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Paper Citation Record · LEDGER

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition

As of 16 August 2026, this Paper Citation Record lists 100 of 296 outbound references and 0 inbound Pith citation observations for arXiv:2608.12632.

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

pith.paper-citation-record.v1
2608.12632 v1

Coverage vector

measured 100 of 296 reference resolution

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Reference resolution

100 of 296 outbound references displayed

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Outbound references

Observation a9efdcac-b0ce-4183-9d2d-3432b14171cb · outbound

This paper cites Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars

Reference 1

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Observation e86d38b1-77af-4c5c-a129-b7a98b11defb · outbound

This paper cites Investigating Twin Star Equation of States in Light of Recent Astrophysical Observations.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Investigating Twin Star Equation of States in Light of Recent Astrophysical Observations

Reference 2

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Observation 1d8595d7-63b6-43d0-a939-f3bae6fbbe14 · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 3

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Observation 4c4e31b8-4823-402c-94de-f8d840b44f36 · outbound

This paper cites Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State

Reference 4

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Observation 500e6159-9b6e-46d8-ac15-2ae1e174103f · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 5

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Observation eef706a4-cda3-4cec-bef9-91ad4841621a · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 6

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Observation ff299539-979b-43ad-9366-3482682ac79c · outbound

This paper cites Constraining twin stars with cold neutron star cooling data.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Constraining twin stars with cold neutron star cooling data

Reference 7

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Observation 6ae90bbb-21c9-4d6c-8fd4-b06390ae8edf · outbound

This paper cites Hybrid stars with large quark cores within the parity doublet model and modified NJL model.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Hybrid stars with large quark cores within the parity doublet model and modified NJL model

Reference 8

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Observation 09b91625-20b5-450b-96be-ded217d4c8f6 · outbound

This paper cites Confirming the Existence of Twin Stars in a.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Confirming the Existence of Twin Stars in a

Reference 9

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Observation 639399c0-d41a-4475-beaf-321d6e579349 · outbound

This paper cites Ultracompact hybrid stars consistent with multimessenger astrophysics.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Ultracompact hybrid stars consistent with multimessenger astrophysics

Reference 10

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Observation 03b46342-5e5d-49ef-adc0-84520560f1aa · outbound

This paper cites Comparison of Equations of State for Neutron Stars with First-Order Phase Transitions: A Qualitative Study.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Comparison of Equations of State for Neutron Stars with First-Order Phase Transitions: A Qualitative Study

Reference 11

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Observation d5ad3998-6b16-411b-8cbc-560f5e6ceebb · outbound

This paper cites Is the central compact object in HESS J1731-347 a hybrid star with a quark core? An analysis with the constant speed of sound parametrization.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Is the central compact object in HESS J1731-347 a hybrid star with a quark core? An analysis with the constant speed of sound parametrization

Reference 12

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Observation 47681be3-e496-42e0-b8b0-0f46e79f7a04 · outbound

This paper cites Properties of the Object HESS J1731-347 as a Twin Compact Star.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Properties of the Object HESS J1731-347 as a Twin Compact Star

Reference 13

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Observation 4c2057ea-d08f-4498-aeb7-be2f778a2623 · outbound

This paper cites Twin Stars and the Stiffness of the Nuclear Equation of State:.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Twin Stars and the Stiffness of the Nuclear Equation of State:

Reference 14

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Observation 9629bc02-eedc-4561-89a1-f3922c8cc48f · outbound

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How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 15

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Observation 58de4236-3b8c-4643-bb57-136108206aca · outbound

This paper cites and Koliogiannis, P.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition and Koliogiannis, P

Reference 17

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Observation 28f56b99-9eb3-4b27-a8f4-d1b86466d9bb · outbound

This paper cites Constraining twin stars with GW170817.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Constraining twin stars with GW170817

Reference 18

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Observation a4f80822-aca1-4cca-b891-df827f6a0165 · outbound

This paper cites Constraints on strong phase transitions in neutron stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Constraints on strong phase transitions in neutron stars

Reference 20

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Observation d4493e31-3c99-4f65-b3cd-5eeb907fde0b · outbound

This paper cites Hybrid star properties with the NJL and mean field approximation of QCD models: A Bayesian approach.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Hybrid star properties with the NJL and mean field approximation of QCD models: A Bayesian approach

