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Vacuum Birefringence, Ellipticity, and the Anomalous Magnetic Moment of a Photon

Sree Ram Valluri, Farrukh Chishtie, Wieslaw J. Mielniczuk

Abstract

We study photon propagation in a strong magnetic field $B\sim B_{\rm{cr}}$, where $B_{\rm cr}= \frac{m^2}{e} \simeq 4.4 \times 10^{13}$ Gauss is the Schwinger critical field. We show that the expected value of the Hamiltonian of a quantized photon for a perpendicular mode is a convex function of the magnetic field $B$. We find that the anomalous magnetic moment of a photon in the one-loop approximation is a non-decreasing function of the magnetic field $B$ in the range $0\leq B \leq 30 \, B_{\rm cr}$. We find that the anomalous magnetic moment $μ_γ$ of a photon for $B=30\, B_{\rm cr}$ is $\sim 8/3$ of the anomalous magnetic moment of a photon for $B = 1/2 ~ B_{\rm cr}$. We establish new connections between $μ_γ$, vacuum birefringence, and directly measurable polarization observables. Based on recent experimental observations -- including the ATLAS detection of light-by-light scattering at $8.2σ$ significance, IXPE X-ray polarimetry of magnetars revealing polarization degrees up to 80\%, and continuing PVLAS measurements approaching QED sensitivity -- we provide predictions for ellipticity and polarization degree as important observables for future experiments. Numerical verification of our analytical results confirms the theoretical predictions with high precision.

Vacuum Birefringence, Ellipticity, and the Anomalous Magnetic Moment of a Photon

Abstract

We study photon propagation in a strong magnetic field , where Gauss is the Schwinger critical field. We show that the expected value of the Hamiltonian of a quantized photon for a perpendicular mode is a convex function of the magnetic field . We find that the anomalous magnetic moment of a photon in the one-loop approximation is a non-decreasing function of the magnetic field in the range . We find that the anomalous magnetic moment of a photon for is of the anomalous magnetic moment of a photon for . We establish new connections between , vacuum birefringence, and directly measurable polarization observables. Based on recent experimental observations -- including the ATLAS detection of light-by-light scattering at significance, IXPE X-ray polarimetry of magnetars revealing polarization degrees up to 80\%, and continuing PVLAS measurements approaching QED sensitivity -- we provide predictions for ellipticity and polarization degree as important observables for future experiments. Numerical verification of our analytical results confirms the theoretical predictions with high precision.
Paper Structure (34 sections, 91 equations, 2 figures, 2 tables)

This paper contains 34 sections, 91 equations, 2 figures, 2 tables.

Figures (2)

  • Figure 1: Ellipticity $\chi/(\alpha |\mathbf{k}|\ell\sin^2\theta)$ as a function of $h = B_{\rm cr}/(2B)$. The rapid growth at small $h$ (strong-field regime) reflects the logarithmic structure of the Heisenberg--Euler Lagrangian.
  • Figure 2: Numerical verification of theoretical predictions and comparison with experiments. Top left: Vacuum magnetic birefringence $|\Delta n|$ as a function of $B/B_{\rm cr}$, showing the $\Delta n \propto (B/B_{\rm cr})^2$ scaling. Vertical dashed lines indicate the field strengths probed by PVLAS (laboratory), VLT J1856 (weak field), and magnetars (strong field). Top right: PVLAS measurement compared with QED prediction. The blue curve shows the QED prediction $\Delta n = k_{\rm CM} B^2$; the green line and shaded region show the PVLAS measured value and $1\sigma$ uncertainty. The QED prediction (blue dotted) at $B = 2.5$ T lies within a factor of $\sim 5$ of current sensitivity. Bottom left: IXPE magnetar observations compared with theoretical expectations. Magnetars probe fields of $B = 3$--$45\,B_{\rm cr}$, in the strong-field regime where polarization effects are large. The high observed polarization degrees (15--65%) provide strong evidence for vacuum birefringence. Bottom right: Normalized photon magnetic moment $m\mu_\gamma/(\alpha|\mathbf{k}|\sin^2\theta)$ as a function of $B/B_{\rm cr}$, confirming the monotonic increase toward the asymptotic value of $2/3$ (dashed line), consistent with Eq. (\ref{['eq:mu_gamma_exact']}).