Stability of extended scalar diquark stars vis-à-vis soliton stars

Details Stability of extended scalar diquark stars vis-à-vis soliton stars Stability of extended scalar diquark stars vis-à-vis soliton stars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003prama..60..461k&link_type=abstract

Pramana, vol. 60, Issue 3, p.461

Physics

3

Stability Of Stars, Diquark Gluon Plasma, Scalar Diquark, Diquark Stars, Soliton Stars, \Phi^4-Theory.

Scientific paper

Motivated by relatively large values of the maximum mass (M = 8.92M_{odot}) and radius (R = 50.7 km) obtained for an extended scalar diquark star within the framework of an effective phi^4-theory (S K Karn et al [1]) some interesting observations are made with regard to the stability of stellar objects describable in general in terms of the polynomial field theories.

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