Reference 21

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Observation 4c0c721e-282d-41ec-8a0f-d1765248e01e · outbound

This paper cites Hybrid Star Models in the Light of New Multimessenger Data , volume=.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Hybrid Star Models in the Light of New Multimessenger Data , volume=

Reference 22

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Observation 5cde9147-5690-4d51-a012-385b0da45580 · outbound

This paper cites New class of hybrid EoS and Bayesian M-R data analysis.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition New class of hybrid EoS and Bayesian M-R data analysis

Reference 23

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How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 24

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This paper cites On the Possibility of Stable Quark and Pion Condensed Stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition On the Possibility of Stable Quark and Pion Condensed Stars

Reference 25

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This paper cites Phase Transitions in Neutron Stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Phase Transitions in Neutron Stars

Reference 26

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Observation d250f4d9-ebfd-4964-9eb9-d8c3bfe2f2dc · outbound

This paper cites Signals of the QCD phase transition in core-collapse supernovae.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Signals of the QCD phase transition in core-collapse supernovae

Reference 27

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Observation 72c0c5cd-94e3-4375-9b00-5254630b0c61 · outbound

This paper cites Accessibility of color superconducting quark matter phases in heavy-ion collisions.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Accessibility of color superconducting quark matter phases in heavy-ion collisions

Reference 28

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This paper cites Non-Identical Neutron Star Twins.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Non-Identical Neutron Star Twins

Reference 29

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How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition and Greiner, C

Reference 30

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This paper cites Trace anomaly as signature of conformality in neutron stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Trace anomaly as signature of conformality in neutron stars

Reference 31

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This paper cites Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Formation of twin compact stars in low-mass X-ray binaries: Implications on eccentric and isolated millisecond pulsar populations

Reference 32

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Observation ebce2899-1f00-46b0-b667-3ea36adc6072 · outbound

This paper cites Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model

Reference 33

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Observation 00d9e6dd-8809-4bff-abb2-335eff3cba29 · outbound

This paper cites Simultaneous explanation of XTE J1814-338 and HESS J1731-347 objects using ${K^{-}}$ and ${\bar{K}^{0}}$ condensates.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Simultaneous explanation of XTE J1814-338 and HESS J1731-347 objects using ${K^{-}}$ and ${\bar{K}^{0}}$ condensates

Reference 34

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This paper cites Exploring pathways to forming twin stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Exploring pathways to forming twin stars

Reference 35

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This paper cites Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations

Reference 36

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This paper cites How the QCD trace anomaly behaves at the core of twin stars?.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition How the QCD trace anomaly behaves at the core of twin stars?

Reference 37

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This paper cites 2025 , version =.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition 2025 , version =

Reference 38

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.751481Z digest=sha256:e8e4fc81dccd34f08d388d8957845a09365a31baf3c6aac36ba3a4cdcdfd987f

Observation f63e1dd3-4bf5-46e1-b559-c4f0cfc48c70 · outbound

This paper cites Strange stars - linear approximation of the EOS and maximum QPO frequency.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Strange stars - linear approximation of the EOS and maximum QPO frequency

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.758072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.758072Z digest=sha256:fe9a741ad4f60ea101c020fe40b06637a0d327a75b80f156bf3f213c28c56432

Observation 179b007f-611f-4a02-b101-92f160e861b4 · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 40

Resolution
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no resolver link, observed 2026-08-16T00:09:04.800118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.800118Z digest=sha256:efec4c28e3ce47f6afa3a8e2eabce8693d96ebe50fb284a60a97666edb75a7a3

Observation d03e555d-d4ea-4537-8aba-c6a2b5a20eff · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.804502Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.804502Z digest=sha256:02829de509c1a849fcb5027faefc8f946fcbebfcbb88c8be3cd4b327cbf2bdcf

Observation 3e56a3f9-976c-4f48-b7fd-2019467c8da6 · outbound

This paper cites A Massive Pulsar in a Compact Relativistic Binary.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition A Massive Pulsar in a Compact Relativistic Binary

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.808351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.808351Z digest=sha256:ac943e6e3c2b16d75bf8b873ca41d3651cefb73a9d8d9bac312ab0e60035c339

