The influence of inelastic neutrino reactions with light nuclei on the standing accretion shock instability in core-collapse supernovae

Shun Furusawa, Hiroki Nagakura, Kohsuke Sumiyoshi, Shoichi Yamada

    Research output: Contribution to journalArticle

    27 Citations (Scopus)

    Abstract

    We perform numerical experiments to investigate the influence of inelastic neutrino reactions with light nuclei on the standing accretion shock instability (SASI). The time evolution of shock waves is calculated with a simple light-bulb approximation for the neutrino transport and a multi-nuclei equation of state. The neutrino absorptions and inelastic interactions with deuterons, tritons, helions, and alpha particles are taken into account in the hydrodynamical simulations. In addition, the effects of ordinary charged-current interactions with nucleons is addressed in the simulations. Axial symmetry is assumed but no equatorial symmetry is imposed. We show that the heating rates of deuterons reach as high as ∼10% of those of nucleons around the bottom of the gain region. On the other hand, alpha particles are heated near the shock wave, which is important when the shock wave expands and the density and temperature of matter become low. It is also found that the models with heating by light nuclei evolve differently in the non-linear phase of SASI than do models that lack heating by light nuclei. This result is because matter in the gain region has a varying density and temperature and therefore sub-regions appear that are locally rich in deuterons and alpha particles. Although the light nuclei are never dominant heating sources and they work favorably for shock revival in some cases and unfavorably in other cases, they are non-negligible and warrant further investigation.

    Original languageEnglish
    Article number78
    JournalAstrophysical Journal
    Volume774
    Issue number1
    DOIs
    Publication statusPublished - 2013 Sep 1

    Fingerprint

    supernovae
    neutrinos
    shock
    accretion
    shock wave
    nuclei
    alpha particles
    heating
    deuterons
    shock waves
    nucleons
    symmetry
    equation of state
    luminaires
    simulation
    equations of state
    temperature
    interactions
    approximation
    particle

    Keywords

    • equation of state
    • hydrodynamics
    • neutrinos
    • supernovae: general

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    The influence of inelastic neutrino reactions with light nuclei on the standing accretion shock instability in core-collapse supernovae. / Furusawa, Shun; Nagakura, Hiroki; Sumiyoshi, Kohsuke; Yamada, Shoichi.

    In: Astrophysical Journal, Vol. 774, No. 1, 78, 01.09.2013.

    Research output: Contribution to journalArticle

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