Chiral magnetohydrodynamic turbulence in core-collapse supernovae

Youhei Masada, Kei Kotake, Tomoya Takiwaki, Naoki Yamamoto

研究成果: Article査読

25 被引用数 (Scopus)

抄録

Macroscopic evolution of relativistic charged matter with chirality imbalance is described by the chiral magnetohydrodynamics (chiral MHD). One such astrophysical system is high-density lepton matter in core-collapse supernovae where the chirality imbalance of leptons is generated by the parity-violating weak processes. After developing the chiral MHD equations for this system, we perform numerical simulations for the real-time evolutions of magnetic and flow fields and study the properties of the chiral MHD turbulence. In particular, we observe the inverse cascade of the magnetic energy and the fluid kinetic energy. Our results suggest that the chiral effects that have been neglected so far can reverse the turbulent cascade direction from direct to inverse cascade, which would impact the magnetohydrodynamics evolution in the supernova core toward explosion.

本文言語English
論文番号083018
ジャーナルPhysical Review D
98
8
DOI
出版ステータスPublished - 2018 10月 15

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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