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| Autores principales: | , , |
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| Formato: | Preprint |
| Publicado: |
2026
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| Acceso en línea: | https://arxiv.org/abs/2602.06815 |
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| _version_ | 1866915780373774336 |
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| author | Jacobsen, Rafael Bán Farias, Ricardo Luciano Sonego Dexheimer, Veronica |
| author_facet | Jacobsen, Rafael Bán Farias, Ricardo Luciano Sonego Dexheimer, Veronica |
| contents | In this work, we present the first extension of the Many-Body Forces (MBF) Model to finite temperature. The MBF Model describes nuclear matter in a relativistic quantum hadrodynamics formalism that takes many-body forces into account through a field dependence of the nuclear interaction coupling constants. Assuming nuclear matter to be charge neutral, beta-equilibrated, and populated by the baryon octet, electrons, and muons, we explore the parameters of the model, three different hyperon coupling schemes (also introduced here for the first time in MBF), and temperature effects to describe basic properties of nuclear matter, including the speed of sound, compressibility, and adiabatic index. We also investigate the mass-radius relation of compact stars by solving the Tolman-Oppenheimer-Volkoff equations at zero and finite temperature, including scenarios with fixed entropy per baryon. Our original results at finite temperature open the path to a new description of proto-neutron stars. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_06815 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Many-body effects on dense matter with hyperons at finite temperature Jacobsen, Rafael Bán Farias, Ricardo Luciano Sonego Dexheimer, Veronica Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Theory In this work, we present the first extension of the Many-Body Forces (MBF) Model to finite temperature. The MBF Model describes nuclear matter in a relativistic quantum hadrodynamics formalism that takes many-body forces into account through a field dependence of the nuclear interaction coupling constants. Assuming nuclear matter to be charge neutral, beta-equilibrated, and populated by the baryon octet, electrons, and muons, we explore the parameters of the model, three different hyperon coupling schemes (also introduced here for the first time in MBF), and temperature effects to describe basic properties of nuclear matter, including the speed of sound, compressibility, and adiabatic index. We also investigate the mass-radius relation of compact stars by solving the Tolman-Oppenheimer-Volkoff equations at zero and finite temperature, including scenarios with fixed entropy per baryon. Our original results at finite temperature open the path to a new description of proto-neutron stars. |
| title | Many-body effects on dense matter with hyperons at finite temperature |
| topic | Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Theory |
| url | https://arxiv.org/abs/2602.06815 |