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相关论文: Exploring the String Axiverse with Precision Black…

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The post-inflationary Peccei-Quinn (PQ) symmetry breaking scenario provides a unique opportunity to pinpoint the QCD axion dark matter mass, which is a crucial input for laboratory experiments that are designed for probing specific mass…

高能物理 - 唯象学 · 物理学 2025-02-18 Mathieu Kaltschmidt , Javier Redondo , Ken'ichi Saikawa , Alejandro Vaquero

A model is presented in the philosophy of the "String Axiverse" of Arvanitaki et al (arXiv:0905.4720v2 [hep-th]) that incorporates a coupling of ultralight axions to their corresponding moduli through the mass term. The light fields roll in…

宇宙学与河外天体物理 · 物理学 2015-03-19 David J. E. Marsh

There are strong interests in considering ultra-light scalar fields (especially axion) around a rapidly rotating black hole because of the possibility of observing gravitational waves from axion condensate (axion cloud) around black holes.…

广义相对论与量子宇宙学 · 物理学 2021-03-08 Hidetoshi Omiya , Takuya Takahashi , Takahiro Tanaka

Cold dark matter axions produced in the post-inflationary Peccei-Quinn symmetry breaking scenario serve as clear targets for their experimental detection, since it is in principle possible to give a sharp prediction for their mass once we…

高能物理 - 唯象学 · 物理学 2024-10-16 Ken'ichi Saikawa , Javier Redondo , Alejandro Vaquero , Mathieu Kaltschmidt

We show that primordial black holes (PBHs) develop non-negligible spins through Hawking emission of the large number of axion-like particles generically present in string theory compactifications. This is because scalars can be emitted in…

宇宙学与河外天体物理 · 物理学 2021-10-27 Marco Calzà , John March-Russell , João G. Rosa

We propose heavy axions as a natural superheavy dark matter candidate in string theory, with the relic density of dark matter originating in quantum fluctuations during cosmic inflation. String Theory is well known for the possibility of…

高能物理 - 理论 · 物理学 2025-04-21 Siyang Ling , Andrew J. Long , Evan McDonough , Alex Hayes

We review current cosmological constraints on the axion. We describe the basic mechanisms by which axions are created in the early universe, focussing on the standard thermal scenario where the dominant process is through axion radiation by…

天体物理学 · 物理学 2016-08-30 R. A. Battye , E. P. S. Shellard

Axions are hypothetical pseudoscalar particles introduced initially as a solution to the Strong CP problem in Quantum Chromodynamics (QCD), and they also arise naturally in a broad class of low-energy compactifications of string theory.…

高能物理 - 唯象学 · 物理学 2025-12-24 Amedeo M. Favitta

We explore the influence of the axion-plasmon on the optical properties of the charged black hole and show how the axion-plasmon coupling modifies the motion of photons around the charged black hole. We then explore in details observational…

广义相对论与量子宇宙学 · 物理学 2024-06-21 Yovqochev Pahlavon , Farruh Atamurotov , Kimet Jusufi , Mubasher Jamil , Ahmadjon Abdujabbarov

We study numerically the axisymmetric relativistic Bondi-Hoyle accretion of a supersonic ideal gas onto a fixed Schwarzschild background space-time described with horizon penetrating coordinates. We verify that a nearly stationary shock…

高能天体物理现象 · 物理学 2013-04-11 F. D. Lora-Clavijo , F. S. Guzman

Gravitational wave observations have recently revealed with high significance, and high precision, the existence of $\mathcal{O}(100) \, M_\odot$ rapidly rotating black holes, allowing gravitational wave events to be used for the first time…

高能物理 - 唯象学 · 物理学 2026-03-30 Andrea Caputo , Gabriele Franciolini , Samuel J. Witte

Axion-gluon interaction induces quadratic couplings between the axion and the matter fields. We find that, if the axion is an ultralight dark matter field, it induces small oscillations of the mass of the hadrons as well as other nuclear…

高能物理 - 唯象学 · 物理学 2024-01-15 Hyungjin Kim , Gilad Perez

Axion strings are horizon-size topological defects that may be produced in the early Universe. Ultra-light axion-like particles may form strings that persist to temperatures below that of big bang nucleosynthesis. Such strings have been…

高能物理 - 唯象学 · 物理学 2023-08-04 Joshua N. Benabou , Malte Buschmann , Soubhik Kumar , Yujin Park , Benjamin R. Safdi

We show results for the expected reach of the network of experiments that is being set up globally with the aim of detecting the "invisible" axion, in light of a non-standard thermal history of the universe. Assuming that the axion is the…

宇宙学与河外天体物理 · 物理学 2019-06-19 Nicklas Ramberg , Luca Visinelli

In the string theory, the fundamental blocks of nature are not particles but one-dimensional strings. Therefore, a generalization of this idea is to think of it as a cloud of strings. Rodrigues et al. embedded the black bounces spacetime…

广义相对论与量子宇宙学 · 物理学 2023-03-17 Yi Yang , Dong Liu , Zhaoyi Xu , Zheng-Wen Long

We show that axion phenomenology may be significantly different than conventionally assumed in theories which exhibit late phase transitions (below the QCD scale). In such theories one can find multiple pseudoscalars with axion-like…

高能物理 - 唯象学 · 物理学 2009-11-11 David B. Kaplan , Kathryn M. Zurek

Ultralight bosons, as important candidates of dark matter, can condense around spinning black holes (BHs) to form long-lived ``boson clouds'' due to superradiance instability. The boson-BH system can be observed through gravitational wave…

广义相对论与量子宇宙学 · 物理学 2022-04-06 Rong-Zhen Guo , Chen Yuan , Qing-Guo Huang

One of the leading candidates for dark matter is axion or axion-like particle in a form of Bose-Einstein condensate (BEC). In this paper, we present an analysis of 17 high-resolution galactic rotation curves from "The H{\footnotesize I}…

星系天体物理 · 物理学 2014-08-04 Ming-Hua Li , Zhi-Bing Li

Unveiling the dark sector of the Universe is one of the leading efforts in theoretical physics. Among the many models proposed, axions and axion-like particles stand out due to their solid theoretical foundation, capacity to contribute…

宇宙学与河外天体物理 · 物理学 2024-11-05 S. Arcari , N. Bartolo , A. Greco , A. Gruppuso , M. Lattanzi , P. Natoli

Understanding axion cosmology has important experimental consequences since it constrains the range of allowed values for the axion mass. In the standard thermal scenario, which assumes Peccei-Quinn symmetry restoration after inflation, an…

天体物理学 · 物理学 2007-05-23 R. A. Battye , E. P. S. Shellard