Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Effects of self-gravity of the accretion disk around rapidly rotating
  black hole in long GRBs   We prescribe a method to study the effects of self-gravity of accretion disk
around a black hole associated with long Gamma Ray Bursts (GRBs) in an evolving
background Kerr metric. This is an extension to our previous work where we
presented possible constraints for the final masses and spins of these
astrophysical black holes. Incorporating the self-force of the accreting cloud
around the black hole is a very important aspect due to the transient nature of
the event, in which a huge amount of mass is accreted and changes the
fundamental black hole parameters i.e. its mass and spin, during the process.
Understanding of the GRBs engine is important because they are possible sources
of high-energy particles and gravitational waves as most of the energy released
from the dynamical evolution is in the form of gravitational radiation. Here,
we describe the analytical framework we developed to employ in our numerical
model. The numerical studies are planned for the future work.

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The categories of this paper are: cmp-lg
12
The categories of this paper are: nucl-th
19
The categories of this paper are: eess
22
The categories of this paper are: chao-dyn
8
The categories of this paper are: hep-ex
28
The categories of this paper are: alg-geom
2
The categories of this paper are: math
0
The categories of this paper are: hep-ph
27
The categories of this paper are: comp-gas
35
The categories of this paper are: mtrl-th
37
The categories of this paper are: supr-con
33
The categories of this paper are: plasm-ph
32
The categories of this paper are: atom-ph
3
The categories of this paper are: physics
9
The categories of this paper are: nlin
21
The categories of this paper are: adap-org