Paper Citation Record · LEDGER

Constraining Hamiltonians from chiral effective field theory with neutron-star data

As of 23 August 2026, this Paper Citation Record lists 94 of 94 outbound references and 4 inbound Pith citation observations for arXiv:2601.05999.

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2601.05999 v2

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measured 94 of 94 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-04T00:40:16.148665Z

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 4 of 4 inbound itemization

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Source: paper_references, paper_reference_links, observed 2026-08-15T22:22:01.873335Z

measured 1 of 1 external citation measurements

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Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 50be1a8c-1d52-483f-9a36-b714bc54281d · outbound

This paper cites The Physics of Neutron Stars.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The Physics of Neutron Stars

Reference 1

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Observation 2946d89b-af55-484f-a600-8737dedf73b7 · outbound

This paper cites Measuring the neutron star equation of state using X-ray timing.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Measuring the neutron star equation of state using X-ray timing

Reference 2

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Observation a1e75f51-5dbf-4367-8bb4-6c9d571c6e68 · outbound

This paper cites Chatziioannou, H.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Chatziioannou, H

Reference 3

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Observation ebbda794-a643-438e-9cb1-b62f960fd267 · outbound

This paper cites Modern Theory of Nuclear Forces.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Modern Theory of Nuclear Forces

Reference 4

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Observation d3825543-47a8-46e6-9099-6b369e54679d · outbound

This paper cites Chiral effective field theory and nuclear forces.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Chiral effective field theory and nuclear forces

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:04.822404Z

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Observation b4fa526d-6460-4434-8886-7345fb1ed62b · outbound

This paper cites Accurate Charge-Dependent Nucleon-Nucleon Potential at Fourth Order of Chiral Perturbation Theory.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Accurate Charge-Dependent Nucleon-Nucleon Potential at Fourth Order of Chiral Perturbation Theory

Reference 6

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Observation 301c6bfd-4809-4f1e-8fe2-a31cdc59a51e · outbound

This paper cites The two-nucleon system at next-to-next-to-next-to-leading order.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The two-nucleon system at next-to-next-to-next-to-leading order

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:05.138241Z

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Observation 6ef97f59-169a-47c0-bc06-73726012800f · outbound

This paper cites Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions

Reference 8

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Observation 2697fb68-68bb-4a85-a4ac-4ac5d94fa068 · outbound

This paper cites Minimally non-local nucleon-nucleon potentials with chiral two-pion exchange including $\Delta$'s.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Minimally non-local nucleon-nucleon potentials with chiral two-pion exchange including $\Delta$'s

Reference 9

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Observation 361c103c-7ffb-48d0-956f-6930d23226b9 · outbound

This paper cites Semilocal momentum-space regularized chiral two-nucleon potentials up to fifth order.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Semilocal momentum-space regularized chiral two-nucleon potentials up to fifth order

Reference 10

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Observation 42c94d7c-a16e-4039-affe-a1e18ed8b4da · outbound

This paper cites High-quality two-nucleon potentials up to fifth order of the chiral expansion.

Constraining Hamiltonians from chiral effective field theory with neutron-star data High-quality two-nucleon potentials up to fifth order of the chiral expansion

Reference 11

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Observation 74d92bfd-8753-43f2-ba8e-ad62ea3c12ed · outbound

This paper cites Maximally local two-nucleon interactions at N$^3$LO in $\Delta$-less chiral effective field theory.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Maximally local two-nucleon interactions at N$^3$LO in $\Delta$-less chiral effective field theory

Reference 12

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Observation 41f662d9-05ef-46aa-b6b7-c3bc458ddf61 · outbound

This paper cites Navratil, V.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Navratil, V

Reference 13

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Observation 8fefc1c2-65e6-4dfa-9891-fd8123da4ed9 · outbound

This paper cites Three-Nucleon Low-Energy Constants from the Consistency of Interactions and Currents in Chiral Effective Field Theory.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Three-Nucleon Low-Energy Constants from the Consistency of Interactions and Currents in Chiral Effective Field Theory

