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• W2149409449 abstract "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." @default.
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• W2149409449 date "2011-11-15" @default.
• W2149409449 modified "2023-10-01" @default.
• W2149409449 title "Spin down of rotating compact magnetized strange stars in general relativity" @default.
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• W2149409449 doi "https://doi.org/10.1007/s10509-011-0912-6" @default.
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