Observation b72978b7-c438-4d55-8210-071dffb4f8bc · outbound

This paper cites A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.812525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.812525Z digest=sha256:809270669983dfcfda05b717fccee6163b297eb2baa66a3c6d3ef6763eda1408

Observation 1e333661-5fec-4524-ad8c-810e82481119 · outbound

This paper cites Quark-Nuclear Hybrid EoS with Excluded Volume Effects.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Quark-Nuclear Hybrid EoS with Excluded Volume Effects

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.816829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.816829Z digest=sha256:6843d4896aeecce1b7ca3f836864cf642c2dd2293648bb2f266cfe4984e28974

Observation 01b1e81c-7ea8-40bf-b2d2-69343e69db1e · outbound

This paper cites Third family of compact stars within a nonlocal chiral quark model equation of state.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Third family of compact stars within a nonlocal chiral quark model equation of state

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.821324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.821324Z digest=sha256:80a4a837602c14e4b8a8e9ec30e2930508a17bc349afd6ea5034309be066b07f

Observation e15a447b-693a-454e-8914-d5b89c019e59 · outbound

This paper cites Mixed phase effects on high-mass twin stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Mixed phase effects on high-mass twin stars

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.826381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.826381Z digest=sha256:751ed4347a30ded3d82f2c26fbff2252dfc2ebbce640d2f5622a520e65aaad84

Observation 1c629a14-3cab-4d25-b559-f67a06305daa · outbound

This paper cites Robustness of third family solutions for hybrid stars against mixed phase effects.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Robustness of third family solutions for hybrid stars against mixed phase effects

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.857036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.857036Z digest=sha256:5f0d175df3c37a8aa84ad0225cdcc63317f7f09a67dfd6be317b32772fbf8c89

Observation 2facf3cd-07df-4d79-9ca4-8e2bc1d05d6a · outbound

This paper cites Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.862396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.862396Z digest=sha256:a8a434b12b7ea2114dd004bd9e223f9a4cff08eb2266e277946e5cdee8b312a0

Observation bb20adc1-b4b4-426c-8f33-52433df62749 · outbound

This paper cites Tripling Fluctuations and Peaked Sound Speed in Fermionic Matter.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Tripling Fluctuations and Peaked Sound Speed in Fermionic Matter

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.867179Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.867179Z digest=sha256:ddfef23fc21b4d58273805aefd6bf9a325f1069e7a741f70e768a47e9e843ec8

Observation 9ec10476-ce20-40c1-82ae-df0c3e4e8b48 · outbound

This paper cites Bayesian inference favors quark matter in neutron star interiors.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Bayesian inference favors quark matter in neutron star interiors

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.872380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.872380Z digest=sha256:33db8875ea16b666876ea1486e3624e0b0cde4a9291e40073c1c203e956ea76f

Observation d96e041f-d178-4d25-a7b7-17d2e00bd47c · outbound

This paper cites Gravitational waves from neutron star mergers and their relation to the nuclear equation of state.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Gravitational waves from neutron star mergers and their relation to the nuclear equation of state

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.952945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.952945Z digest=sha256:8e8abd504f21223597091fc5f3a0e98f4b5bde82f00fab90c072bb70f4e7581e

Observation 5012a1dc-a565-4070-a4de-32b1bae43a4a · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.996351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.996351Z digest=sha256:8f3395785f218604aebd089f95a52ece34eb9eaa47d53e79898d932602766dae

Observation e4d1c11c-a705-4dbe-b2c3-9d0d5119a6ab · outbound

This paper cites Thankful and Gandolfi, Stefano and Tews, Ingo and Radice, David and Steiner, Andrew W.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Thankful and Gandolfi, Stefano and Tews, Ingo and Radice, David and Steiner, Andrew W

Reference 54

Resolution
malformed identifier
no resolver link, observed 2026-08-16T00:09:05.000739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.000739Z digest=sha256:c1018fbc999a2e603f8268d100655304cff5950b56c11bc6de105e52b258ace9

Observation 62b8226a-7378-4c5f-964f-b14301e17776 · outbound

This paper cites Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.005933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.005933Z digest=sha256:a4682c5da7b0317b98c1c670e9b973676587c14e3b8ebdbe6a20ac2b66e7825b

Observation 74cf75ba-97d4-4690-ac59-b844bdf6bd2d · outbound

This paper cites The NewAthena mission concept in the context of the next decade of X-ray astronomy.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition The NewAthena mission concept in the context of the next decade of X-ray astronomy