Reference 14

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Observation 472da770-833a-4f5a-a100-31161f6fb24b · outbound

This paper cites Improved nuclear matter calculations from chiral low-momentum interactions.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Improved nuclear matter calculations from chiral low-momentum interactions

Reference 15

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Observation 957bc8a9-c247-4926-9e29-64b66afb3148 · outbound

This paper cites Chiral Three-Nucleon Interactions in Light Nuclei, Neutron-$\alpha$ Scattering, and Neutron Matter.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Chiral Three-Nucleon Interactions in Light Nuclei, Neutron-$\alpha$ Scattering, and Neutron Matter

Reference 16

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Observation 917bbdb7-a4f6-47d5-be33-5d14145712b9 · outbound

This paper cites Light-nuclei spectra from chiral dynamics.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Light-nuclei spectra from chiral dynamics

Reference 17

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Observation c13cf8e8-47e8-4c0d-a69e-e3f652062089 · outbound

This paper cites Few- and many-nucleon systems with semilocal coordinate-space regularized chiral two- and three-body forces.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Few- and many-nucleon systems with semilocal coordinate-space regularized chiral two- and three-body forces

Reference 18

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Observation 406f01c5-ca44-4b80-be98-5771c8ce8dbb · outbound

This paper cites Neutron matter from local chiral effective field theory interactions at large cutoffs.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Neutron matter from local chiral effective field theory interactions at large cutoffs

Reference 19

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Observation 36ac2d26-32ad-4b1f-9ecd-f33bba6db1f3 · outbound

This paper cites Curry, K.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Curry, K

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:07.003940Z

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Observation c882a254-91d3-4ea2-a330-62565eafc3bf · outbound

This paper cites Accurate nuclear radii and binding energies from a chiral interaction.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Accurate nuclear radii and binding energies from a chiral interaction

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:07.138376Z

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Observation bd25eb37-3e71-4f44-bebe-1ff14296331f · outbound

This paper cites Neutron-rich nuclei and neutron skins from chiral low-resolution interactions.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Neutron-rich nuclei and neutron skins from chiral low-resolution interactions

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:07.270221Z

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Observation 58ec98fc-d6f5-422c-9f31-8e0e4ff27e7b · outbound

This paper cites Ab initio limits of atomic nuclei.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Ab initio limits of atomic nuclei

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:07.440742Z

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Observation fbcd05d4-d242-466d-92d8-c2f68becad7c · outbound

This paper cites Converged ab initio calculations of heavy nuclei.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Converged ab initio calculations of heavy nuclei

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:07.540207Z

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Observation e12e609a-7d30-4506-a805-19cedb597c0f · outbound

This paper cites Ab initio predictions link the neutron skin of ${}^{208}$Pb to nuclear forces.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Ab initio predictions link the neutron skin of ${}^{208}$Pb to nuclear forces

Reference 25

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Observation b833d12e-ab31-4a7b-a9c0-4313055996aa · outbound

This paper cites Normal ordering of three-nucleon interactions for ab initio calculations of heavy nuclei.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Normal ordering of three-nucleon interactions for ab initio calculations of heavy nuclei

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:07.815982Z

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Observation cb7e63c4-0788-4873-b817-c91660b79e02 · outbound

This paper cites Impact of two-body currents on magnetic dipole moments of nuclei.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Impact of two-body currents on magnetic dipole moments of nuclei

Reference 27

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Observation 16386899-59d5-4db3-9eb1-d444d2b659b1 · outbound

This paper cites Probing new bosons and nuclear structure with ytterbium isotope shifts.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Probing new bosons and nuclear structure with ytterbium isotope shifts

Reference 28

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Observation 422b4a8d-ac0f-41d3-af45-eb4fc1e20b7c · outbound

