Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies

Camelio, Giovanni; Lovato, Alessandro; Gualtieri, Leonardo; Benhar, Omar; Pons, José A.; Ferrari, Valeria

doi:10.1103/PhysRevD.96.043015

Title: Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies

Journal Article · Wed Aug 30 00:00:00 EDT 2017 · Physical Review D

DOI:https://doi.org/10.1103/PhysRevD.96.043015· OSTI ID:1415938

Camelio, Giovanni ^[1]; Lovato, Alessandro ^[2]; Gualtieri, Leonardo ^[3]; Benhar, Omar ^[3]; Pons, José A. ^[4]; Ferrari, Valeria ^[3]

Univ. di Roma, Roma (Italy). Dipartimento di Fisica; Stockholm Univ. (Sweden). Astronomy and Oskar Klein Centre
Argonne National Lab. (ANL), Argonne, IL (United States). Physics Division
Univ. di Roma, Roma (Italy). Dipartimento di Fisica
Univ. d'Alacant, Alacant (Spain). Dept. de Fisica Aplicada

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. Here, 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.

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Research Organization:: Argonne National Lab. (ANL), Argonne, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Nuclear Physics (NP)

Grant/Contract Number:: AC02-06CH11357; StronGrHEP-690904; AYA2015-66899-C2-2-P

OSTI ID:: 1415938

Alternate ID(s):: OSTI ID: 1377655

Journal Information:: Physical Review D, Vol. 96, Issue 4; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 44 works

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