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pith:JI2LSR7M

pith:2026:JI2LSR7MXGDFGJICC6Q3PTKLNL
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The impact of flickering variability and magnetisation on the dynamics, stability and morphology of radio-loud AGN jets

Alex J. Cooper, Emma L. Elley, Henry Whitehead, James H. Matthews

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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\usepackage{pith}
\pithnumber{JI2LSR7MXGDFGJICC6Q3PTKLNL}

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2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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Claims

C1strongest claim

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.

C2weakest assumption

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.

C3one line summary

High magnetization and flickering variability in relativistic MHD simulations create asymmetrical cocoons and broken jet morphologies in AGN jets.

References

68 extracted · 68 resolved · 14 Pith anchors

[1] Simulating the dynamics and non-thermal emission of relativistic magnetized jets I. Dynamics. , keywords =. doi:10.1093/mnras/staa2934 , archivePrefix =. 2009.10475 , primaryClass = 2009 · doi:10.1093/mnras/staa2934
[2] Modelling the Kinked Jet of the Crab Nebula · doi:10.1093/mnras/stt1632
[3] D., & Znajek, R · doi:10.1093/mnras/179.3.433
[4] D., & Payne, D · doi:10.1093/mnras/199.4.883
[5] A simple analytical model of magnetic jets. , keywords =. doi:10.1093/mnrasl/slac060 , archivePrefix =. 2204.11637 , primaryClass = · doi:10.1093/mnrasl/slac060
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

Aliases

arxiv: 2605.13469 · arxiv_version: 2605.13469v1 · doi: 10.48550/arxiv.2605.13469 · pith_short_12: JI2LSR7MXGDF · pith_short_16: JI2LSR7MXGDFGJIC · pith_short_8: JI2LSR7M
Agent API
Verify this Pith Number yourself
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())"
# expect: 4a34b947ecb98653250217a1b7cd4b6afbfb5ca72be165a91da71f957cd82afb
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "03cc3eda30561037889387fb53d7e02265b0adbcef2c640c4835a27291ba2efb",
    "cross_cats_sorted": [
      "astro-ph.GA"
    ],
    "license": "http://creativecommons.org/licenses/by-sa/4.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2026-05-13T12:56:29Z",
    "title_canon_sha256": "eb02d814f27fded28b86f8bf23085e0a38655cd07fda6d8f5039be3f7ec8770b"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.13469",
    "kind": "arxiv",
    "version": 1
  }
}