Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-12T14:48:39.985824Z
Paper Citation Record · LEDGER
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
As of 21 August 2026, this Paper Citation Record lists 79 of 79 outbound references and 3 inbound Pith citation observations for arXiv:2411.14930.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:28:07.416341Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T22:47:13.386560Z
Reference resolution
79 of 79 outbound references displayed
- verified exact11
- verified fuzzy9
- unresolved59
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 79ff458c-20cc-4965-a5bb-d9a900eef2e5 · outbound
This paper cites New constraints on radii and tidal deformabilities of neutron stars from GW170817.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state New constraints on radii and tidal deformabilities of neutron stars from GW170817
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.623289Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5f4c1195-e3d6-4002-ae07-0a51655d24cd · outbound
This paper cites From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.628866Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 14584ece-9cfb-4694-840a-1bf10f48763e · outbound
This paper cites Interacting quark matter equation of state for compact stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Interacting quark matter equation of state for compact stars
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.633221Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 241f6fc9-4125-40ab-8bf1-87e5a07d8a07 · outbound
This paper cites Constraining neutron star matter with QCD.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Constraining neutron star matter with QCD
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.637758Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fee429bc-a871-4cb0-b324-37f14bb31ede · outbound
This paper cites Equation of state and neutron star properties constrained by nuclear physics and observation.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Equation of state and neutron star properties constrained by nuclear physics and observation
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.642359Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 23e6d826-57f2-45e4-b3e3-d46edd2b0da5 · outbound
This paper cites Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.647554Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 031384af-8701-424e-a890-324de4420957 · outbound
This paper cites Statistical Model for a Complete Supernova Equation of State.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Statistical Model for a Complete Supernova Equation of State
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.653024Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4b9310ad-36e0-447e-8812-e8fa182ef2e9 · outbound
This paper cites New Equations of State in Simulations of Core-Collapse Supernovae.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state New Equations of State in Simulations of Core-Collapse Supernovae
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.657712Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 01247319-fe17-440d-8022-99aa9201593c · outbound
This paper cites Neutron matter at finite temperature based on chiral effective field theory interactions.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Neutron matter at finite temperature based on chiral effective field theory interactions
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.662690Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 08459f19-4e3d-4524-98e5-9bd796b5e18c · outbound
This paper cites Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.667616Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 943c4443-37d0-41b6-97c4-bb09831ec596 · outbound
This paper cites Tabulated Equations of State From Models Informed by Chiral Effective Field Theory.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Tabulated Equations of State From Models Informed by Chiral Effective Field Theory
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.672354Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 39e321b7-4b22-4e1f-b00a-d567849dc0da · outbound
This paper cites Pulsar J0453+1559: A Double Neutron Star System with a Large Mass Asymmetry.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Pulsar J0453+1559: A Double Neutron Star System with a Large Mass Asymmetry
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.677149Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9f7245e6-58ff-4846-8d17-780fb74ebe84 · outbound
This paper cites Doroshenko, V.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Doroshenko, V
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:42.014097Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 318aa8cd-6f6e-485e-9e79-4d6af992b4b5 · outbound
This paper cites On the minimum mass of neutron stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state On the minimum mass of neutron stars
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.686203Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e15ae581-ac13-423a-a31e-4609666f1f39 · outbound
This paper cites Stockinger et al., Mon.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Stockinger et al., Mon
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.691139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4e2a8791-2773-48a1-bc8d-4578da5bc581 · outbound
This paper cites The minimum neutron star mass in neutrino-driven supernova explosions.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state The minimum neutron star mass in neutrino-driven supernova explosions
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.695483Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e3e12da0-e2f5-410e-90ec-d8517b5e3fc0 · outbound
This paper cites A NICER View of PSR J1231$-$1411: A Complex Case.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state A NICER View of PSR J1231$-$1411: A Complex Case
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.700322Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d032ea5f-b7f1-4da4-8e3b-17407340f0e9 · outbound
This paper cites Burrows and J.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Burrows and J
Reference 18
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.999806Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 25d2db5e-ac24-4a34-801b-606f7c573714 · outbound
This paper cites Burrows and J.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Burrows and J
Reference 19
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.983914Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation f02b0ce6-5d3d-4bf7-b671-0fe37e2ad8a0 · outbound
This paper cites Ledoux-Convection in Protoneutron Stars --- a Clue to Supernova Nucleosynthesis?.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Ledoux-Convection in Protoneutron Stars --- a Clue to Supernova Nucleosynthesis?
