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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…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-18 Ozgur Erken , Pierre Sikivie , Heywood Tam , Qiaoli Yang

The evidence is that the mass of the universe is dominated by an exotic nonbaryonic form of matter largely draped around the galaxies. It approximates an initially low pressure gas of particles that interact only with gravity, but we know…

Cosmology and Nongalactic Astrophysics · Physics 2017-01-23 P. J. E. Peebles

We consider the possibility that the dark matter, which is required to explain the dynamics of the neutral hydrogen clouds at large distances from the galactic center, could be in the form of a Bose-Einstein condensate. To study the…

Astrophysics · Physics 2010-10-27 C. G. Boehmer , T. Harko

The nature of the cosmological dark matter remains elusive. Recent studies have advocated the possibility that dark matter could be composed of ultra-light, self-interacting bosons, forming a Bose-Einstein condensate in the very early…

Cosmology and Nongalactic Astrophysics · Physics 2014-04-22 Tanja Rindler-Daller , Paul R. Shapiro

The cosmological scenario where the Peccei-Quinn symmetry is broken after inflation is investigated. In this scenario, topological defects such as strings and domain walls produce a large number of axions, which contribute to the cold dark…

High Energy Physics - Phenomenology · Physics 2015-08-12 Masahiro Kawasaki , Ken'ichi Saikawa , Toyokazu Sekiguchi

Existing searches for cosmic axions relics have relied heavily on the axion being non-relativistic and making up dark matter. However, light axions can be copiously produced in the early Universe and remain relativistic today, thereby…

High Energy Physics - Phenomenology · Physics 2022-11-10 Jeff A. Dror , Hitoshi Murayama , Nicholas L. Rodd

We analyze the behavior of axion dark matter before it falls into a galactic gravitational potential well. The axions thermalize sufficiently fast by gravitational self-interactions that almost all go to their lowest energy state consistent…

Astrophysics of Galaxies · Physics 2015-06-16 N. Banik , P. Sikivie

A Bose star passing through cold molecular clouds may capture atoms, molecules and dust particles. The observational signature of such an event would be a relatively small amount of matter that is gravitationally bound. This binding may…

High Energy Physics - Phenomenology · Physics 2024-11-18 V. V. Flambaum , I. B. Samsonov

Axions and axion-like particles are ubiquitous in extensions of the Standard Model and offer a unifying framework for addressing open problems in cosmology. Depending on their mass and interactions, axions can act as dark matter, drive…

High Energy Physics - Phenomenology · Physics 2026-05-01 Luca Visinelli

Many theoretically well-motivated extensions of the Standard Model of particle physics predict the existence of the axion and further ultralight axion-like particles. They may constitute the mysterious dark matter in the universe and solve…

High Energy Physics - Phenomenology · Physics 2015-06-16 Andreas Ringwald

Light Axionic Dark Matter, motivated by string theory, is increasingly favored for the "no-WIMP era". Galaxy formation is suppressed below a Jeans scale, of $\simeq 10^8 M_\odot$ by setting the axion mass to, $m_B \sim 10^{-22}$eV, and the…

Cosmology and Nongalactic Astrophysics · Physics 2017-12-01 Ivan De Martino , Tom Broadhurst , S. -H. Henry Tye , Tzihong Chiueh , Hsi-Yu Schive , Ruth Lazkoz

Ordinary baryonic particles (such as protons and neutrons) account for only one-sixth of the total matter in the Universe. The remainder is a mysterious "dark matter" component, which does not interact via electromagnetism and thus neither…

Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detection of various plausible baryonic candidates for dark matter inferred, e.g., from galaxy rotation curves and from cluster of galaxy velocity…

Astrophysics · Physics 2007-05-23 David N. Spergel

The vorticity equation stemming from the modified Navier-Stokes equation gives a solution for a flat profile of the orbital speed of spiral galaxies. Solutions disclose existence of the Gaussian vortex clouds, the coherent vortices with…

General Physics · Physics 2016-07-26 Valeriy I. Sbitnev

Hidden photons and axion-like particles are candidates for cold dark matter if they were produced non-thermally in the early universe. We conducted a search for both of these bosons using 800 live-days of data from the XMASS detector with…

The axion is a motivated dark matter candidate, so it would be interesting to find features in Large Scale Structures specific to axion dark matter. Such features were proposed for a Bose Einstein condensate of axions, leading to confusion…

High Energy Physics - Phenomenology · Physics 2015-06-19 Sacha Davidson

In the same way as the realization of some of the famous gedanken experiments imagined by the founding fathers of quantum mechanics has recently led to the current renewal of the interpretation of quantum physics, it seems that the most…

General Relativity and Quantum Cosmology · Physics 2021-11-19 Gilles Cohen-Tannoudji , Jean-Pierre Gazeau

I present an introduction and topical review on axions as a dark matter candidate. Emphasis is placed on issues surrounding the cosmology of axion dark matter that are relevant for present-day searches, including: early-Universe production…

High Energy Physics - Phenomenology · Physics 2024-05-28 Ciaran A. J. O'Hare

We show that if dark matter consists of QCD axions in the post-inflationary scenario more than ten percent of it efficiently collapses into Bose stars at matter-radiation equality. Such a result is mostly independent of the present…

High Energy Physics - Phenomenology · Physics 2024-08-22 Marco Gorghetto , Edward Hardy , Giovanni Villadoro

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,…

High Energy Physics - Phenomenology · Physics 2009-11-06 P. Sikivie , Q. Yang