Primordial Black Holes as Dark Matter

By K. Jedamzik. 2001

393 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/d04d51f479976c810388c8e717c470f494b7a32c

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Citations in the corpus

Gravitational waves from primordial black hole mergers (2017, background): “The abundance of PBH dark matter (DM) over a broad mass range 10−18 − 104M is severely constrained [14, 15], and even if the PBHs make up all the DM, the present binary formation rate [16, 17] for a uniform PBH distribution has to be enhanced by a factor of O(108) to reach the merger rates indicated”
Dark matter direct-detection experiments (2015, background): “constraints mentioned above, are primordial black holes [36][37].”
Solving puzzles of GW150914 by primordial black holes (2016, background): “Constraints on PBH fraction in DM, f = ρPBH/ρDM, where the PBH mass distribution is taken as ρPBH(M) = M (2)dN/dM (see [38]).”
Primordial Black Holes from Polynomial Potentials in Single Field Inflation (2017, neutral): “[13] for a review of these constraints).”
Reconstructing the spectral shape of a stochastic gravitational wave background with LISA (2019, neutral): “[119–121] for general reviews, and refs.”
Science with the space-based interferometer LISA. IV: probing inflation with gravitational waves (2016, background): “Due to their nongaussian nature, sourced scalar perturbations with amplitude As = O ( 10−4 − 10−3 ) (the precise value depending on the scale) can lead to PBHs [98] in excess to the current bounds [99, 100].”
WIMP dark matter candidates and searches—current status and future prospects (2017, background): “However, there are many limits on PBHs as DM; see [41, 42].”
Primordial black holes as dark matter candidates (2021, background): “3Although BC’s first two papers were on PBHs [4, 20] and are his most cited ones, suggesting that his career has been downhill since the start, his 2016 paper with FK and Sandstad [8] is rapidly catching up!”
On primordial black holes from an inflection point (2017, background): “Although there are many possible astrophysical constraints on PBHs, those are questionable [3], [4] and thus, until further solid astrophysical arguments are given, one should seriously consider the possibility that”
Gravitational wave signatures of inflationary models from Primordial Black Hole dark matter (2017, background): “Analogously to the previous subsection, in the left panel of figure 11 we show a bump in the primordial curvature perturbations that saturates the present PBH bounds, given by neutron star capture [74].”
Massive Primordial Black Holes as Dark Matter and their detection with Gravitational Waves (2017, background): “They range from early to late epochs of the evolution of the Universe, with different probes (electromagnetic and gravitational waves) and different frequencies (from nHz to GHz and from meV to tens of GeV).”