This paper cites Structure of the doubly magic nuclei $^{208}$Pb and $^{266}$Pb from ab initio computations.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Structure of the doubly magic nuclei $^{208}$Pb and $^{266}$Pb from ab initio computations

Reference 29

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Observation 1f76f126-a9fb-4dfa-8330-c967c45b74cf · outbound

This paper cites Ab initio calculations of beta-decay half-lives for $N=50$ neutron-rich nuclei.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Ab initio calculations of beta-decay half-lives for $N=50$ neutron-rich nuclei

Reference 30

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Observation 351250b0-597a-4d96-a99e-d7eb8169ca62 · outbound

This paper cites r-Process Nucleosynthesis With Ab Initio Nuclear Masses Around The N=82 Shell Closure.

Constraining Hamiltonians from chiral effective field theory with neutron-star data r-Process Nucleosynthesis With Ab Initio Nuclear Masses Around The N=82 Shell Closure

Reference 31

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Observation f6286789-ca6d-43f4-8147-e1cba56bc5bd · outbound

This paper cites Chiral three-nucleon forces and neutron matter.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Chiral three-nucleon forces and neutron matter

Reference 32

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Observation b4607df8-7ad7-400c-88c6-46ca9acef0e3 · outbound

This paper cites Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory

Reference 33

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Observation 66a94c48-d8ca-4bb2-bffb-1a4296f647a5 · outbound

This paper cites Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation

Reference 34

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Observation 3815bef0-97a8-4dad-b8a3-40d92f74ff5c · outbound

This paper cites Quantifying uncertainties and correlations in the nuclear-matter equation of state.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Quantifying uncertainties and correlations in the nuclear-matter equation of state

Reference 35

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Observation 9df369ef-06c4-477a-86ab-a18522a6d8ff · outbound

This paper cites Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials

Reference 36

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Observation 950781a9-65d0-4737-9420-4b04083f0dfb · outbound

This paper cites Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator

Reference 37

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Observation 622e1b04-0742-40ae-ac49-78f484527542 · outbound

This paper cites Marino, W.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Marino, W

Reference 38

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Observation 240ad456-b565-4eb9-87a9-5573736a796d · outbound

This paper cites Constraining three-nucleon forces with multimessenger data.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Constraining three-nucleon forces with multimessenger data

Reference 39

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Observation 81efcf58-c1e2-4a86-a85e-953b8e2414fa · outbound

This paper cites Sensitivity of Neutron Star Observations to Three-nucleon Forces.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Sensitivity of Neutron Star Observations to Three-nucleon Forces

Reference 40

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Observation f4eb37c4-d04a-4211-a127-310f11c02ff1 · outbound

This paper cites Revealing the strength of three-nucleon interactions with the Einstein Telescope.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Revealing the strength of three-nucleon interactions with the Einstein Telescope

Reference 41

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This paper cites Somasundaram, I.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Somasundaram, I

Reference 42

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Observation 69fbed90-209a-46f2-98d9-03a21ce89109 · outbound

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

Constraining Hamiltonians from chiral effective field theory with neutron-star data A Massive Pulsar in a Compact Relativistic Binary

Reference 43

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Observation cd5a40e7-63ab-4b78-bdd9-6dcebb145e51 · outbound

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

Constraining Hamiltonians from chiral effective field theory with neutron-star data The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars

Reference 44

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Observation c2c81743-60ee-4743-b723-6546fe12b27e · outbound

This paper cites Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620

Reference 45

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Observation 90808e26-4499-4c5e-acec-233b3b079cd3 · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Constraining Hamiltonians from chiral effective field theory with neutron-star data GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 46

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Observation ebb2b362-98f9-4c14-9c93-9e9d4e7756eb · outbound

This paper cites An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451.

