Neutron star: from the extreme turbulence of supernova outburst to the reference regularity of coherent pulsar radiation

Precise measurements of the second derivative of the rotation period according to the observed long-period second pulsars allow revealing a correlation between the period and the derivatives in a braking index n = 2 - PP''/P'², which indicates a coherence of pulse radiation of a monotonous decelerating neutron star. The braking index value n = -(0,9 ± 0,2), which also extends to millisecond pulsars, allows making a conclusion about the coherence origin at the stage of a neutron star formation along with the stellar core collapse during the supernova outburst. Deceleration of a neutron star expressed by the derivatives of a rotation period at the epoch of the outburst is interpreted as the result of magnetic induction interaction between a supernova magnetic field and circum stellar electron-positron plasma through the open field lines. The paper discusses the magnetic induction braking mechanism of neutron stars. It presents a comparative analysis of the matched rotation parameters of the second and millisecond pulsars, which create two disjoint clusters during the neutron stars evolution.

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