3/2}(f) \le g_{3/2}(1)</math>, a stronger condition is

: <math>\frac{\lambda^3}{v} > g_{3/2}(1),</math>

which defines a transition between a gas phase and a condensed phase. On the critical region it is possible to define a critical temperature and thermal wavelength:

: <math>\lambda_c^3 = g_{3/2}(1)v = \zeta(3/2) v,</math>

: <math>T_\text{c} = \frac{2\pi \hbar^2}{m k_\text{B} \lambda_c^2},</math>

recovering the value indicated on the previous section. The critical values are such that if <math>T < T_\text{c}</math> or <math>\lambda > \lambda_\text{c}</math>, we are in the presence of a Bose–Einstein condensate.
Understanding what happens with the fraction of particles on the fundamental level is crucial. As so, write the equation of state for <math>f = 1</math>, obtaining

: <math>\frac{\langle n_0\rangle}{N} = 1 - \left(\frac{\lambda_\text{c}}{\lambda}\right)^3</math> and equivalently <math>\frac{\langle n_0\rangle}{N} = 1 - \left(\frac{T}{T_\text{c}}\right)^{3/2}.</math>

So, if <math>T \ll T_\text{c}</math>, the fraction <math>\frac{\langle n_0 \rangle}{N} \approx 1</math>, and if <math>T \gg T_\text{c}</math>, the fraction <math>\frac{\langle n_0 \rangle}{N} \approx 0</math>. At temperatures near to absolute 0, particles tend to condense in the fundamental state, which is the state with momentum <math>\vec{p} = 0</math>.

== Experimental observation ==

=== Superfluid helium-4 ===
{{Main article|Superfluid helium-4}}
In 1938, [[Pyotr Leonidovich Kapitsa|Pyotr Kapitsa]], [[John F. Allen (physicist)|John Allen]] and [[Don Misener]] discovered that [[helium-4]] became a new kind of fluid, now known as a [[superfluid]], at temperatures less than 2.17&nbsp;K (the [[lambda point]]). Superfluid helium has many unusual properties, including zero [[viscosity]] (the ability to flow without dissipating energy) and the existence of [[quantum vortex|quantized vortices]]. It was quickly believed that the superfluidity was due to partial Bose–Einstein condensation of the liquid. In fact, many properties of superfluid helium also appear in gaseous condensates created by Cornell, Wieman and Ketterle (see below). Superfluid helium-4 is a liquid rather than a gas, which means that the interactions between the atoms are relatively strong; the original theory of Bose–Einstein condensation must be heavily modified in order to describe it. Bose–Einstein condensation remains, however, fundamental to the superfluid properties of helium-4. Note that [[helium-3]], a [[fermion]], also enters a [[superfluid]] phase (at a much lower temperature) which can be explained by the formation of bosonic [[Cooper pairs]] of two atoms (see also [[fermionic condensate]]).

=== Dilute atomic gases ===
The first "pure" Bose–Einstein condensate was created by [[Eric Cornell]], [[Carl Wieman]], and co-workers at [[JILA]] on 5 June 1995.<ref name=":0" /> They cooled a dilute vapor of approximately two thousand [[rubidium|rubidium-87]] atoms to below 170&nbsp;nK using a combination of [[laser cooling]] (a technique that won its inventors [[Steven Chu]], [[Claude Cohen-Tannoudji]], and [[William D. Phillips]] the 1997 [[Nobel Prize in Physics]]) and [[magnetic evaporative cooling]]. About four months later, an independent effort led by [[Wolfgang Ketterle]] at [[Massachusetts Institute of Technology|MIT]] condensed [[sodium|sodium-23]]. Ketterle's condensate had a hundred times more atoms, allowing important results such as the observation of [[quantum mechanics|quantum mechanical]] [[Interference (wave propagation)|interference]] between two different condensates. Cornell, Wieman and Ketterle won the 2001 [[Nobel Prize in Physics]] for their achievements.<ref name="nobel">{{cite web |url=http://nobelprize.org/nobel_prizes/physics/laureates/2001/cornellwieman-lecture.pdf |archive-url=https://ghostarchive.org/archive/20221009/http://nobelprize.org/nobel_prizes/physics/laureates/2001/cornellwieman-lecture.pdf |archive-date=2022-10-09 |url-status=live |title=Eric A. Cornell and Carl E. Wieman&nbsp;— Nobel Lecture |publisher=nobelprize.org}}</ref>

A group led by [[Randall G. Hulet|Randall Hulet]] at Rice University announced a condensate of [[lithium]] atoms only one month following the JILA work.<ref name=Bradley:1995/> Lithium has attractive interactions, causing the condensate to be unstable and collapse for all but a few atoms. Hulet's team subsequently showed the condensate could be stabilized by confinement quantum pressure for up to about 1000 atoms. Various isotopes have since been condensed.

==== Velocity-distribution data graph ====
In the image accompanying this article, the velocity-distribution data indicates the formation of a Bose–Einstein condensate out of a gas of [[rubidium]] atoms. The false colors indicate the number of atoms at each velocity, with red being the fewest and white being the most. The areas appearing white and light blue are at the lowest velocities. The peak is not infinitely narrow because of the [[uncertainty principle|Heisenberg uncertainty principle]]: spatially confined atoms have a minimum width velocity distribution. This width is given by the curvature of the magnetic potential in the given direction. More tightly confined directions have bigger widths in the ballistic velocity distribution. This [[anisotropy]] of the peak on the right is a purely quantum-mechanical effect and does not exist in the thermal distribution on the left. This graph served as the cover design for the 1999 textbook ''Thermal Physics'' by Ralph Baierlein.<ref>{{cite book |url=https://archive.org/details/thermalphysics00ralp|url-access=registration|title=Thermal Physics|author=Baierlein, Ralph |publisher=Cambridge University Press|year=1999|isbn=978-0-521-65838-6}}</ref>

=== Quasiparticles ===
{{Main|Bose–Einstein condensation of quasiparticles}}Bose–Einstein condensation also applies to [[quasiparticle]]s in solids. [[Magnon]]s, [[excitons]], and [[polaritons]] have integer spin which means they are [[bosons]] that can form condensates.<ref>Monique Combescot and Shiue-Yuan Shiau, "Excitons and Cooper Pairs: Two Composite Bosons in Many-Body Physics", Oxford University Press ({{ISBN|9780198753735}})</ref>

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. In 1999 condensation was demonstrated in antiferromagnetic {{chem|[[Thallium|Tl]]|[[Copper|Cu]]|[[Chlorine|Cl]]|3}},<ref name=Nikuni:1999/> at temperatures as great as 14&nbsp;K. The high transition temperature (relative to atomic gases) is due to the magnons' small mass (near that of an electron) and greater achievable density. In 2006, condensation in a [[ferromagnetism|ferromagnetic]] yttrium-iron-garnet thin film was seen even at room temperature,<ref name=Demokritov:2006/><ref>[https://www.uni-muenster.de/Physik.AP/Demokritov/en/Forschen/Forschungsschwerpunkte/mBECfnP.html ''Magnon Bose Einstein Condensation'' made simple] {{Webarchive|url=https://web.archive.org/web/20210627170551/https://www.uni-muenster.de/Physik.AP/Demokritov/en/Forschen/Forschungsschwerpunkte/mBECfnP.html |date=27 June 2021 }}. Website of the "Westfählische Wilhelms Universität Münster" Prof.Demokritov. Retrieved 25 June 2012.</ref> with optical pumping.

