2019
DOI: 10.1016/j.physletb.2019.01.056
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Axion–photon mixing in quantum field theory and vacuum energy

Abstract: We analyze axion-photon mixing in the framework of quantum field theory. The condensate structure of the vacuum for mixed fields induces corrections to the oscillation formulae and leads to non-zero energy of the vacuum for the component of the photon mixed with the axion. This energy generates a new effect of the vacuum polarization and it has the state equation of the cosmological constant, w = −1. This result holds for any homogeneous and isotropic curved space-time, as well as for diagonal metrics. Numeric… Show more

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Cited by 34 publications
(31 citation statements)
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“…As shown in Ref. [41], the off-diagonal components of Ξ µν (x) are zero for a homogeneous and isotropic universe, as well as for diagonal metrics, thus the energy density and pressure are ρ = g 00 Ξ 00 , and p = −g jj Ξ jj (no summation on the index j is intended), respectively. Then, we obtain the state equation of the cosmological constant: p = −ρ , where…”
Section: Axion-photon Mixing In Curved Space-time and Vacuum Polarizamentioning
confidence: 91%
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“…As shown in Ref. [41], the off-diagonal components of Ξ µν (x) are zero for a homogeneous and isotropic universe, as well as for diagonal metrics, thus the energy density and pressure are ρ = g 00 Ξ 00 , and p = −g jj Ξ jj (no summation on the index j is intended), respectively. Then, we obtain the state equation of the cosmological constant: p = −ρ , where…”
Section: Axion-photon Mixing In Curved Space-time and Vacuum Polarizamentioning
confidence: 91%
“…Finally, we note that the presence of a gas in the conversion region increases the oscillation rate because the gas induces the effective mass of photon m γ = c 2 ω P . However, the plasma presence reduces the value of |Υ k | 2 , which in any case remain detectable [41].…”
Section: Axion-photon Mixingmentioning
confidence: 96%
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“…Indeed, as demonstrated by Capolupo et al [23], in the quantum field theoretical framework axions and photons exhibit considerable mixing, which is somewhat similar to the mixing and oscillations of the neutrino flavors. Following [23], let us consider either one of the waveguides shown in Fig.4(a,b), which is subjected to a DC magnetic field B0 directed along the y coordinate. For the guided photon propagation along the x direction, the photon polarizations decouple, and the axion-photon mixing matrix for the state of polarization parallel to B0 may be obtained as…”
mentioning
confidence: 84%
“…We have several examples of such phenomenon both in the bosonic and fermionic sectors. In the first sector we have mixing among axion-photon [4][5][6], ηη ′ [7], neutral kaons [8] and B meson [9]. In the second one we can find the neutrino flavor oscillations [10,11], the neutron-antineutron oscillations that could be observed in the next generation of experiments using slow neutrons with kinetic energies of a few meV [12], and the quark mixing [13].…”
Section: Introductionmentioning
confidence: 99%