Quark-hadron phase transition in massive gravity
arXiv:1511.09294 · doi:10.1016/j.aop.2016.08.018
Abstract
We study the quark hadron phase transition in the framework of massive gravity. We show that the modification of the FRW cosmological equations leads to the quark hadron phase transition in the early massive Universe. Using numerical analysis, we consider that a phase transition based on the chiral symmetry breaking after the electroweak transition, occurred at approximately seconds after the Big Bang to convert a plasma of free quarks and gluons into hadrons.
13 pages, 8 figures. arXiv admin note: substantial text overlap with arXiv:0807.3066 by other authors
References in corpus (17)
- The order of the quantum chromodynamics transition predicted by the standard model of particle physics
- Resummation of Massive Gravity
- Full result for the QCD equation of state with 2+1 flavors
- The QCD transition temperature: results with physical masses in the continuum limit II.
- Equation of state and QCD transition at finite temperature
- Lattice QCD calculation of form factors describing the rare decays and
- Exact Schwarzschild-de Sitter black holes in a family of massive gravity models
- The recovery of General Relativity in massive gravity via the Vainshtein mechanism
- Lattice QCD Calculation for the Physical Equation of State
- Phase conversion in a weakly first-order quark-hadron transition
- The order, shape and critical point for the quark-gluon plasma phase transition
- Quark-Gluon Bags with Surface Tension
- The thermodynamics for a hadronic gas of fireballs with internal color structures and chiral fields
- Quark-Hadron Phase Transitions in Brane-World Cosmologies
- Mean Field Effects In The Quark-Gluon Plasma
- Quark-hadron phase transition in Brans-Dicke brane gravity
- Horava-Lifshitz cosmology, entropic interpretation and quark-hadron phase transition