Analysis of the gravitational wave background using gamma-ray pulsar timing arrays with next-generation detectors

被引：0
|
作者：
Xie, Zhen [1 ,2 ,3 ]
Zhang, Zhipeng [1 ,2 ,3 ]
Wang, Jieshuang [4 ]
Yang, Ruizhi [1 ,2 ,3 ]
机构：
[1] Univ Sci & Technol China, Deep Space Explorat Lab, Sch Phys Sci, Hefei 230026, Peoples R China
[2] Univ Sci & Technol China, Sch Phys Sci, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
[3] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
[4] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
来源：
PHYSICAL REVIEW D | 2023年 / 108卷 / 08期
关键词：
CHERENKOV TELESCOPES; RADIATION; LIMITS;
D O I：
10.1103/PhysRevD.108.083020
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this work, we investigate the potential of gamma-ray pulsar time array (PTA) on gravitational wave 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.
引用
收藏
页数：6
相关论文
共 50 条
  • [1] A gamma-ray pulsar timing array constrains the nanohertz gravitational wave background
    Ajello, M.
    Atwood, W. B.
    Baldini, L.
    Ballet, J.
    Barbiellini, G.
    Bastieri, D.
    Bellazzini, R.
    Berretta, A.
    Bhattacharyya, B.
    Bissaldi, E.
    Blandford, R. D.
    Bloom, E.
    Bonino, R.
    Bruel, P.
    Buehler, R.
    Burns, E.
    Buson, S.
    Cameron, R. A.
    Caraveo, P. A.
    Cavazzuti, E.
    Cibrario, N.
    Ciprini, S.
    Clark, C. J.
    Cognard, I
    Coronado-Blazquez, J.
    Crnogorcevic, M.
    Cromartie, H.
    Crowter, K.
    Cutini, S.
    D'Ammando, F.
    De Gaetano, S.
    de Palma, F.
    Digel, S. W.
    Di Lalla, N.
    Dirirsa, F. Fana
    Di Venere, L.
    Dominguez, A.
    Ferrara, E. C.
    Fiori, A.
    Franckowiak, A.
    Fukazawa, Y.
    Funk, S.
    Fusco, P.
    Gammaldi, V
    Gargano, F.
    Gasparrini, D.
    Giglietto, N.
    Giordano, F.
    Giroletti, M.
    Green, D.
    SCIENCE, 2022, 376 (6592) : 521 - +
  • [2] On measuring the gravitational-wave background using Pulsar Timing Arrays
    van Haasteren, Rutger
    Levin, Yuri
    McDonald, Patrick
    Lu, Tingting
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 395 (02) : 1005 - 1014
  • [3] GRAVITATIONAL WAVES A gamma-ray pulsar timing array
    不详
    SCIENCE, 2022, 376 (6592) : 472 - 472
  • [4] Cosmography with next-generation gravitational wave detectors
    Chen, Hsin-Yu
    Ezquiaga, Jose Maria
    Gupta, Ish
    CLASSICAL AND QUANTUM GRAVITY, 2024, 41 (12)
  • [5] Seeing the gravitational wave universe Pulsar timing arrays will be a window into the gravitational wave background
    Mingarelli, Chiara M. F.
    Casey-Clyde, J. Andrew
    SCIENCE, 2022, 378 (6620) : 592 - 593
  • [6] Quantum gravitational signatures in next-generation gravitational wave detectors
    Das, Saurya
    Shankaranarayanan, S.
    Todorinov, Vasil
    PHYSICS LETTERS B, 2022, 835
  • [7] Gravitational wave research using pulsar timing arrays
    George Hobbs
    Shi Dai
    National Science Review, 2017, 4 (05) : 707 - 717
  • [8] Gravitational wave research using pulsar timing arrays
    Hobbs, George
    Dai, Shi
    NATIONAL SCIENCE REVIEW, 2017, 4 (05) : 707 - 717
  • [9] Chirality of the gravitational-wave background and pulsar-timing arrays
    Belgacem, Enis
    Kamionkowski, Marc
    PHYSICAL REVIEW D, 2020, 102 (02)
  • [10] Prospects for gravitational wave astronomy with next generation large-scale pulsar timing arrays
    Wang, Yan
    Mohanty, Soumya D.
    12TH EDOARDO AMALDI CONFERENCE ON GRAVITATIONAL WAVES (AMALDI 12), 2018, 957
12345