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Paper Citation Record · LEDGER

Building Neutron Stars with the MUSES Calculation Engine

As of 14 August 2026, this Paper Citation Record lists 100 of 181 outbound references and 11 inbound Pith citation observations for arXiv:2502.07902.

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

pith.paper-citation-record.v1
2502.07902 v1

Coverage vector

measured 100 of 181 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-08T11:32:34.572430Z

measured 111 of 111 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:31:32.607156Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-04T16:19:57.329674Z

Reference resolution

100 of 181 outbound references displayed

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  • verified fuzzy0
  • unresolved96
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Outbound references

Observation 47cc3d64-cdef-43e5-8246-07f28f37b765 · outbound

This paper cites Every point along any curve represents a single, sta- ble, neutron star solution.

Building Neutron Stars with the MUSES Calculation Engine Every point along any curve represents a single, sta- ble, neutron star solution

Reference 1

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Observation 5c4d8680-45b3-407e-9328-ad71ef47d2d8 · outbound

This paper cites The spin-correction to the non- rotating (TOV) mass at O(ϵ2) is given by Eq.

Building Neutron Stars with the MUSES Calculation Engine The spin-correction to the non- rotating (TOV) mass at O(ϵ2) is given by Eq

Reference 2

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Observation c6495a88-e664-41aa-b9af-390b424fca4c · outbound

This paper cites The size of each layer of a neutron star strongly depends on the maximum central density, which in turn produces a given mass and radius of the star.

Building Neutron Stars with the MUSES Calculation Engine The size of each layer of a neutron star strongly depends on the maximum central density, which in turn produces a given mass and radius of the star

Reference 3

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Observation 69504760-e205-4cf1-b293-57e14ea296e1 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 4

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Observation 397d7d05-3deb-45df-b204-0a71582604aa · outbound

This paper cites Default input format for the Flavor Equilibration module in MUSES.

Building Neutron Stars with the MUSES Calculation Engine Default input format for the Flavor Equilibration module in MUSES

Reference 5

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Observation 89cd89b9-e7f3-4cc1-bbc0-37803b878209 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 6

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Observation e42a0fc5-3515-45a3-9fea-272f734d030b · outbound

This paper cites For a derivation and in-depth discussion of these quanti- ties, see Refs.

Building Neutron Stars with the MUSES Calculation Engine For a derivation and in-depth discussion of these quanti- ties, see Refs

Reference 7

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Observation 229c6ed3-f777-47d7-b7d6-f997036fe0aa · outbound

This paper cites From hadrons to quarks in neutron stars: a review.

Building Neutron Stars with the MUSES Calculation Engine From hadrons to quarks in neutron stars: a review

Reference 8

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Observation 56eceef5-339d-4667-8a7e-ed2c018f2cdb · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 9

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Observation eaf2f9bd-febb-44c3-8c16-6cb0546545de · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 10

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Observation 42c62f37-70c1-4874-83a2-c39885c7fb56 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 11

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Observation 236b97f5-d156-4cfc-8f41-5d3ad68668cf · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 12

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Observation fb9b2dfd-44a2-4257-9319-02f2fa969da4 · outbound

This paper cites Ivanenko and D.

Building Neutron Stars with the MUSES Calculation Engine Ivanenko and D

Reference 13

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Observation 03a49b1b-bb49-454f-9493-c642a982d30e · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 14

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Observation 7e5108dd-4c30-4602-bc53-1633eb6eb8d4 · outbound

This paper cites Burrows and J.

Building Neutron Stars with the MUSES Calculation Engine Burrows and J

Reference 15

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Observation 603862ff-594b-49ff-b280-6dec23bc22ae · outbound

This paper cites Explosion Mechanisms of Core-Collapse Supernovae.

Building Neutron Stars with the MUSES Calculation Engine Explosion Mechanisms of Core-Collapse Supernovae

Reference 16

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Observation 1b764492-97f6-4bbf-b0d9-4b4cc768d926 · outbound

This paper cites The QCD equation of state from the lattice.

Building Neutron Stars with the MUSES Calculation Engine The QCD equation of state from the lattice

Reference 17

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Observation 883f4c63-2639-475b-a4f0-c682cd248f9e · outbound

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

Building Neutron Stars with the MUSES Calculation Engine Equations of state for supernovae and compact stars

Reference 18

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Observation cd8d7e84-5e66-43f8-a9c3-1f8b40985305 · outbound

This paper cites CompOSE - CompStar Online Supernovae Equations of State.

Building Neutron Stars with the MUSES Calculation Engine CompOSE - CompStar Online Supernovae Equations of State

Reference 19

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Observation 0915d101-744f-48be-902f-b2fce42c6824 · outbound

This paper cites CompOSE Reference Manual.

