논문 상세보기

THREE-DIMENSIONAL SIMULATION OF A ROTATING CORE-COLLAPSE SUPERNOVA KCI 등재

  • 언어ENG
  • URLhttps://db.koreascholar.com/Article/Detail/385673
구독 기관 인증 시 무료 이용이 가능합니다. 3,000원
천문학논총 (Publications of the Korean Astronomical Society)
한국천문학회 (Korean Astronomical Society)
초록

Multi-dimensionality in the inner working of core-collapse supernovae has long been considered one of the most important ingredients to understand the explosion mechanism. We perform a series of numerical experiments to explore how rotation impacts the 3-dimensional hydrodynamics of core-collapse supernova. We employ a light-bulb scheme to trigger explosions and a three-species neutrino leakage scheme to treat deleptonization effects and neutrino losses from the neutron star interior. We find that the rotation can help the onset of neutrino-driven explosions for models in which the initial angular momentum is matched to that obtained from recent stellar evolutionary calculations (~ 0:3 - 3 rad s-1 at the center). For models with larger initial angular momenta, a shock surface deforms to be oblate due to larger centrifugal force. This makes a gain region, in which matter gains energy from neutrinos, more concentrated around the equatorial plane. As a result, the preferred direction of the explosion in 3-dimensional rotating models is perpendicular to the spin axis, which is in sharp contrast to the polar explosions around the axis that are often obtained from 2-dimensional simulations.

목차
ABSTRACT
1. INTRODUCTION
2. RESULTS
3. CONCLUSIONS
REFERENCES
저자
  • Ko Nakamura(Faculty of Science and Engineering, Waseda University)
  • Takami Kuroda(Department of Physics, University of Basel)
  • Tomoya Takiwaki(National Astronomical Observatory of Japan/RIKEN)
  • Kei Kotake(National Astronomical Observatory of Japan/Department of Applied Physics, Fukuoka University)