Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches | Paper Citation Record

Observation ec536b32-ed39-459e-9596-c6c38ae7d488 · outbound

This paper cites Physics of Neutron Star Crusts.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Physics of Neutron Star Crusts

Reference 1

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Observation 3dda9f9c-05cb-4c9f-9bd0-dd9995140463 · outbound

This paper cites Modelling neutron star mountains.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Modelling neutron star mountains

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Observation db223af4-72bf-4bb2-b10f-1ab6d7d63d5c · outbound

This paper cites Neutrino transport in general relativistic neutron star merger simulations.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutrino transport in general relativistic neutron star merger simulations

Reference 3

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Observation a6b79d6c-2816-410f-93d9-6dac7444f024 · outbound

This paper cites Composition and structure of protoneutron stars.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Composition and structure of protoneutron stars

Reference 4

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Observation 1d110e57-685d-4da5-99ad-280a8d7b5f69 · outbound

This paper cites Neutron Star Cooling.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutron Star Cooling

Reference 5

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Observation 2df4fc2a-1194-433d-a0c9-5680d330cc6e · outbound

This paper cites Evolution of protoneutron stars.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Evolution of protoneutron stars

Reference 6

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Observation 0d7c927f-944a-433b-a701-5ff2267f07fa · outbound

This paper cites The proto-neutron star inner crust in the liquid phase.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches The proto-neutron star inner crust in the liquid phase

Reference 7

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Observation 1cf140fb-ec03-4917-a7ee-42ba8d217976 · outbound

This paper cites Impact of the hot inner crust on compact stars at finite temperature.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Impact of the hot inner crust on compact stars at finite temperature

Reference 8

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Observation 001022b6-7b08-4a2f-8411-71fcd243ebaa · outbound

This paper cites Assessing the joint effect of temperature and magnetic field on the neutron star equation of state.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Assessing the joint effect of temperature and magnetic field on the neutron star equation of state

Reference 9

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Observation 93f0ad8e-5081-4cf4-9709-17ae29ab9b88 · outbound

This paper cites A generalized equation of state for hot, dense matter.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches A generalized equation of state for hot, dense matter

Reference 10

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Observation 58e6f1a3-06ff-4be7-a7e4-fa2eca6e608d · outbound

This paper cites Equations of state for supernovae and compact stars.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Equations of state for supernovae and compact stars

Reference 11

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Observation 3be798ac-080b-4174-af8f-c07dc490cd35 · outbound

This paper cites Open-source nuclear equation of state framework based on the liquid-drop model with Skyrme interaction.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Open-source nuclear equation of state framework based on the liquid-drop model with Skyrme interaction

Reference 12

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Observation 413c00de-7c36-481d-99a6-46ec4f49880e · outbound

This paper cites Finite-temperature equations of state of compact stars with hyperons: three-dimensional tables.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Finite-temperature equations of state of compact stars with hyperons: three-dimensional tables

Reference 13

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Observation eee4882b-0dde-4ed2-ade4-4bcae935920e · outbound

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Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Unresolved cited work

Reference 14

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Observation b627a7d4-58f9-4335-adcd-b2a0d39aee8e · outbound

This paper cites Neutron stars and the nuclear equation of state.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutron stars and the nuclear equation of state

Reference 15

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Observation 48cd8e00-749e-4fd4-8566-a094c5d1f67a · outbound

This paper cites Crystallization of the inner crust of a neutron star and the influence of shell effects.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Crystallization of the inner crust of a neutron star and the influence of shell effects

Reference 16

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Observation b0e2d287-0749-4b67-a1ef-12aeb0cdfc95 · outbound

This paper cites Selfconsistent semiclassical description of average nuclear properties a link between microscopic and macroscopic models.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Selfconsistent semiclassical description of average nuclear properties a link between microscopic and macroscopic models

Reference 17

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Observation 95bacee7-0df8-4683-85e5-076214235103 · outbound

This paper cites Extended Thomas–Fermi theory at finite temperature.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Extended Thomas–Fermi theory at finite temperature

Reference 18

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Observation a463183b-7b2f-4c4d-be35-d620b2e06b1f · outbound

This paper cites Relativistic Equation of State for core-collapse Supernova Simulations.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Relativistic Equation of State for core-collapse Supernova Simulations

Reference 19

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Observation 5ec915b7-fb95-4810-bc93-3314e6a1f992 · outbound

This paper cites Equation of state of stellar nuclear matter in the temperature-dependent extended Thomas–Fermi formalism.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Equation of state of stellar nuclear matter in the temperature-dependent extended Thomas–Fermi formalism

