Pith. sign in

Paper Citation Record · LEDGER

Employing deep-learning techniques for the conservative-to-primitive recovery in binary neutron star simulations

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2503.08289.

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

pith.paper-citation-record.v1
2503.08289 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:28:25.293324Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T07:29:39.528067Z

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 b588c6ad-7c05-4de6-8fc0-1211f0f75d08 · inbound

A "Neural" Riemann solver for Relativistic Hydrodynamics cites this paper.

A "Neural" Riemann solver for Relativistic Hydrodynamics Employing deep-learning techniques for the conservative-to-primitive recovery in binary neutron star simulations

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-07T14:28:25.293324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:28:25.293324Z digest=sha256:e55a0461c9802baea01251b82d3ce1c08c5aea90115142e6faa289bea0a998d7

Observation 1758ad42-2fd3-4cc8-8f34-67c8a122fe09 · inbound

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning cites this paper.

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning Employing deep-learning techniques for the conservative-to-primitive recovery in binary neutron star simulations

Reference 79

Resolution
verified exact
arxiv_id, observed 2026-07-04T07:29:39.529589Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-26T13:20:12.147520Z digest=sha256:3507bfca37993cbe6c125e3ba69ddf108483da4b7ebecd64d9c26c93ff982598