Building Neutron Stars with the MUSES Calculation Engine CompOSE Reference Manual

Reference 20

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Observation 787b59b9-c639-4973-9efc-05bd2771fcfa · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 21

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Observation b6b1dde7-46eb-49c0-af44-4a55c82d66f1 · outbound

This paper cites Quick Guides for Use of the CompOSE Data Base.

Building Neutron Stars with the MUSES Calculation Engine Quick Guides for Use of the CompOSE Data Base

Reference 22

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Observation 75e7ccd9-7fb6-4662-babe-b9b9bca96194 · outbound

This paper cites Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model.

Building Neutron Stars with the MUSES Calculation Engine Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model

Reference 23

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Observation 62b45531-e96c-45fd-9b0d-38aab7ccc391 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 24

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Observation c7de8269-8b45-403a-84ce-1b06dac9776b · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 25

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Observation 1fa6eb41-47e5-4d5a-859b-ed494bce41fb · outbound

This paper cites Tidal Love numbers of neutron stars.

Building Neutron Stars with the MUSES Calculation Engine Tidal Love numbers of neutron stars

Reference 26

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Observation 1c1dd176-574c-48c4-a666-2479ea177241 · outbound

This paper cites Constraining neutron star tidal Love numbers with gravitational wave detectors.

Building Neutron Stars with the MUSES Calculation Engine Constraining neutron star tidal Love numbers with gravitational wave detectors

Reference 27

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Observation 0724c312-c512-4873-9df5-f1bf31f765cb · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 28

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Observation e44d8c77-9883-4ed6-83c8-7de669170b82 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 29

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Observation 96b59719-58a1-42d2-be87-912aab948feb · outbound

This paper cites Thermal-FIST: A package for heavy-ion collisions and hadronic equation of state.

Building Neutron Stars with the MUSES Calculation Engine Thermal-FIST: A package for heavy-ion collisions and hadronic equation of state

Reference 30

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Observation 10e75f4f-6aab-4424-9cad-31e1415192b1 · outbound

This paper cites io/ (2024).

Building Neutron Stars with the MUSES Calculation Engine io/ (2024)

Reference 31

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Observation e5940163-a22c-448a-be2e-5ee0ba859780 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 32

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Observation 47a2a629-57ff-41ea-810e-97db2b86c69b · outbound

This paper cites Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory.

Building Neutron Stars with the MUSES Calculation Engine Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory

Reference 33

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Observation 54099434-6e3d-4a03-9a52-4dde0e044b2a · outbound

This paper cites Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations.

Building Neutron Stars with the MUSES Calculation Engine Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations

Reference 34

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Observation e86147eb-420c-4b2a-9891-a2d8c3c9480a · outbound

This paper cites Steiner and S.

Building Neutron Stars with the MUSES Calculation Engine Steiner and S

Reference 35

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Observation 86e4a145-f91f-41bc-8689-d4c0917cb1a1 · outbound

This paper cites Roy, Crust DFT EoS tables.

Building Neutron Stars with the MUSES Calculation Engine Roy, Crust DFT EoS tables

Reference 36

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Observation 55b07719-6ad6-4b82-a93d-334b32e60387 · outbound

This paper cites Chiral effective field theory and nuclear forces.

Building Neutron Stars with the MUSES Calculation Engine Chiral effective field theory and nuclear forces

Reference 37

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Observation 50b23f84-2c08-4820-b6f9-04d9ee64d024 · outbound

This paper cites Chiral Effective Field Theory and the High-Density Nuclear Equation of State.

Building Neutron Stars with the MUSES Calculation Engine Chiral Effective Field Theory and the High-Density Nuclear Equation of State

Reference 38

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Observation 15ccfa6a-d028-490d-86ad-435d7d6fe28b · outbound

This paper cites Friedenberg and J.

Building Neutron Stars with the MUSES Calculation Engine Friedenberg and J

Reference 39

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Observation bb1ac1ad-057c-496c-ba7e-f96fe9f186d5 · outbound

This paper cites Nuclear thermodynamics from chiral low-momentum interactions.

Building Neutron Stars with the MUSES Calculation Engine Nuclear thermodynamics from chiral low-momentum interactions

Reference 40

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.366058Z digest=sha256:aee699bb8d20837eb16fbd9bdce17b23e08c7d46fa55caa4ff46702eacd57f35

Observation ab780c18-5765-4cc3-8811-65fd977400c0 · outbound

This paper cites Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory.

Building Neutron Stars with the MUSES Calculation Engine Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.369450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.369450Z digest=sha256:1c119e87069ab544ac54e78b3142f304580b829005860068684a51245bd5cd42

Observation 1a025b28-aecd-424e-95d7-1f9f87847164 · outbound

This paper cites Proto-Neutron and Neutron Stars in a Chiral SU(3) Model.