Reference 20

Resolution: verified exact; doi, observed 2026-08-07T14:10:15.214895Z

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Observation 1a33c267-33bb-4a0f-8bc0-c5520aa8be74 · outbound

This paper cites Semi-classical equation of state and specific-heat expressions with proton shell corrections for the inner crust of a neutron star.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Semi-classical equation of state and specific-heat expressions with proton shell corrections for the inner crust of a neutron star

Reference 21

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T14:10:16.501026Z

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Observation 01d0fda8-8c70-48fa-8e64-c10c91dd3578 · outbound

This paper cites A statistical model for a complete supernova equation of state.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches A statistical model for a complete supernova equation of state

Reference 22

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Observation 9aa3d3af-41ef-4614-89ce-f076b8d790c1 · outbound

This paper cites Nuclear Statistical Equilibrium Equation of State for Core Collapse.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Nuclear Statistical Equilibrium Equation of State for Core Collapse

Reference 23

Resolution: verified exact; doi, observed 2026-08-07T14:10:15.031666Z

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Observation 9720deac-8a3a-4209-ae26-02be402d8973 · outbound

This paper cites Core-collapse Supernova Equations of State Based on Neutron Star Observations.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Core-collapse Supernova Equations of State Based on Neutron Star Observations

Reference 24

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Observation 6dd12139-3412-4544-901e-cc09158a1993 · outbound

This paper cites New Equations of State Based on the Liquid Drop Model of Heavy Nuclei and Quantum Approach to Light Nuclei for Core-collapse Supernova Simulations.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches New Equations of State Based on the Liquid Drop Model of Heavy Nuclei and Quantum Approach to Light Nuclei for Core-collapse Supernova Simulations

Reference 25

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Observation f4aef39c-bd5d-4f3c-9ccc-8de4109dd7d8 · outbound

This paper cites Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces

Reference 26

Resolution: verified exact; doi, observed 2026-08-07T14:10:14.886957Z

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Observation e1ddd41f-3f41-4e48-9e7b-03e9a4672bdb · outbound

This paper cites Neutron star crust properties: Comparison between the compressible liquid-drop model and the extended Thomas–Fermi approach.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutron star crust properties: Comparison between the compressible liquid-drop model and the extended Thomas–Fermi approach

Reference 27

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Observation f8ff3501-c9cc-4001-89fa-09e0cf14814b · outbound

This paper cites Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas

Reference 28

Resolution: verified exact; doi, observed 2026-08-07T14:10:14.735747Z

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Observation 0a74a026-a411-4909-a745-58fdc3877163 · outbound

This paper cites Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals—I.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals—I

Reference 29

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Observation 52b455b3-51a7-48ab-8c38-1cd3d537aea0 · outbound

This paper cites Inner crust of a neutron star at the point of crystallization in a multicomponent approach.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Inner crust of a neutron star at the point of crystallization in a multicomponent approach

Reference 30

Resolution: verified exact; doi, observed 2026-08-07T14:10:14.592698Z

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Observation 50adee53-11a7-420a-8207-044fb231fa5b · outbound

This paper cites The proto-neutron star inner crust in a multi-component plasma approach.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches The proto-neutron star inner crust in a multi-component plasma approach

Reference 31

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Observation 4dc8f3b7-feb5-4665-9c38-167df330719f · outbound

This paper cites Neutron Stars 1: Equation of State and Structure; Springer: New York, NY, USA 2007.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutron Stars 1: Equation of State and Structure; Springer: New York, NY, USA 2007

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T14:10:16.366622Z

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Observation d33c4826-cd76-44d2-8370-6ea75bcb35d2 · outbound

This paper cites On the accuracy of the single-nucleus approximation in the equation of state of hot, dense matter.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches On the accuracy of the single-nucleus approximation in the equation of state of hot, dense matter

Reference 33

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Observation 07042966-a4ac-49d0-a1fd-82229f9a711c · outbound

This paper cites Prior Probability Distributions of Neutron Star Crust Models.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Prior Probability Distributions of Neutron Star Crust Models

Reference 34

Resolution: verified exact; doi, observed 2026-08-07T14:10:14.356667Z

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Observation eeee1362-4f56-4de4-affc-dd4f87985414 · outbound

This paper cites Uncertainties in the pasta-phase properties of catalysed neutron stars.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Uncertainties in the pasta-phase properties of catalysed neutron stars

Reference 35

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Observation 856ffc48-51dd-4ce7-99da-e7835281f713 · outbound

This paper cites Pasta properties of the neutron star within effective relativistic mean-field model.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Pasta properties of the neutron star within effective relativistic mean-field model

