Spacetime Foam and Dark Energy

dc.creatorNg, Y. Jack
dc.date2008-08-08
dc.date.accessioned2026-07-07T13:10:17Z
dc.date.available2026-07-07T13:10:17Z
dc.descriptionDue to quantum fluctuations, spacetime is foamy on small scales. The degree of foaminess is found to be consistent with the holographic principle. One way to detect spacetime foam is to look for halos in the images of distant quasars. Applying the holographic foam model to cosmology we "predict" that the cosmic energy density takes on the critical value; and basing only on existing archived data on active galactic nuclei from the Hubble Space Telescope, we also "predict" the existence of dark energy which, we argue, is composed of an enormous number of inert "particles" of extremely long wavelength. We speculate that these "particles" obey infinite statistics.
dc.description6 pages, LaTeX, talk given at the Fourth International Workshop on the Dark Side of the Universe in Cairo (June 1-5, 2008), to appear in the Proceedings
dc.identifierhttps://arxiv.org/abs/0808.1261
dc.identifierhttp://arxiv.org/abs/0808.1261
dc.identifierAIP Conf.Proc.1115:74-79,2009
dc.identifierdoi:10.1063/1.3131531
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228972
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.subjectQuantum Physics
dc.titleSpacetime Foam and Dark Energy
dc.typetext

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