pith:7ZKQ4CW7
Non-thermal Synchrotron Emission and Polarization Signatures during Black Hole Flux Eruptions
Anisotropic non-thermal electrons are essential for interpreting time-variable EHT polarimetric observations of black hole flux eruptions.
arxiv:2512.06803 v2 · 2025-12-07 · astro-ph.HE · gr-qc
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Claims
Incorporating anisotropic non-thermal electrons is essential for a physically self-consistent interpretation of time-variable EHT polarimetric observations.
Non-thermal electrons are accelerated from the thermal background through magnetic reconnection and follow beamed or loss-cone pitch-angle distributions that remain fixed during the eruption.
Non-thermal electrons with anisotropic pitch angles during flux eruptions produce flux outbursts, localized brightening, and suppressed linear polarization in black hole disk images.
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| First computed | 2026-05-20T00:00:29.747108Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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Canonical record JSON
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