Next: Related Publications
Up: Astrophysical Fluid as an
Previous: Research Accomplished
We would like to extend our calculation to study the stability and non linear
behaviour in magneto-fluid, by studying the transonic properties of
the magneto hydrodynamic (MHD) accretion (initially using Newtonian/Post
Newtonian, and finally general relativistic frame work)flow onto astrophysical black hole.
By introducing an effective Lyapunov exponent, we will
investigate the chaotic behaviour in relativistic astro-fluid.
Such study will be useful to explain the variability/micro variability in AGN
spectra.
Tapas Kumar Das
2009-01-17