GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes
GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes
The LIGO detection of the gravitational wave transient GW150914, from the inspiral and merger of two black holes with masses ≳30M⊙, suggests a population of binary black holes with relatively high mass. This observation implies that the stochastic gravitational-wave background from binary black holes, created from the incoherent superposition of …