Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2105.04629.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:50:24.776698Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-01T12:05:42.997528Z
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 61ab390d-bc8a-4fd5-9ccc-949073a9b406 · inbound
Simultaneous description of high density QCD matter in heavy ion collisions and neutron star observations cites this paper.
Simultaneous description of high density QCD matter in heavy ion collisions and neutron star observations Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 42
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-10T16:50:24.776698Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5b9613c0-77dc-4c2b-97ee-186a1d2b6cf5 · inbound
Kaon Modification in Pion Medium cites this paper.
Kaon Modification in Pion Medium Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T17:47:56.924339Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 43fb7420-0adf-4e58-bb7d-276cd1bd3b6b · inbound
Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries cites this paper.
Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T10:19:22.530314Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 328c6730-5d6f-4a11-8664-32f1e4fd80c3 · inbound
Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter cites this paper.
Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 43
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T00:00:31.483864Z
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.
Observation bea3db85-cbe9-4d55-8010-3dbba4a9a893 · inbound
Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter cites this paper.
Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T23:10:16.355514Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aa13c2bc-f76f-4cbd-a483-839b8daacb74 · inbound
Resolution-matched nuclear geometry and the nucleon-size ambiguity in relativistic heavy-ion collisions cites this paper.
Resolution-matched nuclear geometry and the nucleon-size ambiguity in relativistic heavy-ion collisions Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T22:01:53.559815Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5a671fb1-b9b3-4f60-9cf9-ee03d073d898 · inbound
Cooling of Hybrid Stars with a 2SC+$<dd>$ Phase cites this paper.
Cooling of Hybrid Stars with a 2SC+$<dd>$ Phase Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T12:05:42.999277Z
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.
Observation 6be29e9d-731a-4fd6-a804-82838046236f · inbound
Cooling of Hybrid Stars with a 2SC+$<dd>$ Phase cites this paper.
Cooling of Hybrid Stars with a 2SC+$<dd>$ Phase Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:06:07.075111Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0e293f02-162c-4ecf-9d46-a10f37cbba9f · inbound
Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars cites this paper.
Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T16:06:33.449984Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.