Very high frequency gravitational wave background in the universe

Abbott B; Akishin P G Bogolyubov P N Pisarev A F; Allen B; Astone; Barrau A Boudoul G Derome L; Bekenstein J D; Bessonov E G; Bisnovatyi-Kogan G S; Bochkarev N G; Braginskii V B; Chavda A L; Cutler C; G S Bisnovatyi-Kogan; Galtsov D V; Galtsov D V; Galtsov D V; Gertsenshtein M E; Grishchuk L P; Grishchuk L P; Grishchuk L P; Grishchuk L P; Hawking S W; Kuchiev M Yu; Landau L D; Landau L D; Mironovskii B N; Nakamura T Sasaki M Tanaka T Thorne K S; Naselskij P D; Novikov I D; Novikov I D; Page D N; Peebles P J E; Pisarev A F; Rudenko V N; Rudenko V N; Rudenko V N; Servin M Brodin G; Shoemaker D; V N Rudenko; Weinberg S; Zeldovich Y B; Zeldovich Ya B; Zeldovich Ya B

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Very high frequency gravitational wave background in the universe

Abstract

Astrophysical sources of high frequency gravitational radiation are considered in association with a new interest to very sensitive HFGW receivers required for the laboratory GW Hertz experiment. A special attention is paid to the phenomenon of primordial black holes evaporation. They act like black body to all kinds of radiation, including gravitons, and, therefore, emit an equilibrium spectrum of gravitons during its evaporation. Limit on the density of high frequency gravitons in the Universe is obtained, and possibilities of their detection are briefly discussed.Comment: 14 page

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Last time updated on 03/12/2019