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245 10 $a Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries / $c Tong Liu ... [et al.].
490 0# $a Trabajos publicados del IAR ; $v no. 1390
520 ## $a Fast radio bursts (FRBs) are radio transients lasting only about a few milliseconds. They seem to occur at cosmological distances. We propose that these events can originate in the collapse of the magnetospheres of Kerr–Newman black holes (KNBHs). We show that the closed orbits of charged particles in the magnetospheres of these objects are unstable. After examining the dependencies on the specific charge of the particle and the spin and charge of the KNBH, we conclude that the resulting timescale and radiation mechanism fit well with extant observations of FRBs. Furthermore, we argue that the merger of a KNBH binary is a plausible central engine for the potential gamma-ray or radio afterglow following certain FRBs and can also account for gravitational wave (GW) events like GW 150914. Our model leads to predictions that can be tested by combined multiwavelength electromagnetic and GW observations.
773 0# $7 ||as $t The astrophysical journal $d Institute of Physics $x 0004-637X $g Vol. 826, Issue 1, (2016), id. 82
700 1# $a Liu, Tong.
700 1# $a Romero, G. E. $q (Gustavo Esteban)
700 1# $a Liu, Mo-Lin.
700 1# $a Li, Ang.
653 ## $a Fast radio bursts.
653 ## $a Gamma-rays.
653 ## $a Black holes.
653 ## $a Black hole binaries.
653 ## $a Kerr-Newman black holes.
040 ## $a AR-BaBIR

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