Matching the observational value of the cosmological constant\(^{\star }\)

DOI10.1016/S0370-2693(01)00921-2zbMath0971.83098arXivhep-th/0007094OpenAlexW4289254347MaRDI QIDQ5942453

Emilio Elizalde

Publication date: 29 August 2001

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

Full work available at URL: https://arxiv.org/abs/hep-th/0007094

zbMATH Keywords

universeboundary condition compactificationCasimir effect

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (8)

Vacuum densities for a charged scalar field in de Sitter space-time with compact dimensions ⋮ Multi-(super)graviton theory on topologically non-trivial backgrounds ⋮ DIRICHLET CASIMIR ENERGY FOR A SCALAR FIELD IN A SPHERE: AN ALTERNATIVE METHOD ⋮ CASIMIR ENERGY, FERMION FRACTIONALIZATION AND STABILITY OF A FERMI FIELD IN AN ELECTRIC POTENTIAL IN (1+1) DIMENSIONS ⋮ Finite temperature Casimir effect in Kaluza-Klein spacetime ⋮ On gravitational Casimir effect and Stefan-Boltzmann law at finite temperature ⋮ Matching the observed cosmological constant with vacuum energy density in AdS ⋮ Revisiting vacuum energy in compact spacetimes

Cites Work

• Constraints on theories with large extra dimensions
• The neutrino problem in cosmology
• Complete determination of the singularity structure of zeta functions
• Analysis of an inhomogeneous generalized Epstein–Hurwitz zeta function with physical applications
• Ten Physical Applications of Spectral Zeta Functions
• Zeta-function regularization is uniquely defined and well
• Black hole explosions?
• The cosmological constant
• Unnamed Item

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