Bound on induced gravitational wave background from primordial black holes TeX Export

@article{citeulike:6074004, abstract = {The today's energy density of the induced (second order) gravitational wave background in the frequency region \$\sim 10^{-3} - 10^3\$ 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 \$\sim 40\$ Hz (which is the region explored by LIGO detector), the value of the induced part of \$\Omega\_{GW}\$ cannot exceed \$(1-3)\times 10^{-7}\$. The spread of values of the bound is caused by the uncertainty in parameters of the gravitational collapse of black holes.}, archivePrefix = {arXiv}, author = {Bugaev, Edgar and Klimai, Peter}, citeulike-article-id = {6074004}, citeulike-linkout-0 = {http://arxiv.org/abs/0911.0611}, citeulike-linkout-1 = {http://arxiv.org/pdf/0911.0611}, day = {3}, eprint = {0911.0611}, keywords = {black, gravitational, holes, primordial, second-order, waves}, month = {Nov}, posted-at = {2009-11-05 11:34:29}, priority = {2}, title = {Bound on induced gravitational wave background from primordial black holes}, url = {http://arxiv.org/abs/0911.0611}, year = {2009} }

TY - JOUR ID - citeulike:6074004 L3 - citeulike-article-id:6074004 N2 - The today's energy density of the induced (second order) gravitational wave background in the frequency region $\sim 10^{-3} - 10^3$ 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 $\sim 40$ Hz (which is the region explored by LIGO detector), the value of the induced part of $\Omega_{GW}$ cannot exceed $(1-3)\times 10^{-7}$. The spread of values of the bound is caused by the uncertainty in parameters of the gravitational collapse of black holes. TI - Bound on induced gravitational wave background from primordial black holes KW - black KW - gravitational KW - holes KW - primordial KW - second-order KW - waves AU - Bugaev, Edgar AU - Klimai, Peter PY - 2009/Nov/03/ UR - http://arxiv.org/abs/0911.0611 ER -