Charged particle spectra in16O induced nuclear collisions at the CERN SPS

1988 ◽  
Vol 38 (1-2) ◽  
pp. 51-57 ◽  
Author(s):  
◽  
R. Albrecht ◽  
T. C. Awes ◽  
C. Baktash ◽  
P. Beckmann ◽  
...  
1998 ◽  
Vol 57 (5) ◽  
pp. 2536-2546 ◽  
Author(s):  
H. W. Barz ◽  
J. P. Bondorf ◽  
J. J. Gaardhøje ◽  
H. Heiselberg

2019 ◽  
Vol 1258 ◽  
pp. 012010
Author(s):  
M. Ayaz Ahmad ◽  
Jalal Hasan Baker ◽  
Mir Hashim Rasool ◽  
Shafiq Ahmad ◽  
R. Dobra ◽  
...  

2002 ◽  
Vol 66 (1) ◽  
Author(s):  
Q. H. Zhang ◽  
V. Topor Pop ◽  
S. Jeon ◽  
C. Gale

2010 ◽  
Vol 686 (2-3) ◽  
pp. 152-161 ◽  
Author(s):  
N.-E. Bomark ◽  
S. Lola ◽  
P. Osland ◽  
A.R. Raklev

2007 ◽  
Vol 16 (07n08) ◽  
pp. 1790-1799 ◽  
Author(s):  
ALEXANDRU JIPA ◽  
CĂLIN BEŞLIU ◽  
ION SORIN ZGURĂ ◽  
OANA RISTEA ◽  
CĂTĂLIN RISTEA ◽  
...  

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.


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