pith:4G6FLXKI
Theoretical and Observational Bounds on Dynamical Chern-Simons Gravity as an Effective Field Theory
Dynamical Chern-Simons gravity corrections must be extremely small on macroscopic scales to satisfy causality and unitarity.
arxiv:2604.07332 v2 · 2026-04-08 · hep-th · astro-ph.CO · gr-qc · hep-ph
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\pithnumber{4G6FLXKIDHBAREGATYYOPHQGJQ}
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Record completeness
Claims
any dCS corrections to gravitational dynamics should likely be very small on macroscopic systems of observational interest, such as in late-time merging black holes.
The choice of scale in the gravitational species bound and the validity of the specific N-fermion UV completion with (pseudo) Yukawa coupling are sufficient to constrain the effective theory.
Dynamical Chern-Simons gravity is bounded by causality and perturbativity to produce only tiny corrections on macroscopic gravitational systems.
Formal links
Receipt and verification
| First computed | 2026-06-03T01:05:50.316745Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e1bc55dd4819c20890c09e30e79e064c2cc819575ef607ed28216814193abdbe
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4G6FLXKIDHBAREGATYYOPHQGJQ \
| 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: e1bc55dd4819c20890c09e30e79e064c2cc819575ef607ed28216814193abdbe
Canonical record JSON
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"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
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"submitted_at": "2026-04-08T17:49:22Z",
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