Speaker
Dr
Miljenko Cemeljic
(SGMK, CAMK & ASIAA)
Description
We perform the first numerical simulations of a thin accretion disc in pseudo-potential for Reissner-Nordstrom naked singularity. The obtained results share the positions of the zero gravity sphere and maximal rotational velocity with the analytical solutions and the general relativistic simulations. They also show the characteristic shape of the
innermost part of the disc, matching the analytical solutions.
Primary author
Dr
Miljenko Cemeljic
(SGMK, CAMK & ASIAA)