Pith. sign in

Paper Citation Record · LEDGER

Quantum Computers will constrain the Equation of State of Neutron Stars

As of 14 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.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:22:36.910849Z

measured 58 of 58 standing notices

One-hop event checks from named stored sources.

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

measured 0 of 0 inbound itemization

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

  • verified exact17
  • verified fuzzy8
  • unresolved32
  • parse uncertain0
  • malformed identifier1
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

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

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.952553Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.709847Z digest=sha256:8eead49488f76fc0deb9c55d3ff841e5864293a450d88abc157c9ea588d834c6

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

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.943274Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.714808Z digest=sha256:6d34a60483a5654b4b3400f0c1551b4185fe87499ba6f36f1e7adfd7876d6eca

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

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.934120Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.719658Z digest=sha256:640ed92274b603f78c500476274c070f6e32fbc2cd600a401be25f1032f7d4e8

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

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.924888Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.724540Z digest=sha256:40227d857e93ae24dc885d1ed115ca499d5e2176d8539243ff3df141fb97ed8e

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

Resolution
malformed identifier
no resolver link, observed 2026-08-10T04:22:36.729748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.729748Z digest=sha256:a0d1ded5ccb64c0c67508e3073807c2c4792462865a543a0c9eb89eaf1cc922c

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.760211Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.734264Z digest=sha256:6be17830a66bb4385fc9ed15c6f542cdb54d6a4a1b1fbb29ede741eac109485f

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

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.911112Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.738565Z digest=sha256:f9f70eed7c059b6f092be603ddea9ca33a94f87462cb13da3b759a1f53a1da61

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.741860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.741860Z digest=sha256:3972d444a428393227c638df136935ee47f6a30b4172f03c8ac614af7828d901

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.694941Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.744800Z digest=sha256:911c54c68a4bc1bdf3c3df89a282461f22f97b0d26cbcdd4d3a8e9aed6942cc3

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.682743Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.748539Z digest=sha256:531e030f065296a0a3e72a3c1b9f7e6b2eb8742f692cf95920b59a6e11739efb

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.670126Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.751874Z digest=sha256:1ba2bfe84421a83962bdedb0533ac94eb45aa1266529c8673ae75b433d2e0981

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.756366Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.756366Z digest=sha256:f9d22a04696a4729d93cdc83332efbcd870bdf9be647aeaf3ee7c6310cdbef34

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.649292Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.759647Z digest=sha256:833654a0ecc648637c78673f899f3740fed237e1088f7eb1dc94b3bb6ba16100

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.637105Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.763190Z digest=sha256:8c54bb50d025e7952158e9c2f67c1b9e74ee9009e55bb1539c0000b878354791

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

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.901410Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.766333Z digest=sha256:d89f9aa13458443042b0b67d41e8f776f743ad58f77e76a6fc5701fc17a329a3

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

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.892890Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.768845Z digest=sha256:7bad7bc7d481a73e723e5ac4cdd1c2d6bc7df06fa1dc8e3ca2c68c68bf60c480

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.624285Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.771895Z digest=sha256:9f37d927fd8be2dab6ebfa5995f7ab2deb6cc152d47439ebfba61cfd585a68a6

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.775205Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.775205Z digest=sha256:cbac7537149a4eff7013dad0c969af49d9390ce53714cf9f355263639ae9dd32

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.778352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.778352Z digest=sha256:c3d3589c8584d6ceb06075766218eb05c2bb719ab1071238a0259afa6e4808ce

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.782599Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.782599Z digest=sha256:ef7a73072fdb8d0d7917ef7fc1447ebcbb6a01da3b4a0cd985903b8fd59a3464

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.786283Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.786283Z digest=sha256:9d476fb733505e24735181c87d584c9caf5199b2221b9d2c4ad3585e1f509b85

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

This paper cites an unresolved cited work.

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

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.790013Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.790013Z digest=sha256:009f5abf897dd65f87e803d364f7a72fd7f06be2acccbb6ce5a58643306dac71

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.793287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.793287Z digest=sha256:aa46b6705e3d4b91c2b647dab2946fd223e652c84ffb70540d2ad66e3492c0df

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.517842Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.796035Z digest=sha256:0a93d281e87b4d67a864c8c39d8fb4cebb6db5c8ef7e19ee89589388ebab3aa9

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

This paper cites an unresolved cited work.

