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pith:L45EFLT7

pith:2026:L45EFLT7KT4T5YILF3MN6E6WUV
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Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance

Dong Lai, Tu Guo

Resonant Compton scattering can wash out the 90-degree polarization angle swing caused by QED vacuum resonance in magnetar X-rays.

arxiv:2603.08119 v2 · 2026-03-09 · astro-ph.HE

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\pithnumber{L45EFLT7KT4T5YILF3MN6E6WUV}

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Record completeness

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

C1strongest claim

sufficiently strong RCS can wash out the PA swing caused by vacuum resonance. Furthermore, in addition to the QED vacuum resonance effect, significant relativistic signatures arising from plasma drift velocity (β0 ≳ 0.5) may introduce an extra 90° PA swing in the spectrum.

C2weakest assumption

treating vacuum-resonance-induced mode conversion as an input and employing a first-order approximation in RCS optical depth; the validity of the linearization for the range of optical depths and geometries considered is not demonstrated in the abstract.

C3one line summary

A first-order semi-analytical framework shows resonant Compton scattering can erase or add 90-degree polarization angle swings in magnetar soft X-ray spectra depending on magnetic twist and plasma drift velocity.

References

37 extracted · 37 resolved · 1 Pith anchors

[1] Beloborodov, A. M. 2002, Astrophys. J. Lett., 566, L85, doi: 10.1086/339511 2002 · doi:10.1086/339511
[2] 2022, MNRAS, 514, 5024, doi: 10.1093/mnras/stac1571 2022 · doi:10.1093/mnras/stac1571
[3] C., & Thompson, C 1992 · doi:10.1086/186413
[4] 2003, MNRAS, 344, 1000, doi: 10.1046/j.1365-8711.2003.06897.x 2003 · doi:10.1046/j.1365-8711.2003.06521.x
[5] 2003, MNRAS, 344, 1000, doi: 10.1046/j.1365-8711.2003.06897.x 2003 · doi:10.1046/j.1365-8711.2003.06047.x

Formal links

1 machine-checked theorem link

Receipt and verification
First computed 2026-05-17T23:38:59.710573Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

5f3a42ae7f54f93ee10b2ed8df13d6a543dd1359070fa221412dd45fcf8bc242

Aliases

arxiv: 2603.08119 · arxiv_version: 2603.08119v2 · doi: 10.48550/arxiv.2603.08119 · pith_short_12: L45EFLT7KT4T · pith_short_16: L45EFLT7KT4T5YIL · pith_short_8: L45EFLT7
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/L45EFLT7KT4T5YILF3MN6E6WUV \
  | 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: 5f3a42ae7f54f93ee10b2ed8df13d6a543dd1359070fa221412dd45fcf8bc242
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "eb4d6cae726da127a120af31f9fe9e1f437c4cad1ca5c606385c9e05a84a4935",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2026-03-09T08:59:51Z",
    "title_canon_sha256": "357017e22b7399d8d3cf6ee96dae7819b19120032a5b6f3b3e5d3c119ed3de07"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2603.08119",
    "kind": "arxiv",
    "version": 2
  }
}