[[Exciton]]s, electron-hole pairs, were predicted to condense at low temperature and high density by Boer et al., in 1961.{{citation needed|date=May 2020}} Bilayer system experiments first demonstrated condensation in 2003, by Hall voltage disappearance.<ref name="Eisenstein04">{{Cite journal|title = Bose–Einstein condensation of exciton polaritons|date = 2004|journal = Nature|doi = 10.1038/nature03081 |arxiv=cond-mat/0404113|volume=432|pages=691–694|author=Eisenstein, J., MacDonald, A|issue = 7018|pmid = 15592403|s2cid = 1538354}}</ref> Fast optical exciton creation was used to form condensates in sub-kelvin {{chem|Cu|2|O}} in 2005 on.{{citation needed|date=May 2020}}

[[Bose–Einstein condensation of polaritons|Polariton condensation]] was first detected for [[exciton-polaritons]] in a quantum well microcavity kept at 5&nbsp;K.<ref name="ReferenceA">{{Cite journal|title = Bose–Einstein condensation of exciton polaritons|date = 28 September 2006|journal = Nature|doi = 10.1038/nature05131|pmid = 17006506|volume=443 |issue = 7110|pages=409–414|bibcode = 2006Natur.443..409K |author=Kasprzak J, Richard M, Kundermann S, Baas A, Jeambrun P, Keeling JM, Marchetti FM, Szymańska MH, André R, Staehli JL, Savona V, Littlewood PB, Deveaud B, Dang|s2cid = 854066}}</ref> Quasiparticle BECs have been achieved at room-temperature, for example, in microcavity-coupled organic semiconductors and plasmon-exciton polaritons in periodic arrays of metal nanoparticles coupled to dye molecules.<ref name=Hakala:2018/><ref name=Väkeväinen:2020/><ref name=Moilanen:2021/>

=== In zero gravity ===
In June 2020, the [[Cold Atom Laboratory]] experiment on board the [[International Space Station]] successfully created a BEC of rubidium atoms and observed them for over a second in free-fall. Although initially just a proof of function, early results showed that, in the microgravity environment of the ISS, about half of the atoms formed into a magnetically insensitive halo-like cloud around the main body of the BEC.<ref>[https://www.newscientist.com/article/mg24632862-300-exotic-fifth-state-of-matter-made-on-the-international-space-station/#ixzz6PPDVqP7C Exotic fifth state of matter made on the International Space Station] {{Webarchive|url=https://web.archive.org/web/20200615045241/https://www.newscientist.com/article/mg24632862-300-exotic-fifth-state-of-matter-made-on-the-international-space-station/#ixzz6PPDVqP7C |date=15 June 2020 }}, New Scientist, by Jonathan O’Callaghan, 11 June 2020</ref><ref name="AvelineWilliams2020">{{cite journal|display-authors=1|last1=Aveline|first1=David C.|last2=Williams|first2=Jason R.|last3=Elliott|first3=Ethan R.|last4=Dutenhoffer|first4=Chelsea|last5=Kellogg|first5=James R.|last6=Kohel|first6=James M.|last7=Lay|first7=Norman E.|last8=Oudrhiri|first8=Kamal|last9=Shotwell|first9=Robert F.|last10=Yu|first10=Nan|last11=Thompson|first11=Robert J.|title=Observation of Bose–Einstein condensates in an Earth-orbiting research lab|journal=Nature|volume=582|issue=7811|year=2020|pages=193–197|issn=0028-0836|doi=10.1038/s41586-020-2346-1|pmid=32528092|bibcode=2020Natur.582..193A|s2cid=219568565}}</ref>

== Models ==

=== Bose Einstein's non-interacting gas ===
{{Main|Bose gas}}
Consider a collection of ''N'' non-interacting particles, which can each be in one of two [[quantum state]]s, <math>|0\rangle</math> and <math>|1\rangle</math>. If the two states are equal in energy, each different configuration is equally likely.

If we can tell which particle is which, there are <math>2^N</math> different configurations, since each particle can be in <math>|0\rangle</math> or <math>|1\rangle</math> independently. In almost all of the configurations, about half the particles are in <math>|0\rangle</math> and the other half in <math>|1\rangle</math>. The balance is a statistical effect: the number of configurations is largest when the particles are divided equally.

If the particles are indistinguishable, however, there are only <math>N+1</math> different configurations. If there are <math>K</math> particles in state <math>|1\rangle</math>, there are <math>N-K</math> particles in state <math>|0\rangle</math>. Whether any particular particle is in state <math>|0\rangle</math> or in state <math>|1\rangle</math> cannot be determined, so each value of <math>K</math> determines a unique quantum state for the whole system.

Suppose now that the energy of state <math>|1\rangle</math> is slightly greater than the energy of state <math>|0\rangle</math> by an amount <math>E</math>. At temperature <math>T</math>, a particle will have a lesser probability to be in state <math>|1\rangle</math> by <math>e^{-E/kT}</math>. In the distinguishable case, the particle distribution will be biased slightly towards state <math>|0\rangle</math>. But in the indistinguishable case, since there is no statistical pressure toward equal numbers, the most-likely outcome is that most of the particles will collapse into state <math>|0\rangle</math>.

In the distinguishable case, for large ''N'', the fraction in state <math>|0\rangle</math> can be computed. It is the same as flipping a coin with probability proportional to <math>\exp{(-E/T)}</math> to land tails.

In the indistinguishable case, each value of <math>K</math> is a single state, which has its own separate Boltzmann probability. So the probability distribution is exponential:

:<math>\,
P(K)= C e^{-KE/T} = C p^K.
</math>

For large <math>N</math>, the normalization constant <math>C</math> is <math>1-p</math>. The expected total number of particles not in the lowest energy state, in the limit that <math>N\rightarrow \infty</math>, is equal to
: <math>\sum_{n>0} C n p^n=p/(1-p) </math>
It does not grow when ''N'' is large; it just approaches a constant. This will be a negligible fraction of the total number of particles. So a collection of enough Bose particles in thermal equilibrium will mostly be in the ground state, with only a few in any excited state, no matter how small the energy difference.

Consider now a gas of particles, which can be in different momentum states labeled <math>|k\rangle</math>. If the number of particles is less than the number of thermally accessible states, for high temperatures and low densities, the particles will all be in different states. In this limit, the gas is classical. As the density increases or the temperature decreases, the number of accessible states per particle becomes smaller, and at some point, more particles will be forced into a single state than the maximum allowed for that state by statistical weighting. From this point on, any extra particle added will go into the ground state.

To calculate the transition temperature at any density, integrate, over all momentum states, the expression for maximum number of excited particles, <math>p/(1-p)</math>:

:<math>\,
 N = V \int {d^3k \over (2\pi)^3} {p(k)\over 1-p(k)} = V \int {d^3k \over (2\pi)^3} {1 \over e^{k^2\over 2mT}-1} </math>
:<math>\,
p(k)= e^{-k^2\over 2mT}.
</math>

When the integral (also known as [[Bose–Einstein integral]]) is evaluated with factors of <math>k_B</math> and <math>\hbar</math> restored by dimensional analysis, it gives the critical temperature formula of the preceding section. Therefore, this integral defines the critical temperature and particle number corresponding to the conditions of negligible [[chemical potential]] <math>\mu</math>. In [[Bose–Einstein statistics]] distribution, <math>\mu</math> is actually still nonzero for BECs; however, <math>\mu</math> is less than the ground state energy. Except when specifically talking about the ground state, <math>\mu</math> can be approximated for most energy or momentum states as&nbsp;<math>\mu \approx 0</math>.

=== Bogoliubov theory for weakly interacting gas ===
[[Nikolay Bogolyubov|Nikolay Bogoliubov]] considered perturbations on the limit of dilute gas,<ref name=Bogoliubov:1947/> finding a finite pressure at zero temperature and positive chemical potential. This leads to corrections for the ground state. The Bogoliubov state has pressure <math>(T=0)</math>: <math>P = gn^2/2</math>.

The original interacting system can be converted to a system of non-interacting particles with a dispersion law.

=== Gross–Pitaevskii equation ===
{{Main|Gross–Pitaevskii equation}}

In some simplest cases, the state of condensed particles can be described with a nonlinear Schrödinger equation, also known as Gross–Pitaevskii or Ginzburg–Landau equation. The validity of this approach is actually limited to the case of ultracold temperatures, which fits well for the most alkali atoms experiments.

