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Paper Citation Record · LEDGER

Quantum Computers will constrain the Equation of State of Neutron Stars

As of 10 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 0 inbound Pith citation observations for arXiv:2608.06515.

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

pith.paper-citation-record.v1
2608.06515 v1

Coverage vector

measured 58 of 58 reference resolution

Typed states for the displayed outbound observations.

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One-hop event checks from named stored sources.

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Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

58 of 58 outbound references displayed

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  • verified fuzzy8
  • unresolved32
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External citation measurements

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Outbound references

Observation 9645008c-c25c-453b-8059-656b0540f0a8 · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 1

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Observation e74393ef-e8c6-4c02-82e1-bbd2b47999bb · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 2

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Observation 74a01b06-cab8-42c4-9dad-5f937ff0bc30 · outbound

This paper cites Note that, as a consequence of the gluon polarization ba- sis Eq.

Quantum Computers will constrain the Equation of State of Neutron Stars Note that, as a consequence of the gluon polarization ba- sis Eq

Reference 3

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Observation 6e8cf5ac-9636-484c-b55d-1a9d0a171481 · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 4

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Observation b2077252-ffe3-4d33-9d4a-b634896af81d · outbound

This paper cites Exp” denoting an exponential function fit, see Eq. (72) and “Fraction.

Quantum Computers will constrain the Equation of State of Neutron Stars Exp” denoting an exponential function fit, see Eq. (72) and “Fraction

Reference 5

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Observation bb324ffc-3bab-46fe-8e98-56ce72ce0d02 · outbound

This paper cites Neutron stars as probes of dark matter.

Quantum Computers will constrain the Equation of State of Neutron Stars Neutron stars as probes of dark matter

Reference 6

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Observation 2e1c98f4-f6e6-4023-87f1-7963acf9140e · outbound

This paper cites Cano and J.

Quantum Computers will constrain the Equation of State of Neutron Stars Cano and J

Reference 7

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Observation 958f0214-54e4-4683-b361-ae490bde31f8 · outbound

This paper cites Cano and J.

Quantum Computers will constrain the Equation of State of Neutron Stars Cano and J

Reference 8

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Observation 07e3e0ef-2e78-453d-bcc9-f3abc0474dd7 · outbound

This paper cites Influence of dark matter on hybrid and twin stars.

Quantum Computers will constrain the Equation of State of Neutron Stars Influence of dark matter on hybrid and twin stars

Reference 9

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Observation 31316bab-6384-437a-8f67-0368ef979a76 · outbound

This paper cites A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter.

Quantum Computers will constrain the Equation of State of Neutron Stars A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter

Reference 10

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Observation be409df8-e4fe-41b6-a474-3bf0a6003302 · outbound

This paper cites Testing gravity with the latent heat of neutron star matter.

Quantum Computers will constrain the Equation of State of Neutron Stars Testing gravity with the latent heat of neutron star matter

Reference 11

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Observation 1470fd41-184f-4032-929b-8db000055676 · outbound

This paper cites Bayesian Inference of Neutron Star Properties in $f(Q)$ Gravity Using NICER Observations.

Quantum Computers will constrain the Equation of State of Neutron Stars Bayesian Inference of Neutron Star Properties in $f(Q)$ Gravity Using NICER Observations

Reference 12

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Observation 6620e9d3-7669-40a0-8792-7deed238f4d3 · outbound

This paper cites Covariant Tolman-Oppenheimer-Volkoff equations in Energy-Momentum Squared Gravity.

Quantum Computers will constrain the Equation of State of Neutron Stars Covariant Tolman-Oppenheimer-Volkoff equations in Energy-Momentum Squared Gravity

Reference 13

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Observation ec8e001a-9666-4442-b222-c82c43556e80 · outbound

This paper cites Regulator-independent equations of state for neutron stars generated from first principles.

Quantum Computers will constrain the Equation of State of Neutron Stars Regulator-independent equations of state for neutron stars generated from first principles

Reference 14

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Observation 33deb34e-7143-493d-9f23-ece845ac713b · outbound

This paper cites Lope Oter, A.

