Mixing of the photon with low-mass particles

TLDR

Photons can mix with low‑mass bosons such as axions and gravitons via a two‑photon vertex when external electromagnetic fields are present. The authors develop a formalism to study photon–boson beam evolution in external fields and apply it to axion detection through magnetically induced vacuum birefringence. The formalism models photon–axion (or graviton) transitions in external fields, including vacuum birefringence measurements, pulsar magnetic fields, and adiabatic propagation in extended systems such as magnetic white dwarf magnetospheres. QED nonlinearities produce magnetic birefringence far stronger than axion effects, suppressing transitions near pulsars, but plasma refractive effects can cancel this QED contribution, allowing resonant photon–axion transitions analogous to the MSW effect, leading to conclusions that differ from recent discussions.

Abstract

Photons can mix with low-mass bosons in the presence of external electromagnetic fields if these particles---not necessarily of spin 1---couple by a two-photon vertex. Important examples are the hypothetical axion (spin 0) and graviton (spin 2). We develop a formalism which is adapted to study the evolution of a photon (axion, graviton) beam in the presence of external fields. We apply our results to discuss the possibility of detecting axions by a measurement of the magnetically induced birefringence of the vacuum. We also discuss photon-axion (graviton) transitions in pulsar magnetic fields. The QED-induced nonlinearity of Maxwell's equations causes magnetic birefringence effects which are much stronger than the axion-induced effects in the range of axion parameters allowed by astrophysical constraints. Also, this QED effect induces an index of refraction for photons in vacuum which is so large near pulsars that photon-axion (graviton) transitions are strongly suppressed. However, this QED effect can be canceled by plasma refractive effects, leading to degeneracy between photons and axions so that resonant transitions can occur in analogy with the Mikheyev-Smirnov-Wolfenstein effect. The adiabatic condition can be met only in spatially extended systems, possibly in the magnetosphere of magnetic white dwarfs. Our conclusions differ substantially from several recent discussions of various aspects of these mixing phenomena.