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Constraints on the velocity of gravitational waves from the NANOGrav 15-year data set

Yan-Chen Bi1,2,§, Yu-Mei Wu2,3,*, Zu-Cheng Chen4,5,6,7,†, and Qing-Guo Huang1,2,3,‡

  • 1CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 2School of Physical Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, China
  • 3School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, UCAS, Hangzhou 310024, China
  • 4Department of Physics and Synergetic Innovation Center for Quantum Effects and Applications, Hunan Normal University, Changsha, Hunan 410081, China
  • 5Institute of Interdisciplinary Studies, Hunan Normal University, Changsha, Hunan 410081, China
  • 6Department of Astronomy, Beijing Normal University, Beijing 100875, China
  • 7Advanced Institute of Natural Sciences, Beijing Normal University, Zhuhai 519087, China

  • *Corresponding author: ymwu@ucas.ac.cn
  • †Corresponding author: zuchengchen@hunnu.edu.cn
  • ‡Corresponding author: huangqg@itp.ac.cn
  • §biyanchen@itp.ac.cn

Phys. Rev. D 109, L061101 – Published 21 March, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.L061101

Abstract

General relativity predicts that gravitational waves propagate at the speed of light. Although ground-based gravitational-wave detectors have successfully constrained the velocity of gravitational waves in the high-frequency range, extending this constraint to the lower frequency range remains a challenge. In this work, we utilize the deviations in the overlap reduction function for a gravitational-wave background within pulsar timing arrays to investigate the velocity of gravitational waves in the nanohertz frequency band. By analyzing the NANOGrav 15-year data set, we obtain a well-constrained lower bound for the velocity of gravitational waves that v≳0.85c at the 3σ credible level, where c is the speed of light.

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