This approach originates from the assumption that the state of the BEC can be described by the unique wavefunction of the condensate <math>\psi(\vec{r})</math>. For a [[Schrödinger field|system of this nature]], <math>|\psi(\vec{r})|^2</math> is interpreted as the particle density, so the total number of atoms is <math>N=\int d\vec{r}|\psi(\vec{r})|^2</math>

Provided essentially all atoms are in the condensate (that is, have condensed to the ground state), and treating the bosons using [[mean-field theory]], the energy (E) associated with the state <math>\psi(\vec{r})</math> is:

:<math>E=\int
d\vec{r}\left[\frac{\hbar^2}{2m}|\nabla\psi(\vec{r})|^2+V(\vec{r})|\psi(\vec{r})|^2+\frac{1}{2}U_0|\psi(\vec{r})|^4\right]</math>

Minimizing this energy with respect to infinitesimal variations in <math>\psi(\vec{r})</math>, and holding the number of atoms constant, yields the Gross–Pitaevski equation (GPE) (also a non-linear [[Schrödinger equation]]):

:<math>i\hbar\frac{\partial \psi(\vec{r})}{\partial t} = \left(-\frac{\hbar^2\nabla^2}{2m}+V(\vec{r})+U_0|\psi(\vec{r})|^2\right)\psi(\vec{r})</math>

where:

:{|cellspacing="0" cellpadding="0"
|-
| <math>\,m</math>
| &nbsp;is the mass of the bosons,
|-
| <math>\,V(\vec{r})</math>
| &nbsp;is the external potential, and
|-
| <math>\,U_0</math>
| &nbsp;represents the inter-particle interactions.
|}

In the case of zero external potential, the dispersion law of interacting Bose–Einstein-condensed particles is given by so-called Bogoliubov spectrum (for <math>\ T= 0</math>):

:<math> {\omega _p} = \sqrt {\frac{{{p^2}}}{{2m}}\left( {\frac{{{p^2}}}{{2m}} + 2{U_0}{n_0}} \right)} </math>

The Gross-Pitaevskii equation (GPE) provides a relatively good description of the behavior of atomic BEC's. However, GPE does not take into account the temperature dependence of dynamical variables, and is therefore valid only for <math>\ T= 0</math>.
It is not applicable, for example, for the condensates of excitons, magnons and photons, where the critical temperature is comparable to room temperature.

==== Numerical solution ====
The Gross-Pitaevskii equation is a partial differential equation in space and time variables. Usually it does not have analytic solution and
different numerical methods, such as split-step
[[Crank–Nicolson method|Crank–Nicolson]]<ref>{{cite journal
 |author=P. Muruganandam and S. K. Adhikari
 |year=2009
 |title=Fortran Programs for the time-dependent Gross-Pitaevskii equation in a fully anisotropic trap
 |journal=Comput. Phys. Commun.
 |volume=180 |issue=3 |pages=1888–1912
 |doi=10.1016/j.cpc.2009.04.015
|bibcode=2009CoPhC.180.1888M|arxiv=0904.3131|s2cid=7403553
 }}</ref>
and [[Fourier spectral]]<ref>{{cite journal
 |author=P. Muruganandam and S. K. Adhikari
 |year=2003
 |title=Bose–Einstein condensation dynamics in three dimensions by the pseudospectral and finite-difference methods
 |journal=J. Phys. B
 |volume=36 |issue= 12|pages=2501–2514
 |doi=10.1088/0953-4075/36/12/310
 |bibcode=2003JPhB...36.2501M|arxiv=cond-mat/0210177|s2cid=13180020
 }}</ref> methods, are used for its solution. There are different Fortran and C programs for its solution for [[contact interaction]]<ref>{{cite journal
 |author=D. Vudragovic|display-authors=et al
 |year=2012
 |title=C Programs for the time-dependent Gross-Pitaevskii equation in a fully anisotropic trap
 |journal= Comput. Phys. Commun.
 |volume=183 |issue=9 |pages=2021–2025
 |doi=10.1016/j.cpc.2012.03.022
  |bibcode=2012CoPhC.183.2021V|arxiv=1206.1361|s2cid=12031850
 }}</ref><ref>
{{cite journal
 |author=L. E. Young-S.|display-authors=et al
 |year=2016
 |title=OpenMP Fortran and C Programs for the time-dependent Gross-Pitaevskii equation in a fully anisotropic trap
 |journal= Comput. Phys. Commun.
 |volume=204 |issue=9 |pages=209–213
 |doi=10.1016/j.cpc.2016.03.015
 |bibcode=2016CoPhC.204..209Y|arxiv=1605.03958|s2cid=206999817
 }}</ref>
and long-range [[dipolar interaction]]<ref>
{{cite journal
 |author=K. Kishor Kumar|display-authors=et al
 |year=2015
 |title=Fortran and C Programs for the time-dependent dipolar Gross-Pitaevskii equation in a fully anisotropic trap
 |journal= Comput. Phys. Commun.
 |volume=195 |pages=117–128
 |doi=10.1016/j.cpc.2015.03.024
 |bibcode=2015CoPhC.195..117K|arxiv=1506.03283|s2cid=18949735
 }}</ref> which can be freely used.

==== Weaknesses of Gross–Pitaevskii model ====
The Gross–Pitaevskii model of BEC is a physical [[approximation]] valid for certain classes of BECs. By construction, the [[Gross–Pitaevskii equation|GPE]] uses the following simplifications: it assumes that interactions between condensate particles are of the contact two-body type and also neglects anomalous contributions to [[self-energy]].<ref>Beliaev, S. T. Zh. Eksp. Teor. Fiz. 34, 417–432 (1958) [Soviet Phys. JETP 7, 289 (1958)]; ibid. 34, 433–446 [Soviet Phys. JETP 7, 299 (1958)].</ref> These assumptions are suitable mostly for the dilute three-dimensional condensates. If one relaxes any of these assumptions, the equation for the condensate [[wavefunction]] acquires the terms containing higher-order powers of the wavefunction. Moreover, for some physical systems the amount of such terms turns out to be infinite, therefore, the equation becomes essentially non-polynomial. The examples where this could happen are the Bose–Fermi composite condensates,<ref name=Schick:1971/><ref name=Kolomeisky:1992/><ref name=Kolomeisky:2000/><ref name=Chui:2004/> effectively lower-dimensional condensates,<ref>
{{cite journal
 |author1=L. Salasnich
 |author2=A. Parola
 |author3=L. Reatto |name-list-style=amp
 |year=2002
 |title=Effective wave equations for the dynamics of cigar-shaped and disk-shaped Bose condensates
 |journal=Phys. Rev. A
 |volume=65 |issue=4 |page=043614
 |arxiv=cond-mat/0201395
 |bibcode = 2002PhRvA..65d3614S
 |doi=10.1103/PhysRevA.65.043614|s2cid=119376582
 }}
</ref> and dense condensates and [[superfluid]] clusters and droplets.<ref>
{{cite journal
 |author1=A. V. Avdeenkov
 |author2=K. G. Zloshchastiev
 |year=2011
 |title=Quantum Bose liquids with logarithmic nonlinearity: Self-sustainability and emergence of spatial extent
 |journal=J. Phys. B: At. Mol. Opt. Phys.
 |volume=44 |issue=19 |pages=195303
 |arxiv=1108.0847
 |bibcode=2011JPhB...44s5303A
 |doi=10.1088/0953-4075/44/19/195303|s2cid=119248001
 }}
</ref> It is found that one has to go beyond the Gross-Pitaevskii equation. For example, the logarithmic term <math>\psi \ln |\psi|^2 </math> found in the [[Logarithmic Schrödinger equation]] must be added to the Gross-Pitaevskii equation along with a [[Vitaly Ginzburg|Ginzburg]]–Sobyanin contribution to correctly determine that the speed of sound scales as the cubic root of pressure for Helium-4 at very low temperatures in close agreement with experiment.<ref>{{cite journal|author1=T.C Scott|author2=K. G. Zloshchastiev|title=Resolving the puzzle of sound propagation in liquid helium at low temperatures|journal=Low Temperature Physics|volume=45|issue=12|year=2019|pages=1231–1236|doi=10.1063/10.0000200|arxiv=2006.08981|bibcode=2019LTP....45.1231S|s2cid=213962795}}</ref>

==== Other ====
However, it is clear that in a general case the behaviour of Bose–Einstein condensate can be described by coupled evolution equations for condensate density, superfluid velocity and distribution function of elementary excitations. This problem was solved in 1977 by Peletminskii et al. in microscopical approach. The Peletminskii equations are valid for any finite temperatures below the critical point. Years after, in 1985, Kirkpatrick and Dorfman obtained similar equations using another microscopical approach. The Peletminskii equations also reproduce Khalatnikov hydrodynamical equations for superfluid as a limiting case.

