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SPIN EVOLUTION OF ISOLATED NEUTRON STARS:
SPINDOWN THEOREM.
V.M.Lipunov and S.B.Popov
Department of Physics, Moscow University,
119899, Moscow, Russia
Sternberg Astronomical Institute,
Universitetsky pr. 13, Moscow, Russia
In this article we give detail consideration of the possible scenario of evolution of isolated neutron stars (INS's).
The new points of our consideration:
-we give additional arguments for the short time scale of the Ejector stage ( yrs ).
-we proposed specific SPINDOWN THEOREM and give some arguments for its validity. Discovery of accreting INS's will means that SPINDOWN THEOREM is true.
-we consider firstly evolution of spin period of a NS on the accretion stage and predict that its period sec and INS's can be observed as pulsating X-ray sources.
-we consider new idea of stochastic acceleration of the very old NS's due to accretion of turbulizated interstellar medium.
-last point means that INS can be spin up and spin down with equal probability.