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.010672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.010672Z digest=sha256:29ab99e1937de11b92387cf35021f1fb32ae0786549e96576b88eb1ae3603bea

Observation baf6876a-d6d4-48b9-af63-c4a48ef87822 · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.016251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.016251Z digest=sha256:9522f40b01ed6b2df448ffb79f5cd10b319b4698ce837177895e499df12f33c2

Observation a71ef57f-3bfd-4490-aab0-06ef3a60ca3c · outbound

This paper cites Bernoulli.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Bernoulli

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.022362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.022362Z digest=sha256:a223ce1c0dc0dd4dca6130c19bd8951aaae41fb53a6a3cac5c6a517c31b27aa6

Observation 47336996-7f26-4fe0-bbb4-44e03080ddda · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.044993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.044993Z digest=sha256:6711542ca55469f1f0608bd875779b10bbcbc85f8dd4ed8665ea7b0e5104834d

Observation fde0c831-19d0-4fdb-8799-725ee78fcdd9 · outbound

This paper cites https://global.oup.com/academic/product/microeconomic-theory-9780195073409.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition https://global.oup.com/academic/product/microeconomic-theory-9780195073409

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.126339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.126339Z digest=sha256:96bc6cb38bf88a8abffc1c82ba69f4cca8ea57c0a56c928dec3063d3e0fc8c3c

Observation 1ff7c7dc-f3df-40a4-8e4a-972427ac466c · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.187554Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.187554Z digest=sha256:83abd047f9e3274e1d6da7e162596df0ed3ab23cb7b0e31d042dad4bc86ae4f0

Observation cb7a5f54-0ba9-424f-83e1-f3a2ddff96e2 · outbound

This paper cites Properties of the QCD Matter -- An Experimental Review of Selected Results from RHIC BES Program.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Properties of the QCD Matter -- An Experimental Review of Selected Results from RHIC BES Program

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.191994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.191994Z digest=sha256:4a0d93984c75a9156c6c55695dad7f3a63d571e73576c1d0b8836879614cc002

Observation b809b2a4-53ac-4ecc-8a7c-fe7a2d07813c · outbound

This paper cites Is there a "$\Delta$-isobar puzzle" in the physics of neutron stars?.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Is there a "$\Delta$-isobar puzzle" in the physics of neutron stars?

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.196570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.196570Z digest=sha256:d6abea82ac517b1964032d5b15d189aec63c21f253f9de8d9d586ff8d547c384

Observation 4fb18a29-e02e-4f34-a246-5fc096dca850 · outbound

This paper cites Critical Density and Impact of $\Delta (1232)$ Resonance Formation in Neutron Stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Critical Density and Impact of $\Delta (1232)$ Resonance Formation in Neutron Stars

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.201560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.201560Z digest=sha256:434111241bfd2bae663e95c65ef70b3e0e6b7f58ab3c1f39ee1f4ca2f00cc53f

Observation e4bb7a35-55c7-4aef-8510-0db5a9772cd1 · outbound

This paper cites Beyond ^ 2/3 Scaling: Microscopic Origins and Multimessengers of High-Density Nuclear Symmetry Energy.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Beyond ^ 2/3 Scaling: Microscopic Origins and Multimessengers of High-Density Nuclear Symmetry Energy

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.206838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.206838Z digest=sha256:917cac12587a93ee94af6be35e9f33ef7645904fa77241ab14c14d1bbd906548

Observation 2de6813a-08c3-4a24-8fd9-a7e5278d64fe · outbound

This paper cites Coleman and Lamb, Frederick K.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Coleman and Lamb, Frederick K

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.211921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.211921Z digest=sha256:6854b954be4bb28a72c5dae31abfe439e58d1bc52e7c15ede8e60495235cb0ea

Observation f941c840-16cb-40c4-b907-6b1133b3521e · outbound

This paper cites Dense matter in neutron stars with eXTP.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Dense matter in neutron stars with eXTP

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.216974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.216974Z digest=sha256:703f47e5d31c579b5b377fdb93353d1499236cdc4412774aa44ae395bf76acf8

Observation 7c52b9f7-f095-4d19-b4e6-1230935bc78b · outbound

This paper cites 2025 , note =.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition 2025 , note =

