Doubly Special Relativity as a Limit of Gravity

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dc.creatorImilkowska, Katarzyna
dc.creatorKowalski-Glikman, Jerzy
dc.date2005-06-15
dc.date2005-06-17
dc.date.accessioned2026-07-07T10:28:10Z
dc.date.available2026-07-07T10:28:10Z
dc.descriptionDoubly Special Relativity (DSR) is a theory with two observer-independent scales, of velocity and mass, which is expected to replace Special Relativity at ultra-high energies. In these notes we first discuss the postulates of DSR, and then turn to presenting arguments supporting the hypothesis that DSR can be regarded as a flat space, semiclassical limit of gravity. The notes are based on the talk presented at the conference ``Special Relativity -- Will it Survive the Next 100 Years?''
dc.description26 pages, Submitted to Lecture Notes in Physics
dc.identifierhttps://arxiv.org/abs/gr-qc/0506084
dc.identifierhttp://arxiv.org/abs/gr-qc/0506084
dc.identifierLect.NotesPhys.702:279-298,2006
dc.identifierdoi:10.1007/3-540-34523-X_10
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177358
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDoubly Special Relativity as a Limit of Gravity
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