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Can black hole MACHO binaries be detected by the Brazilian spherical antenna?
J. C. N. de Araujo, O. D. Miranda, C. S. Castro +2
Different studies show that dark matter of non-baryonic origin might exist. There have been experimental evidences that at least one form of dark matter has been detected through m…
Gravitational wave background from Population III black hole formation
J. C. N. de Araujo, O. D. Miranda, O. D. Aguiar
We study the generation of a stochastic gravitational wave (GW) background produced from a population of core-collapse supernovae, which form black holes in scenarios of structure…
Possible Strong Gravitational Wave Sources for the LISA Antenna
J. C. N. de Araujo, O. D. Miranda, O. D. Aguiar
Recently Fuller & Shi proposed that the gravitational collapse of supermassive objects () could be a cosmological source of -ray bursts (GRBs). The major…
Stochastic background of gravitational waves
J. C. N. de Araujo, O. D. Miranda, O. D. Aguiar
A continuous stochastic background of gravitational waves (GWs) for burst sources is produced if the mean time interval between the occurrence of bursts is smaller than the average…