Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies
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Título: | Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies |
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Autor/es: | Camelio, Giovanni | Lovato, Alessandro | Gualtieri, Leonardo | Benhar, Omar | Pons, José A. | Ferrari, Valeria |
Grupo/s de investigación o GITE: | Astrofísica Relativista |
Centro, Departamento o Servicio: | Universidad de Alicante. Departamento de Física Aplicada |
Palabras clave: | Proto-neutron star | Nuclear many-body equation of state | Neutrino luminosity | Gravitational wave frequencies |
Área/s de conocimiento: | Astronomía y Astrofísica |
Fecha de publicación: | 30-ago-2017 |
Cita bibliográfica: | Physical Review D. 2017, 96: 043015. doi:10.1103/PhysRevD.96.043015 |
Resumen: | In a core-collapse supernova, a huge amount of energy is released in the Kelvin-Helmholtz phase subsequent to the explosion, when the proto-neutron star cools and deleptonizes as it loses neutrinos. Most of this energy is emitted through neutrinos, but a fraction of it can be released through gravitational waves. We model the evolution of a proto-neutron star in the Kelvin-Helmholtz phase using a general relativistic numerical code, and a recently proposed finite temperature, many-body equation of state; from this we consistently compute the diffusion coefficients driving the evolution. To include the many-body equation of state, we develop a new fitting formula for the high density baryon free energy at finite temperature and intermediate proton fraction. We estimate the emitted neutrino signal, assessing its detectability by present terrestrial detectors, and we determine the frequencies and damping times of the quasinormal modes which would characterize the gravitational wave signal emitted in this stage. |
Patrocinador/es: | This work has been partially supported by “NewCompStar,” COST Action MP1304, by the H2020-MSCA-RISE-2015 Grant No. StronGrHEP-690904, by INFN (through grant TEONGRAV), and supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357 (A. L.). J. A. P. acknowledges support by the Spanish MINECO Grant No. AYA2015-66899-C2-2-P. |
URI: | http://hdl.handle.net/10045/69067 |
ISSN: | 2470-0010 (Print) | 2470-0029 (Online) |
DOI: | 10.1103/PhysRevD.96.043015 |
Idioma: | eng |
Tipo: | info:eu-repo/semantics/article |
Derechos: | © 2017 American Physical Society |
Revisión científica: | si |
Versión del editor: | http://dx.doi.org/10.1103/PhysRevD.96.043015 |
Aparece en las colecciones: | INV - Astrofísica Relativista - Artículos de Revistas Investigaciones financiadas por la UE |
Archivos en este ítem:
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2017_Camelio_etal_PhysRevD.pdf | 855,21 kB | Adobe PDF | Abrir Vista previa | |
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