Sigma model Q-balls and Q-stars

Yosef Verbin

نتاج البحث: نشر في مجلةمقالةمراجعة النظراء


A new kind of Q-balls is found: Q-balls in a nonlinear sigma model. Their main properties are presented together with those of their self-gravitating generalization, sigma model Q-stars. A simple special limit of solutions which are bound by gravity alone ("sigma stars") is also discussed briefly. The analysis is based on calculating the mass, global U(1) charge and binding energy for families of solutions parametrized by the central value of the scalar field. Two kinds (differing by the potential term) of the new sigma model Q-balls and Q-stars are analyzed. They are found to share some characteristics while differing in other respects like their properties for weak central scalar fields which depend strongly on the form of the potential term. They are also compared with their ordinary counterparts and although similar in some respects, significant differences are found like the existence of an upper bound on the central scalar field. A special subset of the sigma model Q-stars contains those which do not possess a flat space limit. Their relation with sigma star solutions is discussed.

اللغة الأصليةالإنجليزيّة
رقم المقال085018
دوريةPhysical Review D - Particles, Fields, Gravitation and Cosmology
مستوى الصوت76
رقم الإصدار8
المعرِّفات الرقمية للأشياء
حالة النشرنُشِر - 22 أكتوبر 2007


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