Listening for dark photon radio signals from the Galactic Center

doi:10.1103/PhysRevD.107.115035

CORC > 理论物理研究所 > 中国科学院理论物理研究所 > 理论物理所科研产出 > 理论物理所1978-2010年知识产出

	Listening for dark photon radio signals from the Galactic Center
	Hardy, Edward ; Song, Ningqiang 1
刊名	PHYSICAL REVIEW D
	2023
卷号	107 期号:11 页码:115035
关键词	MAGNETIC WHITE-DWARFS X-RAY-EMISSION HYDROGEN LINES HIDDEN-SECTOR MASS CONSTRAINTS POLARIZATION DISPERSION RADIATION SEARCH
ISSN号	2470-0010
DOI	10.1103/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
内容类型	期刊论文
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
推荐引用方式 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.