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相关论文: Axion Cloud Decay due to the Axion-photon Conversi…

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Black holes can amplify incoming bosonic waves via rotational superradiance, inducing bound states of ultralight bosons around them. This phenomenon has the potential to confine the parameter spaces of new bosons. Axions and axion-like…

高能天体物理现象 · 物理学 2023-11-06 Zhiren Wang , Avery E. Broderick

The presence of axions introduces new diagrams at one-loop order to the two-photon decays of the neutral pion through axion-pion mixing. In this work, we calculate this correction, missing in all current calculations, in the framework of…

高能物理 - 唯象学 · 物理学 2025-03-17 Zhen-Yan Lu , Yang Huang , Ji-Gui Cheng , Qi Lu , Shu-Peng Wang

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

Cosmological moduli generically come to dominate the energy density of the early universe, and thereby trigger an early matter dominated era. Such non-standard cosmological histories are expected to have profound effects on the evolution…

高能物理 - 唯象学 · 物理学 2025-06-13 Robert Wiley Deal , Leia Barrowes , John T. Giblin, , Kuver Sinha , Scott Watson , Fred C. Adams

We consider a cosmological scenario in which the very early Universe experienced a transient epoch of matter domination due to the formation of a large population of primordial black holes (PBHs) with masses $M \lesssim 10^{9}\,\textrm{g}$,…

高能物理 - 唯象学 · 物理学 2021-09-03 Francesco Schiavone , Daniele Montanino , Alessandro Mirizzi , Francesco Capozzi

We study the cosmological evolution of the QCD axion coupled to hidden photons. For a moderately strong coupling, the motion of the axion field leads to an explosive production of hidden photons by tachyonic instability. We use lattice…

高能物理 - 唯象学 · 物理学 2018-05-23 Naoya Kitajima , Toyokazu Sekiguchi , Fuminobu Takahashi

The axion photon system in an external magnetic field, when for example considered with the geometry of the experiments exploring axion photon mixing, displays a continuous axion-photon duality symmetry in the limit the axion mass is…

高能物理 - 理论 · 物理学 2008-11-26 E. I. Guendelman

We study the propagation of photons in a homogeneous axion dark matter background. When the axion decay into two photons is stimulated, the photon field exhibits a parametric instability in a small bandwidth centered on one half of the…

高能物理 - 唯象学 · 物理学 2020-04-07 Ariel Arza

We discuss the appearance at the QCD phase transition, and the subsequent decay, of axion walls bounded by strings in N=1 axion models. We argue on intuitive grounds that the main decay mechanism is into barely relativistic axions. We…

高能物理 - 唯象学 · 物理学 2009-10-31 S. Chang , C. Hagmann , P. Sikivie

Lasing of ultralight axion condensate into photons can be sensitive to the presence of a background plasma owing to its coupling to electromagnetism. Such a scenario is particularly relevant for superradiant axion condensate around stellar…

高能物理 - 唯象学 · 物理学 2018-11-21 Srimoyee Sen

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

The relic density of dark matter in the $\Lambda$CDM model restricts the parameter space for a cosmological axion field, constraining the axion decay constant, the initial amplitude of the axion field and the axion mass. It is shown via…

高能物理 - 唯象学 · 物理学 2024-01-23 Filippo Anzuini , Angelo Maggi

The properties of axions that constitute 100% of cold dark matter (CDM) depend on the tensor-to-scalar ratio $r$ at the end of inflation. If $r=0.20^{+0.07}_{-0.05}$ as reported by the BICEP2 collaboration, then "half" of the CDM axion…

高能物理 - 唯象学 · 物理学 2014-07-09 L. Visinelli , P. Gondolo

Superradiant instability of rotating black holes (BHs) leads to the formation of a cloud of ultralight bosons, such as axions. When the BH with the cloud belongs to a binary system and is in an inspiraling orbit, the resonant transition…

广义相对论与量子宇宙学 · 物理学 2023-05-24 Takuya Takahashi , Hidetoshi Omiya , Takahiro Tanaka

Relativistic axions are good candidates for the dark radiation for which there are mounting observational hints. The primordial decays of heavy fields produce axions which are ultra-energetic compared to thermalised matter and inelastic…

高能物理 - 唯象学 · 物理学 2015-06-15 Joseph P. Conlon , M. C. David Marsh

Rapidly rotating black holes are known to develop instabilities in the presence of a sufficiently light boson, a process which becomes efficient when the boson's Compton wavelength is roughly the size of the black hole. This phenomenon,…

高能物理 - 唯象学 · 物理学 2021-01-04 Diego Blas , Samuel J. Witte

We present a brief overview of the ongoing searches for the axion particle via its coupling to photons. Both the classical QCD axions and more recently proposed Axion-Like-Particles are considered. Astrophysical bounds on the axion-photon…

高能物理 - 唯象学 · 物理学 2013-09-27 G. Carosi , A. Friedland , M. Giannotti , M. J. Pivovaroff , J. Ruz , J. K. Vogel

By coupling to both the Higgs and electroweak gauge sectors, an axion can generate the matter-antimatter asymmetry in the universe via electroweak baryogenesis when the axion decay constant lies within the range of approximately $10^5$ and…

高能物理 - 唯象学 · 物理学 2025-02-11 Kwang Sik Jeong , Ju Hyeong Kang , Shota Nakagawa

In the presence of a magnetic field, axions can convert into photons and vice versa. The phenomenology of the conversion is captured by a system of two coupled Klein-Gordon equations, which, assuming that the axion is relativistic, is…

高能物理 - 唯象学 · 物理学 2025-03-24 Clemente Smarra , Pierluca Carenza

We studied the collapse of rotating molecular cloud cores with inclined magnetic fields, based on three-dimensional numerical simulations.The numerical simulations start from a rotating Bonnor-Ebert isothermal cloud in a uniform magnetic…

天体物理学 · 物理学 2009-11-11 Masahiro N. Machida , Tomoaki Matsumoto , Tomoyuki Hanawa , Kohji Tomisaka