中国科学:物理学 力学 天文学(英文版)2024,Vol.67Issue(11) :55-62.DOI:10.1007/s11433-024-2445-1

Footprints of axion-like particle in pulsar timing array data and James Webb Space Telescope observations

Shu-Yuan Guo Maxim Khlopov Xuewen Liu Lei Wu Yongcheng Wu Bin Zhu
中国科学:物理学 力学 天文学(英文版)2024,Vol.67Issue(11) :55-62.DOI:10.1007/s11433-024-2445-1

Footprints of axion-like particle in pulsar timing array data and James Webb Space Telescope observations

Shu-Yuan Guo 1Maxim Khlopov 2Xuewen Liu 1Lei Wu 3Yongcheng Wu 3Bin Zhu1
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作者信息

  • 1. Department of Physics,Yantai University,Yantai 264005,China
  • 2. Institute of Physics,Southern Federal University,Rostov on Don 344090,Russia;National Research Nuclear University MEPhI(Moscow Engineering Physics Institute),Moscow 115409,Russia;Virtual Institute of Astroparticle Physics,Paris 75018,France
  • 3. Department of Physics and Institute of Theoretical Physics,Nanjing Normal University,Nanjing 210023,China
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Abstract

Several pulsar timing array(PTA)collaborations have recently reported the evidence for a stochastic gravitational-wave back-ground(SGWB),which can unveil the formation of primordial seeds of inhomogeneities in the early universe.With the SGWB parameters inferred from PTAs data,we can make a prediction of the seeds for early galaxy formation from the domain walls in the axion-like particles(ALPs)field distribution.This also naturally provides a solution to the observation of high redshifts by the James Webb Space Telescope.The predicted photon coupling of the ALP is within the reach of future experimental searches.

Key words

stochastic gravitational-wave background/pulsar timing array/axion-like particle/JWST

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出版年

2024
中国科学:物理学 力学 天文学(英文版)
中国科学院

中国科学:物理学 力学 天文学(英文版)

CSTPCD
影响因子:0.91
ISSN:1674-7348
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