Paper Citation Record · LEDGER

Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2406.13717.

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

pith.paper-citation-record.v1
2406.13717 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:21:42.891574Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T16:19:57.284731Z

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 7ce1f718-f815-4d10-87ee-1f52cd127246 · inbound

Building Neutron Stars with the MUSES Calculation Engine cites this paper.

Building Neutron Stars with the MUSES Calculation Engine Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-08T11:32:34.453445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b0d1bec3-b832-4557-8eec-73fb886bbab8 · inbound

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars cites this paper.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.597991Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 775af8ef-89d5-494a-a35a-fb1732c27b5b · inbound

Classification of color superconductivity by one-gluon exchange helicity amplitudes and renormalization group equations cites this paper.

Classification of color superconductivity by one-gluon exchange helicity amplitudes and renormalization group equations Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-05T15:53:22.585083Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f8774cc-aa0e-4ce7-b941-0d625d6fdfc7 · inbound

Neutrino absorption in two-flavor color-superconducting quark matter cites this paper.

Neutrino absorption in two-flavor color-superconducting quark matter Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-05T10:17:57.017374Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation beaedda9-c175-406d-9595-49bf1b4d7636 · inbound

Bulk viscosity from neutron decays to dark baryons in neutron star matter cites this paper.

Bulk viscosity from neutron decays to dark baryons in neutron star matter Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 130

Resolution: verified exact; arxiv_id, observed 2026-05-18T12:46:23.853491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 6641382a-92b2-462f-bae1-82cb99596bf9 · inbound

Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers cites this paper.

Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-22T12:54:52.482346Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 104fdf87-edfd-4b52-bbe1-5bdd6e19f2fd · inbound

Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars cites this paper.

Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 73

Resolution: verified exact; arxiv_id, observed 2026-06-29T10:13:18.007740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 2ed51122-3c41-48e8-8305-3356633b6388 · inbound

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine cites this paper.

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 157

Resolution: verified exact; arxiv_id, observed 2026-07-04T16:19:57.286169Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation eb36e55c-343c-41d0-bc0c-6cd6e93c820f · inbound

Transport properties in binary neutron star mergers: Effect of magnetic field cites this paper.

Transport properties in binary neutron star mergers: Effect of magnetic field Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-16T00:21:42.891574Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.