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The axion is a motivated cold dark matter candidate, which it would be interesting to distinguish from weakly interacting massive particles. Sikivie has suggested that axions could behave differently during non-linear galaxy evolution, if…

高能物理 - 唯象学 · 物理学 2015-06-16 Sacha Davidson , Martin Elmer

We show that cold dark matter axions thermalize and form a Bose-Einstein condensate. We obtain the axion state in a homogeneous and isotropic universe, and derive the equations governing small axion perturbations. Because they form a BEC,…

高能物理 - 唯象学 · 物理学 2009-11-06 P. Sikivie , Q. Yang

QCD axions are a well-motivated candidate for cold dark matter. Cold axions are produced in the early universe by vacuum realignment, axion string decay and axion domain wall decay. We show that cold axions thermalize via their…

宇宙学与河外天体物理 · 物理学 2017-06-27 Nilanjan Banik , Pierre Sikivie

Recently there has been significant interest in the claim that dark matter axions gravitationally thermalize and form a Bose-Einstein condensate with cosmologically long-range correlation. This has potential consequences for galactic scale…

宇宙学与河外天体物理 · 物理学 2015-11-18 Alan H. Guth , Mark P. Hertzberg , C. Prescod-Weinstein

If cold dark matter elementary particles form a Bose-Einstein condensate, their superfluidity may distinguish them from other forms of cold dark matter, including creation of quantum vortices. We demonstrate here that such vortices are…

宇宙学与河外天体物理 · 物理学 2014-04-22 Tanja Rindler-Daller , Paul R. Shapiro

Cold dark matter axions thermalize through gravitational self-interactions and form a Bose-Einstein condensate when the photon temperature reaches approximately 500 eV. Axion Bose-Einstein condensation provides an opportunity to distinguish…

宇宙学与河外天体物理 · 物理学 2011-11-18 Ozgur Erken , Pierre Sikivie , Heywood Tam , Qiaoli Yang

We show that Dark Matter consisting of bosons of mass of about 1eV or less has critical temperature exceeding the temperature of the universe at all times, and hence would have formed a Bose-Einstein condensate at very early epochs. We also…

广义相对论与量子宇宙学 · 物理学 2015-06-18 Saurya Das , Rajat K. Bhaduri

We study the Bose condensation of scalar dark matter in the presence of both gravitational and self-interactions. Axions and other scalar dark matter in gravitationally bound miniclusters or dark matter halos are expected to condense into…

高能物理 - 唯象学 · 物理学 2020-11-18 Kay Kirkpatrick , Anthony E. Mirasola , Chanda Prescod-Weinstein

Axions differ from the other cold dark matter candidates in that they form a degenerate Bose gas. It is shown that their huge quantum degeneracy and large correlation length cause cold dark matter axions to thermalize through gravitational…

宇宙学与河外天体物理 · 物理学 2013-05-30 O. Erken , P. Sikivie , H. Tam , Q. Yang

Standard thermodynamical results of ideal Bose gases are used to study the possible formation of a cosmological Bose-Einstein condensate in Scalar Field Dark Matter models; the main hypothesis is that the boson particles were in thermal…

广义相对论与量子宇宙学 · 物理学 2010-10-27 L. Arturo Ureña-López

The formation of a dense Bose-Einstein condensate in dark spin states of two-dimensional dipolar excitons is shown to be driven by a dynamical transition to the long-lived dark states. The condensate is stabilized by strong dipole-dipole…

量子气体 · 物理学 2018-05-09 Yotam Mazuz-Harpaz , Maxim Khodas , Ronen Rapaport

Cold dark matter axions form a Bose-Einstein condensate if the axions thermalize. Recently, it was found that they do thermalize when the photon temperature reaches T ~ 100 eV(f/10^12GeV)^1/2 and that they continue to do so thereafter. We…

高能物理 - 唯象学 · 物理学 2014-11-20 Q. Yang

We report the formation of Bose-Einstein condensates into non-equilibrium states. Our condensates are much longer than equilibrium condensates with the same number of atoms, show strong phase fluctuations, and have a dynamical evolution…

We explore the viability of a boson dark matter candidate with an asymmetry between the number densities of particles and antiparticles. A simple thermal field theory analysis confirms that, under certain general conditions, this component…

宇宙学与河外天体物理 · 物理学 2016-04-27 Anthony Aguirre , Alberto Diez-Tejedor

We prove two equilibrium properties of a system of interacting atoms in three or higher dimensional continuous space. (i) If the particles interact via pair potentials of a nonnegative Fourier transform, their self-organization into…

数学物理 · 物理学 2023-05-31 Andras Suto

It was shown in ref. [1] that cold dark matter axions reach thermal contact with baryons, and therefore cool them, shortly after the axions thermalize among themselves and form a Bose-Einstein condensate. The recent observation by the EDGES…

宇宙学与河外天体物理 · 物理学 2018-08-02 Pierre Sikivie

By improving the Bose-Einstein condensate model of dark matter through the repulsive three-particle interaction to better reproduce observables such as rotation curves, both different thermodynamic phases and few-particle correlations are…

星系天体物理 · 物理学 2022-11-22 A. M. Gavrilik , A. V. Nazarenko

It is shown, that Bose-Einstein condensation can occur not only in spatially extended equilibrium systems, but also in the systems far from thermal equilibrium, which show order-disorder phase transition. The investigation is performed by…

软凝聚态物质 · 物理学 2007-05-23 Kestutis Staliunas

In the setting of the principle of local equilibrium which asserts that the temperature is a function of the energy levels of the system, we exhibit plenty of steady states describing the condensation of free Bosons which are not in thermal…

数学物理 · 物理学 2016-06-22 Luigi Accardi , Francesco Fidaleo

The phenomenon of Bose-Einstein condensation is traditionally associated with and experimentally verified for low temperatures: either of nano-Kelvin scale for alkali atoms [1-3] or room temperatures for quasi-particles [4,5] or photons in…

等离子体物理 · 物理学 2020-02-04 M. A. Prakapenia , G. V. Vereshchagin
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