根据对炽星的超高能量观测推测暗光子参数

IF 4.8 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS
Tian-Ci Liu, Ming-Xuan Lu, Xiao-Song Hu
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引用次数: 0

摘要

暗光子是标准模型之外的一种新的规玻色子,是暗物质(DM)的一种候选物质。暗光子暗物质(DPDM)通过动能混合与电磁场相互作用,这就意味着可以用银河系外的甚高能(VHE)源来进行约束。在这项工作中,我们试图从蓝星的宿主星系、星系际介质和银河系中的光子-暗光子散射过程来约束动能混合。来自蓝星的VHE光子会穿过超大质量黑洞周围的致密DM尖峰,在那里DPDM的吸收会显著增强。根据对马尔卡里安(Mrk)421和马尔卡里安501的观测,在95(\%\)置信水平下,动力学混合被约束为(\epsilon \sim 10^{-7}\),质量范围为(m_\textrm{D}\sim 0.03 {-} 1\)eV。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Constraining dark photon parameters based on the very high energy observations of blazars

Constraining dark photon parameters based on the very high energy observations of blazars

Dark photon is a new gauge boson beyond the Standard Model as a kind of dark matter (DM) candidate. Dark photon dark matter (DPDM) interacts with electromagnetic fields via kinetic mixing, implicating an approach to give a constraint with extragalactic very high energy (VHE) sources. In this work, we attempt to constrain the kinetic mixing from the photon-dark photon scattering process in the host galaxy of blazar, the intergalactic medium and the Milky Way. The VHE photons from a blazar would pass through a dense DM spike around the supermassive black hole where the absorption from DPDM is dramatically enhanced. The kinetic mixing is constrained to be \(\epsilon \sim 10^{-7}\) at a 95\(\%\) confidence level with \(m_\textrm{D}\sim 0.03 {-} 1\) eV mass range from the observations of Markarian (Mrk) 421 and Mrk 501.

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来源期刊
The European Physical Journal C
The European Physical Journal C 物理-物理:粒子与场物理
CiteScore
8.10
自引率
15.90%
发文量
1008
审稿时长
2-4 weeks
期刊介绍: Experimental Physics I: Accelerator Based High-Energy Physics Hadron and lepton collider physics Lepton-nucleon scattering High-energy nuclear reactions Standard model precision tests Search for new physics beyond the standard model Heavy flavour physics Neutrino properties Particle detector developments Computational methods and analysis tools Experimental Physics II: Astroparticle Physics Dark matter searches High-energy cosmic rays Double beta decay Long baseline neutrino experiments Neutrino astronomy Axions and other weakly interacting light particles Gravitational waves and observational cosmology Particle detector developments Computational methods and analysis tools Theoretical Physics I: Phenomenology of the Standard Model and Beyond Electroweak interactions Quantum chromo dynamics Heavy quark physics and quark flavour mixing Neutrino physics Phenomenology of astro- and cosmoparticle physics Meson spectroscopy and non-perturbative QCD Low-energy effective field theories Lattice field theory High temperature QCD and heavy ion physics Phenomenology of supersymmetric extensions of the SM Phenomenology of non-supersymmetric extensions of the SM Model building and alternative models of electroweak symmetry breaking Flavour physics beyond the SM Computational algorithms and tools...etc.
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