The gravitational wave and short gamma-ray burst GW170817/SHB170817A

被引：0

作者：

De Rujula, A. ^{[1
,2
]}

机构：

[1] Univ Autonoma Madrid, CSIC, Inst Fis Teor, Madrid, Spain

[2] CERN, Div Theory, CH-1211 Geneva 23, Switzerland

来源：

NUOVO CIMENTO C-COLLOQUIA AND COMMUNICATIONS IN PHYSICS | 2023年 / 46卷 / 01期

关键词：

SWIFT-XRT OBSERVATIONS; LIGHT CURVES; EXTENDED EMISSION; ENERGY INJECTION; AFTERGLOWS; ORIGIN; GRBS; SIGNATURE; EVOLUTION; FIREBALLS;

D O I：

10.1393/ncc/i2023-23005-2

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

This event, so far unique, beautifully confirmed the standard views on the gravitational waves produced by a merger of two neutron stars, but its electro-magnetic multi-wavelenth observations disagreed with the numerous initial versions of the "standard fireball model(s)" of gamma ray bursts. Contrariwise, they pro-vided strong evidence in favour of the "cannonball" model. Most uncontroversially, a cannonball was observed at radio wavelengths, with an overwhelming statistical significance (> 17 sigma), and travelling in the plane of the sky, as expected, at an average apparent superluminal velocity Vapp 4 c.

引用

页数：10

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