Van der Waals Plasma Universe During Reissner-Nordstrom Expansion

ORAL

Abstract

A two-component gas, consisting of ultra-relativistic ``normal'' particles with specific charge~$q$/$m$ and ``unusual'' particles with ultra-high charge $Q$ and ultra-high mass $M $described by a Reissner--Nordstr\"{o}m metric, is conceived as a van der Waals gas model of a plasma in early Universe. The model gives rise to an expansion process, Reissner-Nordstrom Expansion, that is analogues to a cosmic expansion during the radiation-dominated era. The Reissner-Nordstrom Expansion is due to the presence of a region with ``gravitational repulsion'' of the Reissner--Nordstr\"{o}m metric with respect to the ``normal'' particles with \textit{sign}($Q)q$/$m \ge -$1. The expansion era naturally ends at recombination. We discuss the equation of state of the two-component van der Waals gas and the range of model parameters within which the proposed expansion process is consistent with the restrictions regarding quantum effects.

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Authors

  • Vesselin Gueorguiev

    Cal State Univ-Stanislaus

  • V.V. Shlyaptseva

    California State University, Dominguez Hills, Univ of California - Irvine, University of Chicago, UC Merced, NINT, Dublin Institute of Technology, Ireland, MIT, NASA/GSFC, CRESST/UMBC \& NASA/GSFC, LLNL, MPI for Plasma Physics, Remeis-Sternwarte/ECAP/FAU, Humboldt State University, University of Nevada Reno, The University of Michigan, University of Nevada, Reno, Lawrence Livermore National Laboratory, Sandia National Laboratories, Los Alamos National Laboratory, Laboratory for Laser Energetics, University of Rochester, Univ of Nevada - Reno, University of Nevada, Reno - Physics Department, Jilin University, China, Department of Physics, University of California, Berkeley, Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Advanced Materials Laboratory, National Institute for Materials Science, Department of Physics \& Astronomy, California State University, Long Beach, CA 90840, UC Santa Barbara, Department of Physics and Astronomy, University of California, Riverside, University of California at Merced, Laboratoire de Physique des Plasmas (CNRS/Ecole Polytechnique/UPMC/Universit\'e Paris Sud), Ecole Polytechnique, 91128 Palaiseau, France, University of Nevada, Reno, NV 89557, USA, University of Nevada, Reno, NV 89557 USA, University of Nevada-Reno

  • V.V. Shlyaptseva

    California State University, Dominguez Hills, Univ of California - Irvine, University of Chicago, UC Merced, NINT, Dublin Institute of Technology, Ireland, MIT, NASA/GSFC, CRESST/UMBC \& NASA/GSFC, LLNL, MPI for Plasma Physics, Remeis-Sternwarte/ECAP/FAU, Humboldt State University, University of Nevada Reno, The University of Michigan, University of Nevada, Reno, Lawrence Livermore National Laboratory, Sandia National Laboratories, Los Alamos National Laboratory, Laboratory for Laser Energetics, University of Rochester, Univ of Nevada - Reno, University of Nevada, Reno - Physics Department, Jilin University, China, Department of Physics, University of California, Berkeley, Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Advanced Materials Laboratory, National Institute for Materials Science, Department of Physics \& Astronomy, California State University, Long Beach, CA 90840, UC Santa Barbara, Department of Physics and Astronomy, University of California, Riverside, University of California at Merced, Laboratoire de Physique des Plasmas (CNRS/Ecole Polytechnique/UPMC/Universit\'e Paris Sud), Ecole Polytechnique, 91128 Palaiseau, France, University of Nevada, Reno, NV 89557, USA, University of Nevada, Reno, NV 89557 USA, University of Nevada-Reno