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Astrophysical stochastic gravitational wave background
Author(s) -
Freitas Pacheco José Antonio
Publication year - 2019
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.201913738
Subject(s) - gravitational wave background , gravitational wave , physics , astronomy , classical mechanics , astrophysics
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.