Building Neutron Stars with the MUSES Calculation Engine Proto-Neutron and Neutron Stars in a Chiral SU(3) Model

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.372874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.372874Z digest=sha256:474b480e3cf433611899b6fcd0b1cfe5351b87ff24f4ea72fff71271695784ca

Observation 056b031a-4404-4f3a-9d7f-e802c905aa9c · outbound

This paper cites A Novel Approach to Model Hybrid Stars.

Building Neutron Stars with the MUSES Calculation Engine A Novel Approach to Model Hybrid Stars

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.376217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.376217Z digest=sha256:c5a70e6d589d7b824453ca62e461cdf2d6a71a1acd806477beb92feed00755de

Observation 05afb77f-d45d-4695-8b62-7bd23a3a0977 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.379608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.379608Z digest=sha256:969553488c1f66de3f259b27679d29b93b5f9e95a238f230b396a453477a3958

Observation 8d8ad9f6-a9fd-4db7-b7da-c35ac5d46df3 · outbound

This paper cites Pelicer, Lepton module (2025).

Building Neutron Stars with the MUSES Calculation Engine Pelicer, Lepton module (2025)

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.382452Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.382452Z digest=sha256:bdb22fd64c7b220f7b672dac35ae397dbcdfbb34a10660d77563769981a78e5c

Observation 13865638-16bd-4499-96ea-ce9bc9f95db6 · outbound

This paper cites Lattice-based equation of state at finite baryon number, electric charge and strangeness chemical potentials.

Building Neutron Stars with the MUSES Calculation Engine Lattice-based equation of state at finite baryon number, electric charge and strangeness chemical potentials

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.385176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.385176Z digest=sha256:da3cd473e4d8e4dfb278bba4c26de70b4819ad90628c61d8cea23684a7a99aab

Observation fe2ce3b2-ba3e-42cc-8458-7b88e6981e1b · outbound

This paper cites Jahan, H.

Building Neutron Stars with the MUSES Calculation Engine Jahan, H

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.388245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.388245Z digest=sha256:21eb1cb9ed66b1e6b643c069b03c296e684af4a3a44e56c6ea8a05b796e847a3

Observation 25b6b9c2-9c9b-4a0b-a0aa-0cfc9bfb7493 · outbound

This paper cites Lattice QCD equation of state at finite chemical potential from an alternative expansion scheme.

Building Neutron Stars with the MUSES Calculation Engine Lattice QCD equation of state at finite chemical potential from an alternative expansion scheme

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.391071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.391071Z digest=sha256:885999ea0beb89100e826a7de1def34e1f7f7c05bf797c585f619018b01cd83e

Observation b9b95d9d-5983-4d71-89aa-c1611810b80d · outbound

This paper cites Finite density QCD equation of state: critical point and lattice-based $T'$-expansion.

Building Neutron Stars with the MUSES Calculation Engine Finite density QCD equation of state: critical point and lattice-based $T'$-expansion

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.394122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.394122Z digest=sha256:52ce0ccbe164114a1ecfadad1d8b35dd5b94e025e32e450ba51568a0595e26e4

Observation 629b55d4-b590-4fd5-8269-a91555bd25d5 · outbound

This paper cites Kahangirwe, J.

Building Neutron Stars with the MUSES Calculation Engine Kahangirwe, J

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.397738Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.397738Z digest=sha256:a3d5b1baf1948b9fdf3d7b52e0ee3e887ebab368339248da27ce68911e8f140b

Observation cafefac6-6766-42d6-9536-a7e6e620a1eb · outbound

This paper cites Correcting event-by-event fluctuations in heavy-ion collisions for exact global conservation laws with the generalized subensemble acceptance method.

Building Neutron Stars with the MUSES Calculation Engine Correcting event-by-event fluctuations in heavy-ion collisions for exact global conservation laws with the generalized subensemble acceptance method

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.400911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.400911Z digest=sha256:85d89b3cc25bd937d5545d61e103494706fb4a3eeb6609d001e9ae39224ac859

Observation 48559e50-bf2f-4312-b2c9-5c59fc5faaa4 · outbound

This paper cites The Large N Limit of Superconformal Field Theories and Supergravity.

Building Neutron Stars with the MUSES Calculation Engine The Large N Limit of Superconformal Field Theories and Supergravity

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.404965Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.404965Z digest=sha256:e50455d059e241253ee758377c709d130cd5f5ca482293f22345568e048b04ea

Observation 8c9b0934-0bc4-47f0-b564-a425e7912d94 · outbound

This paper cites A holographic critical point.

Building Neutron Stars with the MUSES Calculation Engine A holographic critical point

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.408929Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.408929Z digest=sha256:86e26c9e4a3f99a08df45e365d0f6f223cc1183b97c2a7014c29493753639d6a

Observation 598ad784-64bc-46ce-adbd-a93ee05b0eda · outbound

This paper cites Critical point in the phase diagram of primordial quark-gluon matter from black hole physics.