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.222054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.222054Z digest=sha256:80b0d472e9cb6a3b759cf1ebb70678d63b9ea691f37f5bb7884dbe48116f9871

Observation 806db9f6-ee21-4260-a68e-13d850b4666f · outbound

This paper cites Constraining a relativistic mean field model using neutron star mass-radius measurements II: Hyperonic models.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Constraining a relativistic mean field model using neutron star mass-radius measurements II: Hyperonic models

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.257404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.257404Z digest=sha256:31b947eddf7136f5655217d51679c6600bc6db2a33941b066730ae11435ae203

Observation f00138d9-db2d-4f8c-855a-c3546f020226 · outbound

This paper cites 2025 , note =.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition 2025 , note =

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.380708Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.380708Z digest=sha256:12a228c3ca068ad600dfdcefae348ed51e7cfcd5c51e443e0b31081035240102

Observation dc13ee9e-4fe5-465b-b0c5-87664d4ba319 · outbound

This paper cites Color superconductivity in dense quark matter.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Color superconductivity in dense quark matter

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.385067Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.385067Z digest=sha256:a3023a329daeb9b2998fff47e7f2102640e9f208e9b6909994a6c430d82209af

Observation 16206021-7350-4b7d-9b34-7a6d415f9cad · outbound

This paper cites Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.389639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.389639Z digest=sha256:871d7d46a5c6c50794d45b3a2de31c58dd58f87292211073d11bc4eb51ed5f74

Observation 521f5ff7-a167-464c-84bb-ca4e19b26d94 · outbound

This paper cites Bayesian Quantification of Observability and Equation of State of Twin Stars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Bayesian Quantification of Observability and Equation of State of Twin Stars

Reference 73

Resolution
verified exact
doi, observed 2026-08-16T00:09:08.671244Z

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.

source=arxiv_source observed=2026-08-16T00:09:05.394446Z digest=sha256:53e0450a2fcacac54b615f526f5c664669baf59e23e0f7309c26947a36d849c1

Observation 100d29bb-a967-4d8b-bf42-1460857059f4 · outbound

This paper cites 10.1051/0004-6361/201220697.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition 10.1051/0004-6361/201220697

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.399524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.399524Z digest=sha256:51baef8861c99883a26b585bb32d0a5f4be0d255ef1fe3026292d23e0e5796d7

Observation 5b7a3fc6-fb79-4ffa-9f25-b9c6eec53e79 · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.493016Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.493016Z digest=sha256:89d287e05fae356f0dcf71f8aaa7e4814a2d402e19a48f23c555d4950b4205ec

Observation 8bccd3d2-30cf-4ae3-9d55-d0f439bb9d41 · outbound

This paper cites Probing high-density nuclear symmetry energy with $\Xi^{-}/\Xi^{0}$ ratio in heavy-ion collisions at $\sqrt{s_{NN}} \sim 3$ GeV.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Probing high-density nuclear symmetry energy with $\Xi^{-}/\Xi^{0}$ ratio in heavy-ion collisions at $\sqrt{s_{NN}} \sim 3$ GeV

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.496794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.496794Z digest=sha256:ed2de063fe911126fb4df3c5305d774b9ef1ae9f7eaa5ddb6de6c2f72be2fc10

Observation 8b09ce22-fd43-43b3-a1f3-de2385bd74c4 · outbound

This paper cites Formation of superdense hadronic matter in high energy heavy-ion collisions.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Formation of superdense hadronic matter in high energy heavy-ion collisions

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.503407Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.503407Z digest=sha256:f17b6b4de844a09ed8f868e9ca2171fea12a2c82b42884871201c6b171123e18

Observation 79c0eb98-695e-4e66-a44b-9b2601227333 · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.508566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.508566Z digest=sha256:c0e7b11a2b4856f7740354a16827fcbd73526099e96d7a12eb3d5d118436d4fb

Observation ebf24581-3d73-46bd-9731-a8e2fd2e7413 · outbound

This paper cites Impact of Symmetry Energy on Sound Speed and Spinodal Decomposition in Dense Neutron-Rich Matter.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Impact of Symmetry Energy on Sound Speed and Spinodal Decomposition in Dense Neutron-Rich Matter

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.512885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.512885Z digest=sha256:92f03ade7bbf130687126e8569488a726d4c26545caaaf834a489e3448158dc4

