scholarly journals Temporal evolution of tubular initial conditions and their influence on two-particle correlations in relativistic nuclear collisions

2012 ◽  
Vol 712 (3) ◽  
pp. 226-230 ◽  
Author(s):  
R.P.G. Andrade ◽  
F. Grassi ◽  
Y. Hama ◽  
W.-L. Qian
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.


1997 ◽  
Vol 55 (2) ◽  
pp. 874-881 ◽  
Author(s):  
Henning Heiselberg ◽  
Axel P. Vischer

Symmetry ◽  
2021 ◽  
Vol 13 (8) ◽  
pp. 1358
Author(s):  
Yiannis Contoyiannis ◽  
Michael P. Hanias ◽  
Pericles Papadopoulos ◽  
Stavros G. Stavrinides ◽  
Myron Kampitakis ◽  
...  

This paper presents our study of the presence of the unstable critical point in spontaneous symmetry breaking (SSB) in the framework of Ginzburg–Landau (G-L) free energy. Through a 3D Ising spin lattice simulation, we found a zone of hysteresis where the unstable critical point continued to exist, despite the system having entered the broken symmetry phase. Within the hysteresis zone, the presence of the kink–antikink SSB solitons expands and, therefore, these can be observed. In scalar field theories, such as Higgs fields, the mass of this soliton inside the hysteresis zone could behave as a tachyon mass, namely as an imaginary quantity. Due to the fact that groups Ζ(2) and SU(2) belong to the same universality class, one expects that, in future experiments of ultra-relativistic nuclear collisions, in addition to the expected bosons condensations, structures of tachyon fields could appear.


1980 ◽  
Vol 21 (4) ◽  
pp. 1321-1343 ◽  
Author(s):  
A. Sandoval ◽  
H. H. Gutbrod ◽  
W. G. Meyer ◽  
R. Stock ◽  
Ch. Lukner ◽  
...  

2013 ◽  
Vol 719 (4-5) ◽  
pp. 394-398 ◽  
Author(s):  
Jürgen Schukraft ◽  
Anthony Timmins ◽  
Sergei A. Voloshin

1980 ◽  
Vol 295 (4) ◽  
pp. 401-402 ◽  
Author(s):  
H. St�cker ◽  
G. Graebner ◽  
J. A. Maruhn ◽  
W. Greiner

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