Pith Number

pith:6O7LTKUO

pith:2012:6O7LTKUOIWIQHAUCXH3NATFDGZ

not attested not anchored not stored refs resolved

Dynamical Boson Stars

Carlos Palenzuela, Steven L. Liebling

Boson stars are stable scalar field configurations that persist in dynamical general relativity and serve as dark matter sources or black hole mimickers.

arxiv:1202.5809 v5 · 2012-02-27 · gr-qc · astro-ph.HE · hep-ph · hep-th

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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

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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

Boson stars find use in a wide variety of models as sources of dark matter, as black hole mimickers, in simple models of binary systems, and as a tool in finding black holes in higher dimensions with only a single killing vector.

C2weakest assumption

The assumption that scalar field configurations can form stable, non-dispersing, localized energy bundles that persist under dynamical evolution in general relativity, as required for their use in the cited models.

C3one line summary

Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

References

299 extracted · 200 resolved · 130 Pith anchors

[1] Observation of a new particle in the search for the standard model higgs boson with the atlas detector at the lhc.Physics Letters B2012;716(1):1–29 2012 · doi:10.1016/j.physletb.2012.08.020

[2] Observation of Gravitational Waves from a Binary Black Hole Merger 2016 · doi:10.1103/physrevlett.116.061102

[3] Tests of general relativity with GW150914 2016 · doi:10.1103/physrevlett.116.221101

[4] Exploring the Sensitivity of Next Generation Gravitational Wave Detectors 2017 · doi:10.1088/1361-6382/aa51f4

[5] Phys Rev D 105:102001 2022 · doi:10.1103/physrevd.105.102001

Formal links

2 machine-checked theorem links

Cited by

23 papers in Pith

Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object

Strongly Interacting Dark Matter admixed Neutron Stars

Unveiling horizons in quantum critical collapse

Spin-Hair Induced Chaos of Spinning Test Particles in Rotating Hairy Black Holes

Unveiling horizons in quantum critical collapse

Receipt and verification

First computed	2026-05-17T23:37:42.451190Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

f3beb9aa8e4591038282b9f6d04ca3364837394580a6a89b9b94baf9d6f3dd7f

Aliases

arxiv: 1202.5809 · arxiv_version: 1202.5809v5 · doi: 10.48550/arxiv.1202.5809 · pith_short_12: 6O7LTKUOIWIQ · pith_short_16: 6O7LTKUOIWIQHAUC · pith_short_8: 6O7LTKUO

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/6O7LTKUOIWIQHAUCXH3NATFDGZ \
  | 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: f3beb9aa8e4591038282b9f6d04ca3364837394580a6a89b9b94baf9d6f3dd7f

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "40f352e233b6eba7e19c89f5a5d1520acb815628bafdbef557d395d1fbeb3a39",
    "cross_cats_sorted": [
      "astro-ph.HE",
      "hep-ph",
      "hep-th"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "gr-qc",
    "submitted_at": "2012-02-27T00:47:39Z",
    "title_canon_sha256": "774b215cce9b5cf4affce9a51c46c8fc362561bba38d7b1687e90210b8554ce4"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1202.5809",
    "kind": "arxiv",
    "version": 5
  }
}