Baryon-number inhomogeneity generation in the cosmic quark-hadron phase transition

1988 ◽  
Vol 37 (8) ◽  
pp. 2104-2110 ◽  
Author(s):  
Hannu Kurki-Suonio
1994 ◽  
Vol 49 (8) ◽  
pp. 4023-4027 ◽  
Author(s):  
C. P. Singh ◽  
B. K. Patra ◽  
Saeed Uddin

2014 ◽  
Vol 29 (23) ◽  
pp. 1430024 ◽  
Author(s):  
Bikash Sinha

It is entirely plausible under reasonable conditions, that a first-order QCD phase transition occurred from quarks to hadrons when the universe was about a microsecond old. Relics, if there be any, after the quark–hadron phase transition are the most deciding signatures of the phase transition. It is shown in this paper that quark nuggets, the possible relics of first-order QCD phase transitions with baryon number larger than 1043 will survive the entire history of the universe up to now and can be considered as a candidate for the cold dark matter. The spin down core of the neutron star on the high density low temperature end of the QCD phase diagram initiates transition from hadrons to quarks. As the star spins down, the size of the core goes on increasing. Recently discovered massive Pulsar PSRJ 1614-2230 with a mass of 1.97 ± 0.04M⊙ most likely has a strongly interacting core. What possible observables can there be from these neutron stars?


1990 ◽  
Vol 42 (12) ◽  
pp. 3963-3968 ◽  
Author(s):  
Kohsuke Sumiyoshi ◽  
Toshitaka Kajino ◽  
Charles R. Alcock ◽  
Grant 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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