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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4502
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dc.contributor.authorBhattacharjee, P-
dc.date.accessioned2009-06-01T17:29:49Z-
dc.date.available2009-06-01T17:29:49Z-
dc.date.issued1994-
dc.identifier.citationBikash Sinha, Yogendra Pathak Viyogi and Sibaji Raha., eds., Physics and Astrophysics of Quark-Gluon Plasma; proceedings of the Second International Conference held January 19 - 23, 1993, at Variable Energy Cyclotron Centre, Calcutta, India., pp. 231 - 240en
dc.identifier.isbn981-02-1660-2-
dc.identifier.urihttp://hdl.handle.net/2248/4502-
dc.descriptionRestricted Access-
dc.description.abstractThe question of survivability of quark nuggets against the process of baryon evaporation from their surfaces is discussed within the context of a dynamical model, namely, the chromoelectric flux-tube fission model of baryan formation and evaporation. Depending on the temperature at which nuggets are formed in the early universe and the value of the bag constant B, our conservative estimates (we overestimate the baryan evaporation rate) show that quark nuggets with initial baryan number~ 10/sup 44 or more can survive the evaporation process and be present in the universe today.en
dc.language.isoenen
dc.publisherWorld Scientific-
dc.rights© World Scientific-
dc.subjectQuark Nuggetsen
dc.subjectBaryon Evaporationen
dc.subjectDynamical Modelen
dc.subjectChromoelectric Flux-Tube Fission Modelen
dc.subjectCosmological Quark Nuggetsen
dc.titleOn the survivability of cosmological quark nuggetsen
dc.typeArticleen
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