Quantum Computers will constrain the Equation of State of Neutron Stars Lope Oter, A

Reference 15

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Observation 599cf57a-59dd-4989-85d1-16ce18eae6b3 · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 16

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Observation 9dc44c57-df1d-49a8-9a5f-901c0c4b4b8d · outbound

This paper cites Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. V. Improved parametrization of the nucleon density distributions.

Quantum Computers will constrain the Equation of State of Neutron Stars Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. V. Improved parametrization of the nucleon density distributions

Reference 17

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Observation 4671864d-28a6-4a46-a6b4-503e0f3a2a83 · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 18

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Observation 6ac48e12-955e-4a71-bf90-da04037998fb · outbound

This paper cites Komoltsev and A.

Quantum Computers will constrain the Equation of State of Neutron Stars Komoltsev and A

Reference 19

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Observation c1e9db01-fe0e-4d0c-a04c-7e8d068eab4e · outbound

This paper cites Evaluation of phase shifts for non-relativistic elastic scattering using quantum computers.

Quantum Computers will constrain the Equation of State of Neutron Stars Evaluation of phase shifts for non-relativistic elastic scattering using quantum computers

Reference 20

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Observation dbc8acd8-88ee-4157-8c66-15c280f9e6ae · outbound

This paper cites Quantum simulating multi-particle processes in high energy nuclear physics: dijet production and color (de)coherence.

Quantum Computers will constrain the Equation of State of Neutron Stars Quantum simulating multi-particle processes in high energy nuclear physics: dijet production and color (de)coherence

Reference 21

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Observation 003dbaf6-f44e-4b17-97a1-f37479e8b339 · outbound

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 22

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Observation dc38efad-52e3-4398-b555-f8b7a5f65b7b · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 23

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Observation 3a2ff01d-060d-48bb-b832-eb2a47c3c54f · outbound

This paper cites Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model.

Quantum Computers will constrain the Equation of State of Neutron Stars Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model

Reference 24

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Observation 6c274473-fcd1-448f-9141-659a655d0f5e · outbound

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 25

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Observation ce042879-b9c9-46a7-935a-e343774d4931 · outbound

This paper cites Hinderer, B.

Quantum Computers will constrain the Equation of State of Neutron Stars Hinderer, B

Reference 26

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 27

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Observation 1ac6fdee-d4bf-404a-ab26-d53491d27ec5 · outbound

This paper cites Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms.

Quantum Computers will constrain the Equation of State of Neutron Stars Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms

Reference 28

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This paper cites The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation.

Quantum Computers will constrain the Equation of State of Neutron Stars The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation

Reference 29

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This paper cites Moat hyperons in cold neutron stars.

Quantum Computers will constrain the Equation of State of Neutron Stars Moat hyperons in cold neutron stars

Reference 30

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Observation 6945e4ef-14e6-49cb-b897-d5442e436085 · outbound

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 31

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Observation 3ae689ac-8598-4fff-8d35-a1cea789c192 · outbound

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 32

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Observation 8f399a31-11fa-45aa-a3ca-a7470d4c5aa1 · outbound

This paper cites Bulk Viscosity of Two-Flavor Color Superconducting Quark Matter in Neutron Star Mergers.

Quantum Computers will constrain the Equation of State of Neutron Stars Bulk Viscosity of Two-Flavor Color Superconducting Quark Matter in Neutron Star Mergers

Reference 33

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Observation 7d81acf5-de97-403e-827a-476127f78f41 · outbound

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 34

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Observation 0004141e-6198-4601-936a-11f19c0bd078 · outbound

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Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 35

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Observation 58a17b81-0afe-42f3-b08f-7541d8027cf2 · outbound

This paper cites Fernandez, P.

Quantum Computers will constrain the Equation of State of Neutron Stars Fernandez, P

Reference 36

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Observation 09c26cc4-65d9-4079-ba15-77fe8e8ce4f0 · outbound

This paper cites Peruzzo, J.

Quantum Computers will constrain the Equation of State of Neutron Stars Peruzzo, J

Reference 37

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raw_fallback, observed 2026-08-10T04:22:37.828448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.839576Z digest=sha256:a2fd1d23eb09f51f5a2c0816eeef1347b370ddc4dc28fffbeb4d027c03bcc3e9

Observation 7e108228-cd3a-4680-ab32-ae49c26f89b9 · outbound

This paper cites Tilly, H.

