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Unveiling the graviton mass bounds through the analysis of 2023 pulsar timing array data releases

Sai Wang1 and Zhi-Chao Zhao2,*

  • 1Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, the People’s Republic of China
  • 2Department of Applied Physics, College of Science, China Agricultural University, Qinghua East Road, Beijing 100083, the People’s Republic of China

  • *Corresponding author: zhaozc@cau.edu.cn

Phys. Rev. D 109, L061502 – Published 18 March, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.L061502

Abstract

Strong evidence for the Helling-Downs correlation curves have been reported by multiple pulsar timing array (PTA) collaborations in the middle of 2023. In this work, we investigate the graviton mass bounds by analyzing the observational data of the overlap reduction functions from the NANOGrav 15-year data release and CPTA first data release. The results from our data analysis display the state-of-the-art upper limits on the graviton mass at 90% confidence level, namely, mg≲8.6×10−24  eV from NANOGrav and mg≲3.8×10−23  eV from CPTA. We also study the cosmic-variance limit on the graviton mass bounds, i.e., σmgCV=4.8×10−24  eV×f/(10  year)−1, with f being a typical frequency band of PTA observations. This is equivalent to the cosmic-variance limit on the speed of gravitational waves, i.e., σvgCV=0.07c, with c being the speed of light. Moreover, we discuss potential implications of these results for scenarios of ultralight tensor dark matter.

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