Lepton Asymmetry Generated or Erased Across a Bounce

This paper computes a specific neutrino quantity in a cosmology whose collapse is regulated by a maximum density, the Aldred Limit evaluated on its neutron branch at 9.72e+54 grams per cubic centimetre. A lepton asymmetry much larger than the baryon asymmetry is not excluded a priori, because charge neutrality constrains only the charged leptons. Whether a bounce would erase a pre-existing asymmetry, or generate one, decides what range of asymmetries a post-bounce universe can inherit. The calculation gives the following headline values: T_bounce_MeV = 1045027636488.8951, initial_asymmetry = 0.01, survival_fraction = 1.0, observed_bound = asymmetry below 0.01 from nucleosynthesis (order of magnitude), rhoA_kg_m3 = 9.717779835388742e+57. Each value is obtained from stated assumptions by the deposited script and is compared with published observational values where such values exist. Where the computed frame effect is far below observational reach, that negative result is stated plainly rather than softened. This study is simulated and computed from stated assumptions; it is not a measurement.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-11
DOI
https://doi.org/10.5281/zenodo.24129755
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
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article

Lepton Asymmetry Generated or Erased Across a Bounce

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Lepton Asymmetry Generated or Erased Across a Bounce

William Alexander Aldred
article en

Abstract

This paper computes a specific neutrino quantity in a cosmology whose collapse is regulated by a maximum density, the Aldred Limit evaluated on its neutron branch at 9.72e+54 grams per cubic centimetre. A lepton asymmetry much larger than the baryon asymmetry is not excluded a priori, because charge neutrality constrains only the charged leptons. Whether a bounce would erase a pre-existing asymmetry, or generate one, decides what range of asymmetries a post-bounce universe can inherit. The calculation gives the following headline values: T_bounce_MeV = 1045027636488.8951, initial_asymmetry = 0.01, survival_fraction = 1.0, observed_bound = asymmetry below 0.01 from nucleosynthesis (order of magnitude), rhoA_kg_m3 = 9.717779835388742e+57. Each value is obtained from stated assumptions by the deposited script and is compared with published observational values where such values exist. Where the computed frame effect is far below observational reach, that negative result is stated plainly rather than softened. This study is simulated and computed from stated assumptions; it is not a measurement.

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
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