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pith:HKMNJ22W

pith:2026:HKMNJ22WUGIZRO7J7DXFMVBBCJ
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Stern--Gerlach Spin Sorting in Relativistic Magnetic Reconnection

K. Nykyri

The Stern-Gerlach force sorts particles by magnetic moment projection across reconnection current sheets near magnetars without altering the reconnection rate.

arxiv:2605.16243 v1 · 2026-05-15 · physics.plasm-ph · astro-ph.HE

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Record completeness

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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 further show, using electron--positron particle-in-cell simulations, that the SG force sorts particles by magnetic-moment projection into opposite sides of a Harris current sheet without measurably changing the global reconnection rate in the tested regime.

C2weakest assumption

The assumption that the fully projected branch parameter Ξ₀ = <Z>/r_L and its effective version Ξ_Eff = P_eff Ξ₀ correctly capture the accumulated SG cross-sheet displacement relative to the relativistic Larmor radius during a diffusion-region transit (as defined in the introduction of the control parameter).

C3one line summary

Introduces the parameter Ξ_Eff to quantify Stern-Gerlach spin sorting in reconnection and reports PIC simulations showing particle sorting by magnetic moment without altering the global reconnection rate.

References

42 extracted · 42 resolved · 2 Pith anchors

[1] M. A. Shay, J. F. Drake, B. N. Rogers, and R. E. Denton, Geophysical Research Letters26, 2163 (1999) 1999
[2] J. F. Drake and M. Swisdak, Physics of Plasmas21, 072903 (2014) 2014
[3] J. T. Dahlin, J. F. Drake, and M. Swisdak, Physics of Plasmas21, 092304 (2014) 2014
[4] J. L. Burchet al., Science352, aaf2939 (2016) 2016
[5] K. Nykyri, A. Otto, E. Adamson, E. Dougal, and J. Mumme, Journal of Geophysical Research: Space Physics116(2011) 2011

Formal links

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Receipt and verification
First computed 2026-05-20T00:01:59.771281Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

3a98d4eb56a19198bbe9f8ee5654211279f09ef737d64fac8755bf9b48bc8390

Aliases

arxiv: 2605.16243 · arxiv_version: 2605.16243v1 · doi: 10.48550/arxiv.2605.16243 · pith_short_12: HKMNJ22WUGIZ · pith_short_16: HKMNJ22WUGIZRO7J · pith_short_8: HKMNJ22W
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HKMNJ22WUGIZRO7J7DXFMVBBCJ \
  | 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: 3a98d4eb56a19198bbe9f8ee5654211279f09ef737d64fac8755bf9b48bc8390
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "0253230bd942b461817a17701cf6f0538c11699801741e5d7b08d80e1c96d4bd",
    "cross_cats_sorted": [
      "astro-ph.HE"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "physics.plasm-ph",
    "submitted_at": "2026-05-15T17:48:48Z",
    "title_canon_sha256": "f9f2fe76a161b301422c5794c0fd4f5a804b1c08b035285e4c4049845c15ac66"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.16243",
    "kind": "arxiv",
    "version": 1
  }
}