Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:15:02.503901Z
Paper Citation Record · LEDGER
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
As of 16 August 2026, this Paper Citation Record lists 48 of 48 outbound references and 0 inbound Pith citation observations for arXiv:1908.09534.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
48 of 48 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation a057bc98-677d-4467-bafc-8c22ac51f785 · outbound
This paper cites Three Lectures on Hadron Physics.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Three Lectures on Hadron Physics
Reference 1
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- raw_fallback, observed 2026-08-14T11:15:03.085733Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation eb75b26d-1c5f-46ed-b3d0-ffb8eb926ea1 · outbound
This paper cites Critical point of QCD at finite T and mu, lattice results for physical quark masses.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Critical point of QCD at finite T and mu, lattice results for physical quark masses
Reference 2
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- raw_fallback, observed 2026-08-14T11:15:03.074639Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 0fdd931c-eac6-43a6-8512-417920da4acd · outbound
This paper cites The Order of the quantum chromodynamics transition predicted by the standard model of particle physics.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars The Order of the quantum chromodynamics transition predicted by the standard model of particle physics
Reference 3
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- raw_fallback, observed 2026-08-14T11:15:03.063029Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c247bad2-1b55-45b4-8d9c-97c8cf275ea6 · outbound
This paper cites The QCD Equation of State toO(µ6 B) from Lattice QCD.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars The QCD Equation of State toO(µ6 B) from Lattice QCD
Reference 4
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- raw_fallback, observed 2026-08-14T11:15:03.050146Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 417d36eb-ff8d-4885-b571-6b6cd614ebd4 · outbound
This paper cites The QCD equation of state at finite density from analytical continuation.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars The QCD equation of state at finite density from analytical continuation
Reference 5
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:03.039060Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c30e1158-c892-4b1d-bb45-905959d8ce41 · outbound
This paper cites Chiral crossover in QCD at zero and non-zero chemical potentials.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Chiral crossover in QCD at zero and non-zero chemical potentials
Reference 6
- Resolution
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- no resolver link, observed 2026-08-14T11:15:02.344628Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 13e9e66f-1e6c-449a-9610-96d3a9b83a8a · outbound
This paper cites Towards a Unified Quark-Hadron Matter Equation of State for Applications in Astrophysics and Heavy-Ion Collisions.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Towards a Unified Quark-Hadron Matter Equation of State for Applications in Astrophysics and Heavy-Ion Collisions
Reference 7
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- raw_fallback, observed 2026-08-14T11:15:03.027706Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 03a3d603-64e8-479a-a270-01a71a3297d6 · outbound
This paper cites A Novel Approach to Model Hybrid Stars.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars A Novel Approach to Model Hybrid Stars
Reference 8
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:03.016715Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6092fd08-5018-41be-a26a-c94e517a39b6 · outbound
This paper cites An Effective chiral Hadron-Quark Equation of State.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars An Effective chiral Hadron-Quark Equation of State
Reference 9
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:03.004945Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 001a7a0b-6929-42b9-9b5c-749fadd497eb · outbound
This paper cites Net-baryon number fluctuations in the Hybrid Quark-Meson-Nucleon model at finite density.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Net-baryon number fluctuations in the Hybrid Quark-Meson-Nucleon model at finite density
Reference 10
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- raw_fallback, observed 2026-08-14T11:15:02.993482Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 0bb5c5a7-3875-4a70-8eb3-767197cc1974 · outbound
This paper cites Chiral symmetry restoration by parity doubling and the structure of neutron stars.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Chiral symmetry restoration by parity doubling and the structure of neutron stars
Reference 11
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- raw_fallback, observed 2026-08-14T11:15:02.980520Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 400a9d2f-87d6-43a4-8280-17e12a478dc9 · outbound
This paper cites Quarks and Gluons at High Temperatures and Densities.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Quarks and Gluons at High Temperatures and Densities
Reference 12
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- raw_fallback, observed 2026-08-14T11:15:02.968912Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 3954d665-2bf6-4774-a2d3-1c6cfb7bdab3 · outbound
This paper cites Equations of state for supernovae and compact stars.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Equations of state for supernovae and compact stars
Reference 13
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- raw_fallback, observed 2026-08-14T11:15:02.957280Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c1fff2e4-4702-4149-a36b-8d32ef833405 · outbound
This paper cites The state of matter in simulations of core-collapse supernovae—Reflections and recent developments.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars The state of matter in simulations of core-collapse supernovae—Reflections and recent developments
Reference 14
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- raw_fallback, observed 2026-08-14T11:15:02.945456Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 69587593-b1b4-4a01-8b4b-b62072b6c1dd · outbound
