Nonthermal particle production in Einstein-Cartan gravity with modified Holst term and nonminimal couplings

Nonthermal fermionic particle production is investigated in Einstein-Cartan modified gravity with a modified Holst term and nonminimal 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 nonminimal couplings destabilize the vacuum. Evaluating the nonthermal 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.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-11-21
DOI
https://doi.org/10.1103/physrevd.110.103537
Citations
3
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.99
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article

Nonthermal particle production in Einstein-Cartan gravity with modified Holst term and nonminimal couplings

Naoki Yoshioka, Tomohiro Inagaki
3 citations
Physical review. D/Physical review. D.
Cosmology and Gravitation Theories
0.99
article

Nonthermal particle production in Einstein-Cartan gravity with modified Holst term and nonminimal couplings

Naoki Yoshioka, Tomohiro Inagaki
article en
3 citations

Abstract

Nonthermal fermionic particle production is investigated in Einstein-Cartan modified gravity with a modified Holst term and nonminimal 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 nonminimal couplings destabilize the vacuum. Evaluating the nonthermal 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.

Physical review. D/Physical review. D.Vol. 110(10)
Hiroshima University (JP)
Openalex Percentile: Top 22%
Cosmology and Gravitation Theories
0.99
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