Non-thermal particle production in Einstein-Cartan gravity with modified Holst term and non-minimal couplings

TL;DR

This paper explores non-thermal fermionic particle production in a modified Einstein-Cartan gravity framework, revealing how pseudoscalar fields influence early universe inflation and particle generation.

Contribution

It introduces the Einstein-Cartan pseudoscalaron and analyzes its role in inflation and non-thermal particle production with non-minimal couplings.

Findings

Pseudoscalaron drives inflation when potential dominates.

Non-minimal couplings destabilize the vacuum post-inflation.

Model parameters can enhance preheating and reheating processes.

Abstract

Non-thermal fermionic particle production is investigated in Einstein-Cartan modified gravity with a modified Holst term and non-minimal couplings between the spin connection and a fermion. By using the auxiliary field method, the theory is rewritten into a pseudoscalar-tensor theory with Einstein-Hilbert action and canonical kinetic and potential terms for a pseudoscalar field. The introduced field is called Einstein-Cartan pseudoscalaron. If the potential energy of the Einstein-Cartan pseudoscalaron dominates the energy density of the early universe, it causes inflationary expansion. After the end of inflation, the pseudoscalaron develops a large value and the non-minimal couplings destabilize the vacuum. Evaluating the non-thermal fermionic particle production process, we obtain the mass and the helicity dependences of the produced particle number density. We show the model parameters to enhance the preheating and reheating processes.