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===Strong force phase transition===
This conclusion assumes the simplest scenario at the time of the transition, and first- or second-order transitions are possible in the presence of a quark, baryon or neutrino [[chemical potential]], or strong magnetic fields.<ref name="Boeckel2011">{{cite journal |last1=Boeckel |first1=Tillman |last2=Schettler |first2=Simon |last3=Schaffner-Bielich |first3=Jurgen |title=The Cosmological QCD Phase Transition Revisited |journal=Prog. Part. Nucl. Phys. |date=2011 |volume=66 |issue=2 |pages=266–270 |doi=10.1016/j.ppnp.2011.01.017|arxiv=1012.3342|bibcode=2011PrPNP..66..266B |s2cid=118745752 }}</ref><ref name="Schwarz2009">{{cite journal |last1=Schwarz |first1=Dominik J. |last2=Stuke |first2=Maik |title=Lepton asymmetry and the cosmic QCD transition |journal=JCAP |date=2009 |volume=2009 |issue=11 |pages=025 |doi=10.1088/1475-7516/2009/11/025|arxiv=0906.3434|bibcode=2009JCAP...11..025S |s2cid=250761613 }}</ref><ref name="Cao2023">{{cite journal |last1=Cao |first1=Gaoging |title=First-order QCD transition in a primordial magnetic field |journal=Phys. Rev. D |date=2023 |volume=107 |issue=1 |pages=014021 |doi=10.1103/PhysRevD.107.014021|arxiv=2210.09794
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