Maximum latent heat of neutron star matter without GR
We show how the specific latent heat is relevant to characterize the first-order phase transitions in neutron stars. Our current knowledge of this dynamical quantity strongly depends on the uncertainty bands of Chiral Perturbation Theory and of pQCD calculations and can be used to diagnose progress...
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| Format: | Article |
| Language: | English |
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EDP Sciences
2022-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2022/02/epjconf_vconf2021_07007.pdf |
| _version_ | 1819121392106340352 |
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| author | Lope-Oter Eva |
| author_facet | Lope-Oter Eva |
| author_sort | Lope-Oter Eva |
| collection | DOAJ |
| description | We show how the specific latent heat is relevant to characterize the first-order phase transitions in neutron stars. Our current knowledge of this dynamical quantity strongly depends on the uncertainty bands of Chiral Perturbation Theory and of pQCD calculations and can be used to diagnose progress on the equation of state. We state what is known to be hadron-model independent and without feedback from neutron star observations and, therefore, they can be used to test General Relativity as well as theories beyond GR, such as modified gravity. |
| first_indexed | 2024-12-22T06:35:50Z |
| format | Article |
| id | doaj.art-8bb942f0648c4302aa9b9abcd926cf5f |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-22T06:35:50Z |
| publishDate | 2022-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-8bb942f0648c4302aa9b9abcd926cf5f2022-12-21T18:35:36ZengEDP SciencesEPJ Web of Conferences2100-014X2022-01-012580700710.1051/epjconf/202225807007epjconf_vconf2021_07007Maximum latent heat of neutron star matter without GRLope-Oter Eva0Dept. Física Teórica and IPARCOS, Univ. Complutense de MadridWe show how the specific latent heat is relevant to characterize the first-order phase transitions in neutron stars. Our current knowledge of this dynamical quantity strongly depends on the uncertainty bands of Chiral Perturbation Theory and of pQCD calculations and can be used to diagnose progress on the equation of state. We state what is known to be hadron-model independent and without feedback from neutron star observations and, therefore, they can be used to test General Relativity as well as theories beyond GR, such as modified gravity.https://www.epj-conferences.org/articles/epjconf/pdf/2022/02/epjconf_vconf2021_07007.pdf |
| spellingShingle | Lope-Oter Eva Maximum latent heat of neutron star matter without GR EPJ Web of Conferences |
| title | Maximum latent heat of neutron star matter without GR |
| title_full | Maximum latent heat of neutron star matter without GR |
| title_fullStr | Maximum latent heat of neutron star matter without GR |
| title_full_unstemmed | Maximum latent heat of neutron star matter without GR |
| title_short | Maximum latent heat of neutron star matter without GR |
| title_sort | maximum latent heat of neutron star matter without gr |
| url | https://www.epj-conferences.org/articles/epjconf/pdf/2022/02/epjconf_vconf2021_07007.pdf |
| work_keys_str_mv | AT lopeotereva maximumlatentheatofneutronstarmatterwithoutgr |