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Listening for dark photon radio signals from the Galactic Center

文献类型:期刊论文

作者Hardy, Edward; Song, Ningqiang1
刊名PHYSICAL REVIEW D
出版日期2023
卷号107期号:11页码:115035
ISSN号2470-0010
关键词MAGNETIC WHITE-DWARFS X-RAY-EMISSION HYDROGEN LINES HIDDEN-SECTOR MASS CONSTRAINTS POLARIZATION DISPERSION RADIATION SEARCH
DOI10.1103/PhysRevD.107.115035
英文摘要Dark photon dark matter that has a kinetic mixing with the Standard Model photon can resonantly convert in environments where its mass mA, coincides with the plasma frequency. We show that such conversion in neutron stars or accreting white dwarfs in the Galactic Center can lead to detectable radio signals. Depending on the dark matter spatial distribution, future radio telescopes could be sensitive to values of the kinetic mixing parameter that exceed current constraints by orders of magnitude for mA, & ISIN; (6 x 10-6, 7 x 10-4) eV.
学科主题Astronomy & Astrophysics ; Physics
语种英语
源URL[http://ir.itp.ac.cn/handle/311006/28015]  
专题理论物理研究所_理论物理所1978-2010年知识产出
作者单位1.Univ Liverpool, Dept Math Sci, Liverpool L69 7ZL, England
2.Chinese Acad Sci, Inst Theoret Phys, Beijing 100190, Peoples R China
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GB/T 7714
Hardy, Edward,Song, Ningqiang. Listening for dark photon radio signals from the Galactic Center[J]. PHYSICAL REVIEW D,2023,107(11):115035.
APA Hardy, Edward,&Song, Ningqiang.(2023).Listening for dark photon radio signals from the Galactic Center.PHYSICAL REVIEW D,107(11),115035.
MLA Hardy, Edward,et al."Listening for dark photon radio signals from the Galactic Center".PHYSICAL REVIEW D 107.11(2023):115035.

入库方式: OAI收割

来源:理论物理研究所

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