Non-vanishing cosmological constant \(\Lambda\), phase transitions, and \(\Lambda\)-dependence of high energy processes

DOI10.1016/S0370-2693(02)02022-1zbMath0995.83086arXivhep-th/0203150OpenAlexW1540518897WikidataQ56624964 ScholiaQ56624964MaRDI QIDQ1601262

Freydoon Mansouri

Publication date: 25 June 2002

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0203150

zbMATH Keywords

energy scaleasymptotic space-time symmetrylocal energy-momentum tensor contribution

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (6)

De Sitter relativity: a natural scenario for an evolving \({\Lambda}\) ⋮ de Sitter-invariant special relativity and the dark energy problem ⋮ \(\Lambda\) and the Heisenberg principle ⋮ De Sitter relativity: a new road to quantum gravity? ⋮ IS PHYSICS ASKING FOR A NEW KINEMATICS? ⋮ De Sitter-invariant special relativity and galaxy rotation curves

Cites Work

• Unnamed Item
• THE STRUCTURE OF ADS BLACK HOLES AND CHERN–SIMONS THEORY IN 2 + 1 DIMENSIONS
• The cosmological constant problem
• Discrete Series for the Universal Covering Group of the 3 + 2 de Sitter Group
• Représentations intégrables du groupe de De Sitter
• SPIN ½ WAVE EQUATION IN DE-SITTER SPACE

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