Reference 37

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Observation 06ee09fa-58c9-4e79-a2f3-4e5e55b40d18 · outbound

This paper cites Structure of neutron star crusts from new Skyrme effective interactions constrained by chiral effective field theory.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Structure of neutron star crusts from new Skyrme effective interactions constrained by chiral effective field theory

Reference 38

Resolution: verified exact; doi, observed 2026-08-07T14:10:14.192344Z

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Observation 07140886-6a98-434f-bd7c-13c3094b8d47 · outbound

This paper cites Pasta Phases in Neutron Star Mantle: Extended Thomas–Fermi vs.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Pasta Phases in Neutron Star Mantle: Extended Thomas–Fermi vs

Reference 39

Resolution: verified exact; doi, observed 2026-08-07T14:10:14.055739Z

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Observation 9cd51b3c-ea2a-4fac-8b09-27eb625d18d6 · outbound

This paper cites Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals

Reference 40

Resolution: verified exact; doi, observed 2026-08-07T14:10:13.881150Z

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Observation 08388249-f39f-4c7b-8a25-88483a2c7329 · outbound

This paper cites Proto-neutron star evolution with improved charged-current neutrino–nucleon interactions.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Proto-neutron star evolution with improved charged-current neutrino–nucleon interactions

Reference 42

Resolution: verified exact; doi, observed 2026-08-07T14:10:13.729163Z

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Observation bb626cf7-5724-43f9-9891-731054722839 · outbound

This paper cites Beta Equilibrium Under Neutron Star Merger Conditions.Universe 2021, 7, 399.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Beta Equilibrium Under Neutron Star Merger Conditions.Universe 2021, 7, 399

Reference 43

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Observation 62a936e0-dce0-40d8-856a-186a0ec521b0 · outbound

This paper cites Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:09.139030Z

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Observation a2fd1530-6625-4e13-96ca-3f3757da819c · outbound

This paper cites On the Constitution of Metallic Sodium.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches On the Constitution of Metallic Sodium

Reference 45

Resolution: verified exact; doi, observed 2026-08-07T14:10:13.528395Z

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Observation 33bb6418-337d-427a-8d1c-0a498aaeb708 · outbound

This paper cites On the Constitution of Metallic Sodium.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches On the Constitution of Metallic Sodium

Reference 46

Resolution: verified exact; doi, observed 2026-08-07T14:10:13.385294Z

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Observation 7cb18e15-a1f7-48f3-b76f-f1b1bd78672c · outbound

This paper cites Neutron star matter.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutron star matter

Reference 47

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T14:10:16.220977Z

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Observation 86aaff9d-7823-48d6-b984-e5f341166239 · outbound

This paper cites Energy and Pressure of a Zero-Temperature Plasma.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Energy and Pressure of a Zero-Temperature Plasma

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:09.546919Z

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Observation 206d616e-d545-485d-80af-085d145e1f71 · outbound

This paper cites Neutron star matter at sub-nuclear densities.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutron star matter at sub-nuclear densities

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:09.632687Z

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Observation 1ae8a2f5-1790-464c-b1f0-3615b9dc664e · outbound

This paper cites A mean-field calculation of the equation of state of supernova matter.Nucl.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches A mean-field calculation of the equation of state of supernova matter.Nucl

Reference 50

Resolution: verified exact; doi, observed 2026-08-07T14:10:13.222868Z

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Observation 3de07f17-5992-4b0f-b668-c8346fd758a5 · outbound

This paper cites Validity of the Wigner-Seitz approximation in neutron star crust.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Validity of the Wigner-Seitz approximation in neutron star crust

Reference 51

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Observation 714cf848-f672-4e6b-8ad4-843487159e88 · outbound

This paper cites Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree- Fock method at finite temperature: Core-collapse supernovae.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree- Fock method at finite temperature: Core-collapse supernovae

Reference 52

Resolution: malformed identifier; no resolver link, observed 2026-08-07T14:10:09.913252Z

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Observation 90f3e0dd-cef8-423f-80a0-138f62ef6831 · outbound

This paper cites Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.020867Z

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Observation 1dd71482-8822-4ae7-91b0-6dcf6f1cd11e · outbound

This paper cites On the Fermi functions I −(n+1/2).

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches On the Fermi functions I −(n+1/2)

Reference 54

Resolution: verified exact; doi, observed 2026-08-07T14:10:12.991301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f8b95a46-4467-47b2-b308-ef698959baec · outbound

This paper cites Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.186481Z

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Unavailable: canonical work link unavailable.

