Astrophysical stochastic gravitational wave background

被引：2

作者：

de Freitas Pacheco, Jose Antonio ^{[1
]}

机构：

[1] Univ Cote Azur, Observ Cote Azur, F-06304 Nice, France

来源：

ASTRONOMISCHE NACHRICHTEN | 2019年 / 340卷 / 9-10期

关键词：

binaries; gravitational wave; LIGO; magnetars; supernova; VIRGO; CORE-COLLAPSE; NEUTRON-STAR; SIMULATIONS; POPULATION; EVOLUTION; BINARIES; RATES;

D O I：

10.1002/asna.201913738

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The stochastic gravitational wave background produced by supernovas, magnetars, and merger of binaries constituted of a pair of compact objects is reviewed and updated. The merger of systems composed of two black holes dominates by far the background signal, whose amplitude in the range 10-100 Hz is above the sensitivity of the planned Einstein laser interferometer (ET). The background signal at 25 Hz estimated by the laser interferometric gravitational observatory (LIGO)-VIRGO collaboration, based on the available merger detection data, is in good agreement with the present theoretical predictions.

引用

页码：935 / 944

页数：10

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