High energy effects on D-brane and black hole emission rates

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dc.contributor.authorDas, Saurya
dc.contributor.authorDasgupta, Arundhati
dc.contributor.authorSarkar, Tapobrata
dc.date.accessioned2016-04-06T22:45:58Z
dc.date.available2016-04-06T22:45:58Z
dc.date.issued1997
dc.descriptionSherpa Romeo green journal. Permission to archive final published version.en_US
dc.description.abstractWe study the emission of scalar particles from a class of near-extremal five-dimensional black holes and the corresponding D-brane configuration at high energies. We show that the distribution functions and the black hole greybody factors are modified in the high energy tail of the Hawking spectrum in such a way that the emission rates exactly match. We extend the results to charged scalar emission and to four dimensions.en_US
dc.description.peer-reviewYesen_US
dc.identifier.citationDas, S., Dasgupta, A., & Sarkar, T. (1997). High energy effects on D-brane and black hole emission rates. Physical Review D, 55(12), 7693-7700. http://dx.doi.org/10.1103/PhysRevD.55.7693en_US
dc.identifier.urihttps://hdl.handle.net/10133/4460
dc.language.isoen_CAen_US
dc.publisherAmerican Physical Societyen_US
dc.publisher.facultyArts and Scienceen_US
dc.publisher.institutionInstitute of Mathematical Sciences (India)en_US
dc.publisher.urlhttps://doi.org/10.1103/PhysRevD.55.7693
dc.subjectD-branesen_US
dc.subjectBlack holesen_US
dc.subjectHigh energyen_US
dc.subjectEmission ratesen_US
dc.titleHigh energy effects on D-brane and black hole emission ratesen_US
dc.typeArticleen_US
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