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Is PSR J0514-4002E in a PBH-NS Binary?

Science China Physics, Mechanics & Astronomy(2025)

Hunan Normal University Institute of Interdisciplinary Studies | Advanced Institute of Natural Sciences Department of Astronomy

Cited 1|Views3
Abstract
Recent pulsar timing observations using MeerKAT of the eccentric binary millisecond pulsar, PSR J0514–4002E, have unveiled a companion with a mass in the mass gap, ranging from 2.09 M⊙ to 2.71 M⊙. This challenges conventional astrophysical scenarios for black hole formation. In this paper, we present an alternative explanation: PSR J0514–4002E could be in a PBH-NS binary, with the companion potentially being a primordial black hole formed during the early Universe’s first-order phase transition. The associated stochastic gravitational-wave background generated during this phase transition can account for the observed signal from the pulsar timing array, and the abundance of primordial black holes is consistent with constraints from LIGO-Virgo-KAGRA.
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PSR J0514–4002E,primordial black hole,pulsar timing array,first-order phase transition
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要点】:本文提出了一种新的解释,认为PSR J0514-4002E所在的二元系统中,其伴星可能是一个在早期宇宙相变过程中形成的原初黑洞,这一假设可以解释观测到的随机引力波背景。

方法】:作者通过分析MeerKAT对PSR J0514-4002E的脉冲计时观测数据,发现其伴星质量位于质量间隙中,从而提出了PSR J0514-4002E存在于一个原初黑洞-中子星二元星系的新观点。

实验】:利用MeerKAT进行脉冲计时观测,分析PSR J0514-4002E的观测数据,未提及具体数据集名称,但通过观测结果提出了新的理论模型,并计算出原初黑洞丰度与LIGO-Virgo-KAGRA的限制相符。