Conveners
Session 3
- Chair: João Rosa
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Dan Hooper (Fermilab/University of Chicago)17/06/2024, 14:00
Cosmology textbooks typically assume that the early universe was dominated by relativistic particles. But if even a relatively small number of black holes were created after inflation, they would have constituted an increasingly large fraction of the total energy density as the universe expanded. I’ll argue that it is well-motivated to scenarios in which the early universe included an era in...
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Volodymyr Takhistov (QUP, KEK)17/06/2024, 14:30
We present a new general paradigm for the production of dark matter (DM) relic abundance, regurgitated DM, based on the evaporation of early Universe primordial black holes (PBHs) themselves formed from DM particles. We discuss a minimal realization of the model with dark sector in which a first-order phase transition results in the formation of Fermiball remnants that collapse to PBHs, which...
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Suruj Jyoti Das (Institute for Basic Science, CTPU)17/06/2024, 15:00
We explore the possibility of dynamically producing the observed matter-antimatter asymmetry of the Universe entirely from the evaporation of primordial black holes (PBH), that are formed in an inflaton-dominated
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background. Considering the inflaton $(\phi)$ to oscillate in a monomial
potential $V(\phi)\propto\phi^n$, we show that it is possible to obtain
the desired baryon asymmetry via... -
Jacob Gunn (University of Naples Federico II)17/06/2024, 15:20
The parameter spaces of leptogenesis and ultralight ($M_{\rm PBH} \leq 10^9$g) Primordial Black Holes (PBHs) are notoriously difficult to constrain, but while experiments struggle to probe sterile neutrino masses heavier than a few GeV, the new window into the early universe opened by Gravitational Wave (GW) astronomy offers realistic hopes of detecting GW signals associated with PBHs. Since...
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