Can an off-axis gamma-ray burst jet in GW170817 explain all the electromagnetic counterparts?

• 井岡, 邦仁

  Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University

• 中村, 卓史

  enter for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University･JapanDepartment of Physics, Kyoto University

抄録

Gravitational waves from a merger of two neutron stars (NSs) were discovered for the first time in GW170817, together with diverse electromagnetic (EM) counterparts. To make constraints on a relativistic jet from the NS merger, we calculate the EM signals in (1) the short gamma-ray burst sGRB 170817A from an off-axis jet, (2) the optical–infrared macronova (or kilonova), especially the blue macronova, from a jet-powered cocoon, and (3) the X-ray and radio afterglows from the interaction between the jet and interstellar medium. We find that a typical sGRB jet is consistent with these observations, and there is a parameter space to explain all the observations in a unified fashion with an isotropic energy ～ 10⁵¹ - 10⁵² erg, opening angle ～ 20°, and viewing angle ～ 30°. The off-axis emission is less de-beamed than the point-source case because the viewing angle is comparable to the opening angle. We also analytically show that the jet energy accelerates a fair fraction of the merger ejecta to a sub-relativistic velocity ～0.3 - 0.4c as a cocoon in a wide parameter range. The ambient density might be low ～ 10⁻³ - 10⁻⁶ cm⁻³, which can be tested by future observations of radio flares and X-ray remnants.

収録刊行物

• Progress of Theoretical and Experimental Physics

  Progress of Theoretical and Experimental Physics 2018 (4), 043E02-, 2018-04

  Physical Society of Japan

キーワード

• General Physics and Astronomy

詳細情報

• CRID: 1050845763140658304
• NII論文ID: 120006591359
• ISSN: 20503911
• DOI: 10.1093/ptep/pty036
• HANDLE: 2433/237302
• Web Site: http://academic.oup.com/ptep/article-pdf/2018/4/043E02/24691106/pty036.pdf
• 本文言語コード: en
• 資料種別: journal article
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