ON A “MICROSCOPIC HUBBLE CONSTANT” FROM RELATIVISTIC NUCLEAR COLLISIONS

Author:

JIPA ALEXANDRU1,BEŞLIU CĂLIN1,ZGURĂ ION SORIN2,RISTEA OANA1,RISTEA CĂTĂLIN23,HORBUNIEV AMELIA1,ARSENE IONUţ24,ARGINTARU DĂNUŢ5,CĂLIN MARIUS1,EŞANU TIBERIU1,COVLEA VANEA1,ILIESCU BOGDAN1

Affiliation:

1. Atomic and Nuclear Physics Chair, Faculty of Physics, University of Bucharest, Romania

2. Institute of Space Sciences, Bucharest-Măgurele, Romania

3. “Niels Bohr” Institute, University of Copenhagen, Denmark

4. Physics Department, University of Oslo, Norway

5. Institute of Civilian Marine Constantza, Romania

Abstract

Similarities between cosmological scenarios on the Universe evolution after “Big Bang” and the behavior of the highly excited nuclear matter formed in relativistic nuclear collisions, immediately after collisions, are considered to do an estimation of a “microscopic Hubble parameter/constant” for the expansion rate in relativistic nuclear collisions, similar with the cosmological Hubble constant. Temporal connections between the evolution of the nuclear matter after impact and the scenarios on the Universe evolution after “Big Bang” are introduced. Experimental results on participants, fireball sizes (identical particle interferometry), densities, particle spectra and temperatures have been used. A “Hubble scale” for temporal evolution can be obtained. Satisfactory agreement with Buda-Lund model estimations has been obtained.

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Nuclear and High Energy Physics

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