Building Neutron Stars with the MUSES Calculation Engine Critical point in the phase diagram of primordial quark-gluon matter from black hole physics

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.412608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.412608Z digest=sha256:7970098d96c0b58f731c5ddb4726b1f8abedcb49e47ef3ed5bc805a37b206406

Observation 89b1c6f5-a68a-4116-8d28-034e1f44fbef · outbound

This paper cites Hot and dense quark-gluon plasma thermodynamics from holographic black holes.

Building Neutron Stars with the MUSES Calculation Engine Hot and dense quark-gluon plasma thermodynamics from holographic black holes

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.416132Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.416132Z digest=sha256:f784983e46fe7489614f046ee70875b6871beb05a2866eb7f186dab6db83179a

Observation 5423a689-f081-4296-b5eb-b5dea2b614b1 · outbound

This paper cites Hot QCD Phase Diagram From Holographic Einstein-Maxwell-Dilaton Models.

Building Neutron Stars with the MUSES Calculation Engine Hot QCD Phase Diagram From Holographic Einstein-Maxwell-Dilaton Models

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.419200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.419200Z digest=sha256:8220a9fbd560ee562f23db85e30773cd08ff77ad57b9ffbb80f51f8f09159116

Observation ce5d2da9-40ba-4b9d-bd65-85840560e7f2 · outbound

This paper cites Bayesian location of the QCD critical point from a holographic perspective.

Building Neutron Stars with the MUSES Calculation Engine Bayesian location of the QCD critical point from a holographic perspective

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.422258Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.422258Z digest=sha256:05df905ff08cf39e3433627a5aa7bb34e8477d22c1e9730605cec83b4e4fb690

Observation a307b3d7-dced-4d1f-a258-bd0e680d06d4 · outbound

This paper cites Yang and M.

Building Neutron Stars with the MUSES Calculation Engine Yang and M

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.425328Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.425328Z digest=sha256:de6935ca09cc20f7f499c1bc409d1b6aec0d3cc823140f6919185118e4683eb2

Observation 81e4d004-8984-4933-a991-afe7e59ad1cd · outbound

This paper cites Hippert, J.

Building Neutron Stars with the MUSES Calculation Engine Hippert, J

Reference 59

Resolution
verified exact
doi, observed 2026-08-08T11:32:34.911917Z

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.

source=pdf_text observed=2026-08-08T11:32:34.428148Z digest=sha256:b96733f08d22dc27d76290c4ee0398d5cdb14afb3166a0b34ffe0e300f7e129b

Observation 092e7e36-c165-4200-8f22-8c49a70e146f · outbound

This paper cites Pelicer, Equation of state synthesis (2025).

Building Neutron Stars with the MUSES Calculation Engine Pelicer, Equation of state synthesis (2025)

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.431765Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.431765Z digest=sha256:ab6eb0b2c74052ba22a319f7053e9c39a155e4e504139484970d932cf3433193

Observation f82b0794-ff20-448a-bfa4-bba4537448c8 · outbound

This paper cites Lee, Lattice Effective Field Theory Simulations of Nuclei (2025), arXiv:2501.03303 [nucl-th].

Building Neutron Stars with the MUSES Calculation Engine Lee, Lattice Effective Field Theory Simulations of Nuclei (2025), arXiv:2501.03303 [nucl-th]

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.435194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.435194Z digest=sha256:6ee13da2687c109feb09506e18fec0dd27f132d293ffc053a1c205d5d6efa3bc

Observation 572960e8-b7cb-4d40-bad3-61063051a6ee · outbound

This paper cites BSQ Conserved Charges in Relativistic Viscous Hydrodynamics solved with Smoothed Particle Hydrodynamics.

Building Neutron Stars with the MUSES Calculation Engine BSQ Conserved Charges in Relativistic Viscous Hydrodynamics solved with Smoothed Particle Hydrodynamics

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.438448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.438448Z digest=sha256:a7bbe7f1d09a7be2d6ecd658337dea1f8a657687039df41290e4a0bf4de4426b

Observation 96e9f3d3-e0cc-4f59-bcdb-45ea45fc1a3b · outbound

This paper cites Unlocking "imprints" of conserved charges in the initial state of heavy-ion collisions.

Building Neutron Stars with the MUSES Calculation Engine Unlocking "imprints" of conserved charges in the initial state of heavy-ion collisions

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.442071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.442071Z digest=sha256:f7a40395e5d759535c1f7fbb62b5402ecc4a04bfa7b524cab2e795d6d0f68a27

Observation 804404cf-491f-4500-8f78-0e2d823a818c · outbound

This paper cites Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter.

Building Neutron Stars with the MUSES Calculation Engine Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.446118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.446118Z digest=sha256:df59de59dd4fe0c76c295d447ffacc45d8f11630b01730edfed5333fc28e21c3

Observation 65ccdfc6-6bcf-4549-a6a6-ecd896f1d5b6 · outbound

This paper cites Isospin Equilibration in Neutron Star Mergers.

