Pith Number

pith:2HAK3U56

pith:2022:2HAK3U56LRVAIFXY4ZJ7ECHO57

not attested not anchored not stored refs pending

Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca

23 M. McCaughan, A. Camsonne, A. Deshpande, A. Narayan, A. Rathnayake, A. Shahinyan, A. Yoon, A. Zec, B. Blaikie, B. Pandey, B. Quinn, B.T. Reed, B. Wojtsekhowski, B. Yale, C. Ayerbe Gayoso, C. Clarke, C. Feldman, C. Gal, C. Ghosh, C. Jantzi, C.J. Horowitz, C. Keppel, C. Metts, C. Palatchi, D. Adhikari, D. Androic, D. Bhatta Pathak, D. Bhetuwal, D.C. Jones, D. Dutta (9), D.E. King, D. Gaskell, D. McNulty, D. Meekins, D. Nikolaev, D.S. Armstrong, E. Fuchey, E.W. Wertz, F. Hauenstein, G.D. Cates, G. Leverick, G.M. Urciuoli, H. Albataineh, H. Bhatt, H. Liu, I. Halilovic, J. Boyd, J.C. Cornejo, J.F. Benesch, J. Mammei, J. Napolitano, J.-O. Hansen, J. Pan, J. Zhang, K.A. Aniol, K.D. Paschke, K.S. Kumar, M. Gericke, M.L. Pitt, M. M. Dalton, M. Mihovilovic, M.M. Mondal, M.N.H. Rashad, M. Petrusky, M. Thiel, N. Lashley-Colthirst, N. Liyanage, O. Hassan, P. Datta, P.E. Reimer, P.M. King, P. Souder, Q. Campagna, R. Mammei, R. Michaels, R. Radloff, R. Richards, R.S. Beminiwattha, S. Covrig Dusa, S. Jian, S. Johnston, S. Kakkar, S. Katugampola, S.K. Barcus, S. Park, S. Premathilake, S. Rahman, S. Riordan, S. Seeds, T. Averett, T. Gautam, T. Kutz, T. Ye, V. Bellini, V. Owen, W. Henry, W. Xiong, W. Zhang, X. Zheng, Y. Chen, Y.R. Roblin, Y. Tian

arxiv:2205.11593 v2 · 2022-05-23 · nucl-ex · nucl-th

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{2HAK3U56LRVAIFXY4ZJ7ECHO57}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Cited by

6 papers in Pith

Ab initio calculations of parity-violating electron scattering off $^{48}$Ca and $^{208}$Pb

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis

Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure

Bayesian Inference of the Landau Parameter $G'_0$ from Joint Gamow-Teller Measurements

Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons

Receipt and verification

First computed	2026-07-05T04:52:56.369157Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

d1c0add3be5c6a0416f8e653f208eeefd5564284fe03746ed430f662329abe14

Aliases

arxiv: 2205.11593 · arxiv_version: 2205.11593v2 · doi: 10.48550/arxiv.2205.11593 · pith_short_12: 2HAK3U56LRVA · pith_short_16: 2HAK3U56LRVAIFXY · pith_short_8: 2HAK3U56

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/2HAK3U56LRVAIFXY4ZJ7ECHO57 \
  | 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: d1c0add3be5c6a0416f8e653f208eeefd5564284fe03746ed430f662329abe14

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "e5cf9c0ac75f21e10670633cccf024a58b5cbb58d81d5a5008cea30d047a10c1",
    "cross_cats_sorted": [
      "nucl-th"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "nucl-ex",
    "submitted_at": "2022-05-23T19:46:18Z",
    "title_canon_sha256": "3194715abf37895227c7f9784c20b41f6ece69543d14158c950faedd5e0fa241"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2205.11593",
    "kind": "arxiv",
    "version": 2
  }
}