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Faculty of Physics |
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Fax : 972-8-9465110 Bldg.:K.B. Weissman Institute of Physical Sciences Rm.: P259 Email: fnusov@wicc.weizmann.ac.il Secretariat:
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2. A common feature of neutron stars is a very strong magnetic field at their surface, up to million billion Gauss that is about billion times more than the strength of magnetic fields generated in scientific laboratories on the Earth. We consider the properties of matter in such a strong magnetic field. 3. In 1984 Witten proposed that strange matter made of
quarks is the ground state. If this idea is true,
at least some of the compact objects known to astronomers
as radio pulsars, accreting X-ray sources, X-ray and
gamma-ray bursters, etc. might be strange-quark-matter stars,
not neutron stars as usually assumed. We study the properties of
strange-quark-matter stars. The main goal of our research is toinvestigate
the physical processes at, and radiation from, the surface of
strange-quark-matter stars, with a view to suggesting good observational
signatures that will distinguish them from neutron stars.
1. Usov V.V. Millisecond pulsars with extremely strong magnetic fields as a cosmological source of gamma-ray bursts. Nature, 357, 472, 1992 2. Smolsky M.V. and Usov V.V. Relativistic beam -- magnetic barrier collision and nonthermal radiation of cosmological gamma-ray bursters. Astrophys. J.461, 858, 1996 3. Usov V.V. Bare quark matter surfaces of strange stars
and e+e- emission. Phys. Rev.
Letters 80, 230, 1998
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