Constraining Hamiltonians from chiral effective field theory with neutron-star data An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451

Reference 47

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Observation dff96c33-062d-45bb-984f-1335bc7c9007 · outbound

This paper cites The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data

Reference 48

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Observation 064ae173-e264-4b46-9520-7ad5c0001006 · outbound

This paper cites A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 49

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Observation 46723c6f-0699-4c3a-a06f-03fda4419092 · outbound

This paper cites Mauviardet al., A NICER view of the 1.4 solar- mass edge-on pulsar PSR J0614–3329, arXiv:2506.14883 [astro-ph.HE] (2025).

Constraining Hamiltonians from chiral effective field theory with neutron-star data Mauviardet al., A NICER view of the 1.4 solar- mass edge-on pulsar PSR J0614–3329, arXiv:2506.14883 [astro-ph.HE] (2025)

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Observation c1b7e4f4-4180-4fc9-a6f5-ff7e7f904e98 · outbound

This paper cites Towards accelerated nuclear-physics parameter estimation from binary neutron star mergers: Emulators for the Tolman-Oppenheimer-Volkoff equations.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Towards accelerated nuclear-physics parameter estimation from binary neutron star mergers: Emulators for the Tolman-Oppenheimer-Volkoff equations

Reference 51

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Observation a00ab3a6-9896-47e8-b18b-91bf621ea371 · outbound

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Constraining Hamiltonians from chiral effective field theory with neutron-star data Unresolved cited work

Reference 52

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Observation 2730089c-9540-4ed3-9676-d6cc6015413d · outbound

This paper cites Quantum Monte Carlo methods for nuclear physics.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Quantum Monte Carlo methods for nuclear physics

Reference 53

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Observation 62776a2b-d736-444f-a63d-a100b4915a67 · outbound

This paper cites Quantum Monte Carlo Methods in Nuclear Physics: Recent Advances.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Quantum Monte Carlo Methods in Nuclear Physics: Recent Advances

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Observation b7c3c03a-760d-4c86-93ef-d49d67a8c382 · outbound

This paper cites Roy-Steiner-equation analysis of pion-nucleon scattering.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Roy-Steiner-equation analysis of pion-nucleon scattering

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Observation e8f3cc9b-1475-4b7b-bb72-a470f2c40314 · outbound

This paper cites Reconciling threshold and subthreshold expansions for pion-nucleon scattering.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Reconciling threshold and subthreshold expansions for pion-nucleon scattering

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Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:11.070143Z

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Observation 9ed7a7c1-c37e-497e-b890-c3d584f25a64 · outbound

This paper cites an unresolved cited work.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:11.304858Z

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Observation 9f72d46a-eb54-4444-9646-7e718cb12e73 · outbound

This paper cites Parametric Matrix Models.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Parametric Matrix Models

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:11.494096Z

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Observation f7c6e340-3467-4643-81a5-0a4475b9b1df · outbound

This paper cites Frame, R.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Frame, R

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:11.661375Z

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Observation 772b345a-eb2b-4f57-af3d-42336cf21104 · outbound

This paper cites Eigenvector Continuation as an Efficient and Accurate Emulator for Uncertainty Quantification.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Eigenvector Continuation as an Efficient and Accurate Emulator for Uncertainty Quantification

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:11.842975Z

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Observation 28fec56c-4b19-4c8b-9f8d-660569953aca · outbound

This paper cites Training and Projecting: A Reduced Basis Method Emulator for Many-Body Physics.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Training and Projecting: A Reduced Basis Method Emulator for Many-Body Physics

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.007397Z

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Observation 979bc6d9-b037-46ef-8c15-d88a7adc121a · outbound

This paper cites BUQEYE Guide to Projection-Based Emulators in Nuclear Physics.