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

Reference 25

Resolution
verified exact
raw_fallback, observed 2026-08-10T04:22:37.503871Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.800313Z digest=sha256:906544e8eee795d77425eacc7a4aef592cf38c66275a91f03923ebda349db29d

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.804434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.804434Z digest=sha256:922f8e3032d240df7c087b037e26202f4a082e0e2add6addbdedd119168c2b87

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.807292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.807292Z digest=sha256:b949738224f6c1af78c8830b793cf205cdf9a2ceadf687f9a99ceeeb3c70792b

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.434878Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.810991Z digest=sha256:4494e5ca8a26922e176e9b1d773bd660fe05bc478b2114444a593b9aa8cd6c59

Observation f2902824-c0ff-407d-abd6-897d7ba5d011 · outbound

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.814284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.814284Z digest=sha256:fd56baca04e6db63cf2bc7f28c2c2edc4b1e5e995240b2e49c370e9db1d7628a

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

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:22:37.413539Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.817016Z digest=sha256:116fb7b86dda06dea0d174bf1b8a72ba40541529f62ebc6349b12a9316e7a71e

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

This paper cites an unresolved cited work.

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

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.820432Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.820432Z digest=sha256:edbf9fa497c483ba3621a9cccdb46570e3eb68eab8c09bd47437679308f4f826

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

This paper cites an unresolved cited work.

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

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.823742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.823742Z digest=sha256:2105e03acc59750c1f281863d4065e67006e20726ed93e7b8b88d8b36dce1429

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

Resolution
unresolved
no resolver link, observed 2026-08-10T04:22:36.826590Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:22:36.826590Z digest=sha256:91cd0fa6355ee7fe90a7462247b4f741c56830f7f7e610be2dcf74996d360ed7

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

This paper cites an unresolved cited work.

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

Reference 34

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.856490Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.830664Z digest=sha256:814eb3084ceaeb67712987397dae5b3ee974d45a764ce042e9fab73698132a08

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

This paper cites an unresolved cited work.

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

Reference 35

Resolution
unresolved
raw_fallback, observed 2026-08-10T04:22:37.847329Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.833557Z digest=sha256:45da8e796f3d7010a029ca637774b43d5523e3f059e42056dab76410bbfb1309

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

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T04:22:37.837828Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-10T04:22:36.836538Z digest=sha256:58d053f18ec784ca7b371481dd0ad9e2f1f987aeb0b9e5d655cdd49316fb0688

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

Resolution
verified fuzzy
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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.839576Z digest=sha256:4fcdf45725c01fbaea14cfcc11722c252bab37fa41f70810a83a9b02e57f9fa1

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.842330Z digest=sha256:e421a9691ad82cc523dc84201f51888911b9b64c98f1b9d17c79d94442e043f6

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=sha256:4982ea8486032bd026e7f423500cc5484dfd1a59408afb90b38c55bc710c4803

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.848899Z digest=sha256:dde15a4150694cb8343996408c6a5f78a9637b675f64f536b30ccb6310f45f34

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=sha256:39f0230719458e4b61c19fac4189925f89ca7020c00e8daaf7d78892bed80a4c

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.855819Z digest=sha256:9f7131d4e9e142fbb98419731f415af76fc80c966985d923fe6ebf5d1c0b2aad

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:a7f23b09873f0c22485c79f7bc536c6204b49ffcc99dacdc4a088a1be22fd988

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:eaaa0b8bd5f8127104194f91097ab99cd306310267aad30914f1b621fd99736f

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.865094Z digest=sha256:a3b29d6ef1a4e629e7f50fe5869e7051bd4cf455a8382300088cc3853115f545

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=sha256:7b2707cff1d480ee09f5cd20166aae44f36aa14692d22ba5888c79e34c928129

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.873015Z digest=sha256:615663e4889b2c871e446dc6788fc697d746ce7af92208e87174ca3336e79b9e

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=sha256:05d3fde86e18d17b9799347d237a85b9c207df8c51ac4dbad24cb7d49cf77e6f

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.879894Z digest=sha256:af9327342c2908b080129870ea79b71cf58acc3e0408a6e3560d16ea1e9641fa

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=sha256:1ea1b71fd676c6ce1fdb13fdc74d93b1dd41d258721d571009b85aad3bf7a47b

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.886694Z digest=sha256:23eaca219b3bbb5badae54476ab4a475b2c5d561fab4116070abb18883b95b0e

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.889792Z digest=sha256:2365574f16adc06b055b075f0edca58f170853ed752c7c1002e5f83c5a87384b

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.893336Z digest=sha256:ae2ee87c35159341f4ad1dabf9dcd8a882f7cb14728733002cf8e1ae4d47d14b

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=sha256:61618a6a4fad0eed0e364153a4239259a564d09dcb5de68cd121358a3d4ced79

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=sha256:682b4c15aa4c3bc56c044e97bceec1580c1a1f049ecf0c483f32448141fe7771

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=sha256:8807e22fa02bf58e0c33e4c16310b570c23958fc00eeb6e5551c38e212898f6c

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.907761Z digest=sha256:074ebe490509a4e5a4037c8a02b5b0b874dcd59ddf21ca620290c74e65657a9d

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-10T04:22:36.910849Z digest=sha256:1277355caa84878a1fbd1a4d1abdfdf5f1db9b1334bb1a54f787bb19233f9b7e

Pith citing papers

No inbound Pith citation observations are available.