Building Neutron Stars with the MUSES Calculation Engine Isospin Equilibration in Neutron Star Mergers

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.449865Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.449865Z digest=sha256:cdcd0bb791981d0ecd678729b0ad13eeff6006a8d254246c6bff77e555d688c6

Observation 7ce1f718-f815-4d10-87ee-1f52cd127246 · outbound

This paper cites Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter.

Building Neutron Stars with the MUSES Calculation Engine Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.453445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.453445Z digest=sha256:9ff525460773cbbc7ceb98ef3dbecb65050a992d34b965a1a358b8be3375f13c

Observation 99913c22-7c67-4931-b0f8-5db6bb5fc8a2 · outbound

This paper cites Alford and Z.

Building Neutron Stars with the MUSES Calculation Engine Alford and Z

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.456735Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.456735Z digest=sha256:f0460a280d519224879fc8f43d6c3549a6b17f7c3641527175649acd3db70266

Observation 91ea837c-a954-40f6-ae70-30b0f41c2bc5 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.459668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.459668Z digest=sha256:e80926f2e889a737f65cc36d8fc394e6bddc61c699cc33dcf0768356d2298380

Observation 3bbd1da0-f276-4d5b-af82-66f42adfa38a · outbound

This paper cites Bejger and P.

Building Neutron Stars with the MUSES Calculation Engine Bejger and P

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.462408Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.462408Z digest=sha256:88a1614e9473016491deec5fcf09b066e81ba5c9efd374733327a6baefe16481

Observation 66bfac5e-0da5-4a58-8983-f8104144b8a4 · outbound

This paper cites Why I-Love-Q.

Building Neutron Stars with the MUSES Calculation Engine Why I-Love-Q

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.466135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.466135Z digest=sha256:e9b11738c1c851deb05fca5d2f9c89816f61724d0635e5e635f53c8a7c9c8489

Observation 7fd01bce-d0d0-4a0e-9587-6141fd1e6a0b · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.469427Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.469427Z digest=sha256:199a1430808f293249e27042dbcf5eb943f47fdcacb34636583625101ae5d956

Observation c9b14c00-7e25-40bf-a306-d185bfa4545c · outbound

This paper cites Structure in the speed of sound: from neutron stars to heavy-ion collisions.

Building Neutron Stars with the MUSES Calculation Engine Structure in the speed of sound: from neutron stars to heavy-ion collisions

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.472047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.472047Z digest=sha256:bca19f54bc8b55baf4c15a3022d2f374c4129f0dc9eedff8baffe94dd07065f2

Observation a5527661-5ffd-4a33-b4e3-fe2ef64d1474 · outbound

This paper cites Core-collapse supernova equations of state based on neutron star observations.

Building Neutron Stars with the MUSES Calculation Engine Core-collapse supernova equations of state based on neutron star observations

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.476005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.476005Z digest=sha256:2760980895eb62b1c6076083a57dca206d91ac862c24dadd37991d7598e3024e

Observation 6be711c8-f166-4ce1-b605-cf98c9120dcd · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.479853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.479853Z digest=sha256:121bcff9ae0391944353900089124f518bd278f66bc0d419c31f920f76194abc

Observation 670ec502-943e-410b-ad68-153e07dd5bb1 · outbound

This paper cites Nuclear ground-state masses and deformations: FRDM(2012).

Building Neutron Stars with the MUSES Calculation Engine Nuclear ground-state masses and deformations: FRDM(2012)

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.483445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.483445Z digest=sha256:8b1733240570d53ee9d1cefb7f486f4bac38af0a260742fe9ff58d2d54ec31e6

Observation e7425ba4-7980-4aaa-ad01-2587257e2e1d · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.487833Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.487833Z digest=sha256:55ad0c931ea712b09e54b53bc22fd6dcd2178467357f1cf0187aa1db2ec3f657

Observation d7c9c029-1b92-468c-b1ca-c28336bec218 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.491195Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.491195Z digest=sha256:f066c17cefb4c6a633e3bb2fc01a2c4d2134d9928b1607a1b9bce79944068a67

Observation f6a39022-059c-48b0-a1f0-9048cdc97998 · outbound

This paper cites Kortelainen, J.

Building Neutron Stars with the MUSES Calculation Engine Kortelainen, J

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.494940Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.494940Z digest=sha256:a2fa84b6c0338d586e4a2e4217c2a07af96acbf092cbeb372874f1c74f29b451

Observation c2b2e6d2-fafb-4e75-a9fe-8fc46be9dc20 · outbound

This paper cites Modern Theory of Nuclear Forces.

Building Neutron Stars with the MUSES Calculation Engine Modern Theory of Nuclear Forces

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.498254Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.498254Z digest=sha256:1b9c24ba40ed092953c31da176552cc3c2ad76de7d40ba52555856c956cce436

Observation 973d1825-f9c2-4a56-ac21-161e9ac7c202 · outbound

This paper cites Is nuclear matter perturbative with low-momentum interactions?.