=== Superfluidity of BEC and Landau criterion ===
The phenomena of superfluidity of a Bose gas and superconductivity of a strongly-correlated Fermi gas (a gas of Cooper pairs) are tightly connected to Bose–Einstein condensation. Under corresponding conditions, below the temperature of phase transition, these phenomena were observed in [[helium-4]] and different classes of superconductors. In this sense, the superconductivity is often called the superfluidity of Fermi gas. In the simplest form, the origin of superfluidity can be seen from the weakly interacting bosons model.

== Peculiar properties ==

=== Quantized vortices ===
As in many other systems, [[Vortex|vortices]] can exist in BECs.<ref>
{{Cite journal| doi = 10.1103/PhysRevLett.83.2498| volume = 83| issue = 13| pages = 2498–2501| last1 = Matthews| first1 = M. R.| last2 = Anderson| first2 = B. P.| last3 = Haljan| first3 = P. C.| last4 = Hall| first4 = D. S.| last5 = Wieman| first5 = C. E.| last6 = Cornell| first6 = E. A.| title = Vortices in a Bose-Einstein Condensate| journal = Physical Review Letters| accessdate = 2021-10-20| date = 1999-09-27| arxiv = cond-mat/9908209| bibcode = 1999PhRvL..83.2498M| s2cid = 535347| url = https://link.aps.org/doi/10.1103/PhysRevLett.83.2498}}</ref> 
Vortices can be created, for example, by "stirring" the condensate with lasers,<ref>{{Cite journal| doi = 10.1103/PhysRevLett.84.806| volume = 84| issue = 5| pages = 806–809| last1 = Madison| first1 = K. W.| last2 = Chevy| first2 = F.| last3 = Wohlleben| first3 = W.| last4 = Dalibard| first4 = J.| title = Vortex Formation in a Stirred Bose-Einstein Condensate| journal = Physical Review Letters| accessdate = 2021-10-20| date = 2000-01-31| pmid = 11017378| arxiv = cond-mat/9912015| bibcode = 2000PhRvL..84..806M| s2cid = 9128694| url = https://link.aps.org/doi/10.1103/PhysRevLett.84.806}}</ref> 
rotating the confining trap,<ref>{{Cite journal| doi = 10.1103/PhysRevLett.88.070409| volume = 88| issue = 7| pages = 070409| last1 = Abo-Shaeer| first1 = J. R.| last2 = Raman| first2 = C.| last3 = Ketterle| first3 = Wolfgang| title = Formation and decay of vortex lattices in Bose-Einstein condensates at finite temperatures| journal = Physical Review Letters| date = 2002| pmid = 11863877| arxiv = cond-mat/0108195| bibcode = 2002PhRvL..88g0409A| s2cid = 1599126}}</ref> 
or by rapid cooling across the phase transition.<ref>{{Cite journal| doi = 10.1038/nature07334| volume = 455| issue = 7215| pages = 948–951| last1 = Weiler| first1 = Chad N| last2 = Neely| first2 = Tyler W| last3 = Scherer| first3 = David R| last4 = Bradley| first4 = A S| last5 = Davis| first5 = M J| last6 = Anderson| first6 = B P| title = Spontaneous vortices in the formation of Bose–Einstein condensates| journal = Nature| date = 2008-10-16| arxiv = 0807.3323| bibcode = 2008Natur.455..948W| s2cid = 459795}}</ref> 
The vortex created will be a [[quantum vortex]] with core shape determined by the interactions.<ref>{{Cite journal|last1=Fetter |first1=A. L.|last2=Svidzinsky|first2=A.|title=Vortices in a Trapped Dilute Bose-Einstein Condensate|journal=Journal of Physics: Condensed Matter|year=2001 |volume=13|issue=12|pages=R135–94|doi=10.1088/0953-8984/13/12/201|arxiv=cond-mat/0102003 |s2cid=118913736 }}</ref> Fluid circulation around any point is quantized due to the single-valued nature of the order BEC order parameter or wavefunction,<ref>{{Cite journal| doi = 10.1007/BF02780991| issn = 1827-6121| volume = 6| issue = 2| pages = 279–287| last = Onsager| first = L.| title = Statistical hydrodynamics| journal = Il Nuovo Cimento | accessdate = 2019-11-17| date = 1949-03-01| bibcode = 1949NCim....6S.279O| s2cid = 186224016| url = https://doi.org/10.1007/BF02780991}}</ref> that can be written in the form <math>\psi(\vec{r})=\phi(\rho,z)e^{i\ell\theta}</math> where <math>\rho, z</math> and <math>\theta</math> are as in the [[cylindrical coordinate system]], and <math>\ell</math> is the angular quantum number (a.k.a. the "charge" of the vortex). Since the energy of a vortex is proportional to the square of its angular momentum, in [[trivial topology]] only <math>\ell=1</math> vortices can exist in the [[steady state]]; Higher-charge vortices will have a tendency to split into <math>\ell=1</math> vortices, if allowed by the topology of the geometry.

An axially symmetric (for instance, harmonic) confining potential is commonly used for the study of vortices in BEC. To determine <math>\phi(\rho,z)</math>, the energy of <math>\psi(\vec{r})</math> must be minimized, according to the constraint <math>\psi(\vec{r})=\phi(\rho,z)e^{i\ell\theta}</math>. This is usually done computationally, however, in a uniform medium, the following analytic form demonstrates the correct behavior, and is a good approximation:

:<math>\phi=\frac{nx}{\sqrt{2+x^2}}\,.</math>

Here, <math>n</math> is the density far from the vortex and <math>x=\rho/(\ell \xi)</math>, where <math>\xi=1/\sqrt{8\pi a_s n_0}</math> is the [[Gross–Pitaevskii equation#Healing length|healing length]] of the condensate.

A singly charged vortex (<math>\ell=1</math>) is in the ground state, with its energy <math>\epsilon_v</math> given by

:<math>\epsilon_v=\pi n
\frac{\hbar^2}{m}\ln\left(1.464\frac{b}{\xi}\right)</math>

where <math>\,b</math>&nbsp;is&nbsp;the farthest distance from the vortices considered.(To obtain an energy which is well defined it is necessary to include this boundary <math>b</math>.)

For multiply charged vortices (<math>\ell >1</math>) the energy is approximated by

:<math>\epsilon_v\approx \ell^2\pi n
\frac{\hbar^2}{m}\ln\left(\frac{b}{\xi}\right)</math>

which is greater than that of <math>\ell</math> singly charged vortices, indicating that these multiply charged vortices are unstable to decay. Research has, however, indicated they are metastable states, so may have relatively long lifetimes.

Closely related to the creation of vortices in BECs is the generation of so-called dark [[soliton]]s in one-dimensional BECs. These topological objects feature a phase gradient across their nodal plane, which stabilizes their shape even in propagation and interaction. Although solitons carry no charge and are thus prone to decay, relatively long-lived dark solitons have been produced and studied extensively.<ref>{{Cite journal| doi = 10.1038/nphys962| issn = 1745-2481| volume = 4| issue = 6| pages = 496–501| last1 = Becker| first1 = Christoph| last2 = Stellmer| first2 = Simon| last3 = Soltan-Panahi| first3 = Parvis| last4 = Dörscher| first4 = Sören| last5 = Baumert| first5 = Mathis| last6 = Richter| first6 = Eva-Maria| last7 = Kronjäger| first7 = Jochen| last8 = Bongs| first8 = Kai| last9 = Sengstock| first9 = Klaus| title = Oscillations and interactions of dark and dark–bright solitons in Bose–Einstein condensates| journal = Nature Physics| accessdate = 2021-10-27| date = 2008-05-04| arxiv = 0804.0544| bibcode = 2008NatPh...4..496B| s2cid = 119300908| url = https://www.nature.com/articles/nphys962}}</ref>

=== Attractive interactions ===
Experiments led by Randall Hulet at Rice University from 1995 through 2000 showed that lithium condensates with attractive interactions could stably exist up to a critical atom number. Quench cooling the gas, they observed the condensate to grow, then subsequently collapse as the attraction overwhelmed the zero-point energy of the confining potential, in a burst reminiscent of a supernova, with an explosion preceded by an implosion.

