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Paper Citation Record · LEDGER

Quantum Computers will constrain the Equation of State of Neutron Stars

As of 11 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.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

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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Observation 820d8194-b5d5-4e10-a7a1-d5ee5c77161e · outbound

This paper cites an unresolved cited work.

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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Observation 291a0f5f-6846-40a2-9c19-076d9fa7b65f · outbound

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=sha256:5379a98ae0ddbda2a113cbe2d1c9582890bfa2b7c9a2d8150b4a31250d7dd527

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

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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=sha256:82a07c3c430495efff41f736c64c468c473b20ba06e68929e6b18b88a96fc024

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:c089e671606dff79146269d40273097c3644981d2b25aaca8cbd7538085567aa

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=sha256:1a2c8e0ccf4fdd31d8cc50704a612a04a6e29e337a846ab1c3fbf230c42ef614

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:e5ad1582d274a9658a01fe567ebc1dae2235f858227b31d61ab17d7267c75251

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=sha256:7cdbc8bc83f3dd566ff4025ef03c103c710993691b94774df213166e17e7a6c0

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:b26c9ae7b917f20ee421195d93ddfcf308aed59bcb917bbf38a17757a5d257f2

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=sha256:04c10f2def0763f04e7260c9778df5ea8ecfa1ecc23e3283f41a452e7454d5cf

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:cc575dd259571dd20d8661a77cd00b569ece9e81d5c00affff7224ff568fb841

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=sha256:6e01df978f495e015003aa6e4d7c11c73b73528f509ebd522eff8affb239afa5

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=sha256:0a7220924a363c2dabc9b5769901f4fef1ac797fa63b3bf05f068ea84aa103e2

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=sha256:4798d748c7142baed89e11a140532063e591a1db7bba87363e46f16351a4ae07

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=sha256:32baca6a89ec2d87c0991c3ef6ee005ac55c918c9331e112cafa90198597c853

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=sha256:7efdf92f3b1e75a7315bc801f32532d8ce6d2b5ce7690b981c5976aaf1fcd3cf

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:d8c799a14dc43c82d28c62ebf524312d071785f6779762f7ee93a8ee96be9913

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:d54945b8966b02e703e14d8683bdd7c15b24cc684093244d6ad65dd603964e02

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=sha256:31246af999810e4d2b4bdaa8899cd789c11f1840af2d675476a51bd1ff8fe878

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=sha256:6d1748c43a69e5bd274ba2920bd1d1cb494c6fa4a8a8f9b58697b7b350983de1

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=sha256:1510cce12216f46a77ff92b5c5646167968fc39ee578e92629c7e5ec59a71f01

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=sha256:4a47fcee87273db9fa166d50adb73f80a2c71561401b9cc27351456b7f4257a9

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=sha256:17cd1062a1024891b361e1196c6b98d2035da4eca9ea4bd218946067d94e64bc

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=sha256:02f838d55b01cb5baddad47d45e6ff3e33837cb2afdb56129b7bf7375bff374c

Pith citing papers

No inbound Pith citation observations are available.