pith:JI2LSR7M
The impact of flickering variability and magnetisation on the dynamics, stability and morphology of radio-loud AGN jets
High magnetization and flickering variability produce asymmetrical cocoons and broken jet beams in radio-loud AGN jets.
arxiv:2605.13469 v1 · 2026-05-13 · astro-ph.HE · astro-ph.GA
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Claims
We find that the constant high magnetisation jets can lead to highly asymmetrical cocoon morphologies, whilst the variable high magnetisation jet can exhibit a broken morphology, caused by a discontinuous jet beam.
The chosen two levels of magnetization and the specific flickering prescription are representative of real AGN jets and that numerical resolution is sufficient to capture the reported instabilities without artifacts.
High magnetization and flickering variability in relativistic MHD simulations create asymmetrical cocoons and broken jet morphologies in AGN jets.
References
Receipt and verification
| First computed | 2026-05-18T02:44:41.574724Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4a34b947ecb98653250217a1b7cd4b6afbfb5ca72be165a91da71f957cd82afb
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/JI2LSR7MXGDFGJICC6Q3PTKLNL \
| 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())"
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Canonical record JSON
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