Testing Gravity with Frequency-Dependent Overlap Reduction Function in Pulsar Timing Array

Fuente: arXiv
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Main Authors: Liang, Qiuyue, Obata, Ippei, Sasaki, Misao
Format: Preprint
Published: 2024
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author Liang, Qiuyue
Obata, Ippei
Sasaki, Misao
author_facet Liang, Qiuyue
Obata, Ippei
Sasaki, Misao
contents The positive evidence of a nano-hertz gravitational wave background recently found by several pulsar timing array (PTA) collaborations opened up a window to test modified gravity theories in a unique frequency band in parallel to other gravitational wave detection experiments. In particular, the overlap reduction function (ORF) in PTA observation is sensitive to the phase velocity of gravitational waves. In this work, we provide analytical expressions for the coefficients of the multipole moments in the ORF, and utilize these analytical results to study constraints on the phase velocity from the frequency dependent overlap reduction function obtained from the Chinese PTA (CPTA) data. While the data contain large error bars yet, interesting constraints are found in the frequency-dependent ORF in the case of subluminal phase velocity. This makes us expect that the nano-hertz band gravitational wave background will become one of the important arenas for exploring modified gravity theories.
format Preprint
id arxiv_https___arxiv_org_abs_2405_11755
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Testing Gravity with Frequency-Dependent Overlap Reduction Function in Pulsar Timing Array
Liang, Qiuyue
Obata, Ippei
Sasaki, Misao
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
The positive evidence of a nano-hertz gravitational wave background recently found by several pulsar timing array (PTA) collaborations opened up a window to test modified gravity theories in a unique frequency band in parallel to other gravitational wave detection experiments. In particular, the overlap reduction function (ORF) in PTA observation is sensitive to the phase velocity of gravitational waves. In this work, we provide analytical expressions for the coefficients of the multipole moments in the ORF, and utilize these analytical results to study constraints on the phase velocity from the frequency dependent overlap reduction function obtained from the Chinese PTA (CPTA) data. While the data contain large error bars yet, interesting constraints are found in the frequency-dependent ORF in the case of subluminal phase velocity. This makes us expect that the nano-hertz band gravitational wave background will become one of the important arenas for exploring modified gravity theories.
title Testing Gravity with Frequency-Dependent Overlap Reduction Function in Pulsar Timing Array
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2405.11755