Spin down of rotating compact magnetized strange stars in general relativity

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 ordinary neutron star of the same mass. Comparison with astrophysical observations on pulsars spindown data may provide an evide...

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Bibliographic Details
Published in:Astrophysics and space science 2012-03, Vol.338 (1), p.157-161
Main Authors: Ahmedov, B. J., Ahmedov, B. B., Abdujabbarov, A. A.
Format: Article
Language:English
Subjects:
Astrobiology
Astronomy
Astrophysics
Astrophysics and Astroparticles
Cosmology
Magnetic fields
Observations and Techniques
Original Article
Physics
Physics and Astronomy
Pulsars
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Stars & galaxies
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Summary: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 ordinary 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.
ISSN:0004-640X
1572-946X
DOI:10.1007/s10509-011-0912-6