Paper Citation Record · LEDGER

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events

As of 12 August 2026, this Paper Citation Record lists 38 of 38 outbound references and 0 inbound Pith citation observations for arXiv:2507.09175.

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

pith.paper-citation-record.v1
2507.09175 v1

Coverage vector

measured 38 of 38 reference resolution

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

Source: cited_works

Reference resolution

38 of 38 outbound references displayed

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External citation measurements

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Outbound references

Observation eed5ad23-efd4-4eba-8c08-599e2031aa32 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 1

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:11:14.838283Z

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Observation 8a878165-1dc9-41c9-9e2f-d3cce2fb1ac4 · outbound

This paper cites For initial data, it has become common practice to excise the surface of the black to avoid this.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events For initial data, it has become common practice to excise the surface of the black to avoid this

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:11:14.755285Z

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Observation 5cdabc00-c772-4d7a-87a3-27bd01d13283 · outbound

This paper cites From the equation of hy- drostatic equilibrium Eqs.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events From the equation of hy- drostatic equilibrium Eqs

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:11:14.610377Z

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Observation b537c391-b732-4872-88a2-00f27cfafcd2 · outbound

This paper cites Ferrari, L.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Ferrari, L

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:19.458735Z

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Observation 9eb8e359-6f6b-4037-a3fd-e10561867ef4 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:19.377239Z

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Observation 29cfccb0-db9a-462c-bc18-4c3a217ef405 · outbound

This paper cites Lanza, Self-gravitating Thin Disks around Rapidly Rotating Black Holes, Astrophys.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Lanza, Self-gravitating Thin Disks around Rapidly Rotating Black Holes, Astrophys

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:19.203465Z

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Observation 07126ab4-a07b-46fa-849f-b9ee9933ced6 · outbound

This paper cites Abbott et al.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Abbott et al

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:19.891341Z

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Observation 93f48c7c-f47e-4ce4-a271-92e650fb9a23 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 8

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:19.722446Z

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Observation d3a4ac6e-8d87-43c3-9354-088723dafbb7 · outbound

This paper cites Kyutoku, M.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Kyutoku, M

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:19.579325Z

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Observation 91570e05-4fa2-435b-9e30-1eec2dc84216 · outbound

This paper cites Masuda and Y.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Masuda and Y

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:18.814750Z

Source-reported events for the cited work

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Observation 74df0c98-2645-4caf-a5eb-fc0f92d25e60 · outbound

This paper cites Korobkin, E.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Korobkin, E

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:18.637943Z

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Observation 9b7eb85b-a533-4b24-8633-06379e4ac5a9 · outbound

This paper cites Blinnikov, A.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Blinnikov, A

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:18.454133Z

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Observation beb961bc-af80-460e-b72a-6ac8cc6ba68f · outbound

This paper cites Nishida and Y.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Nishida and Y

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:19.108435Z

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Observation 97775825-8eca-45ff-87bf-1acdd12df2e7 · outbound

This paper cites The equations result- ing from the spectral representation are solved by using Newton-Raphson iterative method [15].

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events The equations result- ing from the spectral representation are solved by using Newton-Raphson iterative method [15]

Reference 14

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Observation bbc337fc-f967-4a06-88c8-0b805415236a · outbound

This paper cites For binary ID, a bi-spherical decomposition is used for the numerical space resulting in at least twelve domains to resolve the problem efficiently (see [15] and.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events For binary ID, a bi-spherical decomposition is used for the numerical space resulting in at least twelve domains to resolve the problem efficiently (see [15] and

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:11:14.518637Z

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Observation 87174a8c-0c30-4965-8f10-328ce416230a · outbound

This paper cites Nishida, A.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Nishida, A

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:18.974462Z

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Observation 0a1a0bdb-596e-44c4-92c5-bebfdefa2af0 · outbound

This paper cites On the runaway instability of relativistic tori.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events On the runaway instability of relativistic tori

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:10:16.635125Z

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Observation ad2b4100-4a44-4e11-ad8e-f0250ff515e6 · outbound

This paper cites 3+1 Formalism and Bases of Numerical Relativity.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events 3+1 Formalism and Bases of Numerical Relativity

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-06T18:10:14.991292Z

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Observation f8f26337-5921-4969-8949-8b1cd5539f05 · outbound

