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Main Authors: Guo, Shu-Yuan, Khlopov, Maxim, Liu, Xuewen, Wu, Lei, Wu, Yongcheng, Zhu, Bin
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2306.17022
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author Guo, Shu-Yuan
Khlopov, Maxim
Liu, Xuewen
Wu, Lei
Wu, Yongcheng
Zhu, Bin
author_facet Guo, Shu-Yuan
Khlopov, Maxim
Liu, Xuewen
Wu, Lei
Wu, Yongcheng
Zhu, Bin
contents Several Pulsar Timing Array (PTA) collaborations have recently reported the evidence for a stochastic gravitational-wave background (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.
format Preprint
id arxiv_https___arxiv_org_abs_2306_17022
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Footprints of Axion-Like Particle in Pulsar Timing Array Data and James Webb Space Telescope Observations
Guo, Shu-Yuan
Khlopov, Maxim
Liu, Xuewen
Wu, Lei
Wu, Yongcheng
Zhu, Bin
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Several Pulsar Timing Array (PTA) collaborations have recently reported the evidence for a stochastic gravitational-wave background (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.
title Footprints of Axion-Like Particle in Pulsar Timing Array Data and James Webb Space Telescope Observations
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2306.17022