Bare Strange Stars Might Not Be Bare
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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.
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Cite this article:
XU Ren-xin, QIAO Guo-jun. Bare Strange Stars Might Not Be Bare[J]. Chin. Phys. Lett., 1998, 15(12): 934-936.
XU Ren-xin, QIAO Guo-jun. Bare Strange Stars Might Not Be Bare[J]. Chin. Phys. Lett., 1998, 15(12): 934-936.
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XU Ren-xin, QIAO Guo-jun. Bare Strange Stars Might Not Be Bare[J]. Chin. Phys. Lett., 1998, 15(12): 934-936.
XU Ren-xin, QIAO Guo-jun. Bare Strange Stars Might Not Be Bare[J]. Chin. Phys. Lett., 1998, 15(12): 934-936.
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