Building Neutron Stars with the MUSES Calculation Engine Is nuclear matter perturbative with low-momentum interactions?

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.502274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.502274Z digest=sha256:0e3e32c4dfb6b9ec6a70f8bdd6801c100bbf8e52bc4cc32c0b2a1d519b3952a2

Observation 37841fa4-c278-4fbd-a6a1-74ce0d044ac6 · outbound

This paper cites Friedenberg and J.

Building Neutron Stars with the MUSES Calculation Engine Friedenberg and J

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.505789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.505789Z digest=sha256:15221892f70788fc7bc0ba065a17de6b6717b4254acbd354ffeac4ab11971157

Observation dd0918a3-557a-4135-bc92-1d91ab76198f · outbound

This paper cites Weinberg, Nuclear forces from chiral Lagrangians, Phys.

Building Neutron Stars with the MUSES Calculation Engine Weinberg, Nuclear forces from chiral Lagrangians, Phys

Reference 82

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no resolver link, observed 2026-08-08T11:32:34.508617Z

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source=pdf_text observed=2026-08-08T11:32:34.508617Z digest=sha256:e5959322b5f1027fdcba0fa2480f7ceca8e269c3a405397db080f39fb4985adb

Observation 7a2b0bbb-e1f4-4a62-92f5-496d13be380e · outbound

This paper cites Coraggio, A.

Building Neutron Stars with the MUSES Calculation Engine Coraggio, A

Reference 83

Resolution
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no resolver link, observed 2026-08-08T11:32:34.511993Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-08T11:32:34.511993Z digest=sha256:b7b47b24dc1b95103bfb4fdbd8d78155516e581199671bb1d5ad384ca350b530

Observation 682b9979-3bf5-4c6c-bc37-64b7f5a7652d · outbound

This paper cites Reduced regulator dependence of neutron-matter predictions with chiral interactions.

Building Neutron Stars with the MUSES Calculation Engine Reduced regulator dependence of neutron-matter predictions with chiral interactions

Reference 84

Resolution
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no resolver link, observed 2026-08-08T11:32:34.515359Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-08T11:32:34.515359Z digest=sha256:873e4259901c1aa7e73578bde88faa4b48ebd69f38b45a941848565678ae7e7a

Observation 90c3e740-4390-4208-85b5-67917306dbd9 · outbound

This paper cites Density-dependent effective nucleon-nucleon interaction from chiral three-nucleon forces.

Building Neutron Stars with the MUSES Calculation Engine Density-dependent effective nucleon-nucleon interaction from chiral three-nucleon forces

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.519073Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.519073Z digest=sha256:e41454bb1f037665b3299449abab757755f7081e044befec22d3d52b382a65cf

Observation 952dae0b-7f97-42ed-9602-68e7b3eaf3bb · outbound

This paper cites Nuclear chiral dynamics and thermodynamics.

Building Neutron Stars with the MUSES Calculation Engine Nuclear chiral dynamics and thermodynamics

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.522334Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.522334Z digest=sha256:ec0816d23f8605cd029f92b04948483ffd1ce24d10461ea02c46f7d3f48151b6

Observation 57522fa3-cc2a-44cf-aa03-fcf1ed02d292 · outbound

This paper cites Implementing chiral three-body forces in terms of medium-dependent two-body forces.

Building Neutron Stars with the MUSES Calculation Engine Implementing chiral three-body forces in terms of medium-dependent two-body forces

Reference 87

Resolution
verified exact
local_arxiv, observed 2026-08-08T11:32:35.979125Z

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.

source=pdf_text observed=2026-08-08T11:32:34.526008Z digest=sha256:87b2a244adf508eec2865b767b2bed246e43737afdad5bb9761dad8d24447fb8

Observation 5b819f94-c736-46ae-8199-589463953ed1 · outbound

This paper cites Neutron star tidal deformabilities constrained by nuclear theory and experiment.

Building Neutron Stars with the MUSES Calculation Engine Neutron star tidal deformabilities constrained by nuclear theory and experiment

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.529945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.529945Z digest=sha256:3daa151c2f461e1ff3b454e2ea5111c86f95dbf0dcb71407d255ec08a0e8ebf2

Observation bb32fb8c-0c97-482c-8181-68290545c4b8 · outbound

This paper cites Predicting the moment of inertia of pulsar J0737-3039A from Bayesian modeling of the nuclear equation of state.

Building Neutron Stars with the MUSES Calculation Engine Predicting the moment of inertia of pulsar J0737-3039A from Bayesian modeling of the nuclear equation of state

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-08-08T11:32:35.955909Z

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.

source=pdf_text observed=2026-08-08T11:32:34.533733Z digest=sha256:5b43a75f35e46fc4978c753dd79e811a1bd6ec6ee39d63e2a0fba7a67d4c619f

Observation 92be52e9-890e-4111-9a9b-25ab6337e401 · outbound

This paper cites Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817.

