Q Fei - Communications in Theoretical Physics, 2024 - iopscience.iop.org
The recent stochastic signal observed jointly by NANOGrav, parkes pulsar timing array, European pulsar timing array, and Chinese pulsar timing array can be accounted for by …
L Liu, SP Kim - Journal of Cosmology and Astroparticle Physics, 2022 - iopscience.iop.org
We consider the two-body dynamical capture of black holes carrying U (1) charge which can not only correspond to electric or magnetic charge but also have other physical …
A bstract We present current direct and astrophysical limits on the cosmological abundance of black holes with extremal magnetic charge. Such black holes do not Hawking radiate …
D Marín Pina, M Orselli, D Pica - Physical Review D, 2022 - APS
We analyze the formation and evolution of the event horizon of a black hole binary merger when the black holes are charged. We find that the presence of charge influences the …
In this manuscript, we investigate the electromagnetic radiation of a binary system of electrically charged black holes. Using the results of previous works, we compute the …
The stochastic signal detected by the NANOGrav, PPTA, EPTA, and CPTA collaborations can be attributed to gravitational waves induced by the primordial curvature perturbations …
The common-spectrum process, characterized by the Hellings–Downs angular correlation and observed by pulsar timing array collaborations, such as NANOGrav, PPTA, EPTA, and …
The stochastic signal observed by collaborations such as NANOGrav, PPTA, EPTA+ InPTA, and CPTA may originate from gravitational waves induced by primordial curvature …
Black hole binary systems can form and evolve in the inner region of a galaxy, where usually a supermassive black hole is located. These three objects naturally form a triple system …