Lepton asymmetry and the cosmic QCD transition
arXiv:0906.3434 · doi:10.1088/1475-7516/2009/11/025 10.1088/1475-7516/2010/10/E01
Abstract
We study the influence of lepton asymmetry on the evolution of the early Universe. The lepton asymmetry is poorly constrained by observations and might be orders of magnitude larger than the baryon asymmetry , . We find that lepton asymmetries that are large compared to the tiny baryon asymmetry, can influence the dynamics of the QCD phase transition significantly. The cosmic trajectory in the phase diagram of strongly interacting matter becomes a function of lepton (flavour) asymmetry. Large lepton asymmetry could lead to a cosmic QCD phase transition of first order.
23 pages, 14 figures; matches published version, including Erratum. Conclusions, pictures, numerics remained unchanged
References in corpus (15)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The order of the quantum chromodynamics transition predicted by the standard model of particle physics
- Color superconductivity in dense quark matter
- The QCD transition temperature: results with physical masses in the continuum limit
- The transition temperature in QCD
- Improved Calculation of the Primordial Gravitational Wave Spectrum in the Standard Model
- Phase transitions in the early and the present Universe
- Constraining The Universal Lepton Asymmetry
- WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
- Cosmological Structure Formation Creates Large-Scale Magnetic Fields
- Transition temperature in QCD with physical light and strange quark masses
- Exploring the QCD phase diagram
- Quarks in the universe
- Can Electric Charges and Currents Survive in an Inhomogeneous Universe?
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