Constraining Hamiltonians from chiral effective field theory with neutron-star data BUQEYE Guide to Projection-Based Emulators in Nuclear Physics

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.178984Z

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Observation dcd09b05-f158-4488-9795-dddd89190837 · outbound

This paper cites Model reduction methods for nuclear emulators.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Model reduction methods for nuclear emulators

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.330838Z

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Observation 58333c46-4ebb-46fd-946e-b9459841f9c0 · outbound

This paper cites Eigenvector Continuation and Projection-Based Emulators.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Eigenvector Continuation and Projection-Based Emulators

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.434580Z

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Observation c1f17701-531c-446c-8a18-9ff0af0cfc2b · outbound

This paper cites Bayes goes fast: Uncertainty Quantification for a Covariant Energy Density Functional emulated by the Reduced Basis Method.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Bayes goes fast: Uncertainty Quantification for a Covariant Energy Density Functional emulated by the Reduced Basis Method

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.558840Z

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Observation 137118d4-42a6-4160-82be-eb31af9adef0 · outbound

This paper cites The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.675109Z

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Observation 814b468b-78ac-4bcc-ad03-c5cea564f1dc · outbound

This paper cites The equation of state for dense nucleonic matter from a meta-modeling. II. Predictions for neutron stars properties.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The equation of state for dense nucleonic matter from a meta-modeling. II. Predictions for neutron stars properties

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.799606Z

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Observation a9c6add4-95b4-46bd-940e-04ab4b2a7222 · outbound

This paper cites Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:12.918002Z

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Observation 4a6d752d-54f5-4c1e-9286-0a1a6d255657 · outbound

This paper cites A unified equation of state of dense matter and neutron star structure.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A unified equation of state of dense matter and neutron star structure

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.033466Z

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Observation 0ff24775-4025-4984-9ebc-b1aca397a09c · outbound

This paper cites From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter.

Constraining Hamiltonians from chiral effective field theory with neutron-star data From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.133726Z

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Observation a1c886a5-83f3-48f1-ab02-22507098348e · outbound

This paper cites A critical examination of constraints on the equation of state of dense matter obtained from GW170817.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A critical examination of constraints on the equation of state of dense matter obtained from GW170817

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.276442Z

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Observation 031205aa-9fa3-4552-af05-896b469bd4e9 · outbound

This paper cites Equation of state sensitivities when inferring neutron star and dense matter properties.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Equation of state sensitivities when inferring neutron star and dense matter properties

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.429100Z

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Observation 7814dac6-e131-43f9-bb97-03b872650771 · outbound

This paper cites Investigating Signatures of Phase Transitions in Neutron-Star Cores.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Investigating Signatures of Phase Transitions in Neutron-Star Cores

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.604326Z

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Observation b7fed112-c6ef-4ec5-8253-e6269f77b2e4 · outbound

This paper cites GW170817: Measurements of Neutron Star Radii and Equation of State.

Constraining Hamiltonians from chiral effective field theory with neutron-star data GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.720426Z

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Observation b13faac2-d785-40cd-a4c8-c517cf6077b0 · outbound

This paper cites Pratten, L.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Pratten, L

Reference 75

Resolution: verified exact; doi, observed 2026-08-04T00:43:37.864977Z

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No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 3498fa78-781e-4415-87af-b6c3c6143c5b · outbound

This paper cites The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:13.983945Z

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Observation c9aeea1f-02cf-4470-999b-0a8a0b1203f4 · outbound

This paper cites A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.150525Z

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Observation 77ca5ebf-69c2-492c-b583-3af36fb31e6d · outbound

This paper cites The LIGO Open Science Center.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The LIGO Open Science Center

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.306097Z

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Observation cce5b6c3-77dd-4e8b-80d6-b030e9863588 · outbound

This paper cites Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.436968Z

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Observation 6bd5ea0f-5c08-4dee-8f57-c50e332fe1c9 · outbound

This paper cites PyCBC Inference: A Python-based parameter estimation toolkit for compact binary coalescence signals.

