Holography stabilizes the vacuum energy
From MaRDI portal
Publication:2837636
DOI10.1103/PHYSREVLETT.89.081301zbMATH Open1267.83044arXivhep-th/0010145OpenAlexW2035116110WikidataQ64947621 ScholiaQ64947621MaRDI QIDQ2837636
Author name not available (Why is that?)
Publication date: 11 July 2013
Published in: (Search for Journal in Brave)
Abstract: Gravitational holography is argued to render the cosmological constant stable against divergent quantum corrections. This provides a technically natural solution to the cosmological constant problem. Evidence for quantum stability of the cosmological constant is illustrated in a number of examples including, bulk descriptions in terms of delocalized degrees of freedom, boundary screen descriptions on stretched horizons, and non-supersymmetric conformal field theories as dual descriptions of anti-de Sitter space. In an expanding universe, holographic quantum contributions to the stress-energy tensor are argued to be at most of order the energy density of the dominant matter component.
Full work available at URL: https://arxiv.org/abs/hep-th/0010145
No records found.
This page was built for publication: Holography stabilizes the vacuum energy
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q2837636)
