Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current–neutrino interactions and inverse neutron decay

Fischer, Tobias; Guo, Gang; Dzhioev, Alan A.; Martínez-Pinedo, Gabriel; Wu, Meng-Ru; Lohs, Andreas; Qian, Yong-Zhong

doi:10.1103/physrevc.101.025804

Title: Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current–neutrino interactions and inverse neutron decay

Journal Article · Fri Feb 14 00:00:00 EST 2020 · Physical Review. C

DOI:https://doi.org/10.1103/physrevc.101.025804· OSTI ID:1800659

^[1]; Guo, Gang ^[2]; Dzhioev, Alan A. ^[3]; Martínez-Pinedo, Gabriel ^[4];

^[5]; Lohs, Andreas ^[6]; Qian, Yong-Zhong ^[7]

Univ. of Wroclaw (Poland)
GSI Helmholtzzentrum für Schwerioneneforschung, Darmstadt (Germany); Academia Sinica, Taipei (Taiwan)
Joint Inst. for Nuclear Research (JINR), Dubna (Russian Federation)
GSI Helmholtzzentrum für Schwerioneneforschung, Darmstadt (Germany); Technische Univ. Darmstadt (Germany)
Academia Sinica, Taipei (Taiwan); National Center for Theoretical Sciences, Hsinchu (Taiwan)
GSI Helmholtzzentrum für Schwerioneneforschung, Darmstadt (Germany)
Univ. of Minnesota, Minneapolis, MN (United States)

In this work, we investigate the impact of charged-current–neutrino processes on the formation and evolution of neutrino spectra during the deleptonization of proto-neutron stars. To this end we develop the full kinematics of these reaction rates consistent with the nuclear equation of state, including weak magnetism contributions. This allows us to systematically study the impact of inelastic contributions and weak magnetism on the $$ν_e$$ and $$\bar{ν}_e$$ luminosities and average energies. Furthermore, we explore the role of the inverse neutron decay, also known as the direct Urca process, on the emitted spectra of $$\bar{ν}_e$$. This process is commonly considered in the cooling scenario of cold neutron stars but has so far been neglected in the evolution of hot proto-neutron stars. We find that the inverse neutron decay becomes the dominating opacity source for low-energy $$\bar{ν}_e$$. Accurate three-flavor Boltzmann neutrino transport enables us to relate the magnitude of neutrino fluxes and spectra to details of the treatment of weak processes. This allows us to quantify the corresponding impact on the conditions relevant for the nucleosynthesis in the neutrino-driven wind, which is ejected from the proto-neutron star surface during the deleptonization phase.

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Research Organization:: Univ. of Minnesota, Minneapolis, MN (United States)

Sponsoring Organization:: USDOE Office of Science (SC); National Science Centre of Poland (NCN); German Research Foundation (DFG); Taiwan Ministry of Science and Technology (MOST)

Grant/Contract Number:: FG02-87ER40328; UMO-2016/23/B/ST2/00720; 107-2119-674 M-001-038; 108-2112-M-001-010

OSTI ID:: 1800659

Alternate ID(s):: OSTI ID: 1599691

Journal Information:: Physical Review. C, Vol. 101, Issue 2; ISSN 2469-9985

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 28 works

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