Signals of Bursts from the Very Early Universe

Abstract We consider possible observable signals from explosive events in the very early Universe, dubbed “bursts.” These could be expected in connection with massive black hole or “baby Universe” formation. We anticipate that such major disruptions of spacetime would be associated with neutrino and perhaps other pulses. While these seem to be not detectable directly, we discuss how they could lead to potentially observable signals. We analyze how the pulses from very early times may “escape,” that is, propagate to the last scattering epoch at the time t cmb and later, or alternatively be absorbed earlier, i.e., “contained.” The possibly detectable signals include effects on small regions of the cosmic microwave background, a soft X-ray resulting from positron production, or a nonthermal addition to the relic neutrino background.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-10-15
DOI
https://doi.org/10.3847/1538-4357/ae01a4
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

Signals of Bursts from the Very Early Universe

Joseph Silk, L. Stodolsky
The Astrophysical Journal
Cosmology and Gravitation Theories
article

Signals of Bursts from the Very Early Universe

Joseph Silk, L. Stodolsky
article en

Abstract

Abstract We consider possible observable signals from explosive events in the very early Universe, dubbed “bursts.” These could be expected in connection with massive black hole or “baby Universe” formation. We anticipate that such major disruptions of spacetime would be associated with neutrino and perhaps other pulses. While these seem to be not detectable directly, we discuss how they could lead to potentially observable signals. We analyze how the pulses from very early times may “escape,” that is, propagate to the last scattering epoch at the time t cmb and later, or alternatively be absorbed earlier, i.e., “contained.” The possibly detectable signals include effects on small regions of the cosmic microwave background, a soft X-ray resulting from positron production, or a nonthermal addition to the relic neutrino background.

The Astrophysical JournalVol. 992(2)
Centre National de la Recherche Scientifique (FR), Johns Hopkins University (US), Institut d'Astrophysique de Paris (FR), Sorbonne Université (FR), University of Oxford (GB), Max Planck Institute for Physics (DE)
Openalex Percentile: Top 80%
Cosmology and Gravitation Theories
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