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- W2007931415 abstract "The today’s energy density of the induced (second order) gravitational wave background in the frequency region ∼10−3–103 Hz is constrained using the existing limits on primordial black hole production in the early Universe. It is shown, in particular, that at frequencies near ∼40 Hz (which is the region explored by LIGO detector), the value of the induced part of ΩGW cannot exceed (1−3) × 10−7. The spread of values of the bound is caused by the uncertainty in parameters of the gravitational collapse of black holes." @default.
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- W2007931415 date "2010-01-01" @default.
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- W2007931415 title "Bound on induced gravitational wave background from primordial black holes" @default.
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- W2007931415 doi "https://doi.org/10.1134/s0021364010010017" @default.
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