Quantum Computers will constrain the Equation of State of Neutron Stars Tilly, H

Reference 38

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.819246Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.842330Z digest=sha256:2006501b5559efceaa9f38321ec2ba11d6a23af8fe6016d406ffb6e05111ebc3

Observation 34d74509-a2cf-462e-93a7-09fb18bea0ea · outbound

This paper cites Nocedal and S.

Quantum Computers will constrain the Equation of State of Neutron Stars Nocedal and S

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.845759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.845759Z digest=sha256:7045fbeb2beaf3f47121096ca427daec97b8ffb8d5e53f54a9076c300cd2590d

Observation 28913ab4-8313-4714-9c0a-7191b930dda0 · outbound

This paper cites Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis.

Quantum Computers will constrain the Equation of State of Neutron Stars Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.266458Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.848899Z digest=sha256:d564a9806bf366e8c8fbb91612aa8fab5e685aef1692f8e4db1a140551d867aa

Observation eae3eb73-0504-46ac-bb37-c81d1ac4eae3 · outbound

This paper cites On the formation of strange quark stars from supernova in compact binaries.

Quantum Computers will constrain the Equation of State of Neutron Stars On the formation of strange quark stars from supernova in compact binaries

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.851917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.851917Z digest=sha256:259bcd7baa011886924da5c82504c3cab45cc018c4ad8b5217017c0fab238e81

Observation a93231eb-f9e8-4490-8c20-7617f73be10f · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 42

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.804400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.855819Z digest=sha256:822909345805d00bc5672e8be4874fba9b1164fd4948a24018886b715f68eb8a

Observation 6f2e1315-bab5-407f-a330-bbcc34bea0e8 · outbound

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

Quantum Computers will constrain the Equation of State of Neutron Stars Bayesian inference favors quark matter in neutron star interiors

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.858555Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.858555Z digest=sha256:4139556e37c1ea53385bac821cf940397b6e0764d87e98ed2a2283e747d7a644

Observation 10edf9be-d329-4be3-9aa0-b388c75aefaa · outbound

This paper cites Constraints on Phase Transitions in Neutron Star Matter.

Quantum Computers will constrain the Equation of State of Neutron Stars Constraints on Phase Transitions in Neutron Star Matter

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.862182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.862182Z digest=sha256:e5468b1fab2ff73cb23e1db00a797c918fa64bd88bea784c583e26079385a69e

Observation a207b7b2-d6a8-4eb0-8e6c-9091e4b2cf7a · outbound

This paper cites Ridges in rotating neutron-star properties due to first order phase transitions.

Quantum Computers will constrain the Equation of State of Neutron Stars Ridges in rotating neutron-star properties due to first order phase transitions

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.229479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.865094Z digest=sha256:2392476ed38c0db24e6e5d287272604e5f54de733521985a15d5ec42f11c4512

Observation 9b451fb0-3f09-4d24-a724-6f80c82fb040 · outbound

This paper cites Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement.

Quantum Computers will constrain the Equation of State of Neutron Stars Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.868989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.868989Z digest=sha256:e1fb34b4a8fa04eef50ea45551e2032487edbb95b091eb8f0a7ddb6d39ba4983

Observation 90a75974-4b35-4be2-bff2-a29cf6e0bee6 · outbound

This paper cites Pulse Modulation as a Signature of the Asteroid-Neutron Star Collision Model for High-Energy Transients.

Quantum Computers will constrain the Equation of State of Neutron Stars Pulse Modulation as a Signature of the Asteroid-Neutron Star Collision Model for High-Energy Transients

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.207943Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.873015Z digest=sha256:fff0fdb533e3ae8a3ccefee49ba6b8bcb05deb056775cad7eb6c4fe09e8ad052

Observation 37c912c2-42a0-440b-acbe-01364be4db01 · outbound

This paper cites Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers.

Quantum Computers will constrain the Equation of State of Neutron Stars Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.876474Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.876474Z digest=sha256:116d7ce871c4966d5c6c8f7acc5fde210d922a80d330570ef7386d3f031f2271

Observation daa12519-ec94-4ad5-8626-cba696f2bcfb · outbound

This paper cites Gorda, A.

