53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
The influence of space curvature on the input of pulsar magnetic field outside star to effective moment of inertia of neutron star and its influence on pulsar braking indexes is considered. It is shown that it leads to the changing of braking indexes estimates only in two or ten times. So a majority of pulsar braking indexes may be explained by a simple model of neutron star precessed due to its anomalous torque as well as without taking into account the space curvature influence nearby neutron star.
stars: neutron; stars: magnetic field
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