Forschungsergebnisse und Animationen
2020
Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity

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.
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)