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pith:KAYYTXFQ

pith:2019:KAYYTXFQHYKQBS4TJNPYKNCBDP
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PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

A. J. Dittmann, A. K. Harding, F. K. Lamb, G. Prigozhin, J. M. Lattimer, K. C. Gendreau, K. S. Wood, M. C. Miller, P. S. Ray, R. Foster, R. M. Ludlam, S. Bogdanov, S. Guillot, S. Mahmoodifar, S. M. Morsink, T. Enoto, T. E. Strohmayer, T. Okajima, W. C. G. Ho, Y. Soong, Z. Arzoumanian

Bayesian modeling of NICER X-ray pulses from PSR J0030+0451 yields a neutron star radius near 13 km and mass of 1.44 solar masses, improving constraints on the equation of state above nuclear density.

arxiv:1912.05705 v1 · 2019-12-12 · astro-ph.HE · nucl-th

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1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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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.

Claims

C1strongest claim

We show that our measurements of Re and M for PSR J0030+0451 improve the astrophysical constraints on the equation of state of cold, catalyzed matter above nuclear saturation density.

C2weakest assumption

The analysis assumes that the observed X-ray waveform is produced by a small number of uniform-temperature oval emitting regions whose geometry and temperature distribution can be adequately parameterized and that systematic uncertainties in the instrument response and atmosphere model are sub-dominant to the statistical errors.

C3one line summary

Mass and radius of PSR J0030+0451 measured as 1.44 solar masses and 13.02 km, improving astrophysical constraints on the cold dense matter equation of state.

References

75 extracted · 75 resolved · 1 Pith anchors

[1] P., Abbott, R., Abbott, T 2017
[2] 2015, PhRvD, 92, 023012 2015
[3] R., & Ravenhall, D 1998
[4] 1980, ApJ, 235, 534 1980
[5] AlGendy, M., & Morsink, S. M. 2014, ApJ, 791, 78 2014

Formal links

2 machine-checked theorem links

Cited by

26 papers in Pith

Receipt and verification
First computed 2026-05-17T23:38:14.832887Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

503189dcb03e1500cb934b5f8534411bcf357616eb2045de1634f1ad5f72d8ba

Aliases

arxiv: 1912.05705 · arxiv_version: 1912.05705v1 · doi: 10.48550/arxiv.1912.05705 · pith_short_12: KAYYTXFQHYKQ · pith_short_16: KAYYTXFQHYKQBS4T · pith_short_8: KAYYTXFQ
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KAYYTXFQHYKQBS4TJNPYKNCBDP \
  | 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: 503189dcb03e1500cb934b5f8534411bcf357616eb2045de1634f1ad5f72d8ba
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "c21e097227ab655f3a7347ef09dcd0ea576cb15077a179bcf0f7a5376b8075a6",
    "cross_cats_sorted": [
      "nucl-th"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2019-12-12T00:04:41Z",
    "title_canon_sha256": "47daf82093770dab63fc625d977173234a35f1280aabbe15e8571d940cb86dbc"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1912.05705",
    "kind": "arxiv",
    "version": 1
  }
}