Observation 73f0825a-b962-4b3a-97d4-f0ec3be8ca0b · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.517007Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.517007Z digest=sha256:5e0a2e0ab89025ef25fd06c0ac4e206efa65f024909de6c5b48c5e0a805629b2

Observation f3afb230-7c28-452a-9834-6d332e72ed1a · outbound

This paper cites Effect of Cluster Formation on Isospin Asymmetry in the Liquid-Gas Phase Transition Region.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Effect of Cluster Formation on Isospin Asymmetry in the Liquid-Gas Phase Transition Region

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.522204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.522204Z digest=sha256:dab81a7d7a7607dce02c379231e5e32a5d49033d8ced635ab2a9bfb345c5f29e

Observation 27c4a3d3-1009-4f3e-b82e-a729aff352af · outbound

This paper cites Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.574005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.574005Z digest=sha256:a031a13f885c5d40da17fa8f524b0492ac22c13f6b2d4d5b8595799862acc9d6

Observation b7bf7b59-6a77-4f0f-94ed-4bc44b280bd4 · outbound

This paper cites High density symmetry energy: A key to the solution of the hyperon puzzle.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition High density symmetry energy: A key to the solution of the hyperon puzzle

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.578548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.578548Z digest=sha256:559c8c6f4943e87e0588181a3a8e8a075820918b0811a596dd9f28349a851a4b

Observation d9061caf-19da-4814-a1a2-df4ce427f986 · outbound

This paper cites The NICER data and a $\sigma$-field dependent stiffness of the hadronic equation of state.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition The NICER data and a $\sigma$-field dependent stiffness of the hadronic equation of state

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.583154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.583154Z digest=sha256:8d71ded5d0c5e19cbc54b5cf80cd0a1ff6d2ea29e53c21698f5db17b42ede8fa

Observation b21c21ce-8d84-4bd4-ab44-f5b8cdc8a300 · outbound

This paper cites Far-from-equilibrium bulk-viscous transport coefficients in neutron star mergers.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Far-from-equilibrium bulk-viscous transport coefficients in neutron star mergers

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.588155Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.588155Z digest=sha256:146c0c51487d225077c2d5107ca16353d13dff6e06bd96e747f5b5dc6226f3e3

Observation ccdc7ea5-b051-45fe-94bb-252cc786ac52 · outbound

This paper cites Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.593487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.593487Z digest=sha256:e76824323938d9174de6a971a963449e18459f4b47e901015b123a3cf83e75cb

Observation 82381fd5-304e-4a41-948b-2aaf254a2fb8 · outbound

This paper cites Symmetry Energy Expansion with Strange Dense Matter.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Symmetry Energy Expansion with Strange Dense Matter

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.598085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.598085Z digest=sha256:545471a48b1a776fe88ad8ebdef058eb81f6be49630e3fa3a96e562628349f21

Observation 38f91359-ab3e-4203-96a4-0c9e7623894a · outbound

This paper cites Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.642373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.642373Z digest=sha256:f7bb509c1a59cc4f0891c3b3d06f23a5216f46df1adc59ca13353d36d11c83d0

Observation a4695099-c544-4fd5-ae51-cfc37c49463b · outbound

This paper cites Nucleon Effective Masses in Neutron-Rich Matter.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Nucleon Effective Masses in Neutron-Rich Matter

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.747145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.747145Z digest=sha256:397516c19cab790595114f869b1fb7ad4ee22c58348a4749a3e694c59944d4cb

Observation e0156be1-12f0-4dba-b395-39493a2944b7 · outbound

This paper cites PSR J2222--0137. I. Improved physical parameters for the system.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition PSR J2222--0137. I. Improved physical parameters for the system

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.790208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.790208Z digest=sha256:cda9b50572164ec17c5b5786ca1ac53b34db9cb6a3a1257c8e0e68ad2a45b752

Observation 93efa1a1-b9a8-4b42-9bd4-71b7c65e820c · outbound

This paper cites The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.795661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.795661Z digest=sha256:6a9acf9f8da784d1586f89e787bf630bba7ece1a22673440ee10deea5a6257d8

Observation d79da17e-0176-42c3-9d1e-022bacff07d3 · outbound

This paper cites Thermal X-ray emission identified from the millisecond pulsar PSR J1909-3744.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Thermal X-ray emission identified from the millisecond pulsar PSR J1909-3744

