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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Two-Photon Coupling of Low-M<strong>as</strong>s Bosons 183<br />

5.4.4 Vacuum Birefringence<br />

Besides the conversion between photons and axions there is a more<br />

subtle effect that can serve to search <strong>for</strong> the two-photon vertex of lowm<strong>as</strong>s<br />

pseudoscalars. In an external transverse E or B field the mixing<br />

between the A ∥ component with a leads to a backreaction on A ∥<br />

(Fig. 5.8b) which amounts to a retardation of its ph<strong>as</strong>e. Put another<br />

way, the ∥ and ⊥ polarization states have different refractive indices in<br />

vacuum with an E or B field (vacuum Cotton-Mouton effect). There<strong>for</strong>e,<br />

if one shines a light beam which is linearly polarized at 45 ◦ relative<br />

to a transverse B field, the beam will develop a small degree of elliptic<br />

polarization (Maiani, Petronzio, and Zavattini 1986).<br />

A vacuum Cotton-Mouton effect is expected even in the absence of<br />

axions from the QED amplitude shown in Fig. 5.8a; in the non<strong>for</strong>ward<br />

direction it describes Delbrück scattering on a charged particle. More<br />

generally, an electron loop mediates an effective γγ interaction which<br />

<strong>for</strong> low energies can be described by the Euler-Heisenberg Lagrangian,<br />

L γγ = 2α2 [<br />

(E 2 − B 2 ) 2 + 7(E · B) 2] (5.30)<br />

45m 4 e<br />

(Heisenberg and Euler 1936; see also Itzykson and Zuber 1983).<br />

Fig. 5.8. Vacuum birefringence in the presence of external fields. (a) QED<br />

contribution according to the Euler-Heisenberg γγ interaction. (b) γa or<br />

γπ ◦ oscillations in an external E or B field. (c) Photon birefringence in an<br />

external axion field (axionic domain walls, cosmic axion field). (d) Axionmediated<br />

contribution in a strong E · B field, e.g. near a pulsar.

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