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相关论文: Diluted Axion Star Collisions with Neutron Stars

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If QCD axions form a large fraction of the total mass of dark matter, then axion stars could be very abundant in galaxies. As a result, collisions with each other, and with other astrophysical bodies, can occur. We calculate the rate and…

宇宙学与河外天体物理 · 物理学 2017-05-24 Joshua Eby , Madelyn Leembruggen , Joseph Leeney , Peter Suranyi , L. C. R. Wijewardhana

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 study the nature of phase transitions between dilute and dense axion stars interpreted as self-gravitating Bose-Einstein condensates. We develop a Newtonian model based on the Gross-Pitaevskii-Poisson equations for a complex scalar field…

广义相对论与量子宇宙学 · 物理学 2018-07-18 Pierre-Henri Chavanis

Axion dark matter or any ultralight bosonic dark matter can go through Bose-Einstein condensation due to the large phase density, leading to the formation of axion stars or solitons in dark matter halo centers. The formation rate is…

高能物理 - 唯象学 · 物理学 2025-08-13 Patrick J. Fox , Neal Weiner , Huangyu Xiao

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

In this work we estimate the radius and the mass of a self-gravitating system made of axions. The quantum axion field satisfies the Klein-Gordon equation in a curved space-time and the metric components of this space-time are solutions to…

天体物理学 · 物理学 2009-11-13 J. Barranco , A. Bernal

The anomalous orbits of trans-Neptunian objects can be accounted for by the planet 9 hypothesis. One intriguing possibility is that planet 9 could be a dilute axion star captured by the solar system, with the ratio of the axion star to dark…

高能物理 - 唯象学 · 物理学 2025-01-09 Haoran Di , Haihao Shi , Zhu Yi

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

If dark matter is mainly composed of axions, the density distribution can be nonuniformly distributed, being clumpy instead. By solving the Einstein-Klein-Gordon system of a scalar field with the potential energy density of an axionlike…

宇宙学与河外天体物理 · 物理学 2013-06-17 J. Barranco , A. Carrillo Monteverde , D. Delepine

We present a theoretical model for detecting axions from neutron stars in a QCD phase of quark matter. The axions would be produced from a quark-antiquark pair $u\bar{u}$ or $d\bar{d}$, in loop(s) involving gluons. The chiral anomaly of QCD…

高能天体物理现象 · 物理学 2025-08-11 Bijan Berenji

Axion stars are hypothetical objects formed of axions, obtained as localized and coherently oscillating solutions to their classical equation of motion. Depending on the value of the field amplitude at the core $|\theta_0| \equiv…

宇宙学与河外天体物理 · 物理学 2017-12-13 Luca Visinelli , Sebastian Baum , Javier Redondo , Katherine Freese , Frank Wilczek

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

In this paper we examine the possibility of dilute axion stars converting to photons in the weak, large-scale magnetic field of the Milky Way and show that they can resonate with the surrounding plasma and produce a sizable signal. We…

高能物理 - 唯象学 · 物理学 2023-09-19 A. Kyriazis

The anomalous orbits of Trans-Neptunian Objects (TNOs) can be explained by the Planet 9 hypothesis. We propose that the Planet 9 can be an axion star. Axion stars are gravitational bound clusters condensed by QCD axions or axion-like…

高能物理 - 唯象学 · 物理学 2023-11-29 Haoran Di , Haihao Shi

When axion stars fly through an astrophysical magnetic background, the axion-to-photon conversion may generate a large electromagnetic radiation power. After including the interference effects of the spacially-extended axion-star source and…

高能天体物理现象 · 物理学 2018-04-11 Yang Bai , Yuta Hamada

Probing the QCD axion dark matter (DM) hypothesis is extremely challenging as the axion interacts very weakly with Standard Model particles. We propose a new avenue to test the QCD axion DM via transient radio signatures coming from…

高能物理 - 唯象学 · 物理学 2021-09-22 Sami Nurmi , Enrico D. Schiappacasse , Tsutomu T. Yanagida

Axion-like particles can be abundantly produced through scattering processes in the cores of neutron stars (NSs). If they are ultralight ($m_a \lesssim 10^{-4}$ eV), then they can efficiently convert to detectable photons in the external NS…

高能物理 - 唯象学 · 物理学 2025-12-19 Orion Ning , Kailash Raman , Benjamin R. Safdi

The QCD axion and axion-like particles are compelling candidates for galactic dark matter. Theoretically, axions can convert into photons in the presence of a strong external magnetic field, which means it is possible to search for them…

The QCD axion or axion-like particles are candidates of dark matter of the universe. On the other hand, axion-like excitations exist in certain condensed matter systems, which implies that there can be interactions of dark matter particles…

高能物理 - 唯象学 · 物理学 2021-09-01 So Chigusa , Takeo Moroi , Kazunori Nakayama

The QCD axion is expected to form dense structures known as axion miniclusters if the Peccei-Quinn symmetry is broken after inflation. Miniclusters that have survived until today will interact with neutron stars (NSs) in the Milky Way to…

高能物理 - 唯象学 · 物理学 2021-10-25 Thomas D. P. Edwards , Bradley J. Kavanagh , Luca Visinelli , Christoph Weniger
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