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.799813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.799813Z digest=sha256:6a418bd94750964c677d11f6f15bd4e465ea27bbfbf992245b1940eebfaff1c3

Observation 3e658cf8-7641-4f5f-850f-afaf2b50c5c0 · outbound

This paper cites an unresolved cited work.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Unresolved cited work

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.804983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.804983Z digest=sha256:2e0763781630f7e65a5fa05b70ee5b8f8d54f3c0029ee9ab50c3dd3016bce7db

Observation d402db1b-0ce9-4e91-8417-4a9dd4c20e89 · outbound

This paper cites and others.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition and others

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.809639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.809639Z digest=sha256:a3646372ff311674f163466c4b6d0676b11188ee17a7091865334a7eeeaeb188

Observation 7aa4156a-6a0b-4d46-a7ca-085bf0690878 · outbound

This paper cites PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.848712Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.848712Z digest=sha256:ec4803691031b815e8084e0f5b2de74ed245af28726024fe7afb23c902073e08

Observation a8270474-d351-4f75-97bb-ec551a2b55fa · outbound

This paper cites Neutron Star Observations: Prognosis for Equation of State Constraints.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Neutron Star Observations: Prognosis for Equation of State Constraints

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.868990Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.868990Z digest=sha256:078ec92c6a9943eefd049ae1c48158b6ea55e729e80577a1ffa72856352558b0

Observation 36a0da4e-f716-4f94-b513-01bfe6b7b993 · outbound

This paper cites Astrophys.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Astrophys

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.874850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.874850Z digest=sha256:0a6a569043d0695c76fd69d72401732474f78388f9716fb96b7ab6143db5f036

Observation fa34a150-3b77-465b-b1c4-9d1c4c68032f · outbound

This paper cites A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.880262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.880262Z digest=sha256:66cb8df8809afaf5a12dbc7d9658394fbb678114cf95dd0db6a5b46066d19ba9

Observation 171b7db1-e3f3-4ddd-8c99-3c6c1ef4e1e5 · outbound

This paper cites Influence of Nuclear Reaction Rate Uncertainties on Neutron Star Properties Extracted From X-ray Burst Model-Observation Comparisons.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Influence of Nuclear Reaction Rate Uncertainties on Neutron Star Properties Extracted From X-ray Burst Model-Observation Comparisons

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.885546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.885546Z digest=sha256:29dab65be0e868a5b0de101cbe6988924c01da4a84404c6bbf3a897e1c053511

Observation ec49c10b-17d4-482e-9e11-1b7cc97112c0 · outbound

This paper cites Constraints on neutron star mass and radius in GS 1826-24 from sub-Eddington X-ray bursts.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Constraints on neutron star mass and radius in GS 1826-24 from sub-Eddington X-ray bursts

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.889695Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.889695Z digest=sha256:22d1cfe8d5a3ee8d7c21776f07c380eec11e002f3f8cd8236b58a24e4edf6a88

Observation 932f0641-f5e1-4720-a555-1ab06ccbd069 · outbound

This paper cites Long tails on thermonuclear X-ray bursts from neutron stars: a signature of inward heating?.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Long tails on thermonuclear X-ray bursts from neutron stars: a signature of inward heating?

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.894680Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.894680Z digest=sha256:5c447906e20a1266bbc96f761b7341349b8d65529c2b61ddba6bee866d79c29f

Observation 9416a6d8-f440-4095-a126-3d32a4fdf2c3 · outbound

This paper cites Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:05.932349Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:05.932349Z digest=sha256:af31d6cbcb2c1423b6dcafa6b44e88942cdaba21b09f23e2b5405922d2f9d521

Observation e793d47c-8b9a-462d-b700-c7c6138102c2 · outbound

This paper cites Periodic Thermonuclear X-ray Bursts from GS 1826-24 and the Fuel Composition as a Function of Accretion Rate.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Periodic Thermonuclear X-ray Bursts from GS 1826-24 and the Fuel Composition as a Function of Accretion Rate

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:06.040583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:06.040583Z digest=sha256:7ae370e365d5a3d0db4c0330b7e04eaa53b2b2021590148164f05efb5757930d

Pith citing papers

No inbound Pith citation observations are available.