Reference 20
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:41.115370Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation fe1730c3-80dd-4eeb-bcdf-f81d283ab87b · outbound
This paper cites Proto-neutron star evolution with improved charged-current neutrino-nucleon interactions.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Proto-neutron star evolution with improved charged-current neutrino-nucleon interactions
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.718061Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation da2f933d-db03-43db-9a83-606f83773d87 · outbound
This paper cites Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.722077Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b439c242-b05f-4a44-8048-9f9a1c4dbdc7 · outbound
This paper cites Supernova Neutrinos: Production, Oscillations and Detection.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Supernova Neutrinos: Production, Oscillations and Detection
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.726108Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 00ee69cb-307c-4d5a-89a3-2948804c7f8b · outbound
This paper cites A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.730285Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b918648c-c52a-4fdd-9e42-1ff4bc4f51e5 · outbound
This paper cites Supernova Simulations Confront SN 1987A Neutrinos.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Supernova Simulations Confront SN 1987A Neutrinos
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.734986Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cbbc7ba9-9d7d-4856-950e-9a5639601af4 · outbound
This paper cites Haines et al.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Haines et al
Reference 26
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.895876Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 2b65fb69-81de-4272-a0df-55f210fdcfe9 · outbound
This paper cites Dessart, A.
Reference 27
- Resolution
- verified exact
- raw_fallback, observed 2026-08-12T14:48:40.996537Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 2f005126-0064-4964-8660-eab6b7ea5c52 · outbound
This paper cites Early evolution of newly born proto-neutron stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Early evolution of newly born proto-neutron stars
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.892481Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 4ac5d841-c449-43bf-a67f-9da2855f8b51 · outbound
This paper cites Buras, H.
Reference 29
- Resolution
- verified exact
- raw_fallback, observed 2026-08-12T14:48:40.870546Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 8b73ccbd-591e-4c56-8a1e-412265c96ba2 · outbound
This paper cites Composition and Structure of Protoneutron Stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Composition and Structure of Protoneutron Stars
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.758517Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6261fb97-9170-4272-8f5e-7b8e0f126169 · outbound
This paper cites Neutrino Propagation In Color Superconducting Quark Matter.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Neutrino Propagation In Color Superconducting Quark Matter
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.763216Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2ace2905-0bce-4907-8057-24582db13299 · outbound
This paper cites Strange Quark Matter and Compact Stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Strange Quark Matter and Compact Stars
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.767801Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5e4a8bbd-11d4-4b7c-8d49-b7973ef1193a · outbound
This paper cites NJL-model analysis of dense quark matter.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state NJL-model analysis of dense quark matter
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.772258Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cf9ce2c1-e442-440f-8d90-a7fb89f7dabf · outbound
This paper cites Signals of the QCD phase transition in core-collapse supernovae.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Signals of the QCD phase transition in core-collapse supernovae
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.777106Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 674c47ff-75c9-404c-9319-413cefeaeb46 · outbound
This paper cites Do hyperons exist in the interior of neutron stars ?.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Do hyperons exist in the interior of neutron stars ?
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.781871Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fc790462-d27a-466d-a66a-6eed57f75243 · outbound
This paper cites Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site
Reference 36
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.703414Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 70fe3a06-4c48-44b0-b45f-4dd33b5aa7b0 · outbound
This paper cites Gondek, P.