This paper cites Strange Matter.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Strange Matter
Reference 15
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 07d3849c-71e6-40fa-875e-d359c1353871 · outbound
This paper cites Shapiro Delay Measurement of A Two Solar Mass Neutron Star.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Shapiro Delay Measurement of A Two Solar Mass Neutron Star
Reference 16
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- raw_fallback, observed 2026-08-14T11:15:02.922701Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 11cc764a-ba81-41df-942e-f6527cf8bb30 · outbound
This paper cites The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars
Reference 17
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- raw_fallback, observed 2026-08-14T11:15:02.911663Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 359dbe19-43b0-496b-90e3-84027a156763 · outbound
This paper cites A Massive Pulsar in a Compact Relativistic Binary.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars A Massive Pulsar in a Compact Relativistic Binary
Reference 18
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 1427fa1e-e43f-48a8-ab68-c357023bb0c6 · outbound
This paper cites Vector interaction enhanced bag model for astrophysical applications.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Vector interaction enhanced bag model for astrophysical applications
Reference 19
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- raw_fallback, observed 2026-08-14T11:15:02.888359Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e02aed0f-a050-4f38-bc01-1d74397a1d22 · outbound
This paper cites Simultaneous chiral symmetry restoration and deconfinement— Consequences for the QCD phase diagram.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Simultaneous chiral symmetry restoration and deconfinement— Consequences for the QCD phase diagram
Reference 20
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- raw_fallback, observed 2026-08-14T11:15:02.876405Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 11c1965f-c23c-4d3d-a87b-862683d0f1cc · outbound
This paper cites Consequences of simultaneous chiral symmetry breaking and deconfinement for the isospin symmetric phase diagram.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Consequences of simultaneous chiral symmetry breaking and deconfinement for the isospin symmetric phase diagram
Reference 21
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- raw_fallback, observed 2026-08-14T11:15:02.864268Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d54b27c5-4142-4356-8838-a6e6d0ede7e1 · outbound
This paper cites Vector-Interaction-Enhanced Bag Model.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Vector-Interaction-Enhanced Bag Model
Reference 22
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.852584Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 967b8e83-b026-406e-b8f2-e5ffe5ab6489 · outbound
This paper cites Phase diagram and critical endpoint for strongly-interacting quarks.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Phase diagram and critical endpoint for strongly-interacting quarks
Reference 23
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.841689Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 29ad8ac6-df1d-440b-8b55-d8878bb16096 · outbound
This paper cites Phase structure of three and four flavor QCD.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Phase structure of three and four flavor QCD
Reference 24
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.830442Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 7e1e4a89-c7ca-4b49-afe3-3d98c43eb0a7 · outbound
This paper cites Two point fermion correlation functions at finite density.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Two point fermion correlation functions at finite density
Reference 25
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 55725963-fbc7-4f10-85cf-5a4989a1b8e7 · outbound
This paper cites Dyson-Schwinger equations: Density, temperature and continuum strong QCD.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Dyson-Schwinger equations: Density, temperature and continuum strong QCD
Reference 26
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- raw_fallback, observed 2026-08-14T11:15:02.804774Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 1161c582-ca4a-4578-b9b8-b572ed15a8d2 · outbound
This paper cites Pion form factor from a contact interaction.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Pion form factor from a contact interaction
Reference 27
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.791312Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8cc52d3a-edd4-457e-92a6-eb4b1c0b6774 · outbound
This paper cites Dynamical chiral symmetry breaking, Goldstone’s theorem and the consistency of the Schwinger-Dyson and Bethe-Salpeter Equations.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Dynamical chiral symmetry breaking, Goldstone’s theorem and the consistency of the Schwinger-Dyson and Bethe-Salpeter Equations
Reference 28
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- raw_fallback, observed 2026-08-14T11:15:02.780081Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 3c2a795c-a254-404b-8d62-c14fa7de0372 · outbound
This paper cites Goldstone theorem and diquark confinement beyond rainbow ladder approximation.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Goldstone theorem and diquark confinement beyond rainbow ladder approximation
Reference 29
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- raw_fallback, observed 2026-08-14T11:15:02.767723Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 61851e81-518a-47bc-a8d1-266a7a38a045 · outbound
This paper cites NJL model analysis of quark matter at large density.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars NJL model analysis of quark matter at large density
Reference 30
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- raw_fallback, observed 2026-08-14T11:15:02.755189Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 58061926-42f5-44f0-a422-7f7090db5dc4 · outbound
This paper cites Extended NJL model for light and heavy mesons without q- anti-q thresholds.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Extended NJL model for light and heavy mesons without q- anti-q thresholds
