Analysis of the Gravitational Wave Background Using Gamma-Ray Pulsar Timing Arrays with Next-Generation Detectors
arXiv:2309.13359 · doi:10.1103/PhysRevD.108.083020
Abstract
In this work, we investigate the potential of gamma-ray pulsar time array (PTA) on gravitational waves background (GWB) using future gamma-ray detectors with larger effective areas. We consider both spaceborne detectors and ground-based imaging air Cherenkov telescope arrays (IACTs). We simulated the detected photons from pulsars using the response of hypothetical detectors taking into account the backgrounds and analyzed the sensitivities. Our results showed that thanks to the higher statistics of IACTs, the PTA using IACTs can improve significantly the performance compared with the PTA using Fermi-LAT data.
arXiv comment6 pages, 5 figures, Accepted for publication in PRD
References in corpus (15)
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array
- Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
- Pre-Big-Bang in String Cosmology
- Incremental Fermi Large Area Telescope Fourth Source Catalog
- Development of the Model of Galactic Interstellar Emission for Standard Point-Source Analysis of Fermi Large Area Telescope Data
- Low-frequency gravitational radiation from coalescing massive black hole binaries in hierarchical cosmologies
- Stochastic Gravitational Wave Backgrounds
- PINT: A Modern Software Package for Pulsar Timing
- Astrophysics Milestones For Pulsar Timing Array Gravitational Wave Detection
- Forecast constraints on cosmic string parameters from gravitational wave direct detection experiments
- 5@5 - a 5 GeV energy threshold array of imaging atmospheric Cherenkov telescopes at 5 km altitude
- Limits on Direct Detection of Gravitational Waves
- A Gamma-ray Pulsar Timing Array Constrains the Nanohertz Gravitational Wave Background
- Construction and On-site Performance of the LHAASO WFCTA Camera