Parametric study of flow patterns behind the standing accretion shock wave for core-collapse supernovae

Wakana Iwakami, Hiroki Nagakura, Shoichi Yamada

Research output: Contribution to journalArticle

14 Citations (Scopus)

Abstract

In this study, we conduct three-dimensional hydrodynamic simulations systematically to investigate the flow patterns behind the accretion shock waves that are commonly formed in the post-bounce phase of core-collapse supernovae. Adding small perturbations to spherically symmetric, steady, shocked accretion flows, we compute the subsequent evolutions to find what flow pattern emerges as a consequence of hydrodynamical instabilities such as convection and standing accretion shock instability for different neutrino luminosities and mass accretion rates. Depending on these two controlling parameters, various flow patterns are indeed realized. We classify them into three basic patterns and two intermediate ones; the former includes sloshing motion (SL), spiral motion (SP), and multiple buoyant bubble formation (BB); the latter consists of spiral motion with buoyant-bubble formation (SPB) and spiral motion with pulsationally changing rotational velocities (SPP). Although the post-shock flow is highly chaotic, there is a clear trend in the pattern realization. The sloshing and spiral motions tend to be dominant for high accretion rates and low neutrino luminosities, and multiple buoyant bubbles prevail for low accretion rates and high neutrino luminosities. It is interesting that the dominant pattern is not always identical between the semi-nonlinear and nonlinear phases near the critical luminosity; the intermediate cases are realized in the latter case. Running several simulations with different random perturbations, we confirm that the realization of flow pattern is robust in most cases.

Original languageEnglish
Article number118
JournalAstrophysical Journal
Volume786
Issue number2
DOIs
Publication statusPublished - 2014 May 10

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shock wave
flow pattern
supernovae
shock waves
flow distribution
accretion
luminosity
liquid sloshing
bubble
bubbles
neutrinos
shock
perturbation
simulation
convection
hydrodynamics
trends
rate

Keywords

  • Hydrodynamics
  • Instabilities
  • Supernovae: general

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Parametric study of flow patterns behind the standing accretion shock wave for core-collapse supernovae. / Iwakami, Wakana; Nagakura, Hiroki; Yamada, Shoichi.

In: Astrophysical Journal, Vol. 786, No. 2, 118, 10.05.2014.

Research output: Contribution to journalArticle

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