Building Neutron Stars with the MUSES Calculation Engine Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.537839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.537839Z digest=sha256:af3162d1c857493c3c01382ef0756a007bfd6b468670e5fb95314c5e44d7a02d

Observation c7b7fd2c-119d-42a7-99ff-d14c59ebfb23 · outbound

This paper cites Kohn and J.

Building Neutron Stars with the MUSES Calculation Engine Kohn and J

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.541566Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-08T11:32:34.541566Z digest=sha256:3449e7841e21f050e9fe9b17db5d1872f27bd2355ee575ee2f75a051a709a34e

Observation 3c3e55a1-2615-46b6-a133-d00b99dd933b · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.545615Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:32:34.545615Z digest=sha256:cb9018fc7361d6d4327591dfa085c120eb3afe9c5bdf9f55740a1b8e679b4b1d

Observation e02b0c84-1b65-4c4c-952d-394670c75de1 · outbound

This paper cites Divergence of the isospin-asymmetry expansion of the nuclear equation of state in many-body perturbation theory.

Building Neutron Stars with the MUSES Calculation Engine Divergence of the isospin-asymmetry expansion of the nuclear equation of state in many-body perturbation theory

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.549339Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-08T11:32:34.549339Z digest=sha256:3b2725746d7a3ed695cd9a3532a27f114b4151b438813ebb8ee316148d318102

Observation c61e0d80-d191-47ff-9c31-e93d366016e1 · outbound

This paper cites Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT.

Building Neutron Stars with the MUSES Calculation Engine Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.553312Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-08T11:32:34.553312Z digest=sha256:2e641d7d92917f1039363fe079df59065ca90ae8c7635ac7a3d7a0e7423bf596

Observation acf05089-1282-498c-83ae-a9b433b344fb · outbound

This paper cites Low-momentum NN interactions and all-order summation of ring diagrams of symmetric nuclear matter.

Building Neutron Stars with the MUSES Calculation Engine Low-momentum NN interactions and all-order summation of ring diagrams of symmetric nuclear matter

Reference 95

Resolution
verified exact
local_arxiv, observed 2026-08-08T11:32:35.904646Z

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.

source=pdf_text observed=2026-08-08T11:32:34.556672Z digest=sha256:42c8df09194726b460a72ea8a31b80c2623bfea563b7147bf77211455c512099

Observation 24280343-355f-44f5-99e3-3a04ee39c4d2 · outbound

This paper cites From low-momentum interactions to nuclear structure.

Building Neutron Stars with the MUSES Calculation Engine From low-momentum interactions to nuclear structure

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.559666Z

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source=pdf_text observed=2026-08-08T11:32:34.559666Z digest=sha256:0eb8667210c77b0f2e51647b507eb609e03eaeb16dbdc212728bf42b802f8bde

Observation e8c04d03-cd63-4324-a33a-51b7073fa3f7 · outbound

This paper cites Weinberg, Nonlinear realizations of chiral symmetry, Phys.

Building Neutron Stars with the MUSES Calculation Engine Weinberg, Nonlinear realizations of chiral symmetry, Phys

Reference 97

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no resolver link, observed 2026-08-08T11:32:34.562771Z

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source=pdf_text observed=2026-08-08T11:32:34.562771Z digest=sha256:3a67b6ad3b45fc4fa4691db536861fd7816f189d92fa51f1f19eeab115d4924a

Observation 75cfea4e-b854-4845-9227-5cb1112254a6 · outbound

This paper cites Papazoglou, D.

Building Neutron Stars with the MUSES Calculation Engine Papazoglou, D

Reference 98

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no resolver link, observed 2026-08-08T11:32:34.565648Z

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source=pdf_text observed=2026-08-08T11:32:34.565648Z digest=sha256:edd4a1076b1fd1867bd55bc1ebd722c0af661803c2f9c7283cc20fd2d0237c85

Observation de8d24aa-2cd0-42eb-9566-6c4f113d1119 · outbound

This paper cites an unresolved cited work.

Building Neutron Stars with the MUSES Calculation Engine Unresolved cited work

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.568943Z

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source=pdf_text observed=2026-08-08T11:32:34.568943Z digest=sha256:5cf7c1395a6867ad1f5952bfc18a9d01fe9cb8b6321e56d6d6576712f54bbdec

Observation 106f6b43-973f-48a5-9ebb-685d61009398 · outbound

This paper cites Non-congruence of the nuclear liquid-gas and deconfinement phase transitions.