Further work on attractive condensates was performed in 2000 by the [[JILA]] team, of Cornell, Wieman and coworkers. Their instrumentation now had better control so they used naturally ''attracting'' atoms of rubidium-85 (having negative atom–atom [[scattering length]]). Through [[Feshbach resonance]] involving a sweep of the magnetic field causing spin flip collisions, they lowered the characteristic, discrete energies at which rubidium bonds, making their Rb-85 atoms repulsive and creating a stable condensate. The reversible flip from attraction to repulsion stems from quantum [[Interference (wave propagation)|interference]] among wave-like condensate atoms.

When the JILA team raised the magnetic field strength further, the condensate suddenly reverted to attraction, imploded and shrank beyond detection, then exploded, expelling about two-thirds of its 10,000 atoms. About half of the atoms in the condensate seemed to have disappeared from the experiment altogether, not seen in the cold remnant or expanding gas cloud.<ref name=nobel/> [[Carl Wieman]] explained that under current atomic theory this characteristic of Bose–Einstein condensate could not be explained because the energy state of an atom near absolute zero should not be enough to cause an implosion; however, subsequent mean-field theories have been proposed to explain it. Most likely they formed molecules of two rubidium atoms;<ref name=vanPutten:2010/> energy gained by this bond imparts velocity sufficient to leave the trap without being detected.

The process of creation of molecular Bose condensate during the sweep of the magnetic field throughout the Feshbach resonance, as well as the reverse process, are described by the exactly solvable model that can explain many experimental observations.<ref name="sun-16pra2">{{cite journal|doi=10.1103/PhysRevA.94.033808|title=Landau-Zener extension of the Tavis-Cummings model: Structure of the solution|author1=C. Sun|author2=N. A. Sinitsyn |journal=[[Phys. Rev. A]]|volume=94|issue=3|year=2016|pages=033808|bibcode=2016PhRvA..94c3808S|arxiv=1606.08430|s2cid=119317114}}</ref>

== Current research ==
{{unsolved|physics|How do we rigorously prove the existence of Bose–Einstein condensates for generally interacting systems?}}
Compared to more commonly encountered states of matter, Bose–Einstein condensates are extremely fragile.<ref>{{Cite web|url=http://physicsworld.com/cws/article/news/2013/nov/28/how-to-watch-a-bose-einstein-condensate-for-a-very-long-time|title=How to watch a Bose–Einstein condensate for a very long time - physicsworld.com|website=physicsworld.com|date=28 November 2013|language=en-GB|access-date=2018-01-22}}</ref> The slightest interaction with the external environment can be enough to warm them past the condensation threshold, eliminating their interesting properties and forming a normal gas.<ref>{{cite journal|url=https://www.nist.gov/news-events/news/2001/10/bose-einstein-condensate-new-form-matter |title=Bose-Einstein Condensate: A New Form of Matter |journal=NIST |date=October 9, 2001 |access-date=January 17, 2022 |publisher=[[National Institute of Standards and Technology]]}}</ref>

Nevertheless, they have proven useful in exploring a wide range of questions in fundamental physics, and the years since the initial discoveries by the JILA and MIT groups have seen an increase in experimental and theoretical activity.

Bose–Einstein condensates composed of a wide range of [[isotope]]s have been produced; see below.<ref>{{cite web | url=http://physicsworld.com/cws/article/print/2005/jun/01/ten-of-the-best-for-bec| title=Ten of the best for BEC | publisher=Physicsweb.org | date=1 June 2005 }}</ref>

=== Fundamental research ===

Examples include experiments that have demonstrated [[Interference (wave propagation)|interference]] between condensates due to [[wave–particle duality]],<ref>{{cite web | author=Gorlitz, Axel | url=http://cua.mit.edu/ketterle_group/Projects_1997/Interference/Interference_BEC.htm | title=Interference of Condensates (BEC@MIT) | publisher=Cua.mit.edu | access-date=13 October 2009 | url-status=dead | archive-url=https://web.archive.org/web/20160304092631/http://cua.mit.edu/ketterle_group/Projects_1997/Interference/Interference_BEC.htm | archive-date=4 March 2016}}</ref> the study of [[superfluidity]] and quantized [[vortex|vortices]], the creation of bright matter wave [[soliton]]s from Bose condensates confined to one dimension, and the [[slow light|slowing of light]] pulses to very low speeds using [[electromagnetically induced transparency]].<ref>
{{cite journal
 |author1=Z. Dutton
 |author2=N. S. Ginsberg
 |author3=C. Slowe
 |author4=L. Vestergaard Hau |name-list-style=amp
 |year=2004
 |title=The art of taming light: ultra-slow and stopped light
 |journal=Europhysics News
 |volume=35 |issue=2 |pages=33–39
 |doi=10.1051/epn:2004201
 |bibcode=2004ENews..35...33D|doi-access=free
 }}
</ref> Vortices in Bose–Einstein condensates are also currently the subject of [[analogue gravity]] research, studying the possibility of modeling [[black hole]]s and their related phenomena in such environments in the laboratory.

Experimenters have also realized "[[optical lattice]]s", where the interference pattern from overlapping lasers provides a [[periodic potential]]. These are used to explore the transition between a superfluid and a [[Mott insulator]].<ref>{{cite web | url=http://qpt.physics.harvard.edu/qptsi.html | title=From Superfluid to Insulator: Bose–Einstein Condensate Undergoes a Quantum Phase Transition | publisher=Qpt.physics.harvard.edu | access-date=13 October 2009}}</ref>

They are also useful in studying Bose–Einstein condensation in fewer than three dimensions, for example the [[Lieb–Liniger model]] (an the limit of strong interactions, the [[Tonks–Girardeau gas]]) in 1D and the [[Berezinskii–Kosterlitz–Thouless transition]] in 2D. Indeed, a deep optical lattice allows the experimentalist to freeze the motion of the particles along one or two directions, effectively eliminating one or two dimension from the system.

Further, the sensitivity of the pinning transition of strongly interacting bosons confined in a shallow one-dimensional optical lattice originally observed by Haller<ref>
{{cite journal
 |author1=Elmar Haller
 |author2=Russell Hart
 |author3=Manfred J. Mark
 |author4=Johann G. Danzl
 |author5=Lukas Reichsoellner
 |author6=Mattias Gustavsson
 |author7=Marcello Dalmonte
 |author8=Guido Pupillo
 |author9=Hanns-Christoph Naegerl
 |year=2010
 |title=Pinning quantum phase transition for a Luttinger liquid of strongly interacting bosons
 |journal=Nature Letters
 |volume=466 |issue=7306
 |pages=597–600
 |doi=10.1038/nature09259|pmid=20671704
 |arxiv=1004.3168
 |bibcode=2010Natur.466..597H
 |s2cid=687095
 }}
</ref> has been explored via a tweaking of the primary optical lattice by a secondary weaker one.<ref>
{{cite journal
 |author1=Asaad R. Sakhel
 |year=2016
 |title=Properties of bosons in a one-dimensional bichromatic optical lattice in the regime of the pinning transition: A worm- algorithm Monte Carlo study
 |journal=Physical Review A
 |volume=94 |issue=3
 |pages=033622
 |doi=10.1103/PhysRevA.94.033622|arxiv=1511.00745
 |bibcode=2016PhRvA..94c3622S
 |s2cid=55812834
 }}
</ref> Thus for a resulting weak bichromatic optical lattice, it has been found that the pinning transition is robust against the
introduction of the weaker secondary optical lattice.

