pith:ICGKS7RM
GRRMHD Simulations of State Transitions in Non-Jetted Tidal Disruption Events
GRRMHD simulations show TDE disks become thermally unstable in 17-46 days, causing X-ray luminosity to drop by nearly 100 times.
arxiv:2604.23916 v2 · 2026-04-27 · astro-ph.HE
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Claims
We find that the disk becomes thermally unstable within 17.1-46.5 days depending on the spin of the BH. Thermal spectra show a soft X-ray excess prior to collapse, with a nearly two order of magnitude decline in X-ray luminosity upon disk collapse. The spectral properties and soft X-ray luminosity in our models are similar to the TDE AT2021ehb.
The initial magnetized torus accurately represents the late-stage debris from the cooling envelope model without requiring full self-consistent evolution from the initial stellar disruption; the simulations also assume standard ideal MHD and radiative cooling prescriptions whose validity at these densities is not re-derived here.
GRRMHD simulations of TDE debris disks reveal thermal instability and collapse within weeks, producing soft X-ray excess followed by a sharp luminosity drop that resembles AT2021ehb observations.
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| First computed | 2026-07-02T00:18:29.192930Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
408ca97e2c93816a22ca42a5a4241fd897e381565ba3bea54eab4967f75c66dd
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Canonical record JSON
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