Abstract:
Detailed study of relativistic jets around black hole sources, such as
microquasars and active galactic nuclei (AGNs) is carried out and
the impact of radiation and thermal driving is investigated. Across
the chapters, the analysis is done in various regimes, flat space-time
to curved space-time, fixed to variable adiabatic index relativistic
equation of state, radial to non radial cross section of the jet, Thom-
son (elastic) scattering to Compton scattering regime etc.
Accretion disc plays auxiliary role for generating radiation field, as
well as, geometrically shaping the jet near its base. The disc ra-
diates through thermal, bremsstrahlung, synchrotron and inverse
Compton processes. Jets are taken to be non rotating and axis-
symmetric. Further, relativistic equation of state is used that takes
care of variable adiabatic index at relativistic temperatures, as well
as, composition of the flow. The radiative moments are calculated
using their full relativistic transformations. Bending of photon path
is also considered.