Quantum Computers will constrain the Equation of State of Neutron Stars Gorda, A

Reference 49

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.795373Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.879894Z digest=sha256:edc520cccda7d2b297ab6755fe2b3623ff33e09a14307a98e0b583e6b0a67d43

Observation 5dd20ac4-1664-4f38-aa52-325327c2cb96 · outbound

This paper cites Asymptotically conformal CFL quark matter within a nonlocal chiral quark model.

Quantum Computers will constrain the Equation of State of Neutron Stars Asymptotically conformal CFL quark matter within a nonlocal chiral quark model

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.883451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.883451Z digest=sha256:9f8978f3bd606a96276b66a61684bb4153fc14989737318a16c4571564c620cd

Observation f0f60dec-85d8-4696-af6c-e41205989724 · outbound

This paper cites Ma, Acta Phys.

Quantum Computers will constrain the Equation of State of Neutron Stars Ma, Acta Phys

Reference 51

Resolution
verified exact
raw_fallback, observed 2026-08-10T04:22:37.177818Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.886694Z digest=sha256:64814daf2574541bc84e30ac2b9b0e0a245f571d09bc8d605ae0a9eba67f8bbc

Observation a22daf4e-de7f-4786-aa8d-f776473c8368 · outbound

This paper cites Xiong, Y.

Quantum Computers will constrain the Equation of State of Neutron Stars Xiong, Y

Reference 52

Resolution
verified exact
raw_fallback, observed 2026-08-10T04:22:37.117182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.889792Z digest=sha256:9ce914db04e49d14b3bf8d167df9c69112b664d765484c974b1b1a2a01a6e5c6

Observation 8517fa1e-cc09-43f3-baca-157249b1b0da · outbound

This paper cites Renormalized Effective QCD Hamiltonian: Gluonic Sector.

Quantum Computers will constrain the Equation of State of Neutron Stars Renormalized Effective QCD Hamiltonian: Gluonic Sector

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.036871Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.893336Z digest=sha256:59d1e30ef451a6818ee10588cd1baaa228cdbbb8ef6dd4bceba626985fdaea27

Observation 1c2812e7-bda1-4754-bc8f-7a3ac4124b43 · outbound

This paper cites Buballa, Phys.

Quantum Computers will constrain the Equation of State of Neutron Stars Buballa, Phys

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.897247Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.897247Z digest=sha256:8ffb6f2acf6a9228b33a1e669d230e5b2bff486afe5bd54068a201771b54b71e

Observation 5ab5dae0-3682-4c5d-aa0d-9c63b9af57cb · outbound

This paper cites The Science of the Einstein Telescope.

Quantum Computers will constrain the Equation of State of Neutron Stars The Science of the Einstein Telescope

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.900806Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.900806Z digest=sha256:4c38ff317df8fe6e2ab565f7800820156867c7466212201d96c613bb2702fc63

Observation 5b73d33a-b557-4a3d-a56c-2331b19c1a62 · outbound

This paper cites Di Matteo, A.

Quantum Computers will constrain the Equation of State of Neutron Stars Di Matteo, A

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.904747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.904747Z digest=sha256:9b15def7be7c0a98197155f80f1f03c1f20e163628cc2b1822202aed147886db

Observation 658fff35-3b1e-4e1b-a39f-587522a3fa35 · outbound

This paper cites Siwach and P.

Quantum Computers will constrain the Equation of State of Neutron Stars Siwach and P

Reference 57

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.780351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.907761Z digest=sha256:d6a42857386e82a8a0b4ef307b150a38fa70a5f7f5c4013690f2fb0d4b417299

Observation a8d477a1-4997-480f-940a-09581f784fa9 · outbound

This paper cites an unresolved cited work.

Quantum Computers will constrain the Equation of State of Neutron Stars Unresolved cited work

Reference 58

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.771087Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-10T04:22:36.910849Z digest=sha256:8d5a7c0d68e50a3aa9d5452b59e6511e6b3eb18dfcd0b7b3ad2462ce252f2aae

Pith citing papers

No inbound Pith citation observations are available.