Bare Strange Stars Might Not Be Bare

Chin. Phys. Lett.

1998, Vol. 15

Issue (12): 934-936 DOI:

Original Articles

Bare Strange Stars Might Not Be Bare

XU Ren-xin;QIAO Guo-jun

Department of Geophysics, Peking University, Beijing 100871, and Chinese Academy of Sciences-Peking University Joint Beijing Astrophysical Center, Beijing 100871

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XU Ren-xin, QIAO Guo-jun 1998 Chin. Phys. Lett. 15 934-936

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Abstract It is proposed that the bare strange matter stars might not be bare, and the observed pulsars might be in fact the bare strange stars. As intensely magnetized strange matter stars rotate, the induced unipolar electric fields would be large enough to construct magnetospheres. This situation is very similar to that discussed by many authors for rotating neutron stars. Also, the strange stars with accretion crusts in binaries could act as x-ray pulsars or x-ray bursters. There are some advantages if pulsars are bare strange stars.

Keywords: 97.60.Gb 97.60.Jd 97.60.Sm

Published: 01 December 1998

PACS:	97.60.Gb	(Pulsars)
	97.60.Jd	(Neutron stars)
	97.60.Sm

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y1998/V15/I12/0934

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