Spin Down of Rotating Compact Magnetized Strange Stars in General Relativity

Details Spin Down of Rotating Compact Magnetized Strange Stars in General Relativity Spin Down of Rotating Compact Magnetized Strange Stars in General Relativity

2011-10-30

arxiv.org/abs/1110.6586v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

6 pages; Accepted for publication in Astrophysics and Space Science

Scientific paper

We find that in general relativity slow down of the pulsar rotation due to the magnetodipolar radiation is more faster for the strange star with comparison to that for the neutron star of the same mass. Comparison with astrophysical observations on pulsars spindown data may provide an evidence for the strange star existence and, thus, serve as a test for distinguishing it from the neutron star.

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