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相关论文: Projected bounds on ALPs from Athena

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The surprising discovery by MAGIC of an intense, rapidly varying emission in the energy range 70 - 400 GeV from the flat spectrum radio quasar PKS 1222+216 represents a challenge for all interpretative scenarios. Indeed, in order to avoid…

高能天体物理现象 · 物理学 2013-05-30 F. Tavecchio , M. Roncadelli , G. Galanti , G. Bonnoli

We explore the axion-like particle (ALP)-photon oscillation effect in the $\gamma$-ray spectra of the blazars Markarian 421 (Mrk 421) and PG 1553+113, which are measured by the Major Atmospheric Gamma Imaging Cherenkov Telescopes (MAGIC)…

高能天体物理现象 · 物理学 2022-08-17 Hai-Jun Li , Xiao-Jun Bi , Peng-Fei Yin

The chemical enrichment of the Universe at all scales is related to stellar winds and explosive supernovae phenomena. Metals produced by stars and later spread at the mega-parsec scale through the intra-cluster medium (ICM) become a fossil…

Axions or ALPs are hypothetical particles predicted by BSM theories, which make one of the dark matter candidates. These particles can convert into photons and vice-versa in the presence of magnetic field, with a probability decided by its…

宇宙学与河外天体物理 · 物理学 2024-09-19 Harsh Mehta , Suvodip Mukherjee

The Axion Like Particle (ALP) is a hypothetical pseudo-scalar particle beyond the Standard Model, with a compelling possible connection to dark matter and early universe physics. ALPs can be converted into photons via interactions with…

高能天体物理现象 · 物理学 2020-03-04 Ryo Yamamoto , Noriko Y. Yamasaki , Kazuhisa Mitsuda , Masahiro Takada

Axion-like particles (ALPs), a class of pseudoscalars common to many extensions of the Standard Model, have the capacity to drain energy from the interiors of stars. Consequently, stellar evolution can be used to derive many constraints on…

高能物理 - 唯象学 · 物理学 2021-09-16 Matthew J. Dolan , Frederick J. Hiskens , Raymond R. Volkas

Quiescent hard X-ray and soft gamma-ray emission from neutron stars constitute a promising frontier to explore axion-like-particles (ALPs). ALP production in the core peaks at energies of a few keV to a few hundreds of keV; subsequently,…

高能物理 - 唯象学 · 物理学 2021-07-19 Jean-François Fortin , Huai-Ke Guo , Steven P. Harris , Elijah Sheridan , Kuver Sinha

Photons couple to Axion-Like Particles (ALPs) or more generally to any pseudo Nambu-Goldstone boson in the presence of an external electromagnetic field. Mixing between photons and ALPs in the strong magnetic field of a Gamma-Ray Burst…

高能天体物理现象 · 物理学 2011-03-18 Olga Mena , Soebur Razzaque , F. Villaescusa-Navarro

Axion-like particles (ALPs) may undergo mixing with photons in the presence of astrophysical magnetic fields, leading to alterations in the observed high energy $\gamma$-ray spectra. In this study, we investigate the ALP-photon oscillation…

高能天体物理现象 · 物理学 2024-03-06 Lin-Qing Gao , Xiao-Jun Bi , Jun-Guang Guo , Wenbin Lin , Peng-Fei Yin

In the beyond Standard Model (BSM) scenarios, the possibility of neutrinos decaying into a lighter state is one of the prime quests for the new-generation neutrino experiments. The observation of high-energy astrophysical neutrinos by…

高能天体物理现象 · 物理学 2024-03-08 Bhanu Prakash Pant

Axion-Like Particles (ALPs) are a generic, calculable, and well motivated extension of the Standard Model with far reaching phenomenology. ALPs that couple only to hypercharge represent one subset of such models, coupling the ALP to both…

高能物理 - 唯象学 · 物理学 2021-09-15 Noah Steinberg , James D. Wells

Axion-like particles (ALPs) are light, neutral, pseudo-scalar bosons predicted by several extensions of the Standard Model of particle physics -- such as the String Theory -- and are supposed to interact primarily only with two photons. In…

高能天体物理现象 · 物理学 2019-11-22 Giorgio Galanti

Axion-like particles (ALPs) are pseudo Nambu-Goldstone bosons associated with spontaneously broken global symmetries emerging in many extensions of the Standard Model. Assuming the most general effective Lagrangian up to dimension-5…

高能物理 - 唯象学 · 物理学 2020-12-08 Gholamhossein Haghighat , Daruosh Haji Raissi , Mojtaba Mohammadi Najafabadi

Axion-Like Particles (ALPs) are the focus of intense current research. We analyze photon-ALP conversion in the context of relativistic jet models of Active Galactic Nuclei (AGN) for more than 100 sources. Contrary to previous claims, we…

高能天体物理现象 · 物理学 2009-05-26 Nicola Bassan , Marco Roncadelli

In this paper we outline an experiment to detect the conversion of photons to axion-like particles (ALPs) in a strong magnetic field. We show that by modulating the polarization of the light passing through a Fabry-Perot cavity so that it…

高能物理 - 唯象学 · 物理学 2022-04-13 Richard Creswick , Frank T. Avignone

Burrage, Davis, and Shaw recently suggested exploiting the correlations between high and low energy luminosities of astrophysical objects to probe possible mixing between photons and axion-like particles (ALP) in magnetic field regions.…

宇宙学与河外天体物理 · 物理学 2014-11-21 Guido Walter Pettinari , Robert Crittenden

Axion-like particles (ALPs) can be produced by thermal processes in a stellar interior, escape from the star and, if sufficiently light, be converted into photons in the external Galactic magnetic field. Such a process could produce a…

Axions and axion-like particles (ALPs) appear in many extensions of the Standard Model and are being investigated as promising dark matter (DM) candidates. One viable methodology for their detection involves the investigation of the…

高能天体物理现象 · 物理学 2024-04-18 Wen-Qing Guo , Zi-Qing Xia , Xiaoyuan Huang

The growing interest in axion-like particles (ALPs) stems from the fact that they provide successful theoretical explanations of physics phenomena, from the anomaly of the CP-symmetry conservation in strong interactions to the observation…

高能天体物理现象 · 物理学 2021-06-08 Ivana Batković , Alessandro De Angelis , Michele Doro , Marina Manganaro

We report on a broadband search for axion-like-particle (ALP) interactions using a radio-frequency-operated $^{87}\mathrm{Rb}$ atomic magnetometer. The instrument provides wide spectral coverage and sensitivity to an oscillating…

原子物理 · 物理学 2026-03-31 A. Rigoulet , S. Nanos , I. K. Kominis , D. Antypas