Inferring the cosmological constant in early Universe only by gravitational waves

Fuente: arXiv
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Hauptverfasser: Li, Song, Han, Wen-Biao
Format: Preprint
Veröffentlicht: 2025
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author Li, Song
Han, Wen-Biao
author_facet Li, Song
Han, Wen-Biao
contents The expansion of the Universe is accelerating which can be interpreted as due to the cosmological constant $Λ$. In this study, we investigate the behavior of gravitational waves in the presence of a cosmological constant in the early universe. We rigorously analyze the merger rate of binary primordial black holes (PBHs) and the corresponding signal-to-noise ratio within the framework of Laser Interferometer Space Antenna (LISA). We find that binary PBHs with a total mass of $M_{\mathrm{tot}}=1000M_{\odot}$ and a redshift larger than $z=500$ are the ideal system for studying the effect of the cosmological constant through LISA. By computing the fisher information matrix, we establish that the cosmological constant can be effectively constrained.
format Preprint
id arxiv_https___arxiv_org_abs_2501_12608
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Inferring the cosmological constant in early Universe only by gravitational waves
Li, Song
Han, Wen-Biao
General Relativity and Quantum Cosmology
The expansion of the Universe is accelerating which can be interpreted as due to the cosmological constant $Λ$. In this study, we investigate the behavior of gravitational waves in the presence of a cosmological constant in the early universe. We rigorously analyze the merger rate of binary primordial black holes (PBHs) and the corresponding signal-to-noise ratio within the framework of Laser Interferometer Space Antenna (LISA). We find that binary PBHs with a total mass of $M_{\mathrm{tot}}=1000M_{\odot}$ and a redshift larger than $z=500$ are the ideal system for studying the effect of the cosmological constant through LISA. By computing the fisher information matrix, we establish that the cosmological constant can be effectively constrained.
title Inferring the cosmological constant in early Universe only by gravitational waves
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2501.12608