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The maximum spin of Millisecond Pulsar and the gravitational wave

Published online by Cambridge University Press:  27 October 2016

C. M. Zhang
C. M. Zhang*
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China email: zhangcm@bao.ac.cn
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Abstract

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The gravitational wave radiation will release the energy momentum, which will dissipate the rotation of neutron star while in the accretion process. If the deformation of star is known, then we can estimate the maximum spin frequency of pulsar, based on which we can interpret why the spin periods of all millisecond pulsars cannot be less than one millisecond.

Keywords

neutron starpulsarmillisecond pulsargravitational waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 370 - 371
Copyright
Copyright © International Astronomical Union 2016 

References

Alpar, M. A., Cheng, A. F., Ruderman, M. A., & Shaham, J. 1982, Nature, 300, 728 Google Scholar
Bhattacharya, D. & van den Heuvel, E. P. J. 1991, Phys. Rep., 203, 1 CrossRefGoogle Scholar
Bildsten, L. 1998, ApJ, 501, L89 Google Scholar
Chakrabarty, D. 2005, “Millisecond Pulsars in X-Ray Binaries,” in Binary Radio Pulsars, eds. Rasio, F. A. & Stairs, I. H. (ASP: San Francisco) p. 279 Google Scholar
Ghosh, P. & Lamb, F. K. 1979, ApJ, 234, 296 Google Scholar
Wang, J., Zhang, C. M., Zhao, Y. H., et al. 2011, A&A, 526, A88 Google Scholar
Zhang, C. M. & Kojima, Y. 2006, MNRAS 366 137 (ZK06)Google Scholar