Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: How is Binary Radio-Pulsars with Black Holes Population Rich?   Using "Scenario Machine" we have carried out population synthesis of radio
pulsar with black hole binaries (BH+Psr) in context of the most wide
assumptions about star mass loss during evolution, binary stars mass ratio
distribution, kick velocity and envelope mass lost during collapse. Our purpose
is to display that under any suppositional parameters of evolution scenario
BH+Psr population have to be abundant in Galaxy. It is shown that in the all
models including models evolved by Heger et al. (2002), Woosley et al. (2002),
Heger et al. (2003) expected number of the black holes paired with radio
pulsars is sufficient enough to discover such systems within the next few
years.

34
The categories of this paper are: chem-ph
9
The categories of this paper are: nlin
27
The categories of this paper are: comp-gas
26
The categories of this paper are: bayes-an
18
The categories of this paper are: econ
5
The categories of this paper are: gr-qc
7
The categories of this paper are: hep-th
17
The categories of this paper are: q-fin
32
The categories of this paper are: atom-ph
12
The categories of this paper are: nucl-th
35
The categories of this paper are: mtrl-th
28
The categories of this paper are: alg-geom
29
The categories of this paper are: funct-an
15
The categories of this paper are: nucl-ex
19
The categories of this paper are: eess
22
The categories of this paper are: chao-dyn