Studies of vortices in nonuniform Bose–Einstein condensates<ref>
{{cite journal
 |author1=Roger R. Sakhel
 |author2=Asaad R. Sakhel
 |year=2016
 |title=Elements of Vortex-Dipole Dynamics in a Nonuniform Bose–Einstein Condensate
 |journal=Journal of Low Temperature Physics
 |volume=184 |issue=5–6
 |pages=1092–1113
 |doi=10.1007/s10909-016-1636-3|bibcode=2016JLTP..184.1092S
 |s2cid=124942094
 }}
</ref> as well as excitations of these systems by the application of moving repulsive or attractive obstacles, have also been undertaken.<ref>
{{cite journal
 |author1=Roger R. Sakhel
 |author2=Asaad R. Sakhel
 |author3=Humam B. Ghassib
 |year=2011
 |title=Self-interfering matter-wave patterns generated by a moving laser obstacle in a two-dimensional Bose–Einstein condensate inside a power trap cut off by box potential boundaries
 |journal=Physical Review A
 |volume=84 |issue=3
 |pages=033634
 |doi=10.1103/PhysRevA.84.033634|arxiv=1107.0369
 |bibcode=2011PhRvA..84c3634S
 |s2cid=119277418
 }}
</ref><ref>
{{cite journal
 |author1=Roger R. Sakhel
 |author2=Asaad R. Sakhel
 |author3=Humam B. Ghassib
 |year=2013
 |title=Nonequilibrium Dynamics of a Bose–Einstein Condensate Excited by a Red Laser Inside a Power-Law Trap with Hard Walls
 |journal=Journal of Low Temperature Physics
 |volume=173 |issue=3–4
 |pages=177–206
 |doi=10.1007/s10909-013-0894-6|bibcode=2013JLTP..173..177S
 |s2cid=122038877
 }}
</ref> Within this context, the conditions for order and chaos in the dynamics of a trapped Bose–Einstein condensate have been explored by the application of moving blue and red-[[Laser detuning|detuned]] laser beams (hitting frequencies slightly above and below the resonance frequency, respectively) via the time-dependent Gross-Pitaevskii equation.<ref>
{{cite journal
 |author1=Roger R. Sakhel
 |author2=Asaad R. Sakhel
 |author3=Humam B. Ghassib
 |author4=Antun Balaz
 |year=2016
 |title=Conditions for order and chaos in the dynamics of a trapped Bose–Einstein condensate in coordinate and energy space
 |journal=European Physical Journal D
 |volume=70 |issue=3
 |pages=66
 |doi=10.1140/epjd/e2016-60085-2|arxiv=1604.01349
 |bibcode=2016EPJD...70...66S
 |s2cid=119180702
 }}
</ref>

=== Applications ===

In 1999, Danish physicist [[Lene Hau]] led a team from [[Harvard University]] which [[Slow light|slowed a beam of light]] to about 17 meters per second{{Clarify|date=January 2010|reason=group velocity and not actual velocity?}} using a superfluid.<ref>{{cite web | last = Cromie | first = William J. | title = Physicists Slow Speed of Light | website = The Harvard University Gazette | date = 18 February 1999 | url = http://news.harvard.edu/gazette/1999/02.18/light.html | access-date = 26 January 2008 }}</ref> Hau and her associates have since made a group of condensate atoms recoil from a light pulse such that they recorded the light's phase and amplitude, recovered by a second nearby condensate, in what they term "slow-light-mediated atomic matter-wave amplification" using Bose–Einstein condensates.<ref name=Ginsberg:2007/>

Another current research interest is the creation of Bose–Einstein condensates in microgravity in order to use its properties for high precision [[Atom interferometer|atom interferometry]]. The first demonstration of a BEC in weightlessness was achieved in 2008 at a [[Fallturm Bremen|drop tower]] in Bremen, Germany by a consortium of researchers led by [[Ernst M. Rasel]] from [[Leibniz University Hannover]].<ref>{{Cite journal|last1=Zoest|first1=T. van|last2=Gaaloul|first2=N.|last3=Singh|first3=Y.|last4=Ahlers|first4=H.|last5=Herr|first5=W.|last6=Seidel|first6=S. T.|last7=Ertmer|first7=W.|last8=Rasel|first8=E.|last9=Eckart|first9=M.|date=2010-06-18|title=Bose–Einstein Condensation in Microgravity|journal=Science|language=en|volume=328|issue=5985|pages=1540–1543|doi=10.1126/science.1189164|pmid=20558713|bibcode=2010Sci...328.1540V|s2cid=15194813}}</ref> The same team demonstrated in 2017 the first creation of a Bose–Einstein condensate in space<ref>{{Cite news|url=http://www.dlr.de/dlr/en/desktopdefault.aspx/tabid-10081/151_read-20337/#/gallery/25194|title=MAIUS 1 – First Bose–Einstein condensate generated in space|last=DLR|work=DLR Portal|access-date=2017-05-23|language=en-GB}}</ref> and it is also the subject of two upcoming experiments on the [[International Space Station]].<ref>{{Cite web|url=https://coldatomlab.jpl.nasa.gov/|title=Cold Atom Laboratory|last=Laboratory|first=Jet Propulsion|website=coldatomlab.jpl.nasa.gov|access-date=2017-05-23}}</ref><ref>{{Cite web|url=http://www.lpi.usra.edu/planetary_news/2017/03/13/2017-nasa-fundamental-physics-workshop/|title=2017 NASA Fundamental Physics Workshop {{!}} Planetary News|website=www.lpi.usra.edu|language=en-US|access-date=2017-05-23}}</ref>

Researchers in the new field of [[atomtronics]] use the properties of Bose–Einstein condensates in the emerging quantum technology of matter-wave circuits.<ref>{{Cite journal |last1=Amico |first1=L. |last2=Boshier |first2=M. |last3=Birkl |first3=G. |last4=Minguzzi |first4=A.|author4-link=Anna Minguzzi |last5=Miniatura |first5=C. |last6=Kwek |first6=L.-C. |last7=Aghamalyan |first7=D. |last8=Ahufinger |first8=V. |last9=Anderson |first9=D. |last10=Andrei |first10=N. |last11=Arnold |first11=A. S. |last12=Baker |first12=M. |last13=Bell |first13=T. A. |last14=Bland |first14=T. |last15=Brantut |first15=J. P. |date=25 August 2021 |title=Roadmap on Atomtronics: State of the art and perspective |url=https://avs.scitation.org/doi/10.1116/5.0026178 |journal=AVS Quantum Science |language=en |volume=3 |issue=3 |pages=039201 |doi=10.1116/5.0026178 |arxiv=2008.04439 |bibcode=2021AVSQS...3c9201A |s2cid=235417597 |issn=2639-0213}}</ref><ref>
{{cite journal
 |author=P. Weiss
 |date=12 February 2000
 |title=Atomtronics may be the new electronics
 |journal=Science News Online
 |volume=157 |issue=7 |page=104
 |doi=10.2307/4012185
 |url=http://www.sciencenews.org/view/generic/id/69786
 |jstor=4012185}}
</ref>

In 1970, BECs were proposed by [[Emmanuel David Tannenbaum]] for anti-[[stealth technology]].<ref>{{cite arXiv | last=Tannenbaum| first=Emmanuel David | title=Gravimetric Radar: Gravity-based detection of a point-mass moving in a static background| year=1970| eprint=1208.2377| class=physics.ins-det}}</ref>

