UDC 53
UDC 520
UDC 521
UDC 523
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
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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