35 citations · 69 across the 6 of their papers we have counts for
7 papers
Electromagnetic Signatures From Primordial Black Holes in the Solar System
Alexandra P. Klipfel, David I. Kaiser
Primordial black holes (PBHs) in the asteroid-mass range, with typical masses , have drawn significant recent attention as a v…
Gravitational Ionization by Schwarzschild Primordial Black Holes
Alexandra P. Klipfel, David I. Kaiser
Primordial black holes (PBHs) are theorized to form from the collapse of overdensities in the very early Universe. PBHs in the asteroid-mass range $10^{17} \, {\rm g}\lesssim M \le…
Hawking Radiation Signatures from Primordial Black Holes Transiting the Inner Solar System: Prospects for Detection
Alexandra P. Klipfel, Peter Fisher, David I. Kaiser
Primordial black holes (PBHs) arise from the collapse of density perturbations in the early universe and serve as a dark matter (DM) candidate and a probe of fundamental physics. T…
Gravitational wave signals from primordial black holes orbiting solar-type stars
Vitorio A. De Lorenci, David I. Kaiser, Patrick Peter +2
Primordial black holes (PBHs) with masses between and kg are candidates to contribute a substantial fraction of the total dark matter abundance. When in orbit a…
Ultra-High-Energy Neutrinos from Primordial Black Holes
Alexandra P. Klipfel, David I. Kaiser
The KM3NeT Collaboration recently announced the detection of a neutrino with energy 220 PeV. One possible source of such ultra-high-energy particles is the rapid emission of energe…
Orbital motion of primordial black holes crossing Solar-type stars
Vitorio A. De Lorenci, David I. Kaiser, Patrick Peter
Primordial black holes (PBHs) are hypothetical objects that could have originated from density fluctuations in a very early phase of our Universe. Recent observations restrict the…
Close encounters of the primordial kind: a new observable for primordial black holes as dark matter
Tung X. Tran, Sarah R. Geller, Benjamin V. Lehmann +1
Primordial black holes (PBHs) remain a viable dark matter candidate in the asteroid-mass range. We point out that in this scenario, the PBH abundance would be large enough for at l…