首页|Simulation Study on Constraining Gravitational Wave Propagation Speed by Gravitational Wave and Gamma-ray Burst Joint Observation on Binary Neutron Star Mergers

Simulation Study on Constraining Gravitational Wave Propagation Speed by Gravitational Wave and Gamma-ray Burst Joint Observation on Binary Neutron Star Mergers

扫码查看
Theories of modified gravity suggest that the propagation speed of gravitational waves(GW)vg may deviate from the speed of light c.A constraint can be placed on the difference between c and vg with a simple method that uses the arrival time delay between GW and electromagnetic wave simultaneously emitted from a burst event.We simulated the joint observation of GW and short gamma-ray burst signals from binary neutron star merger events in different observation campaigns,involving advanced LIGO(aLIGO)in design sensitivity and Einstein Telescope(ET)joint-detected with Fermi/GBM.As a result,the relative precision of constraint on vg can reach~10-17(aLIGO)and~10-18(ET),which are one and two orders of magnitude better than that from GW170817,respectively.We continue to obtain the bound of graviton mass mg ≤ 7.1(3.2)×10-20eV with aLIGO(ET).Applying the Standard-Model Extension test framework,the constraint on vg allows us to study the Lorentz violation in the nondispersive,nonbirefringent limit of the gravitational sector.We obtain the constraints of the dimensionless isotropic coefficients(s)(4)00at mass dimension d=4,which are-1×10-15<(s)(4)00<9×10-17 for aLIGO and-4×10-16<(s)(4)00<8×10-18 for ET.

gravitational waves(stars:)gamma-ray burst:generalstars:neutron

Jin-Hui Rao、Shu-Xu Yi、Lian Tao、Qing-Wen Tang

展开 >

Department of Physics,School of Physics and Materials Science,Nanchang University,Nanchang 330031,China

Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China

National Natural Science Foundation of ChinaJiangxi Provincial Natural Science FoundationChinese Academy of SciencesChinese Academy of SciencesChinese Academy of Sciences

1206501720224ACB211001E329A3M1E32983U8E3545KU2

2024

天文和天体物理学研究
中国科学院国家天文台

天文和天体物理学研究

CSTPCD
影响因子:0.406
ISSN:1674-4527
年,卷(期):2024.24(8)