Pith. sign in

Paper Citation Record · LEDGER

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations

As of 17 August 2026, this Paper Citation Record lists 25 of 25 outbound references and 2 inbound Pith citation observations for arXiv:2504.21822.

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

pith.paper-citation-record.v1
2504.21822 v2

Coverage vector

measured 25 of 25 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:59:40.313539Z

measured 27 of 27 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-29T10:03:39.187375Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T18:45:59.206230Z

Reference resolution

25 of 25 outbound references displayed

  • verified exact1
  • verified fuzzy2
  • unresolved22
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation b6d8cc90-d999-49bc-bc4c-23a7edb58e22 · outbound

This paper cites An implementation of the microphysics in full general relativity : General relativistic neutrino leakage scheme.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations An implementation of the microphysics in full general relativity : General relativistic neutrino leakage scheme

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-08-16T04:59:40.574678Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T04:59:40.214863Z digest=sha256:e97504867f0a77f264a64fbd0e5249b85edc5f0b435a6585e26414a05ead518a

Observation 98f67a12-ec43-4dd4-ae65-c5c5fe9cfcf1 · outbound

This paper cites Black Hole-Neutron Star Mergers with a Hot Nuclear Equation of State: Outflow and Neutrino-Cooled Disk for a Low-Mass, High-Spin Case.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Black Hole-Neutron Star Mergers with a Hot Nuclear Equation of State: Outflow and Neutrino-Cooled Disk for a Low-Mass, High-Spin Case

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.219838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.219838Z digest=sha256:720cd7ffa19bf8973339276067d63e8e945132fb575e702e12a5ec3e6dd781ae

Observation 983a0935-2609-4117-8dc4-57cbb96e7aba · outbound

This paper cites Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.224039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.224039Z digest=sha256:cc06adf28437d9985fb236986aab11e6e74f5d8a898f8bf42bcf4791c259467e

Observation bc0e8949-1113-4d6e-a65c-7f92ebde574d · outbound

This paper cites Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.228253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.228253Z digest=sha256:de6bda1d855c8863ce1c96fb9a0340b1bff71c54b496004dfd13b10ff1e76341

Observation 6ad77603-3548-4591-ba0d-4e51a8b770e1 · outbound

This paper cites Neutrino transport in general relativistic neutron star merger simulations.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Neutrino transport in general relativistic neutron star merger simulations

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.232888Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.232888Z digest=sha256:dd2b213898f683015aed36b399f8a6c1fc4c16f4a1e167f205c887dfd980a78d

Observation 630840cd-ff0b-4c2e-934c-f9d42e5e5118 · outbound

This paper cites Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.237318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.237318Z digest=sha256:777afa398273353937c251773b12c4c3f9c8d0bf91f0932034b09fe10ad28473

Observation 5939c864-090e-4fcc-8545-ae875fdd6ea0 · outbound

This paper cites Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.241817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.241817Z digest=sha256:2d9cb5b0c3626c04e41faf79609e24c4b70c2e2f71dc05a417c28b8bb3d02c9a

Observation 8d8c2a57-e9fc-4045-b7a2-b657ad892654 · outbound

This paper cites A New Moment-Based General-Relativistic Neutrino-Radiation Transport Code: Methods and First Applications to Neutron Star Mergers.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations A New Moment-Based General-Relativistic Neutrino-Radiation Transport Code: Methods and First Applications to Neutron Star Mergers

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.245904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.245904Z digest=sha256:96b5719fb87a750800abb4b0d9df812ad998537a18c2f0aa4e0d06147f2cbdf6

Observation f29b8b33-55fe-461f-bfdf-137f805137b6 · outbound

This paper cites Implementation of Monte-Carlo transport in the general relativistic SpEC code.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Implementation of Monte-Carlo transport in the general relativistic SpEC code

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.249855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.249855Z digest=sha256:6a17cc30186e2c79456a86b506ae88aa287b18ddfd7a1d3636faf0670a520ead

Observation 90baa8d7-c2b0-4eb4-80ff-30475fbd69cf · outbound

This paper cites Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.254689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.254689Z digest=sha256:cdde4a1aa2acb93bd1cee219c98c08be448ad5d969cd9b377cee292a947618fc

Observation a353f882-b871-4edb-a34f-af2ab5652017 · outbound

This paper cites Long-term Monte Carlo-based neutrino-radiation hydrodynamics simulations for a black hole-torus system.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Long-term Monte Carlo-based neutrino-radiation hydrodynamics simulations for a black hole-torus system

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.258720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.258720Z digest=sha256:2462719e82d0f63f985e72b8466aca878090179c3568a62c97c41d2cc06211c0

Observation 68545f6f-f5be-44be-acfe-821d521d8a37 · outbound

This paper cites Robustness of neutron star merger simulations to changes in neutrino transport and neutrino-matter interactions.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Robustness of neutron star merger simulations to changes in neutrino transport and neutrino-matter interactions

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.262747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.262747Z digest=sha256:8c035ecaf4ad912771616c9bbba541f067c56694b91797f495ab66110bdd253c

Observation 996d47c7-85e6-4930-9ab8-cf6e6e4d70d1 · outbound

This paper cites Neutrino Flavor Transformation in Neutron Star Mergers.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Neutrino Flavor Transformation in Neutron Star Mergers