=== Isotopes ===

Bose-Einstein condensation has mainly been observed on alkaline atoms, some of which have collisional properties particularly suitable for evaporative cooling in traps, and which where the first to laser-cooled. As of 2021, using ultra-low temperatures of {{val|e=-7|u=K}} or below, Bose–Einstein condensates had been obtained for a multitude of isotopes with more or less ease, mainly of [[alkali metal]], [[alkaline earth metal]], and [[lanthanide]] atoms ({{SimpleNuclide|lithium|7|link=yes}}, {{SimpleNuclide|sodium|23|link=yes}}, {{SimpleNuclide|potassium|39|link=yes}}, {{SimpleNuclide|potassium|41|link=yes}}, {{SimpleNuclide|rubidium|85|link=yes}}, {{SimpleNuclide|Rubidium|87|link=yes}}, {{SimpleNuclide|caesium|133|link=yes}}, {{SimpleNuclide|chromium|52|link=yes}}, {{SimpleNuclide|calcium|40|link=yes}}, {{SimpleNuclide|strontium|84|link=yes}}, {{SimpleNuclide|strontium|86|link=yes}}, {{SimpleNuclide|strontium|88|link=yes}}, {{SimpleNuclide|ytterbium|170|link=yes}}, {{SimpleNuclide|ytterbium|174|link=yes}}, {{SimpleNuclide|ytterbium|176|link=yes}}, {{SimpleNuclide|dysprosium|164|link=yes}}, {{SimpleNuclide|erbium|168|link=yes}}, {{SimpleNuclide|thulium|169|link=yes}}, and metastable {{SimpleNuclide|helium|4|link=yes}} (orthohelium)).<ref>{{cite journal | last1=Schreck | first1=Florian | last2=Druten | first2=Klaasjan van | title=Laser cooling for quantum gases | journal=Nature Physics | volume=17 | issue=12 | date=2021 | issn=1745-2473 | doi=10.1038/s41567-021-01379-w | pages=1296–1304| arxiv=2209.01026 }}</ref><ref>{{cite thesis |last=Stellmer |first=Simon |date=2013 |title=Degenerate quantum gases of strontium |degree=PhD |publisher=University of Innsbruck|url=http://www.ultracold.at/theses/2013-stellmer.pdf}}</ref> Research was finally successful in atomic hydrogen with the aid of the newly developed method of 'evaporative cooling'.<ref>
{{cite journal
 |author1=Dale G. Fried
 |author2=Thomas C. Killian
 |author3=Lorenz Willmann
 |author4=David Landhuis
 |author5=Stephen C. Moss
 |author6=Daniel Kleppner
 |author7=Thomas J. Greytak |name-list-style=amp
 |year=1998
 |title=Bose–Einstein Condensation of Atomic Hydrogen
 |journal=Phys. Rev. Lett.
 |volume=81 |issue=18 |pages=3811
 |doi=10.1103/PhysRevLett.81.3811 |bibcode=1998PhRvL..81.3811F|arxiv = physics/9809017 |s2cid=3174641
 }}
</ref>

In contrast, the superfluid state of {{SimpleNuclide|Helium|4|link=yes}} below {{val|1.17|u=K}} is differs significantly from dilute degenerate atomic gases because the interaction between the atoms is strong. Only 8% of atoms are in the condensed fraction near absolute zero, rather than near 100% of a weakly interacting BEC.<ref>{{cite web | url=https://www.nobelprize.org/nobel_prizes/physics/laureates/2001/advanced-physicsprize2001.pdf |archive-url=https://ghostarchive.org/archive/20221009/https://www.nobelprize.org/nobel_prizes/physics/laureates/2001/advanced-physicsprize2001.pdf |archive-date=2022-10-09 |url-status=live| title=Bose–Einstein Condensation in Alkali Gases | publisher=The Royal Swedish Academy of Sciences | date=2001 | access-date = 17 April 2017 }}</ref>

The [[boson]]ic behavior of some of these alkaline gases appears odd at first sight, because their nuclei have half-integer total spin. It arises from the interplay of electronic and nuclear spins: at ultra-low temperatures and corresponding excitation energies, the half-integer total spin of the electronic shell (one outer electron) and half-integer total spin of the nucleus are coupled by a very weak [[hyperfine structure|hyperfine interaction]].<ref name="f953">{{cite book | last=Dunlap | first=Richard A. | title=Lasers and Their Application to the Observation of Bose-Einstein Condensates | publisher=Iop Concise Physics | date=2019-09-04 | isbn=978-1-64327-693-9 | page=}}</ref> The total spin of the atom, arising from this coupling, is an integer value.<ref>The chemistry of systems at room temperature is determined by the electronic properties, which is essentially fermionic, since room temperature thermal excitations have typical energies much higher than the hyperfine values.</ref> Conversely, alkali isotopes which have an integer nuclear spin (such as {{SimpleNuclide|lithium|6|link=yes}} and {{SimpleNuclide|potassium|40|link=yes}}) are fermions and can form degenerate [[Fermi gas]]es, also called "Fermi condensates".<ref>{{cite conference | last=Greiner | first=Markus | title=AIP Conference Proceedings | chapter=Fermionic Condensates | publisher=AIP | volume=770 | date=2005 | doi=10.1063/1.1928855 | pages=209–217| arxiv=cond-mat/0502539 }}</ref>

Cooling [[fermion]]s to extremely low temperatures has created [[degenerate matter|degenerate]] gases, subject to the [[Pauli exclusion principle]]. To exhibit Bose–Einstein condensation, the fermions must "pair up" to form bosonic compound particles (e.g. [[molecule]]s or [[BCS theory|Cooper pairs]]). The first [[molecule|molecular]] condensates were created in November 2003 by the groups of [[Rudolf Grimm]] at the [[University of Innsbruck]], [[Deborah S. Jin]] at the [[University of Colorado at Boulder]] and [[Wolfgang Ketterle]] at [[Massachusetts Institute of Technology|MIT]]. Jin quickly went on to create the first [[fermionic condensate]], working with the same system but outside the molecular regime.<ref>{{cite web | url=http://physicsworld.com/cws/article/news/2004/jan/28/fermionic-condensate-makes-its-debut|title=Fermionic condensate makes its debut| publisher=Physicsweb.org | date=28 January 2004 }}</ref>

=== Continuous Bose–Einstein condensation ===
Limitations of evaporative cooling have restricted atomic BECs to "pulsed" operation, involving a highly inefficient duty cycle that discards more than 99% of atoms to reach BEC. Achieving continuous BEC has been a major open problem of experimental BEC research, driven by the same motivations as continuous optical laser development: high flux, high coherence matter waves produced continuously would enable new sensing applications.

Continuous BEC was achieved for the first time in 2022 with {{SimpleNuclide|strontium|84|link=yes}}.<ref>
{{cite journal
 |author1=Chun-Chia Chen
 |author2=Rodrigo González Escudero
 |author3=Jiří Minář
 |author4=Benjamin Pasquiou
 |author5=Shayne Bennetts
 |author6=Florian Schreck
 |year=2022
 |title=Continuous Bose–Einstein Condensation
 |journal=[[Nature (journal)|Nature]]
 |volume=606
 |issue=7915
 |pages=683–687
 |doi=10.1038/s41586-022-04731-z|pmid=35676487
 |pmc=9217748
 |bibcode=2022Natur.606..683C
 |s2cid=237532099
 }}</ref>

=== In solid state physics ===

In 2020, researchers reported the development of [[superconductivity|superconducting]] BEC and that there appears to be a "smooth transition between" BEC and [[BCS theory|Bardeen–Cooper–Shrieffer]] regimes.<ref>{{cite news |title=Researchers demonstrate a superconductor previously thought impossible |url=https://phys.org/news/2020-11-superconductor-previously-thought-impossible.html |access-date=8 December 2020 |work=phys.org |language=en}}</ref><ref>{{cite journal |last1=Hashimoto |first1=Takahiro |last2=Ota |first2=Yuichi |last3=Tsuzuki |first3=Akihiro |last4=Nagashima |first4=Tsubaki |last5=Fukushima |first5=Akiko |last6=Kasahara |first6=Shigeru |last7=Matsuda |first7=Yuji |last8=Matsuura |first8=Kohei |last9=Mizukami |first9=Yuta |last10=Shibauchi |first10=Takasada |last11=Shin |first11=Shik |last12=Okazaki |first12=Kozo |title=Bose–Einstein condensation superconductivity induced by disappearance of the nematic state |journal=Science Advances |date=1 November 2020 |volume=6 |issue=45 |pages=eabb9052 |doi=10.1126/sciadv.abb9052 |pmid=33158862 |pmc=7673702 |bibcode=2020SciA....6.9052H |url=|language=en |issn=2375-2548}}</ref>

=== Dark matter ===
P. Sikivie and Q. Yang showed that [[cold dark matter]] [[axions]] would form a Bose–Einstein condensate by [[thermalisation]] because of gravitational self-interactions.<ref>P. Sikivie, Q. Yang; Physical Review Letters,103:111103; 2009</ref> Axions have not yet been confirmed to exist. However the important search for them has been greatly enhanced with the completion of upgrades to the [[Axion Dark Matter Experiment]] (ADMX) at the University of Washington in early 2018.

