Pith. sign in

Paper Citation Record · LEDGER

What's the matter with $\Sigma m_{\nu}$?

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:2503.14470.

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

pith.paper-citation-record.v1
2503.14470 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 15 of 15 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 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:34:27.381038Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T09:36:50.049796Z

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 06bfd022-6f34-4965-83e9-85c1f44a1ae1 · inbound

SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field cites this paper.

SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field What's the matter with $\Sigma m_{\nu}$?

Reference 162

Resolution
malformed identifier
arxiv_id, observed 2026-05-13T19:11:29.270696Z

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=2026-05-13T19:11:25.985677Z digest=sha256:467724a7e8da8e898d6f25b007f3baf28c434c50aa5406aa67a1dcbcf91cf8bd

Observation fb98e5f6-be06-4c3e-9e08-d61c953dbfa9 · inbound

Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data cites this paper.

Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data What's the matter with $\Sigma m_{\nu}$?

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-06T21:34:27.381038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:34:27.381038Z digest=sha256:c0ce2e65f0b8ec2a11cc5b1c5022db1ae3c069aeef983e5e550064f601b9cef7

Observation 8c2a1ba0-424a-4d71-8ef9-e917a6ab0dd0 · inbound

Constraints on Logarithmic Model Extensions of Symmetric Teleparallel Gravity cites this paper.

Constraints on Logarithmic Model Extensions of Symmetric Teleparallel Gravity What's the matter with $\Sigma m_{\nu}$?

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-05T14:44:16.548843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:44:16.548843Z digest=sha256:4b61030202c090cc7e4ac43b4918051129664c0c8b728705e5b3eda78b498f66

Observation 7e7b5841-6a29-440b-8af9-64b5c950a2fb · inbound

Rapid late-time reionization: constraints and cosmological implications cites this paper.

Rapid late-time reionization: constraints and cosmological implications What's the matter with $\Sigma m_{\nu}$?

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-05T14:41:15.503598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:41:15.503598Z digest=sha256:04bcbc2be03515fcafd3b718ace754cf34d630ae1d893fc6a883481cf59db1ae

Observation b081007e-bdc7-4a1d-8f82-ab4ed0fe2309 · inbound

Dynamical Dark Energy or Modified Gravity? Signatures in Gravitational Wave Propagation cites this paper.

Dynamical Dark Energy or Modified Gravity? Signatures in Gravitational Wave Propagation What's the matter with $\Sigma m_{\nu}$?

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-04T21:32:34.617964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T21:32:34.617964Z digest=sha256:114e9d3cbb79de30f5b322e4218401832a0f142d589e7650797e1e5ece7e0b15

Observation 9bb75403-9bec-452c-9b59-aa7749929058 · inbound

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity cites this paper.

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity What's the matter with $\Sigma m_{\nu}$?

Reference 112

Resolution
verified exact
arxiv_id, observed 2026-05-16T18:01:09.143958Z

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=2026-05-16T18:00:59.984076Z digest=sha256:d92c10e4c0e1bb74bb7df13e3a1c2c4050210fbb7060be67d6ad46b8c4739233

Observation 5f9c3479-5dbf-4a20-86a4-21db5cfbc9a4 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions What's the matter with $\Sigma m_{\nu}$?

Reference 152

Resolution
unresolved
no resolver link, observed 2026-08-03T11:11:49.000382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T11:11:49.000382Z digest=sha256:e3863e124da9a9a4846ade4e88435ae29aaee0ab4636f2d367f19dfbf1825de6

Observation 6b3759de-a8ce-4aec-a6ed-db38389794ca · inbound

Neutrino mass limits and decaying dark matter: background evolution versus perturbations cites this paper.

Neutrino mass limits and decaying dark matter: background evolution versus perturbations What's the matter with $\Sigma m_{\nu}$?

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-02T19:14:24.177158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T19:14:24.177158Z digest=sha256:084087b2000d2f0491dae7e3b4ca0726ef14c7cbda4f1b6f7be3a06779372502

Observation b4740707-15cc-4440-88e1-51ea410686f6 · inbound

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe cites this paper.

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe What's the matter with $\Sigma m_{\nu}$?

Reference 10

Resolution
verified exact
arxiv_id, observed 2026-05-12T00:36:14.134677Z

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=2026-05-07T15:00:09.282977Z digest=sha256:44288b54d64f845b11fe499373fad7b2fa39186d049f1aca6bb9d900136bfd82

Observation d786a29c-b918-4aeb-ab04-3dfc18797220 · inbound

A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino cites this paper.

A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino What's the matter with $\Sigma m_{\nu}$?

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-06-29T11:23:21.735846Z

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=2026-06-29T11:15:53.860139Z digest=sha256:464e40217bbe3dca5d6972ae87da563ab568d0b11460f4378bb058b6f943d6d1

Observation 0e6cd5db-05f5-4bb6-84aa-d82d9c977c96 · inbound

The Future of Lepton Flavor cites this paper.

The Future of Lepton Flavor What's the matter with $\Sigma m_{\nu}$?

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-07-02T09:36:50.051191Z

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=2026-06-28T05:25:55.116276Z digest=sha256:ab85ef915fe2f07694a200fd189625e7f4af7f64435a7a00a7a15538b44add80

Observation 02ccc90e-543a-4109-9e75-a6e0c65648ba · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation What's the matter with $\Sigma m_{\nu}$?

Reference 182

Resolution
verified exact
arxiv_id, observed 2026-07-02T06:16:43.523585Z

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=2026-07-02T06:14:20.101706Z digest=sha256:c8d7d4077d285fc8ad528a0a9e42bfeef869b0ed92dab9ae8b78e4162c178c1e

Observation c502b6d6-bddb-4099-baec-f712c40d318e · inbound

Evaporating cosmologically coupled black holes cites this paper.

Evaporating cosmologically coupled black holes What's the matter with $\Sigma m_{\nu}$?

Reference 258

Resolution
unresolved
no resolver link, observed 2026-08-02T03:36:03.722986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T03:36:03.722986Z digest=sha256:9394fe4a15b64391263b493d5c4cff25210f5d1fbbd5f91fb8c848d0d8850ecf

Observation ddfc35e9-f69a-4293-92e4-f4ea15ee0fee · inbound

Measuring Cosmic Neutrino Masses Independently of Dark Energy cites this paper.

Measuring Cosmic Neutrino Masses Independently of Dark Energy What's the matter with $\Sigma m_{\nu}$?

Reference 17

Resolution
unresolved
no resolver link, observed 2026-07-31T06:22:31.479054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T06:22:31.479054Z digest=sha256:82cd694b3345b668cf3cd163d88c0f50c6b56ac716e12f3b071096110f73f4b7

Observation d41c9e86-ee12-4657-9e80-95cb343c86e0 · inbound

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift cites this paper.

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift What's the matter with $\Sigma m_{\nu}$?

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-04T18:21:06.602057Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:21:06.602057Z digest=sha256:e080a195de392bdbf0e9334c3b3b8ca04ca6881242e3858946e84456647d059c