Electromagnetic responses driven by gravitational-wave memory in magnetar-flare outflows

Wen-Biao Han

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arXiv · 2608.10511

Electromagnetic responses driven by gravitational-wave memory in magnetar-flare outflows

Wen-Biao Han

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Abstract

An asymmetric relativistic outflow from a magnetar giant flare produces a step-like gravitational-wave (GW) memory. In the magnetized pair plasma surrounding the star, such GW memory drives transverse electromagnetic (EM) X-mode/fast-magnetosonic responses at the corresponding frequencies. We use this GW-memory spectrum to drive a global wave equation for a cold electron--positron pair plasma. With radiative boundary conditions excluding incoming waves, the driven response forms an outgoing EM mode that reaches the outer boundary of the source region. For central-engine energy-release timescales of $10$, $1$, and $0.15\,\mu\mathrm{s}$, 90\% of the integrated response energy lies below 23.3 kHz, 233 kHz, and 1.51 MHz, respectively. The principal response occupies the 10 kHz--1 MHz frequency band; a substantial extension into the 1--3 MHz frequency band also appears when a submicrosecond asymmetric-energy component is present. The electromagnetic response can escape from the source region and potentially propagate in the interstellar medium.

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Wen-Biao Han. 2026-08-11. Electromagnetic responses driven by gravitational-wave memory in magnetar-flare outflows. https://arxiv.org/abs/2608.10511

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