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A&A 440, L33-L36 (2005)
DOI: 10.1051/0004-6361:200500161
Letter
Newtonian and general relativistic contribution of gravity to surface tension of strange stars
M. Bagchi1, M. Sinha1, M. Dey1, J. Dey1 and S. Bhowmick21 Dept. of Physics, Presidency College, 86/1 College Street, Kolkata 700 073, India
e-mail: mnj2003@vsnl.net; kamal1@vsnl.com; deyjm@giascl101.vsnl.net.in
2 Department of Physics, Barasat Govt. College, Barasat, North 24 Parganas, W. Bengal, India
(Received 1 June 2005 / Accepted 23 July 2005)
Abstract
Surface tension (S) is due to the inward force
experienced by particles at the surface and usually gravitation
does not play an important role in this force. But in compact
stars the gravitational force on the particles is very large and S
is found to depend not only on the interactions in the strange
quark matter, but also on the structure of the star, i.e. on its
mass and radius.
Key words: X-rays: binaries -- stars: fundamental parameters -- relativity -- waves -- dense matter -- equation of state -- gravitation
SIMBAD Objects
© ESO 2005
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