Dynamics of metastable Standard Model particles from long-lived particle decays in the MeV primordial plasma
arXiv:2411.00931 · doi:10.1103/PhysRevD.111.063542
Abstract
We investigate the cosmological impact of hypothetical unstable new physics particles that decay in the MeV-scale plasma of the Early Universe. Focusing on scenarios where the decays produce metastable species such as muons, pions, and kaons, we systematically analyze the dynamics of these particles using coupled Boltzmann equations governing their abundances. Our results demonstrate that the metastable species can efficiently annihilate or interact with nucleons, often leading to their disappearance before decay. The suppression of decay significantly alters the properties of cosmic neutrinos, impacting cosmological observables like Big Bang nucleosynthesis and the Cosmic Microwave Background. To support further studies, we provide two public codes: the Mathematica code that traces the evolution of these metastable particles, as well as the python-based unintegrated neutrino Boltzmann solver that uses this evolution as an input and may be applied to a broad range of scenarios. We then utilize them for studying a few particular new physics models.
Version accepted for the publication in PRD. Companion paper of "New physics decaying into metastable particles: impact on cosmic neutrinos"
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- No Hiding in the Dark: Cosmological Bounds on Heavy Neutral Leptons with Dark Decay Channels
- Precision calculation of with Neutrino Direct Simulation Monte Carlo
- Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look
- Neutrino Emission and Plasma Heating from Primordial Black Holes: An Improved Approach to Constraints