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2020

Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity

Rest-mass density in units of g=cm<sup>3</sup>, temperature (kT) in units of MeV, specific entropy per baryon in units of k, and electron fraction Y<sub>e</sub> for model K8. The rest-mass density, the value of Y<sub>e</sub>, and the temperature of the  atmosphere artificially added are ≈10 g=cm<sup>3</sup>, 0.5, and ≈0.036 MeV=k, respectively.
© S. Fujibayashi (Max-Planck-Institut für Gravitationsphysik), M. Shibata (Max-Planck-Institut für Gravitationsphysik & Yukawa Institute for Theoretical Physics, Kyoto University)

Viscous evolution of disks for Mdisk = 0.1 M⊙

Rest-mass density in units of g=cm3, temperature (kT) in units of MeV, specific entropy per baryon in units of k, and electron fraction Ye for model K8. The rest-mass density, the value of Ye, and the temperature of the  atmosphere artificially added are ≈10 g=cm3, 0.5, and ≈0.036 MeV=k, respectively.

Publication:

1.
DOI
S. Fujibayashi, M. Shibata, S. Wanajo, K. Kiuchi, K. Kyutoku, and Y. Sekiguchi
Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity
Physical Review D 101, 083029 (2020)
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