Reference 37
- Resolution
- verified exact
- raw_fallback, observed 2026-08-12T14:48:40.679991Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 516cce95-2a01-40d3-93fb-66d1393ac3a8 · outbound
This paper cites Proto-Neutron and Neutron Stars in a Chiral SU(3) Model.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Proto-Neutron and Neutron Stars in a Chiral SU(3) Model
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.795384Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63300a19-4693-494c-b4e2-de2858bad8f0 · outbound
This paper cites The maximum and minimum mass of protoneutron stars in the Brueckner theory.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state The maximum and minimum mass of protoneutron stars in the Brueckner theory
Reference 39
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.582602Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 21658481-ff74-4f13-b81f-90c51a02d7c9 · outbound
This paper cites Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.804693Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6844ff18-cdb4-4ed8-a2ee-f4873e405d12 · outbound
This paper cites Neutron matter from chiral effective field theory interactions.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Neutron matter from chiral effective field theory interactions
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.809400Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 849f06c2-53e2-46af-91f0-71d581a2fc9e · outbound
This paper cites Composition and thermodynamics of nuclear matter with light clusters.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Composition and thermodynamics of nuclear matter with light clusters
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.814232Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation afda7189-a8ae-48ae-a03a-641dc8c762db · outbound
This paper cites Core-collapse supernova equations of state based on neutron star observations.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Core-collapse supernova equations of state based on neutron star observations
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.818546Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b87bc62e-b19b-4ef2-ac02-d0dbfce35a2b · outbound
This paper cites Neutrino Emission from Supernovae.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Neutrino Emission from Supernovae
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.823073Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cd970559-05f6-4d1f-a4f5-cafdbe4e9336 · outbound
This paper cites Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.450433Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 556760d5-51b9-401a-9eca-abb5d438c522 · outbound
This paper cites Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.832369Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3bbd90c6-82bd-46f5-8c74-a1dcfcb54c11 · outbound
This paper cites Astrophysical Axion Bounds: The 2024 Edition.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Astrophysical Axion Bounds: The 2024 Edition
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.837207Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d8c73d6d-a6c9-49c6-a4a3-77b1c15b4e6e · outbound
This paper cites Symmetry energy impact in simulations of core-collapse supernovae.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Symmetry energy impact in simulations of core-collapse supernovae
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.842810Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 93f0ac9a-6754-4106-a524-8ffa27e3fd63 · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.847368Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 81a3a3fe-e276-4daf-9a3e-f40fa004592d · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 50
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T14:48:41.792295Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 9bbf6308-7ed5-4d4e-82f3-18760c11ca72 · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 51
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T14:48:41.777028Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 3c7c5c40-bf49-464a-b402-e430825bd805 · outbound
This paper cites Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.861567Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ecc7033b-ad3a-4d60-b053-6cf20dd7264a · outbound
This paper cites Explosion Mechanisms of Core-Collapse Supernovae.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Explosion Mechanisms of Core-Collapse Supernovae
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.866293Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df5be244-a8ed-4364-bdef-40b5d0a73d80 · outbound
This paper cites What Can the Accretion Induced Collapse of White Dwarfs Really Explain?.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state What Can the Accretion Induced Collapse of White Dwarfs Really Explain?
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.871151Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 48a70c58-5602-4b0b-91e0-a54dfef3e612 · outbound
This paper cites The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
Reference 55
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.875749Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 471ed481-24ae-4dc9-904b-3c7335481227 · outbound
This paper cites Multimessenger Emission from the Accretion Induced Collapse of White Dwarfs.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Multimessenger Emission from the Accretion Induced Collapse of White Dwarfs
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.880455Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 11f78fc8-8810-4c87-b647-6601faaa04d9 · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.884595Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b187d420-1360-4090-abfa-152ecb15ec72 · outbound
This paper cites Tolman and P.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Tolman and P
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.888737Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b542c2cd-65db-435d-871f-af9b60e02794 · outbound
This paper cites Klein, Reviews of Modern Physics 21, 531 (1949).
