pith:LO2LDZGC
GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States
The magnetic flux threading the black hole horizon controls jet efficiency, magnetization, and radiative output in three accretion states.
arxiv:2605.17460 v1 · 2026-05-17 · astro-ph.HE
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Claims
The magnetic flux threading the black hole horizon emerges as the fundamental state variable controlling jet efficiency, flow magnetization, and radiative output across all three states.
That the chosen initial magnetic field geometries and the direct scaling of simulated luminosities and variability amplitudes to observed sources (GRS 1915+105, Cyg X-1, HLX-1) capture the dominant physics without missing effects such as radiative cooling or non-ideal MHD.
GRMHD simulations identify magnetic flux through the black hole horizon as the key variable setting jet efficiency and radiative output across MAD, INT, and SANE states, with mappings to temporal classes in GRS 1915+105 and other sources.
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| First computed | 2026-05-20T00:04:40.142826Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5bb4b1e4c21b64fe50b7541d4d683f904f7b1f3623e3bdbb3bd7d0a5ef5e8f05
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/LO2LDZGCDNSP4UFXKQOU22B7SB \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 5bb4b1e4c21b64fe50b7541d4d683f904f7b1f3623e3bdbb3bd7d0a5ef5e8f05
Canonical record JSON
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