Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation
Abstract Gravitational particle production in cosmology is a mechanism through which particles of different natures are produced during the very early universe. It is a general mechanism that explains how the universe became populated with the particles of the Standard Model after cosmic inflation a...
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SpringerOpen
2025-07-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-025-14426-0 |
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| author | Flavio Pineda Luis O. Pimentel |
| author_facet | Flavio Pineda Luis O. Pimentel |
| author_sort | Flavio Pineda |
| collection | DOAJ |
| description | Abstract Gravitational particle production in cosmology is a mechanism through which particles of different natures are produced during the very early universe. It is a general mechanism that explains how the universe became populated with the particles of the Standard Model after cosmic inflation and may also account for the origin of dark matter. In this work, we study the non-perturbative production of massive scalar particles in the Higgs- $$R^2$$ R 2 inflation model, a two-field scalar inflation model within the Einstein frame. We consider spectator scalar fields that are conformally or minimally coupled to the gravitational field through the curvature scalar R which in turn is a time-dependent function determined by the fields driving inflationary dynamics. We numerically compute the production of these particles using the Bogolyubov transformation method for each scenario, aiming to assess the spectrum of the produced particles. For both scenarios, we consider light particles with masses $$m_\chi \ll H_{\textrm{end}}$$ m χ ≪ H end and large masses that exceed the Hubble scale at the end of inflation $$m_\chi \gtrsim H_{\textrm{end}}.$$ m χ ≳ H end . We use these numerical results to calculate the relic abundance $$\Omega _\chi h^2$$ Ω χ h 2 to find out if the model is viable as a dark matter candidate. |
| format | Article |
| id | doaj-art-51d827e19e8a407bb44c552755fe21cf |
| institution | DOAJ |
| issn | 1434-6052 |
| language | English |
| publishDate | 2025-07-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj-art-51d827e19e8a407bb44c552755fe21cf2025-08-20T03:04:17ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-07-0185711710.1140/epjc/s10052-025-14426-0Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflationFlavio Pineda0Luis O. Pimentel1Departamento de Física, Universidad Autónoma MetropolitanaDepartamento de Física, Universidad Autónoma MetropolitanaAbstract Gravitational particle production in cosmology is a mechanism through which particles of different natures are produced during the very early universe. It is a general mechanism that explains how the universe became populated with the particles of the Standard Model after cosmic inflation and may also account for the origin of dark matter. In this work, we study the non-perturbative production of massive scalar particles in the Higgs- $$R^2$$ R 2 inflation model, a two-field scalar inflation model within the Einstein frame. We consider spectator scalar fields that are conformally or minimally coupled to the gravitational field through the curvature scalar R which in turn is a time-dependent function determined by the fields driving inflationary dynamics. We numerically compute the production of these particles using the Bogolyubov transformation method for each scenario, aiming to assess the spectrum of the produced particles. For both scenarios, we consider light particles with masses $$m_\chi \ll H_{\textrm{end}}$$ m χ ≪ H end and large masses that exceed the Hubble scale at the end of inflation $$m_\chi \gtrsim H_{\textrm{end}}.$$ m χ ≳ H end . We use these numerical results to calculate the relic abundance $$\Omega _\chi h^2$$ Ω χ h 2 to find out if the model is viable as a dark matter candidate.https://doi.org/10.1140/epjc/s10052-025-14426-0 |
| spellingShingle | Flavio Pineda Luis O. Pimentel Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation European Physical Journal C: Particles and Fields |
| title | Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation |
| title_full | Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation |
| title_fullStr | Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation |
| title_full_unstemmed | Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation |
| title_short | Non-perturbative approach for scalar particle production in Higgs- $$R^2$$ R 2 inflation |
| title_sort | non perturbative approach for scalar particle production in higgs r 2 r 2 inflation |
| url | https://doi.org/10.1140/epjc/s10052-025-14426-0 |
| work_keys_str_mv | AT flaviopineda nonperturbativeapproachforscalarparticleproductioninhiggsr2r2inflation AT luisopimentel nonperturbativeapproachforscalarparticleproductioninhiggsr2r2inflation |