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pith:KSWSJR4W

pith:2026:KSWSJR4WXMNGMKR6UNA7C4H743
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Resonant shear-flow instability in anisotropic supersonic plasmas with heat flux

Namig S. Dzhalilov

A resonant instability develops in supersonic shear flows of anisotropic collisionless plasmas and disappears in the vortex sheet limit.

arxiv:2605.13056 v1 · 2026-05-13 · astro-ph.SR · physics.plasm-ph

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Record completeness

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4 Citations open
5 Replications open
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Claims

C1strongest claim

The instability is identified as resonant, peaking when the wave phase velocity matches the mean flow velocity, with the growth rate decreasing for higher-order modes... the instability vanishes in the vortex sheet limit, distinguishing it from the classical Kelvin-Helmholtz mechanism. These findings suggest that this specific instability holds significant potential for explaining the problem of observed boundaries between isotropic and anisotropic proton temperature regions in a low-beta solar wind plasma.

C2weakest assumption

The reduction of the governing wave equation to an exactly solvable form assumes a smooth hyperbolic velocity profile together with spatially homogeneous density and magnetic field in the unperturbed state; the 16-moment closure must remain valid throughout the linear growth phase.

C3one line summary

An exact analytical modal analysis yields a resonant shear-flow instability in supersonic anisotropic plasmas that vanishes in the vortex-sheet limit and is distinct from Kelvin-Helmholtz.

References

120 extracted · 120 resolved · 0 Pith anchors

[1] G. K. Batchelor , title =. J. Fluid Mech. , year =
[2] Blumen, W. and Drazin, P. G. and Billings, D. F. , title=. J. Fluid Mech. , volume =. 1975 , doi= 1975
[3] Hunana, P. and Zank, G. P. , title =. Astrophys. J. , volume =. 2017 , doi = 2017
[4] Hunana, P. and Tenerani, A. and Zank, G. P. and Khomenko, E. and Goldstein, M. L. and Webb, G. M. and Cally, P. S. and Collados, M. and Velli, M. and Adhikari, L. , title =. J. Plasma Phys. , volume = 2019
[5] Malara, F. and Settino, A. and Perrone, D. and Pezzi, O. and Guzzi, G. and Valentini, F. , title =. Astrophys. J. , volume =. 2022 , doi = 2022

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-18T03:08:59.196271Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

54ad24c796bb1a662a3ea341f170ffe6c900c0cd50931f5d7b19636d1bec2a6c

Aliases

arxiv: 2605.13056 · arxiv_version: 2605.13056v1 · doi: 10.48550/arxiv.2605.13056 · pith_short_12: KSWSJR4WXMNG · pith_short_16: KSWSJR4WXMNGMKR6 · pith_short_8: KSWSJR4W
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KSWSJR4WXMNGMKR6UNA7C4H743 \
  | 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: 54ad24c796bb1a662a3ea341f170ffe6c900c0cd50931f5d7b19636d1bec2a6c
Canonical record JSON
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    "cross_cats_sorted": [
      "physics.plasm-ph"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-05-13T06:26:54Z",
    "title_canon_sha256": "f7d1f4ddbdc9d7957d2c75f7eb185881d7251ad806257a19d07a21e3573cc840"
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