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Paper Citation Record · LEDGER

Hubble Tension and Cosmological Imprints of $U(1)_X$ Gauge Symmetry: $U(1)_{B_3-3 L_i}$ as a case study

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2312.16304.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2312.16304 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:34.921401Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-11T07:06:01.926625Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 09cdfc64-f5f0-4864-b66f-3ea8c9881c39 · inbound

Can a secluded self-interacting dark sector generate detectable gravitational waves? cites this paper.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Hubble Tension and Cosmological Imprints of $U(1)_X$ Gauge Symmetry: $U(1)_{B_3-3 L_i}$ as a case study

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-08T23:34:34.921401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T23:34:34.921401Z digest=sha256:f97e3f954650b5aae7a34d6a5af223078f1c96ffc58657854c48b60faa383e3c

Observation d1755fb4-7ac0-403f-83e7-fbf327dfc5ce · inbound

New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis cites this paper.

New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis Hubble Tension and Cosmological Imprints of $U(1)_X$ Gauge Symmetry: $U(1)_{B_3-3 L_i}$ as a case study

Reference 184

Resolution
unresolved
no resolver link, observed 2026-08-06T21:08:58.679122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:08:58.679122Z digest=sha256:738c0e13c768420f6ff54f6c453f31fdf0fc7bd7942703d9191810d7b882d109

Observation bf262b53-b785-4642-a1ec-f6a66922d06b · inbound

CMB signatures of gravity-mediated dark radiation in $\mathbf{\Delta N_{\rm eff}}$ cites this paper.

CMB signatures of gravity-mediated dark radiation in $\mathbf{\Delta N_{\rm eff}}$ Hubble Tension and Cosmological Imprints of $U(1)_X$ Gauge Symmetry: $U(1)_{B_3-3 L_i}$ as a case study

Reference 14

Resolution
verified exact
arxiv_id, observed 2026-05-11T07:06:01.930143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-10T17:18:29.352423Z digest=sha256:c42694e16c1663d508da56d213102552a66512493fd4dfa000c00556e202574f