TL;DR
This paper investigates temperature-dependent CPT violation during Big Bang Nucleosynthesis, constraining electron-positron mass asymmetries with a modified BBN code and presenting models for the temperature dependence.
Contribution
It introduces a novel temperature-dependent CPT violation model with $b_0(T) \\propto T^2$ and derives the most stringent early-universe constraints using observational data.
Findings
Electron-positron mass differences are constrained to -6 GeV^{-1} for keV-scale masses.
No 7 overlap in all three observables, but pairwise overlaps constrain parameter space.
Toy models show how 7 temperature dependence can arise from field-theoretic mechanisms.
Abstract
In this study, we explore temperature-dependent CPT violation during Big Bang Nucleosynthesis (BBN) through electron-positron mass asymmetries parametrized by . The scaling naturally evades stringent laboratory bounds at zero temperature while allowing for significant CPT violation at MeV scales in the early universe \cite{ParticleDataGroup:2024cfk}. Using a modified version of the BBN code \faGithub \href{https://github.com/vallima/PRyMordial}{\,\texttt{PRyMordial}} with dynamically-solved chemical potentials and appropriate finite-mass corrections, we constrain electron-positron mass differences from observed abundances of Helium-4, Deuterium, and . We find that must be greater than or approximately equal to GeV for keV-scale mass differences at BBN. All three observables show no simultaneous overlap, though…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Code & Models
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsParticle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions · Dark Matter and Cosmic Phenomena