Building Neutron Stars with the MUSES Calculation Engine Non-congruence of the nuclear liquid-gas and deconfinement phase transitions

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.572430Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-08T11:32:34.572430Z digest=sha256:1e49c865725f2307c32cda60b4d2c4f666051e13949e3df7b106e40000b5f944

Pith citing papers

Observation 09cf1fd1-af28-4b2d-8aa9-4dbd8c97703b · inbound

Symmetry Energy Expansion with Strange Dense Matter cites this paper.

Symmetry Energy Expansion with Strange Dense Matter Building Neutron Stars with the MUSES Calculation Engine

Reference 85

Resolution
verified exact
arxiv_id, observed 2026-05-22T18:21:55.453487Z

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

source=pdf_text observed=2026-05-22T18:20:24.680116Z digest=sha256:ed3d3e44b464c4b23cc50fedb785bbbe72807a072b52d3d1aed9ecf04fdce617

Observation bc31f5f9-cfa7-487d-88b3-f24961c47ade · inbound

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars cites this paper.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Building Neutron Stars with the MUSES Calculation Engine

Reference 21

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unresolved
no resolver link, observed 2026-08-07T15:31:32.607156Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:31:32.607156Z digest=sha256:ed2e8da313165dbf0158b076a97d1ed859455fd39ba4c40b55bd108dac6eba14

Observation e4ef59c1-6842-4388-aa65-af9ec7914ef5 · inbound

Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework cites this paper.

Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework Building Neutron Stars with the MUSES Calculation Engine

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-07T14:28:47.969566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:28:47.969566Z digest=sha256:768122b867e203434cfc3aff7648cdcaa4ea079dcbabeba28830dc260202e067

Observation 27f53119-d009-4668-b935-95395b2db195 · inbound

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation cites this paper.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Building Neutron Stars with the MUSES Calculation Engine

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.947288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.947288Z digest=sha256:a135a5faac817500b256e0d7ae821ebc36fda974bebc0cdf1c4d2c2de4e10a3f

Observation d44737fc-5969-45d2-9b2c-684d03e9a888 · inbound

Toward a Unified Understanding of the Dense Matter Equation of State cites this paper.

Toward a Unified Understanding of the Dense Matter Equation of State Building Neutron Stars with the MUSES Calculation Engine

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-03T20:20:19.172188Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T20:20:19.172188Z digest=sha256:029dc102a44dcd075b07ecd08d05ec0c9020da613cc16ce798fdd52a8d3ba5ab

Observation ecaaad0f-30f3-4868-b0d7-a8ebd7907085 · inbound

Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling cites this paper.

Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling Building Neutron Stars with the MUSES Calculation Engine

Reference 44

Resolution
verified exact
arxiv_id, observed 2026-07-02T19:07:18.441783Z

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.

source=pdf_text observed=2026-06-27T21:37:55.919953Z digest=sha256:e51856753b7704140899584e7b429b52c571fca60b9c865fd753169e398ad655

Observation 40cf57d2-3c85-460c-8380-e9b1f07b63fc · inbound

Scaling of the Surface Free Energy as a Probe of the QCD Critical Region cites this paper.

Scaling of the Surface Free Energy as a Probe of the QCD Critical Region Building Neutron Stars with the MUSES Calculation Engine

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-07-03T18:38:48.969001Z

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.

source=pdf_text observed=2026-06-27T02:47:17.260960Z digest=sha256:9a644355aa8ee2881196473a88354366ce9a4aa25793e5eda71ed83f4c1aea5c

Observation 713046e3-50d7-49f2-975f-e4bf54f73006 · inbound

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine cites this paper.

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine Building Neutron Stars with the MUSES Calculation Engine

Reference 95

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:19:57.331222Z

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.

source=pdf_text observed=2026-06-26T00:47:21.247516Z digest=sha256:c725b4707af85668bc16bcc6fbf6704296bdf68c690445420647c4ba258ce1ab

Observation 17644d04-1653-43c6-9286-d91471e6824c · inbound

Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties cites this paper.

Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties Building Neutron Stars with the MUSES Calculation Engine

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-02T05:44:20.789666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T05:44:20.789666Z digest=sha256:dd2f5eb23da15b2a56b90d0be5a6a8df6cacc45feb7fc789708f3cdbbc530fdb

Observation 1e4afbc3-6fd7-4fb7-bf27-dc301537afd9 · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars Building Neutron Stars with the MUSES Calculation Engine

Reference 293

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:27.394945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:27.394945Z digest=sha256:d32b8a44f756a936cfecbdcf2435c90b7b5a3e6335e5c4cc4c9bac4a2cd2975f

Observation fe49bf93-b53b-4dfa-860d-5ea5f77f64e5 · inbound

Nuclear matter equation of state and astrophysics cites this paper.

Nuclear matter equation of state and astrophysics Building Neutron Stars with the MUSES Calculation Engine

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-01T01:20:21.621988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T01:20:21.621988Z digest=sha256:5941e1802319997268e99716fb3cea7c0d3f24516573e47da8dea8b9be72f4a4