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.266817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.266817Z digest=sha256:c1110d4173dd6e3e27fe9ec6ca211e3008237e0959d608b0b01bce5beaf3f2d0

Observation 01471bf3-1e0b-4b43-bb95-08320ebd8068 · outbound

This paper cites Accurate muonic interactions in neutron star mergers and impact on heavy-element nucleosynthesis.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Accurate muonic interactions in neutron star mergers and impact on heavy-element nucleosynthesis

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.270755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.270755Z digest=sha256:3a470ac75d943cec9f925cefe41977c1621a5b4fa5cefbf253c4bf0b7ad0ce71

Observation 392b7071-c2f0-46e8-8735-cccc3749262c · outbound

This paper cites Mass Ejection from the Remnant of a Binary Neutron Star Merger: Viscous-Radiation Hydrodynamics Study.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Mass Ejection from the Remnant of a Binary Neutron Star Merger: Viscous-Radiation Hydrodynamics Study

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.274778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.274778Z digest=sha256:0e67ccc92793bddab30502bd4c1a33be47e77408d7f265b82b29427691a537c4

Observation 3b03a17d-53d0-48b4-9f98-04c49c959257 · outbound

This paper cites Energy-dependent and energy-integrated two-moment general-relativistic neutrino transport simulations of hypermassive neutron star.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Energy-dependent and energy-integrated two-moment general-relativistic neutrino transport simulations of hypermassive neutron star

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.278621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.278621Z digest=sha256:c99efd3fb89d9c8d82910f42659cee7eb22608743ee8b779027ee3eea30cb3d0

Observation 131fa554-04d2-4316-9b7a-299d01b40cba · outbound

This paper cites Monte-Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamics simulations.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Monte-Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamics simulations

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.282194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.282194Z digest=sha256:e2c1bd6a909a0e646eb0a625fa56e8d8af53847468097aa5d5c5a96a8aa1657d

Observation e24e5339-ec0e-4899-82ff-113440edce43 · outbound

This paper cites The Guided Moments formalism: a new efficient full-neutrino treatment for astrophysical simulations.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations The Guided Moments formalism: a new efficient full-neutrino treatment for astrophysical simulations

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.285964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.285964Z digest=sha256:49b7c8fee2226d6091955ef5cd240e80a686948bfbc86cf8ae07c9d1e6ab22e0

Observation b7cc8dac-24a6-48ef-9e86-17ae87f1ed48 · outbound

This paper cites Neutrino Opacities in Nuclear Matter.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Neutrino Opacities in Nuclear Matter

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.289956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.289956Z digest=sha256:20357b1127a6f1492509671d2e8a473e6932587149c3b8224c3693edab34aa07

Observation 8aa742a7-66c2-4374-84b3-2ddd65256b76 · outbound

This paper cites Banerjee, A.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Banerjee, A

Reference 20

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:59:40.598355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T04:59:40.294194Z digest=sha256:30377838fd005998cf9ccb27b9fc23b2bc2d493b9767bd1fdd3e1caaf4793f3c

Observation 61607616-72bd-4a62-8fa3-6b08739799c3 · outbound

This paper cites Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.297983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.297983Z digest=sha256:cbee80fcf147b5d49a905c1be644bd9ae6f73abb9ddb9dba37b360439ce82076

Observation cebfa847-5b4b-4538-a24d-e1203d5dec2e · outbound

This paper cites Foucart, M.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Foucart, M

Reference 22

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:59:40.587054Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T04:59:40.302271Z digest=sha256:5a523f17f0ee9351e20b8984f77e9448a56c142ab3af5c43014c24589c71bf71

Observation 0bca2e85-319f-40ba-b2c6-1adf012f31ef · outbound

This paper cites Core-collapse supernova equations of state based on neutron star observations.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Core-collapse supernova equations of state based on neutron star observations

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.305792Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.305792Z digest=sha256:665956c750c637dd67cf561c1f07b8f819440a050d55472ff797851a4797dcfc

Observation 2c36a25a-46ed-44f6-a4da-3cd824c31756 · outbound

This paper cites An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.309504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.309504Z digest=sha256:4c5b863e1fdf235edd01daddd3d612f074bc56f45a458a80c0383850970bba81

Observation 139064ff-59b3-4034-a4b1-0c700e38d715 · outbound

This paper cites Monte-Carlo neutrino transport in neutron star merger simulations.

On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations Monte-Carlo neutrino transport in neutron star merger simulations

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-16T04:59:40.313539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:59:40.313539Z digest=sha256:28abea59f12340c4b2f855d8d143987383ae339223f77dcf9ae8d412ce4cd223

Pith citing papers

Observation f786a786-b7f1-4864-9ec4-5ee483601005 · 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 On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-06-29T10:13:18.040024Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-06-29T10:03:39.187375Z digest=sha256:4d80f1d172549ba0a2818127395871d487f9253be0e1cca031afca6e2bf52ed2

Observation a7d16d93-8252-49a6-a7a4-78d816c418c7 · inbound

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers cites this paper.

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers On the difficulty of capturing the distribution function of neutrinos in neutron star merger simulations

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-07-01T18:45:59.207776Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-06-29T01:37:25.342025Z digest=sha256:ac41600eee1ca19844e74f38f6850d3f7e6787bbbd1095fc897a88eaf7471dcc