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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

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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

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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

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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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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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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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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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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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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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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=sha256:5ebb82b60095a2c789df3abb75e52394eb8d5bab36e76ba7562ee8237e1f880b

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
unresolved
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=sha256:202c4cb6cd514ffda4b0335c1a7dfa9b81ff852c1f4d49527daec84225fcfaee

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=sha256:2e84464f1b8515f3f5614b84908d6ae65cc82efc1899839ae1b1818df7114ad4

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=sha256:2943bae2d039a75fe7fbb30409a5813cd089a1bc7531aad8ade6ec3d96df244c

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=sha256:0c6d4c41b664f031e75aa22701533bb5eb713d24df3eb1e13d5f56f2ebc52c7b

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:bf2d1f438007ea3b448704f48984433be300bf97be89c090c9f0ab4dec49a48f

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=sha256:8eaa29c9f12cfb11323314315f85ce2b6f2041a9e22669a6c05434c2aaa4a9d5

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:d69854df22dfeb4d3ab1df7c3f47d9e509dcc90fa63dce0f0021790cd2babfee

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:a06d4faed6e249aa4b885e3001a437ff4260d686472110c064a462220a482dc1

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=sha256:8ab11151637b7636971296a8e97bfcae55f410fe22b2d96187659cdd5a29ce83

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=sha256:1d837cb61fa741dd065fc2251ee51d9e5a6660cc6cd9d421435c0b3c97d8176e

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=sha256:83b782aa26398dd666836036e16bd67b9a673ad0a6c5a73eeca5a2239c497aa1

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=sha256:3625dd1aab2d396e9e19ca6dcbbebeb2166461bda28a7b9c9878bc715bf74eb6

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:e8506c9bc28e69b17574f779cdcb892e6ce25e5520ef6941502592de69bf4381

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=sha256:3a243cefc15cc2f58cbbead4d9cd60a8156f5d912c44d00b2c7e461a9c2a25b3

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:e1cc353f73f33b36a57f96417f990796b867912def6e02325549949594931b44

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=sha256:29fc25914d4fae308d9b72d3778642bc89857b6aa03b773c02e7388d65323d54

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=sha256:5a9a4c1686db09bb4417f4d2c7069d346dedf77ab5843c694198933145b582a3

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=sha256:3ce9ecf3647eff5572beb4e48f20cf203a5faf6b1893bb0f654d2c458ae79390

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:cc0c1116ed3ccda7f3bed098dc35b5f353038faec49e28be7da4871e1c7143d8

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:ffdba8f15803261a7538fc8fdd143858ceeac0d5ab30cf6a3c545fc122c734c9

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=sha256:3fe7fa9aec695f3ef71cb10d3f2f223483d14852bf8669d119ad74a610a73fb7

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=sha256:4f1ca3bb00f48c3ad1b9760f9a73b62668c477eb44e3989ba148404eb7f81068

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:f0070ecb22dd0bed1da4062c84a235635c01b5403a51a3f167117b6df282b4f7

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=sha256:154c8f9c542b23eb7de4c878202414b4f057b7d37e45e55f648b0e85171f48a2

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:f978c26ae50ed8bd534e7120cc96415136416a9d086a7abb584f1615f3a36a74

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=sha256:0dd09154331258c62cf7c2de1eaa063726672dd1448bb2dd0e33e708bd30cb6c

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=sha256:287a2c849c2464b56c0e37f635d279d968cea925ad92be8756a136d0c5b59f2a

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=sha256:751975ff25e35c94ef5d3fe74b3a4aa62b72e5d32668d0a73a0040d30a887a3d

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=sha256:533b02231330f6998427328b4c4708edd4cfd0fee28c9f2edc90b40bcdff35a7

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=sha256:3194cfd08413a3e97f6d8d1fcc23b43bb78c3ae5e8d0d3e5e8494dd1d7fbed42

