Stochastic gravitational-wave background from primordial black hole scenario after GW150914 and GW151226

By Sai Wang, Yi-Fan Wang, Q. Huang, T. Li. 2016

157 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/4c06e1af2baceefc67302e3e33871756c40d5dc2

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Citations in the corpus

• Solar-mass primordial black holes explain NANOGrav hint of gravitational waves (2020, background): “The dark shaded regions at the top are constraints from EROS-2 [88] and MACHO [89] (brown), caustic crossing [90] (purple), Advanced LIGO O2 (subsolar mass range) [91] (gray), Advanced LIGO non-detection of the stochastic GW background [92, 93] (cyan), and the E-mode polarization of the CMB due to t”
• Primordial black holes from a tiny bump/dip in the inflaton potential (2019, methodology): “For constraints on PBH abundance using stochastic gravitational wave background (SGWB) from binary PBH mergers, see [35, 36].”
• Primordial Black Holes as Dark Matter: Recent Developments (2020, unknown): “[226].”
• Generating PBHs and small-scale GWs in two-field models of inflation (2020, background): “mple, the collapse of large scalar uctuations at scale k˘1012 Mpc 1 into M PBH ˘10 12 M PBHs leads to a SBGW that peaks in the frequency band targeted by the future space based GW interferometer LISA [48,49]. According to these results, the duration of the second stage of in ation becomes critical i”