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Constraints on axionlike particles from observations of Mrk 421 using the CLs method

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成果类型:
期刊论文
作者:
Gao, Lin-Qing;Bi, Xiao-Jun;Guo, Jun-Guang;Lin, Wenbin;Yin, Peng-Fei
通讯作者:
Gao, LQ
作者机构:
[Gao, LQ; Gao, Lin-Qing] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.
[Bi, Xiao-Jun; Yin, Peng-Fei] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China.
[Bi, Xiao-Jun] Univ Chinese Acad Sci, Sch Phys Sci, Beijing, Peoples R China.
[Guo, Jun-Guang] Jiaying Univ, Sch Phys & Elect Engn, Meizhou 514015, Peoples R China.
[Lin, Wenbin] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
通讯机构:
[Gao, LQ ] U
Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.
语种:
英文
期刊:
PHYSICAL REVIEW D
ISSN:
2470-0010
年:
2024
卷:
109
期:
6
页码:
063003
基金类别:
National Natural Science Foundation of China [11973025, 12175248]
机构署名:
本校为第一机构
院系归属:
核科学技术学院
数理学院
摘要:
Axionlike 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 effect using the spectra of the blazar Mrk 421 over 15 observation periods measured by Major Atmospheric Gamma Imaging Cherenkov Telescopes (MAGIC) and Fermi Large Area Telescope (Fermi-LAT). Compared with previous studies, we generate mock data under the ALP hypothesis and employ the CLs method to set constraints on the ALP parameters. This method is widely ut...

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