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Klein, Reviews of Modern Physics 21, 531 (1949)
Reference 59
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.742474Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 0ff211e5-6f98-4378-ade9-56a989fad9cd · outbound
This paper cites Thermodynamic Equilibrium in General Relativity.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Thermodynamic Equilibrium in General Relativity
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.896975Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 241407b3-7bbc-4ce8-b81b-8f19bad07cec · outbound
This paper cites A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.901830Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f772cbd7-db97-42d2-b4da-e6bb9bc0bcfe · outbound
This paper cites Goussard, P.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Goussard, P
Reference 62
- Resolution
- verified exact
- raw_fallback, observed 2026-08-12T14:48:40.246074Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 25bd8d13-e3aa-49e2-8755-e0d44635e9e1 · outbound
This paper cites Keil and H.
Reference 63
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.727070Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 3ecd46ac-aaf6-41da-85b1-fbb046e9fe19 · outbound
This paper cites Prakash, J.
Reference 64
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.711900Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation bf07ceff-d0d7-4863-af91-d64ffa84405c · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 65
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T14:48:41.694883Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation cabe3c65-6aba-402d-82f8-bcda3806c535 · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 66
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T14:48:41.578867Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation d43fc115-7d89-4db1-baa2-4dbb493d5568 · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 67
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T14:48:41.517994Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation dae236d2-991d-4193-8e73-38d33db55a33 · outbound
This paper cites an unresolved cited work.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Unresolved cited work
Reference 68
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T14:48:41.503813Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 9535502e-0e94-44df-9bf3-755909f9582c · outbound
This paper cites Kampfer, J.
Reference 69
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.488902Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 0557b78c-6818-4b7c-8155-4ec2695a12ec · outbound
This paper cites Non-Identical Neutron Star Twins.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Non-Identical Neutron Star Twins
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.942790Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a0645001-5f0e-4e9c-b039-48e808fabc88 · outbound
This paper cites Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.947665Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a8e08668-66e4-4296-be93-5203ed6bb27f · outbound
This paper cites Twin Stars within the SU(3) Chiral Quark-Meson Model.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Twin Stars within the SU(3) Chiral Quark-Meson Model
Reference 72
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.128928Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 21e25015-a89c-480c-8fbf-eec1e76dfa67 · outbound
This paper cites Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.957220Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 51a165d6-1815-4150-9c89-4b488be6c318 · outbound
This paper cites Phase Transition to Hyperon Matter in Neutron Stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Phase Transition to Hyperon Matter in Neutron Stars
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.962435Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c3a60e4-59fb-4a74-80f8-ab82b8a9199a · outbound
This paper cites Chabanat, J.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Chabanat, J
Reference 75
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T14:48:41.474949Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 9f0677df-f4ed-45ab-9eea-c35c5897e7e5 · outbound
This paper cites Conditions for Phase Equilibrium in Supernovae, Proto-Neutron and Neutron Stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Conditions for Phase Equilibrium in Supernovae, Proto-Neutron and Neutron Stars
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.971866Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 31ef2cdd-eb5d-4455-9528-d535eb65681b · outbound
This paper cites A new possible quark-hadron mixed phase in protoneutron stars.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state A new possible quark-hadron mixed phase in protoneutron stars
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.976765Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1d723bca-f28c-44e5-b9e3-f8ec9179290a · outbound
This paper cites Hot third family of compact stars and the possibility of core-collapse supernova explosions.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Hot third family of compact stars and the possibility of core-collapse supernova explosions
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.046932Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 1c47bb8d-4575-400a-9e41-4c94448da071 · outbound
This paper cites Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:48:39.985824Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation f01a286e-88d8-41ea-806f-82b5b98d0a6a · inbound
Strongly Interacting Dark Matter admixed Neutron Stars cites this paper.
Strongly Interacting Dark Matter admixed Neutron Stars Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T22:47:13.389016Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation b777e559-8910-49d8-ac41-b57bbc7e6727 · inbound
Constraints on maximum neutron star mass from proto-neutron star evolution cites this paper.
Constraints on maximum neutron star mass from proto-neutron star evolution Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:28:07.416341Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 67f55096-33ec-4304-9abf-5827ab0f3811 · inbound
The petit four of color-superconducting phases in proto-neutron star evolution cites this paper.
The petit four of color-superconducting phases in proto-neutron star evolution Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T04:54:21.953406Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.