The circular loop equation of a cosmic string with time-varying tension in de Sitter spacetimes

dc.creatorLiu, Yunqi
dc.creatorCheng, Hongbo
dc.date2008-01-30
dc.date2008-03-13
dc.date.accessioned2026-07-07T12:55:02Z
dc.date.available2026-07-07T12:55:02Z
dc.descriptionIn this work the equation of circular loops of cosmic string possessing time-dependent tension is studied in the de Sitter spacetime. We find that the cosmic string loops with initial radius $r(t_{0})>0.707L$, L de Sitter radius, should not collapse to form a black holes. It is also found that in the case of $r(t_{0})<0.707L$ a loop of cosmic string whose tension depends on some power of cosmic time can not become a black hole if the power is lower than a critical value which is associated with the initial size of the loop.
dc.description6 pages
dc.identifierhttps://arxiv.org/abs/0801.4615
dc.identifierhttp://arxiv.org/abs/0801.4615
dc.identifierInt.J.Theor.Phys.48:1070-1075,2009
dc.identifierdoi:10.1007/s10773-008-9879-7
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224140
dc.subjectHigh Energy Physics - Theory
dc.titleThe circular loop equation of a cosmic string with time-varying tension in de Sitter spacetimes
dc.typetext

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