The Quark-Hadron Phase Transition and Primordial Nucleosynthesis

1987 ◽  
pp. 378-387
Author(s):  
Craig J. Hogan
1989 ◽  
Vol 8 ◽  
pp. 693-696
Author(s):  
Hubert Reeves

Important progresses have been made in two fronts in the few past years.On the theoretical ground, we have realized the importance of the quark-hadron phase transition as possibly influencing in a major way the yields of die primordial nucleosynthesis isotopes.On the observational ground, the status of lithium as a bona-fide cosmological observable has been confirmed and its primordial abundance can be evaluated with increased confidence.


1987 ◽  
Vol 320 ◽  
pp. 439 ◽  
Author(s):  
C. Alcock ◽  
G. M. Fuller ◽  
G. J. Mathews

2016 ◽  
pp. 4115-4125
Author(s):  
Argha Deb

The event-by-event fluctuation of hadronic patterns is investigated by finding a measure of the non-hadronic regions, the voids, for the experimental data of p-AgBr interactions at 400 GeV/c considering the anisotropy of phase space. Two moments of the event-to-event fluctuation of voids, <Gq> and Sq have been calculated as defined by R. C. Hwa and Q. H. Zhang to quantify the dependence of the voids on the bin sizes. The results suggest that no quark-hadron phase transition of second order have taken place for p-AgBr interactions at 400 GeV/c. The result have been compared with the result of VENUS generated data.


2005 ◽  
Vol 71 (4) ◽  
Author(s):  
Abhijit Bhattacharyya ◽  
Sanjay K. Ghosh ◽  
Matthias Hanauske ◽  
Sibaji Raha

2017 ◽  
Vol 45 ◽  
pp. 1760059
Author(s):  
Clebson A. Graeff ◽  
Débora P. Menezes

We analyse the hadron/quark phase transition described by the Nambu-Jona-Lasinio (NJL) model [quark phase] and the extended Nambu-Jona-Lasinio model (eNJL) [hadron phase]. While the original formulation of the NJL model is not capable of describing hadronic properties due to its lack of confinement, it can be extended with a scalar-vector interaction so it exhibits this property, the so-called eNJL model. As part of this analysis, we obtain the equations of state within the SU(2) versions of both models for the hadron and the quark phases and determine the binodal surface.


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