Cosmic Acceleration from Elementary Interactions

dc.creatorAldrovandi, R.
dc.creatorCuzinatto, R. R.
dc.creatorMedeiros, L. G.
dc.date2005-12-22
dc.date.accessioned2026-07-07T06:53:58Z
dc.date.available2026-07-07T06:53:58Z
dc.descriptionIt is possible to generate an accelerated period of expansion from reasonable potentials acting between the universe particle constituents. The pressure of primordial nucleons interacting via a simple nuclear potential is obtained via Mayer's cluster expansion technique. The attractive part of the potential engenders a negative pressure and may therefore be responsible for the cosmic acceleration.
dc.description4 pages, 3 figures, 1 table
dc.identifierhttps://arxiv.org/abs/gr-qc/0512135
dc.identifierhttp://arxiv.org/abs/gr-qc/0512135
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/105781
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCosmic Acceleration from Elementary Interactions
dc.typetext

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