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:ce65df5540030b71fe0dc05969fb0838c93bcedf8937efde5e66465ab05862ab

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=sha256:5edc9332960743bc11d5304140937db674f9d8a40ca757545e5e98df51a10e14

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=sha256:0d9f5a1b303dd9244eb8c4e7d862aa13b9d8b60cc0d36bec3190d8227bcdf84a

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=sha256:3d75fffc2de704dfeae7d77e10b2be80013224a73e9655fe8d9f44292fefd590

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=sha256:62c96f7755831cf85ca38a6a81f561cfb4e45892e6616c69d9baa92bf4bc976e

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=sha256:32b2f10c65be74d2fe734614ff3315a581ddb4dd94ad8a31c99cd4747e1c0599

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:c04ecaa5dd3c496646eac58706e9f2709c825a3301914e48a0df72d1be756f88

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=sha256:887baa771b655bcc8e8935cb6371658e5407f732f49d5a01ee6be956e76aed00

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:d4f0d59de033c0ed413bdb103a7512cea760e04cb341687d8964c2e6ac5a59f3

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:e21bcf41ea1afbb5633a50d16ff0961ba713016f9456266fc3f23fa4de028155

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:b28f6c671422240b6cf8be03549a64e77084adc6134b426b68b6c643a0d0f0b3

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=sha256:52646dd2c8c52d71687492748c3624ea08b53cdab117cb729f4ac37094ad7154

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=sha256:2f3a87c2495c34e840bb4fd65b4cafc40f9bf32d45481ae986d424d71af8d3e3

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=sha256:4ffa5e57d550547a11487cfe465860875431a92aba4e2dbd9f2ab2913176b5b7

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:bd68ccc6507dfd45daa62ade954c2c396157ec61019bf7d780c4d87d340b286c

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:c9f706f0483f8885b2c925c02c2198c600544873511a3710c339dc8a41355065

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=sha256:709c71bb42915f64857483658e1cd86785f90229bd19200d71ae1320a1f05209

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=sha256:766ea8f4be3537eba666454df0ac8f3350e207c183175f0ad7d908d89d54c733

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:c02937b816a3c6ab5fc4a0692e1587405608afe8deca179836555cbcdb3c4134

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=sha256:0b15336705d2572d4d9f0ece57bbdcd97271b2c529bca4053dacbf6a3ed038fb

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=sha256:9f771ef833dab20ca7a946bc14eac6e582478be25815e0575dcf058eca486b87

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:ee2d684b26373f0c41094be8b9283379c3892d6cb4fe9a158635860a8d584dbf

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=sha256:44c98150cd99b0b2b8bcf502df43784c045171f13755506969847596f7a561e8

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=sha256:92b666f67b5cf0eb099e92866ca0e3563cebaf78da4fb28ee084b1ecef020c56

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:ee5050ab55abdc631bd3b2b22206a4b81dd16fce652bf6c817d9fe7d227e00ac

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=sha256:3dff92d707ded07343b92348dd07df2c2e969bd4e5e6dea3dd68ce1703ba3961

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=sha256:3640314ec07773eb189a5d6c7a87300dd2843edcea547f4f385a4eb13a88141e

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=sha256:766b0ee55d89f3999ef723f6d6161b718bf2e86daa9aeca0015ad61522daaa1d

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=sha256:2292c69dbcb795ea8067c5a965c9e411c421fc8b4135969418d1fea9b8e90fa9

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:f85b6b009278c444a5cb42e3423e8c5e03a6029eec1f808e8f2ebea1200425dd

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=sha256:12532a5474eaeef34c0960bd7ac9c996cda5234d162a14711b12e39ac4464ece

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=sha256:87f93922849588d35d98339e7334ba3ab3cbc9c0e2484597ed760f0a4d1419f7

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:d261a37ab12a4bbd6c8f0619cf0dc71be55abdaeeda0ba97758466dfa0a2d335

Pith citing papers

No inbound Pith citation observations are available.