This paper cites Stripping of a neutron star in a close binary system in a pair with a black hole.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Stripping of a neutron star in a close binary system in a pair with a black hole

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:10:16.450423Z

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Observation efafb3d4-87de-409d-9b73-04beefceaa19 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:18.318103Z

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Observation b93e8432-1c52-4774-84ce-575fb7f38601 · outbound

This paper cites Grandcl´ ement, Kadath: A spectral solver for theoret- ical physics, J.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Grandcl´ ement, Kadath: A spectral solver for theoret- ical physics, J

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:18.218201Z

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Observation 2dc5284f-eceb-4d25-be35-d09f86adefb3 · outbound

This paper cites Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Black hole-neutron star binaries with high spins and large mass asymmetries: I. Properties of quasi-equilibrium sequences

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:10:16.306352Z

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Observation 7b66d554-6c20-4373-9898-ddc336a510bc · outbound

This paper cites Black hole - neutron star binaries with high spins and large mass asymmetries: II. Properties of dynamical simulations.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Black hole - neutron star binaries with high spins and large mass asymmetries: II. Properties of dynamical simulations

Reference 23

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Observation 1905b57b-29a9-408e-80ed-375dc826f2b1 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-06T18:10:15.242918Z

Source-reported events for the cited work

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Observation 6f8043da-86a1-4e79-b506-e50a4b82c368 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 25

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:18.061524Z

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Observation 65b3220b-d5d0-4cbc-875d-fab90596b0c5 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 26

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:17.916913Z

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Observation 7e9a60f9-197c-4de3-9dde-c1bbb2a6e006 · outbound

This paper cites However, in some cases the code does not converge for smaller separations and it is not possible to find a minimum of the binding energy.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events However, in some cases the code does not converge for smaller separations and it is not possible to find a minimum of the binding energy

Reference 27

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Observation 6935d8b0-a252-48d9-ac3e-f6d40081e4be · outbound

This paper cites Shibata, Relativistic formalism for computation of ir- rotational binary stars in quasiequilibrium states, Phys.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Shibata, Relativistic formalism for computation of ir- rotational binary stars in quasiequilibrium states, Phys

Reference 28

Resolution: verified exact; doi, observed 2026-08-06T18:10:15.976417Z

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Observation 76ba28fe-00fc-443e-8de8-98840b1eb03e · outbound

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Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 29

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:17.754152Z

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Observation 590d12a5-362b-4f1d-a6d4-20c4f429a282 · outbound

This paper cites Togashi, K.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Togashi, K

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:17.623839Z

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Observation 7dcc486b-5997-4eed-8b93-cf6bc32e41e4 · outbound

This paper cites Caudill, G.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Caudill, G

Reference 31

Resolution: verified exact; doi, observed 2026-08-06T18:10:15.696726Z

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Observation 9728e98e-ba95-4451-87f4-3381eab3e66e · outbound

This paper cites Taniguchi, T.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Taniguchi, T

Reference 32

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Observation e5cd3bc8-3bae-4a43-a6d6-6f97555b1e52 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 33

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Source-reported events for the cited work

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Observation 1a66bae7-aeb7-4eb3-9d0a-df508f1558ce · outbound

This paper cites Frank, A.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Frank, A

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:17.297034Z

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Observation 223e6d87-27e8-4514-bacd-495168bffa73 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 35

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:17.094038Z

Source-reported events for the cited work

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Observation 046afd15-9f4d-45ef-bc04-1a2e066689c1 · outbound

This paper cites an unresolved cited work.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Unresolved cited work

Reference 36

Resolution: unresolved; raw_fallback, observed 2026-08-06T18:10:16.889272Z

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Observation eb61a0d9-cb87-4e02-ad8f-c491037e419b · outbound

This paper cites Paczy´ nski, Evolutionary processes in close binary sys- tems, Ann.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Paczy´ nski, Evolutionary processes in close binary sys- tems, Ann

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T18:10:16.780845Z

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Observation 7fb3fa7a-93fd-4b59-b45f-d7ef950c03d3 · outbound

This paper cites Roche Lobes in the Second Post-Newtonian Approximation.

Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events Roche Lobes in the Second Post-Newtonian Approximation

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:10:16.116614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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