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相关论文: Decay of Ultralight Axion Condensates

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Stability properties of gravitationally bound condensates composed of ultralight axionic Fuzzy Dark Matter (FDM) are studied. Previous work has shown that astrophysical collisions could make self-gravitating condensates structurally…

宇宙学与河外天体物理 · 物理学 2018-12-11 Joshua Eby , Madelyn Leembruggen , Peter Suranyi , L. C. R. Wijewardhana

Axion-like particle (ALP) dark matter shows distinctive behavior on scales where wavelike effects dominate over self-gravity. Ultralight axions are candidates for fuzzy dark matter (FDM) whose de Broglie wavelength in virialized halos…

宇宙学与河外天体物理 · 物理学 2020-07-15 Jens C. Niemeyer

Ultra light particles $(m_a \sim 10^{-21}eV-10^{-22}eV)$ with axion-like couplings to other particles can be candidates for fuzzy dark matter (FDM) if the axion decay constant $f_a\sim 10^{17}GeV$. If a compact star is immersed in such a…

高能物理 - 唯象学 · 物理学 2020-04-15 Tanmay Kumar Poddar , Subhendra Mohanty , Soumya Jana

We investigate the decay of condensates of scalars in a field theory defined by $V({\cal A})=m{}^2\,f{}^2\,[1-\cos({\cal A}\,/\,f)]$, where $m$ and $f$ are the mass and decay constant of the scalar field. An example of such a theory is that…

高能物理 - 唯象学 · 物理学 2016-05-11 Joshua Eby , Peter Suranyi , L. C. R. Wijewardhana

This is a review on the brief history of the scalar field dark matter model also known as fuzzy dark matter, BEC dark matter, wave dark matter, or ultra-light axion. In this model ultra-light scalar dark matter particles with mass $m =…

宇宙学与河外天体物理 · 物理学 2018-01-24 Jae-Weon Lee

Axion-like dark matter whose symmetry breaking occurs after the end of inflation predicts enhanced primordial density fluctuations at small scales. This leads to dense axion minihalos (or miniclusters) forming early in the history of the…

高能物理 - 唯象学 · 物理学 2023-11-28 Patrick J. Fox , Neal Weiner , Huangyu Xiao

Cosmological structure formation simulations of ultralight axion-like dark matter have shown that an axion star forms at the center of every dark matter halo in the Universe. These axion stars would then form in large numbers during the…

高能物理 - 唯象学 · 物理学 2024-02-12 Miguel Escudero

Axion-like particles are a well-motivated dark matter candidate that can form a condensate with low momentum and high occupation number. In the presence of dark radiation, this condensate loses energy, naturally increasing the energy…

高能物理 - 唯象学 · 物理学 2024-09-24 Daniel Aloni , Hengameh Bagherian , Rashmish K. Mishra

The particle that makes up the dark matter of the universe could be an axion or axion-like particle. A collection of axions can condense into a bound Bose-Einstein condensate called an axion star. It is possible that a significant fraction…

高能物理 - 唯象学 · 物理学 2018-10-30 Eric Braaten , Hong Zhang

Recently there has been much interest in the spatial distribution of light scalar dark matter, especially axions, throughout the universe. When the local gravitational interactions between the scalar modes are sufficiently rapid, it can…

高能物理 - 唯象学 · 物理学 2018-02-19 Enrico D. Schiappacasse , Mark P. Hertzberg

Axions are some of the best motivated particles beyond the Standard Model. We show how the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from $10^{-22}$ eV to $10^7$ GeV, can lead to nongravitational…

宇宙学与河外天体物理 · 物理学 2020-04-15 Asimina Arvanitaki , Savas Dimopoulos , Marios Galanis , Luis Lehner , Jedidiah O. Thompson , Ken Van Tilburg

The axion is arguably one of the best motivated candidates for dark matter. For a decay constant greater than about 10^9 GeV, axions are dominantly produced non-thermally in the early universe and hence are "cold", their velocity dispersion…

高能物理 - 唯象学 · 物理学 2016-12-30 Andreas Ringwald

If the dark matter particles are axions, gravity can cause them to coalesce into axion stars, which are stable gravitationally bound systems of axions. In the previously known solutions for axion stars, gravity and the attractive force…

高能物理 - 唯象学 · 物理学 2016-09-20 Eric Braaten , Abhishek Mohapatra , Hong Zhang

This is a brief review on some properties of galaxies in the fuzzy dark matter model, where dark matter is an ultra-light scalar particle with mass $m = O(10^{-22})eV$. From quantum pressure, dark matter has a halo length scale which can…

星系天体物理 · 物理学 2022-08-30 Jae-Weon Lee

Ultralight axion like particles (ALPs) of mass $m_a\in (10^{-21}\rm{eV}-10^{-22}\rm{eV})$ with axion decay constant $f_a\sim 10^{17}\rm{GeV}$ can be candidates for fuzzy dark matter (FDM). If celestial bodies like Earth and Sun are immersed…

高能物理 - 唯象学 · 物理学 2021-10-08 Tanmay Kumar Poddar

Ultralight scalar dark matter has been proposed to constitute a component of dark matter, though the minimal scenarios have increasingly become constrained. In this work, we analyze scenarios where the dark matter consists of more than one…

高能物理 - 唯象学 · 物理学 2020-10-09 Joshua Eby , Madelyn Leembruggen , Lauren Street , Peter Suranyi , L. C. R. Wijewardhana

Fuzzy dark matter of ultra-light axions has gained attention, largely in light of the galactic scale problems associated with cold dark matter. But the large de Broglie wavelength, believed to possibly alleviate these problems, also leads…

星系天体物理 · 物理学 2020-01-08 Amr El-Zant , Jonathan Freundlich , Francoise Combes , Anaelle Halle

The highly populated, low-energy excitations of a scalar field of mass $m_a\sim 10^{-22}\,\textrm{eV}$ can represent the full dark matter content of the universe and alleviate some tensions in the standard cosmological scenario on…

高能物理 - 唯象学 · 物理学 2017-02-08 Alberto Diez-Tejedor , David J. E. Marsh

Axions and axion-like particles are compelling candidates for the missing dark matter of the universe. As they undergo gravitational collapse, they can form compact objects such as axion stars or even black holes. In this paper, we study…

宇宙学与河外天体物理 · 物理学 2018-10-17 James Y. Widdicombe , Thomas Helfer , David J. E. Marsh , Eugene A. Lim

Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

高能物理 - 唯象学 · 物理学 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler
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