Abstract
General formulas are given for the mean net baryon number produced in the decay of superheavy scalar or vector bosons. These results are used to make rough numerical estimates of the cosmological baryon abundance that would result from such decay processes in the very early universe.
Keywords
Affiliated Institutions
Related Publications
Signatures of relativistic neutrinos in CMB anisotropy and matter clustering
We present a detailed analytical study of ultra-relativistic neutrinos in cosmological perturbation theory and of the observable signatures of inhomogeneities in the cosmic neut...
<i>Planck</i> 2018 results
We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the t...
The Large Scale Structure of Space-Time
Einstein's General Theory of Relativity leads to two remarkable predictions: first, that the ultimate destiny of many massive stars is to undergo gravitational collapse and to d...
Neutrino and dark radiation properties in light of recent CMB observations
Recent cosmic microwave background measurements at high multipoles from the South Pole Telescope and from the Atacama Cosmology Telescope seem to disagree in their conclusions f...
Planck 2018 results. VI. Cosmological parameters
We present cosmological parameter results from the final full-mission Planck\nmeasurements of the CMB anisotropies. We find good consistency with the\nstandard spatially-flat 6-...
Publication Info
- Year
- 1979
- Type
- article
- Volume
- 20
- Issue
- 10
- Pages
- 2484-2493
- Citations
- 176
- Access
- Closed
External Links
Social Impact
Social media, news, blog, policy document mentions
Citation Metrics
Cite This
Identifiers
- DOI
- 10.1103/physrevd.20.2484