Constraining Hamiltonians from chiral effective field theory with neutron-star data PyCBC Inference: A Python-based parameter estimation toolkit for compact binary coalescence signals

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.551075Z

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Observation baf65cb1-bbe3-49f5-9cb9-feb2e0d89984 · outbound

This paper cites Gravitational-wave constraints on the neutron-star-matter Equation of State.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Gravitational-wave constraints on the neutron-star-matter Equation of State

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.681445Z

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Observation 3a940a7b-76da-4819-a31f-ef5a8f1daf0e · outbound

This paper cites Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.808235Z

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Observation aafdec23-f4b6-47c1-8921-cd017e3eb3e6 · outbound

This paper cites Multi-messenger constraints on the neutron-star equation of state and the Hubble constant.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Multi-messenger constraints on the neutron-star equation of state and the Hubble constant

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:14.969271Z

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Observation e3e3378e-7a08-42f8-afe2-e221d9941629 · outbound

This paper cites Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.019768Z

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Observation daa61307-c75f-431d-a55b-212ce29b1cde · outbound

This paper cites The Radius of PSR J0740+6620 from NICER and XMM-Newton Data.

Constraining Hamiltonians from chiral effective field theory with neutron-star data The Radius of PSR J0740+6620 from NICER and XMM-Newton Data

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.087106Z

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Observation 588a032b-54b8-4c90-bf23-f6bdbd320f72 · outbound

This paper cites Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.239346Z

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Observation 04bb7a71-8767-45a5-b42f-086f4a5e1910 · outbound

This paper cites Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.346531Z

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Observation 1fddc885-6cb1-4973-928c-385c8901877f · outbound

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

Constraining Hamiltonians from chiral effective field theory with neutron-star data PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.457970Z

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Observation c9d082dc-e617-4517-a3d5-ffb6982d232c · outbound

This paper cites Local chiral effective field theory interactions and quantum Monte Carlo applications.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Local chiral effective field theory interactions and quantum Monte Carlo applications

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.574343Z

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Observation 3887af1c-b8a4-4c25-9897-249c450c1997 · outbound

This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.715216Z

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Observation a13b9c45-8df1-4d5d-bb8d-721d35a086d7 · outbound

This paper cites A Horizon Study for Cosmic Explorer: Science, Observatories, and Community.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A Horizon Study for Cosmic Explorer: Science, Observatories, and Community

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.854778Z

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Observation b75174c9-ade2-4e45-b5b9-7ae864b47e26 · outbound

This paper cites Punturoet al., The Einstein Telescope: A third- generation gravitational wave observatory, Class.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Punturoet al., The Einstein Telescope: A third- generation gravitational wave observatory, Class

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:15.942206Z

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Observation 592a532b-e55f-42f2-873a-568ad314fc64 · outbound

This paper cites Science Case for the Einstein Telescope.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Science Case for the Einstein Telescope

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:16.063524Z

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Observation 759f58cd-3ec2-40dc-b179-6a97111fa7e7 · outbound

This paper cites an unresolved cited work.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Unresolved cited work

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-04T00:40:16.148665Z

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Pith citing papers

Observation 75c2da3a-8295-47fb-a15b-b0f7bc752bee · inbound

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Conformal prediction for uncertainties in the neutron star equation of state Constraining Hamiltonians from chiral effective field theory with neutron-star data

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-08-04T01:49:24.711121Z

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No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c336e84d-155b-425f-9adc-5ae665a9001b · inbound

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Light nuclear scattering from neural quantum states Constraining Hamiltonians from chiral effective field theory with neutron-star data

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-08-04T01:49:24.711121Z

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No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 5b82c449-73d3-43ae-9651-925e28bd225a · inbound

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Measuring radii of merging neutron stars with interface-mode asteroseismology informed by nuclear theory and experiment Constraining Hamiltonians from chiral effective field theory with neutron-star data

Reference 75

Resolution: verified exact; arxiv_id, observed 2026-08-04T01:49:24.711121Z

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No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 459ff6ed-aa32-4f02-a27d-d4d8a789205b · inbound

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Parametric Matrix Models for Emulation in Nuclear and Many-Body Physics Constraining Hamiltonians from chiral effective field theory with neutron-star data

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Resolution: unresolved; no resolver link, observed 2026-08-15T22:22:01.873335Z

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