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PVLAS experiment, star cooling and BBN constraints: Possible interpretation with temperature dependent gauge symmetry breaking

Jihn E. Kim

Abstract

It is known that the kinetic mixing of photon and another U(1)_ex gauge boson can introduce millicharged particles. Millicharged particles $f$ of mass 0.1 eV can explain the PVLAS experiment. We suggest a temperature dependent gauge symmetry breaking of U(1)_ex for this idea to be consistent with astrophysical and cosmological constraints.

PVLAS experiment, star cooling and BBN constraints: Possible interpretation with temperature dependent gauge symmetry breaking

Abstract

It is known that the kinetic mixing of photon and another U(1)_ex gauge boson can introduce millicharged particles. Millicharged particles of mass 0.1 eV can explain the PVLAS experiment. We suggest a temperature dependent gauge symmetry breaking of U(1)_ex for this idea to be consistent with astrophysical and cosmological constraints.

Paper Structure

This paper contains 12 equations, 3 figures.

Figures (3)

  • Figure 1: Feynman diagrams leading to photon conversions in a magnetic field.
  • Figure 2: Mixing of U(1)$_{\rm em}$ and U(1)$_{\rm ex}$ gauge bosons through a heavy particle $F$.
  • Figure 3: Typical scales of masses and critical temperatures.