In 2014, a potential dibaryon was detected at the [[Forschungszentrum Jülich|Jülich Research Center]] at about 2380 MeV. The center claimed that the measurements confirm results from 2011, via a more replicable method.<ref>{{cite web
|url=https://www.fz-juelich.de/SharedDocs/Pressemitteilungen/UK/EN/2014/14-05-23exotisches-teilchen.html
|title=Forschungszentrum Jülich press release
}}</ref><ref>{{cite web
|url=https://www.theregister.co.uk/AMP/2014/06/10/massive_news_in_the_microworld_a_hexaquark_particle/
|title=Massive news in the micro-world: a hexaquark particle
|website=[[The Register]]
}}</ref> The particle existed for 10<sup>−23</sup> seconds and was named d*(2380).<ref>
{{cite journal
 |author=P. Adlarson|year=2014
 |title=Evidence for a New Resonance from Polarized Neutron-Proton Scattering
 |journal=[[Physical Review Letters]]
 |volume=112 |issue=2 |pages=202301
 |arxiv=1402.6844
 |bibcode=2014PhRvL.112t2301A
 |doi=10.1103/PhysRevLett.112.202301
|s2cid=2280323
 |display-authors=etal}}</ref> This particle is hypothesized to consist of three [[Up quark|up]] and three [[down quark]]s.<ref>
{{cite journal
 |author=M. Bashkanov
 |year=2020
 |title=A new possibility for light-quark dark matter
 |journal=[[Journal of Physics G]]
 |volume=47 |issue=3 |pages=03LT01
 |bibcode=2020JPhG...47cLT01B
 |doi=10.1088/1361-6471/ab67e8
|arxiv=2001.08654
 |s2cid=210861179
 |doi-access=free
 }}</ref> It is theorized that groups of d* (d-stars) could form Bose–Einstein condensates due to prevailing low temperatures in the early universe, and that BECs made of such [[hexaquark]]s with trapped electrons could behave like [[dark matter]].<ref>{{cite web
|url=https://www.livescience.com/hexaquarks-could-explain-dark-matter.html
|title=Did German physicists accidentally discover dark matter in 2014?
|website=[[Live Science]]
|date=9 March 2020
}}</ref><ref>{{cite news
|url=https://www.sciencealert.com/d-star-hexaquark-particles-could-be-responsible-for-creating-dark-matter
|title=Physicists Think We Might Have a New, Exciting Dark Matter Candidate
|newspaper=Sciencealert
|date=4 March 2020
|last1=Starr
|first1=Michelle
}}</ref><ref>{{cite web
|url=https://www.space.com/hexaquarks-big-bang-form-universe-dark-matter.html
|title=Did this newfound particle form the universe's dark matter?
|website=[[Space.com]]
|date=5 March 2020
}}</ref>

== In fiction ==
* In the 2016 film ''[[Spectral]]'', the US military battles mysterious enemy creatures fashioned out of Bose–Einstein condensates.<ref name="Spectral Review">{{Cite web|url=https://arstechnica.com/gaming/2017/07/spectral-movie-science-review/|title=The science of Spectral: Is that really how Bose–Einstein condensate behaves? An actual Bose–Einstein condensate scientist reviews Spectral's science. Plus a response from the film's director, Nic Mathieu.|first=Thilo|last=Stöferle|date=July 18, 2017|website=[[Ars Technica]]|access-date=June 4, 2021}}</ref>
* In the 2003 novel ''[[Blind Lake (novel)|Blind Lake]]'', scientists observe sentient life on a planet 51 light-years away using telescopes powered by Bose–Einstein condensate-based quantum computers.

== See also ==
{{Portal|Physics}}
{{div col|colwidth=22em}}
* [[Atom laser]]
* [[Atomic coherence]]
* [[Bose–Einstein correlations]]
* [[Bose–Einstein condensation: a network theory approach]]
* [[Bose–Einstein condensation of quasiparticles]]
* [[Bose–Einstein statistics]]
* [[Cold Atom Laboratory]]
* [[Electromagnetically induced transparency]]
* [[Fermionic condensate]]
* [[Gas in a box]]
* [[Gross–Pitaevskii equation]]
* [[Macroscopic quantum phenomena]]
* [[Macroscopic quantum self-trapping]]
* [[Slow light]]
* [[Transuranium element#Super-heavy elements|Super-heavy atom]]
* [[Superconductivity]]
* [[Superfluid film]]
* [[Superfluid helium-4]]
* [[Supersolid]]
* [[Tachyon condensation]]
* [[Timeline of low-temperature technology]]
* [[Ultracold atom]]
* [[Wiener sausage]]
{{div col end}}

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== Further reading ==
{{Refbegin|colwidth=60em}}
* {{cite journal |author=S. N. Bose |year=1924 |title=Plancks Gesetz und Lichtquantenhypothese |journal=Zeitschrift für Physik |volume=26 |issue=1 |pages=178–181 |bibcode=1924ZPhy...26..178B |doi=10.1007/BF01327326|s2cid=186235974 }}
* {{cite journal |author=A. Einstein |year=1925 |title=Quantentheorie des einatomigen idealen Gases |journal=Sitzungsberichte der Preussischen Akademie der Wissenschaften |volume=1 |page=3}},
* {{cite journal |author=L. D. Landau |year=1941 |title=The theory of Superfluity of Helium 111 |journal=J. Phys. USSR |volume=5 |pages=71–90}}
* {{cite journal |author=L. D. Landau |year=1941 |title=Theory of the Superfluidity of Helium II |journal=Physical Review |volume=60 |issue=4 |pages=356–358 |bibcode=1941PhRv...60..356L |doi=10.1103/PhysRev.60.356}}
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* Monique Combescot and Shiue-Yuan Shiau, "Excitons and Cooper Pairs: Two Composite Bosons in Many-Body Physics", Oxford University Press ({{ISBN|9780198753735}}).
{{Refend}}

==External links==
{{wikiquote}}
{{Commons category}}
*[https://web.archive.org/web/20100113160458/http://iqoqi.at/bec2009/ Bose–Einstein Condensation 2009 Conference] – Frontiers in Quantum Gases
*[https://web.archive.org/web/20051220142130/http://www.colorado.edu/physics/2000/bec/index.html BEC Homepage] General introduction to Bose–Einstein condensation
*[http://nobelprize.org/physics/laureates/2001/index.html Nobel Prize in Physics 2001] – for the achievement of Bose–Einstein condensation in dilute gases of alkali atoms, and for early fundamental studies of the properties of the condensates
*{{cite journal |doi=10.1063/1.1445529|title=Cornell, Ketterle, and Wieman Share Nobel Prize for Bose–Einstein Condensates|year=2001|last1=Levi|first1=Barbara G.|author-link=Barbara Goss Levi|journal=Physics Today|volume=54|issue=12|pages=14–16|bibcode=2001PhT....54l..14L|doi-access=free}}
*[http://jilawww.colorado.edu/bec/ Bose–Einstein condensates at JILA]
*[http://atomcool.rice.edu/ Atomcool at Rice University]
*[https://web.archive.org/web/20051226061445/http://cua.mit.edu/ketterle_group/home.htm Alkali Quantum Gases at MIT]
*[http://www.physics.uq.edu.au/atomoptics/ Atom Optics at UQ]
*[http://www.lorentz.leidenuniv.nl/history/Einstein_archive/ Einstein's manuscript on the Bose–Einstein condensate discovered at Leiden University]
*[http://xstructure.inr.ac.ru/x-bin/theme3.py?level=2&index1=145786 Bose–Einstein condensate on arxiv.org]
*[http://www.vigyanprasar.gov.in/dream/jan2002/article1.htm Bosons – The Birds That Flock and Sing Together]
*[http://jilawww.colorado.edu/bec/BEC_for_everyone/ Easy BEC machine] – information on constructing a Bose–Einstein condensate machine.
*[http://www.cosmosmagazine.com/features/online/2176/verging-absolute-zero Verging on absolute zero – Cosmos Online] {{Webarchive|url=https://web.archive.org/web/20081122144155/http://www.cosmosmagazine.com/features/online/2176/verging-absolute-zero |date=22 November 2008 }}
*[https://techtv.mit.edu/videos/15968-bose-einstein-condensates-the-coldest-matter-in-the-universe Lecture by W Ketterle at MIT in 2001]
*[https://web.archive.org/web/20110709214322/http://bec.nist.gov/ Bose–Einstein Condensation at NIST] – [[NIST]] resource on BEC

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