Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2571
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dc.contributor.authorde Sabbata, Venzo-
dc.contributor.authorSivaram, C-
dc.date.accessioned2008-07-02T07:18:53Z-
dc.date.available2008-07-02T07:18:53Z-
dc.date.issued1992-01-
dc.identifier.citationAstrophysics and Space Science , Vol. 187, No.1, pp. 149 - 154en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2571-
dc.description.abstractBy introducing torsion in general relativity - that is physically considering the effect of the spin and linking the torsion to defects in the space-time topology - a minimum unit of time can be obtained. In this context the possibility exists of identifying the defects in space-time topology induced by torsion as behaving like a string so that the minimum length, derived by treating the spin as an extra dimension, is related with string tension. Physical implications are considered for field theory (the divergence of self-energy integral is eliminated without introducing any ad hoc cut-off), particle decay, evaporation of black holes, and information theory.en
dc.format.extent502940 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1992Ap%26SS.187..149Den
dc.relation.urihttp://www.springer.com/astronomy/journal/10509en
dc.subjectCosmologyen
dc.subjectField Theory (Physics)en
dc.subjectRelativistic Theoryen
dc.subjectSpace-Time Functionsen
dc.subjectString Theoryen
dc.subjectTorsionen
dc.subjectBlack Holes (Astronomy)en
dc.subjectComputational Astrophysicsen
dc.subjectNuclear Astrophysicsen
dc.subjectQuantum Theoryen
dc.titleTorsion, minimum time, string tension and its physical implications in cosmologyen
dc.typeArticleen
Appears in Collections:IIAP Publications

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