2018
DOI: 10.1016/j.physletb.2018.07.020
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“Invisible” QCD axion rolling through the QCD phase transition

Abstract: The origin of "invisible" axion in four dimensional effective beyond-standard models from string compactification is discussed and its refined passover through the QCD phase transition is presented toward a reliable estimate of the current axion energy density in terms of the initial misalignment angleθ 1 . The explicit examples are presented in a flipped SU(5) GUT model. This allows to introduce a flavor symmetry through string compactification, and hence we also comment on the source of flavor symmetries fro… Show more

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Cited by 12 publications
(12 citation statements)
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“…[120], but adopt a cosmological model, taking into a field theoretic account of 'supercooling' of the light degrees by forming bubbles in the RD universe as shown in Fig. 9, presented recently [121]. We adopt two basic principles: (i) during the first order phase transition the Gibbs free energy is conserved and (ii) the phase transition is completed into the homogenious h-phase by the time t f in the evolving Universe.…”
Section: Qcd Phase Transition In the Rd Universe And Axion Massmentioning
confidence: 99%
See 1 more Smart Citation
“…[120], but adopt a cosmological model, taking into a field theoretic account of 'supercooling' of the light degrees by forming bubbles in the RD universe as shown in Fig. 9, presented recently [121]. We adopt two basic principles: (i) during the first order phase transition the Gibbs free energy is conserved and (ii) the phase transition is completed into the homogenious h-phase by the time t f in the evolving Universe.…”
Section: Qcd Phase Transition In the Rd Universe And Axion Massmentioning
confidence: 99%
“…A view of susceptibility χ (blue curve) during the quark-hadron phase transition, and a typical axion energy density (red curve) for ma = 100 µ eV[121].…”
mentioning
confidence: 99%
“…Moreover, we may consider the environment of the early universe, where the hadron phase is expected to be created in a spatially (presumably almost) homogeneous form, after the QCD phase transition and thermalization of the hadron phase bubbles (even with feasible inhomogeneity by a supercooling) [24]. The homogeneous hadron phase is thermalized with the temperature ∼ 100 MeV [24][25][26], at which all hadrons already become nonrelativistic in the thermal bath with photon (but still strongly interacting each other in the kinetic equilibrium). Then the thermal loop corrections to the dilaton dynamics can safely be neglected (with all exponentially suppressed), so the external EM interactions would be most relevant to the dilaton, as well as the vacuum contributions by strong interactions with pions and dilatons themselves.…”
mentioning
confidence: 99%
“…Moreover, we may consider the environment of the early universe, where the hadron phase is expected to be created in a spatially (presumably almost) homogeneous form, after the QCD phase transition and thermalization of the hadron phase bubbles (even with feasible inhomogeneity by a supercooling) [25]. The homogeneous hadron phase is thermalized with the temperature ∼ 100 MeV [25][26][27], at which all hadrons already become nonrelativistic in the thermal bath with photon (but still strongly interacting each other in the kinetic equilibrium). Then the thermal loop corrections to the dilaton dynamics can safely be neglected (with all exponentially suppressed), so the external EM interactions would be most relevant to the dilaton, as well as the vacuum contributions by strong interactions with pions and dilatons themselves.…”
Section: Jhep10(2020)017mentioning
confidence: 99%