S E M I N A R I

Departament d'Astronomia i Astrofísica
Universitat de València

    A toy model of viscous relativistic thick disk in Schwarzschild spacetime

Sayantani Lahiri

Center of Applied Space Technology and Microgravity (ZARM), Universität Bremen, Alemanya


Seminari del departament d'Astronomia i Astrofísica

Dijous 28 febrer 2019

12:00


Resum

The aim of the work is to explore cumulative effects of the black hole curvature and the shear viscosity on a relativistic thick accretion disk. As an initial step towards this direction, we investigate how they cast their imprints and hence influence the fluid velocity profiles of a disk which can be visualized by studying corresponding isopressure surfaces.