Add to ORKGThe abundance and size distribution of quark nuggets (QN), formed a few microseconds after the big bang due to first order QCD phase transition in the early universe, has been estimated. It appears that stable QNs could be a viable candidate for cosmological dark matter. The evolution of baryon inhomogeneity due to evaporated (unstable) QNs are also examined
False vacuum remnants in first-order phase transitions in the early Universe can form compact objec...
During its hot, dense, early evolution the Universe was a primordial nuclear reactor, synthesizing t...
The possible role of a first order QCD phase transition at nonvanishing quark chemical potential and...
We calculate the size distribution of quark nuggets, which could be formed due to first order QCD ph...
A QCD phase transition in the early universe could have left inhomogeneities in the baryon to photon...
We study the quark-hadron phase transition in the early Universe and the effect of baryon density in...
In the standard hot big bang theory, when the Universe was about 1-10μs old, the cosmological matter...
Borghini N, Cottingham WN, Mau RV. Possible cosmological implications of the quark-hadron phase tran...
Strange quark nuggets (SQNs) could be the relics of the cosmological QCD phase transition, and they ...
The modern phase diagram of strongly interacting matter reveals a rich structure at high-densities ...
We study the quark-hadron transition in the early Universe and compute the amplitude of isothermal b...
A first-order phase transition is likely to have occurred in the early universe at the end of the qu...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
In this paper we consider the Universe at the late stage of its evolution and deep inside the cell o...
We consider the formation of horizon-size primordial black holes (PBH's) from pre-existing density f...
False vacuum remnants in first-order phase transitions in the early Universe can form compact objec...
During its hot, dense, early evolution the Universe was a primordial nuclear reactor, synthesizing t...
The possible role of a first order QCD phase transition at nonvanishing quark chemical potential and...
We calculate the size distribution of quark nuggets, which could be formed due to first order QCD ph...
A QCD phase transition in the early universe could have left inhomogeneities in the baryon to photon...
We study the quark-hadron phase transition in the early Universe and the effect of baryon density in...
In the standard hot big bang theory, when the Universe was about 1-10μs old, the cosmological matter...
Borghini N, Cottingham WN, Mau RV. Possible cosmological implications of the quark-hadron phase tran...
Strange quark nuggets (SQNs) could be the relics of the cosmological QCD phase transition, and they ...
The modern phase diagram of strongly interacting matter reveals a rich structure at high-densities ...
We study the quark-hadron transition in the early Universe and compute the amplitude of isothermal b...
A first-order phase transition is likely to have occurred in the early universe at the end of the qu...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
In this paper we consider the Universe at the late stage of its evolution and deep inside the cell o...
We consider the formation of horizon-size primordial black holes (PBH's) from pre-existing density f...
False vacuum remnants in first-order phase transitions in the early Universe can form compact objec...
During its hot, dense, early evolution the Universe was a primordial nuclear reactor, synthesizing t...
The possible role of a first order QCD phase transition at nonvanishing quark chemical potential and...