Reference 31
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- raw_fallback, observed 2026-08-14T11:15:02.744168Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 297482ea-c145-4206-900d-48ddc87a6c8c · outbound
This paper cites Composition and thermodynamics of nuclear matter with light clusters.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Composition and thermodynamics of nuclear matter with light clusters
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T11:15:02.442495Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc4a6d69-ef60-4049-80e2-8fccc21b47c6 · outbound
This paper cites A New parametrization for the Lagrangian density of relativistic mean field theory.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars A New parametrization for the Lagrangian density of relativistic mean field theory
Reference 33
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- raw_fallback, observed 2026-08-14T11:15:02.726355Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5955b588-6a12-440a-a4fe-13d55c5d4239 · outbound
This paper cites Asymmetric nuclear matter in a parity doublet model with hidden local symmetry.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Asymmetric nuclear matter in a parity doublet model with hidden local symmetry
Reference 34
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- raw_fallback, observed 2026-08-14T11:15:02.715633Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 4d744974-bcc9-4438-a651-97a27b543498 · outbound
This paper cites Constraining the Symmetry Parameters of the Nuclear Interaction.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Constraining the Symmetry Parameters of the Nuclear Interaction
Reference 35
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.704643Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation be01de28-b40f-448e-af2e-40b9f80429bb · outbound
This paper cites Nuclear energy density optimization: Large deformations.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Nuclear energy density optimization: Large deformations
Reference 36
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.693203Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d641f0a2-894b-4901-8f82-229e1aade919 · outbound
This paper cites an unresolved cited work.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Unresolved cited work
Reference 37
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T11:15:02.680903Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation daf934e3-1206-41db-8f2d-7e57eba3e04e · outbound
This paper cites Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817
Reference 38
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.670006Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation dca100f7-673f-4633-b94d-807f20d46e2d · outbound
This paper cites First results on the equation of state constraints from NICER.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars First results on the equation of state constraints from NICER
Reference 39
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.657911Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8a6fde29-6b95-4769-9662-a8ede13e166d · outbound
This paper cites The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars
Reference 40
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.647010Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6d683b55-aaf1-4767-820c-78f95bd09cf1 · outbound
This paper cites Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T11:15:02.476575Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 24ce5bc7-4a22-44a6-81e0-e3085f8fe5d9 · outbound
This paper cites Identifying a first-order phase transition in neutron star mergers through gravitational waves.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Identifying a first-order phase transition in neutron star mergers through gravitational waves
Reference 42
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.635606Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 86d305e2-d5b6-430f-b150-f0245b3e7a97 · outbound
This paper cites A new quark-hadron hybrid equation of state for astrophysics - I.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars A new quark-hadron hybrid equation of state for astrophysics - I
Reference 43
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.623835Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 585b74a0-c47a-4814-ba4c-05edab5eff77 · outbound
This paper cites Detectability of strange matter in heavy ion experiments.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Detectability of strange matter in heavy ion experiments
Reference 44
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.611860Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5b97fe01-2c3c-4efb-9164-c2be7d96d226 · outbound
This paper cites Hyperons and massive neutron stars: Vector repulsion and SU(3) symmetry.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Hyperons and massive neutron stars: Vector repulsion and SU(3) symmetry
Reference 45
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.598466Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 683a698d-5b21-447f-a658-78f8077efb23 · outbound
This paper cites Hyperons in hot dense matter: what do the constraints tell us for equation of state? Publ.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Hyperons in hot dense matter: what do the constraints tell us for equation of state? Publ
Reference 46
- Resolution
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- raw_fallback, observed 2026-08-14T11:15:02.585958Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation acd3ff07-f762-4ffb-af4a-6ce436e31558 · outbound
This paper cites Cosmic Separation of Phases.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Cosmic Separation of Phases
Reference 47
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.573060Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 31c73b95-5b21-41c5-9ecd-44bba1f52c3e · outbound
This paper cites Strange quark stars.
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars Strange quark stars
Reference 48
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T11:15:02.560748Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Pith citing papers
No inbound Pith citation observations are available.