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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

We consider a general class of axion models, including the QCD and string axion, in which the PQ symmetry is broken before or during inflation. Assuming the axion is the dominant component of the dark matter, we discuss axion star formation…

宇宙学与河外天体物理 · 物理学 2020-10-20 Mark P. Hertzberg , Enrico D. Schiappacasse , Tsutomu T. Yanagida

We analyze the dynamics and observational signatures of axion clouds formed via the superradiant instability around primordial black holes, focusing on the mass range $10^{14}-10^{18}$ kg where the latter may account for all the dark…

高能物理 - 唯象学 · 物理学 2023-04-12 Nuno P. Branco , Ricardo Z. Ferreira , João G. Rosa

We study the formation and the subsequent mass growth of axion stars inside axion miniclusters. Numerically solving the Schr\"odinger-Poisson equations with realistic initial conditions we find that the axion stars exhibit similar…

宇宙学与河外天体物理 · 物理学 2019-09-25 Benedikt Eggemeier , Jens C. Niemeyer

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

A fraction of light scalar dark matter, especially axions, may organize into Bose-Einstein condensates, gravitationally bound clumps, "boson stars", and be present in large number in galactic halos today. We compute the expected number of…

高能物理 - 唯象学 · 物理学 2022-06-22 Kohei Fujikura , Mark P. Hertzberg , Enrico D. Schiappacasse , Masahide Yamaguchi

If the symmetry breaking responsible for axion dark matter production occurs during the radiation-dominated epoch in the early Universe, then this produces large amplitude perturbations that collapse into dense objects known as axion…

宇宙学与河外天体物理 · 物理学 2019-08-09 Malcolm Fairbairn , David J. E. Marsh , Jérémie Quevillon , Simon Rozier

Axions are a viable candidate for Cold Dark Matter (CDM) which should generically form minihalos of sub-planetary masses from white-noise isocurvature density fluctuations if the Peccei-Quinn phase transition occurs after inflation. Despite…

宇宙学与河外天体物理 · 物理学 2020-01-22 Liang Dai , Jordi Miralda-Escudé

Dark matter in the form of axions is expected to form miniclusters, and their dense regions can harbor compact axion stars. Such axion stars could be discovered by microlensing events. In particular, some candidate events reported by Subaru…

高能物理 - 唯象学 · 物理学 2023-04-10 Sunao Sugiyama , Masahiro Takada , Alexander Kusenko

Superradiance provides a unique opportunity for investigating dark sectors as well as primordial black holes, which themselves are candidates for dark matter over a wide mass range. Using axion-like particles as an example, we show that…

高能物理 - 唯象学 · 物理学 2025-01-22 James B. Dent , Bhaskar Dutta , Tao Xu

The axion, as a leading dark matter candidate, is the target of many ongoing and proposed experimental searches based on its coupling to photons. Ultralight axions that couple to photons can also cause polarization rotation of light, which…

高能物理 - 唯象学 · 物理学 2024-10-08 Xucheng Gan , Lian-Tao Wang , Huangyu Xiao

Axions are hypothetical pseudoscalar particles that have been regarded as promising dark matter (DM) candidates. On the other hand, extended compact objects such as axion stars, which are supported by gravity and axion self interactions,…

高能物理 - 唯象学 · 物理学 2025-05-09 Jan Tristram Acuña , Kuan-Yen Chou , Po-Yan Tseng

Dark matter may be in the form of non-baryonic structures such as compact subhalos and boson stars. Structures weighing between asteroid and solar masses may be discovered via gravitational microlensing, an astronomical probe that has in…

宇宙学与河外天体物理 · 物理学 2020-04-15 Djuna Croon , David McKeen , Nirmal Raj

It has recently been proposed that massive primordial black holes (PBH) could constitute all of the dark matter, providing a novel scenario of structure formation, with early reionization and a rapid growth of the massive black holes at the…

宇宙学与河外天体物理 · 物理学 2017-10-16 Juan García-Bellido , Sebastien Clesse

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

The classical equations of motion for an axion with potential $V(\phi)=m_a^2f_a^2 [1-\cos (\phi/f_a)]$ possess quasi-stable, localized, oscillating solutions, which we refer to as "axion stars". We study, for the first time, collapse of…

宇宙学与河外天体物理 · 物理学 2017-04-05 Thomas Helfer , David J. E. Marsh , Katy Clough , Malcolm Fairbairn , Eugene A. Lim , Ricardo Becerril

The present surge for the astrophysical relevance of boson stars stems from the speculative possibility that these compact objects could provide a considerable fraction of the non-baryonic part of dark matter within the halo of galaxies.…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Eckehard W. Mielke , Franz E. Schunck

Axion-like particles, which we call axions, can compose the missing dark matter and may form substructures such as miniclusters and axion stars. We obtain the mass distributions of axion stars derived from their host miniclusters in our…

高能物理 - 唯象学 · 物理学 2024-09-23 Dennis Maseizik , Sagnik Mondal , Hyeonseok Seong , Günter Sigl

The QCD axion and axion-like particles, as leading dark matter candidates, can also have interesting implications for dark matter substructures if the Peccei-Quinn symmetry is broken after inflation. In such a scenario, axion perturbations…

高能物理 - 唯象学 · 物理学 2024-09-20 Jae Hyeok Chang , Patrick J. Fox , Huangyu Xiao

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
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