Observation 375b7009-430b-4a1b-8516-67df75c8ba9d · outbound

This paper cites Physical properties of hot, dense matter: The general case.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Physical properties of hot, dense matter: The general case

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.241813Z

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Unavailable: canonical work link unavailable.

Observation 2e4e78a5-7c45-4534-a5e1-685b6516ffec · outbound

This paper cites Isospin-dependent clusterization of neutron-star matter.Nucl.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Isospin-dependent clusterization of neutron-star matter.Nucl

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.398289Z

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Observation 6deb67b0-0029-448e-87f3-4bc8e29b7296 · outbound

This paper cites Equation of state for dense nucleonic matter from metamodeling.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Equation of state for dense nucleonic matter from metamodeling

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.512942Z

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Unavailable: canonical work link unavailable.

Observation 36bcff53-7a19-4ab2-8713-3f9634aed8ce · outbound

This paper cites Structure of matter below nuclear saturation density.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Structure of matter below nuclear saturation density

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.647066Z

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Observation 6751b071-73a9-42a3-b970-d9784ed09773 · outbound

This paper cites Nuclear “pasta” structures and the charge screening effect.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Nuclear “pasta” structures and the charge screening effect

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.775261Z

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Unavailable: canonical work link unavailable.

Observation af71b062-3525-4fdd-ae52-b3215c190aeb · outbound

This paper cites A Survey of the Parameter Space of the Compressible Liquid Drop Model as Applied to the Neutron Star Inner Crust.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches A Survey of the Parameter Space of the Compressible Liquid Drop Model as Applied to the Neutron Star Inner Crust

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:10.883226Z

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Unavailable: canonical work link unavailable.

Observation f2fe2f79-f3a9-4aba-917a-dc7ed3a1fc13 · outbound

This paper cites Nuclear interface energy at finite temperatures.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Nuclear interface energy at finite temperatures

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:11.007908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9536b0e7-a0cc-46a0-a924-0c3295971f04 · outbound

This paper cites Private communications, 2024.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Private communications, 2024

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T14:10:16.096494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2e58e2fd-cdf1-41e8-8b46-4fe0a6a979e0 · outbound

This paper cites Parametrization of the surface energy in the ETF approximation.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Parametrization of the surface energy in the ETF approximation

Reference 64

Resolution: verified exact; doi, observed 2026-08-07T14:10:12.669074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8c5bd8cd-b597-43ff-989c-dda4d495d301 · outbound

This paper cites The AME 2020 atomic mass evaluation (II).

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches The AME 2020 atomic mass evaluation (II)

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:11.420724Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7bfc3256-171b-428e-b99b-c3504280b9f7 · outbound

This paper cites The AME2016 atomic mass evaluation (II).

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches The AME2016 atomic mass evaluation (II)

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:11.533064Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59d121f5-db32-4761-b2ba-f59661c5aac5 · outbound

This paper cites Neutrino-pair bremsstrahlung by electrons in neutron star crusts.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Neutrino-pair bremsstrahlung by electrons in neutron star crusts

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-08-07T14:10:12.473785Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation cc2964d9-f317-4f0e-b8a5-abe34376fe5f · outbound

This paper cites Thermal relaxation in young neutron stars.Mon.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Thermal relaxation in young neutron stars.Mon

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:11.693199Z

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Unavailable: canonical work link unavailable.

Observation f7a5e881-94dd-4cd0-bdf9-c1b6c61b8322 · outbound

This paper cites Role of neutron pairing with density-gradient dependence in the semimicroscopic treatment of the inner crust of neutron stars.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Role of neutron pairing with density-gradient dependence in the semimicroscopic treatment of the inner crust of neutron stars

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:11.796649Z

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Unavailable: canonical work link unavailable.

Observation 0d17f835-845b-44a4-9c6e-4fbf3a424616 · outbound

This paper cites Comparison between the Thomas–Fermi and Hartree–Fock–Bogoliubov Methods in the Inner Crust of a Neutron Star: The Role of Pairing Correlations.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Comparison between the Thomas–Fermi and Hartree–Fock–Bogoliubov Methods in the Inner Crust of a Neutron Star: The Role of Pairing Correlations

Reference 70

Resolution: verified exact; doi, observed 2026-08-07T14:10:12.312109Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2ee3129d-4d93-4873-8a00-803c1ba51466 · outbound

This paper cites Time-Dependent Nuclear Energy-Density Functional Theory Toolkit for Neutron Star Crust: Dynamics of a Nucleus in a Neutron Superfluid.

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches Time-Dependent Nuclear Energy-Density Functional Theory Toolkit for Neutron Star Crust: Dynamics of a Nucleus in a Neutron Superfluid

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T14:10:12.043864Z

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