Pith Number

pith:6WRT4LIZ

pith:2025:6WRT4LIZINRC3UGQYJ23KYKWB5

not attested not anchored not stored refs resolved

Compact Stars in Symmetric Teleparallel Scalar-Tensor Gravity

Andr\'es Lueiza-Colip\'i, Andronikos Paliathanasis, Grigorios Panotopoulos, Nikolaos Dimakis

Symmetric teleparallel scalar-tensor gravity supports viable compact stars through interior solutions matched to extremal Reissner-Nordström exteriors.

arxiv:2510.17066 v2 · 2025-10-20 · gr-qc

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\usepackage{pith}
\pithnumber{6WRT4LIZINRC3UGQYJ23KYKWB5}

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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.

Claims

C1strongest claim

The symmetric teleparallel scalar-tensor theory supports the existence of viable astrophysical objects, demonstrated by constructing interior solutions matched to an extremal Reissner-Nordström exterior.

C2weakest assumption

The assumption that a nontrivial connection can be chosen such that the theory reduces to a genuinely nontrivial limit of general relativity while still admitting analytic solutions via the minisuperspace reduction and variational symmetries (invoked in the abstract when stating that the field equations admit a minisuperspace description and that conservation laws enable reconstruction of analytic black-hole solutions).

C3one line summary

Analytic black-hole solutions are reconstructed via conservation laws from variational symmetries in symmetric teleparallel scalar-tensor gravity, and the theory is shown to support viable compact-star interiors matched to extremal Reissner-Nordström exteriors.

References

72 extracted · 72 resolved · 1 Pith anchors

[1] Tegmark et al., Astrophys 2004

[2] Kowalski et al., Astrophys 2008

[3] Komatsu et al., Astrophys 2009

[4] N. Suzuki et. al., Astrophys. J.746, 85 (2012) 2012

[5] Akrami et al 2020

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-26T01:02:28.988530Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

f5a33e2d1943622dd0d0c275b561560f7a6fab058a0bb3c0127d20bdbbe11b19

Aliases

arxiv: 2510.17066 · arxiv_version: 2510.17066v2 · doi: 10.48550/arxiv.2510.17066 · pith_short_12: 6WRT4LIZINRC · pith_short_16: 6WRT4LIZINRC3UGQ · pith_short_8: 6WRT4LIZ

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/6WRT4LIZINRC3UGQYJ23KYKWB5 \
  | 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: f5a33e2d1943622dd0d0c275b561560f7a6fab058a0bb3c0127d20bdbbe11b19

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "fa9900192eb427a46f1de731865d7935ddb82ea2fa039158a1b4284923ef75ed",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "gr-qc",
    "submitted_at": "2025-10-20T00:45:01Z",
    "title_canon_sha256": "2e1c95acdc7e5b83c7ba8fcc23207b12feab82fce6dc61480289a4deea74688d"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2510.17066",
    "kind": "arxiv",
    "version": 2
  }
}