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Paper Citation Record · LEDGER

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

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 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

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 17 of 17 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:00:37.985704Z

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

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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 b5cac60b-2530-4a94-a04c-1d193bffe4e3 · inbound

Turning a negative neutrino mass into a positive optical depth cites this paper.

Turning a negative neutrino mass into a positive optical depth What's the matter with $\Sigma m_{\nu}$?

Reference 12

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no resolver link, observed 2026-08-16T05:00:37.985704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:00:37.985704Z digest=sha256:3c48440dbfb63d016059feabaf68d5285f31b2804f5b97c640b8af4fe05234ea

Observation 45d1b5c1-9117-4198-9ef3-2136e6987dc3 · inbound

It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2 cites this paper.

It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2 What's the matter with $\Sigma m_{\nu}$?

Reference 23

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unresolved
no resolver link, observed 2026-08-16T04:44:34.565764Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:44:34.565764Z digest=sha256:5dd8ca0eccdc02c9d3c7f557f2752b8982bb22ca1c2032205bc1bc21c1ebbbfb

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

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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 2026-08-22T06:32:14.747728+00:00.

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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

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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=sha256:02e7cd00fa2f67f18caef0b74d1f5ab3f0a0d15c5f4136d15346734a10174f86

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

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:44:16.548843Z digest=sha256:b9e833b29160c056a6a9fd8659444f88872822c46d76f6846375350ecdf6ebd5

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:41:15.503598Z digest=sha256:43523979419022fc09641db5d85dd8a935a28499657df1474f18ecaac63d4a5b

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

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T21:32:34.617964Z digest=sha256:fdafe613e2cf4d8bc61ae264d76dc3d933752b125072ff6d3a986bf65dfea46c

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

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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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-16T18:00:59.984076Z digest=sha256:1801813c5cf6865f1121cd400930a5fd78f1f1aa226f4c32582d36473e3926ff

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

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T11:11:49.000382Z digest=sha256:f34a9c56d14415fbdf0eb8f269d76c41b338e476c3d975933dd7335663ff5a83

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

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T19:14:24.177158Z digest=sha256:566b06c0205fcfffd508ec53a58f5207397812a326970cdfa73d86066529ebad

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

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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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-07T15:00:09.282977Z digest=sha256:659005be01f7892d691bf39f88217789d2c552cbde54a44fda350a95700d82cf

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

Minimal dark $SU(2)$ origin of a massless Dirac neutrino cites this paper.

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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-29T11:15:53.860139Z digest=sha256:32c25c84603d61b02ef8692dd08017f16e03dac3e4e6c32a11f6cc71adbae97c

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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-28T05:25:55.116276Z digest=sha256:3b92cd7ce1d081c1ffdccb62057dcc90a397d5359e13014711e2726b1cb68dc6

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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-02T06:14:20.101706Z digest=sha256:ee06b2a55292853900339390f0d1348ee9ad091349e589b0e2857017252b3e4f

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

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T03:36:03.722986Z digest=sha256:a08e18c25c786e30994fd73bd28b61bc0a53e68a52f31480443f5e949c02cf52

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

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T06:22:31.479054Z digest=sha256:43d0e2de4134257a7844cb4895a57d80e425e564741c9e7bc12cc327b498e3c2

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

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Unavailable: canonical work link unavailable.

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