A little inflation in the early universe at the QCD phase transition

We explore a scenario that allows for a strong first order phase transition of QCD at a non-negligible baryon number in the early Universe and its possible observable consequences. The main assumption is a quasistable QCD-vacuum state that leads to a short period of inflation, consequently diluting...

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Hauptverfasser: Boeckel, Moritz Tillmann (VerfasserIn) , Schaffner-Bielich, Jürgen (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 19 July 2010
In: Physical review letters
Year: 2010, Jahrgang: 105, Heft: 4, Pages: 1-4
ISSN:1079-7114
DOI:10.1103/PhysRevLett.105.041301
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevLett.105.041301
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevLett.105.041301
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Verfasserangaben:Tillmann Boeckel and Jürgen Schaffner-Bielich

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