Fine Structure of Dark Energy and New Physics

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dc.creatorJejjala, Vishnu
dc.creatorKavic, Michael
dc.creatorMinic, Djordje
dc.date2007-05-31
dc.date2007-09-05
dc.date.accessioned2026-07-07T11:16:28Z
dc.date.available2026-07-07T11:16:28Z
dc.descriptionFollowing our recent work on the cosmological constant problem, in this letter we make a specific proposal regarding the fine structure (i.e., the spectrum) of dark energy. The proposal is motivated by a deep analogy between the blackbody radiation problem, which led to the development of quantum theory, and the cosmological constant problem, which we have recently argued calls for a conceptual extension of the quantum theory. We argue that the fine structure of dark energy is governed by a Wien distribution, indicating its dual quantum and classical nature. We discuss a few observational consequences of such a picture of dark energy.
dc.description14 pages, LaTeX, typos fixed, comments, references, and footnotes added, Sec. 4 revised
dc.identifierhttps://arxiv.org/abs/0705.4581
dc.identifierhttp://arxiv.org/abs/0705.4581
dc.identifierAdv.HighEnergyPhys.2007:21586,2007
dc.identifierdoi:10.1155/2007/21586
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192683
dc.subjectHigh Energy Physics - Theory
dc.titleFine Structure of Dark Energy and New Physics
dc.typetext

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