النجوم المغناطيسية: كيف يخدع المجال المغناطيسي الضوء سريع

الملخص الأصلي

كما كتبه المؤلفون، بالإنجليزية arXiv:2605.17048

Magnetars are among the most extreme laboratories in the universe, harboring surface magnetic fields reaching $$10^{15}$$~G. At these supercritical scales, Maxwell's linear electrodynamics is superseded by Nonlinear Electrodynamics (NLED). While vacuum birefringence has provided initial observational evidence for these effects, its broader impact on photon propagation remains largely unexplored. In this work, we demonstrate that NLED significantly alters photon propagation in the vicinity of magnetars, deviating light from standard null-geodesics. We estimate that neglecting these corrections leads to relative errors in inferred stellar radii by means of ray-tracing techniques of approximately $$10\%$$. Furthermore, we find that NLED induces a systematic minimal travel-time delay of approximately $$350~n$$s, a value that already far exceeds the $$100$$~ns temporal resolution of missions like NICER. These results are critical for the interpretation of X-ray pulse profiles from current and future observatories, such as eXTP, which rely on high-precision light-bending and timing models to determine neutron-star masses and radii. Finally, our results underscore the role of magnetars as a vital window into the physics of superdense matter and supercritical fields, and we briefly highlight other astrophysical observables--such as glitches and antiglitches--that may be affected by NLED.