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Paper Citation Record · LEDGER

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster

As of 11 August 2026, this Paper Citation Record lists 69 of 69 outbound references and 0 inbound Pith citation observations for arXiv:2507.11684.

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

pith.paper-citation-record.v1
2507.11684 v1

Coverage vector

measured 69 of 69 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

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

Source: cited_works

Reference resolution

69 of 69 outbound references displayed

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External citation measurements

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Outbound references

Observation 00d8a6d8-472b-421a-bebc-79a9abee9549 · outbound

This paper cites For that we use eq.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster For that we use eq

Reference 1

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This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 2

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Observation bdd1fd7a-4a50-4580-b225-844db4404689 · outbound

This paper cites Therefore, we consid er below only the case α(τ = 0) = 0.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Therefore, we consid er below only the case α(τ = 0) = 0

Reference 3

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Observation f9c5b617-932f-435b-b3db-280dd4b52844 · outbound

This paper cites We conclude that relatively large mass ratios q >∼ 0.04 are preferable.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster We conclude that relatively large mass ratios q >∼ 0.04 are preferable

Reference 4

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This paper cites Note that a reader who is interested in astrophysical applications o nly can omit Section 2-4 and go directly to Section 5, which is written in a self-consistent way.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Note that a reader who is interested in astrophysical applications o nly can omit Section 2-4 and go directly to Section 5, which is written in a self-consistent way

Reference 5

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 6

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 7

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 8

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Reference 9

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 10

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Observation dec4fb28-aa1f-4ba4-8f6a-4fd185e46846 · outbound

This paper cites Massive Black Hole Binary Evolution.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Massive Black Hole Binary Evolution

Reference 11

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Observation 1b278152-c088-4681-8104-9daea8e3badc · outbound

This paper cites Komossa, Mem.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Komossa, Mem

Reference 12

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 13

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This paper cites A massive binary black-hole system in OJ287 and a test of general relativity.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster A massive binary black-hole system in OJ287 and a test of general relativity

Reference 14

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 15

Resolution
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Observation 75667896-1c9e-4055-96f5-370d56746e10 · outbound

This paper cites Gravitational Wave Astronomy: in Anticipation of First Sources to be Detected.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Gravitational Wave Astronomy: in Anticipation of First Sources to be Detected

Reference 16

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Observation b67ee6a8-9b71-45fc-840b-99496c836a44 · outbound

This paper cites Astrophysics with the Laser Interferometer Space Antenna.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Astrophysics with the Laser Interferometer Space Antenna

Reference 17

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Observation e11d1167-bf0a-422a-ab95-df3d99e9c033 · outbound

This paper cites Cosmology with the Laser Interferometer Space Antenna.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Cosmology with the Laser Interferometer Space Antenna

Reference 18

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 19

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Observation 18877a21-0ca9-42fd-afc7-651bd05c68c3 · outbound

This paper cites Changing-Look Inspirals: Trends and Switches in AGN Disk Emission as Signposts for Merging Black Hole Binaries.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Changing-Look Inspirals: Trends and Switches in AGN Disk Emission as Signposts for Merging Black Hole Binaries

Reference 20

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Blaes, M

Reference 21

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 22

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Observation 8f238bac-7551-4242-a78b-fb45b27d4328 · outbound

This paper cites Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation

Reference 23

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Observation 1dcd2bb3-bfe4-4194-96d1-3eb00fb63859 · outbound

This paper cites von Zeipel, Astronomische Nachrichten 183, 345 (1910).

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster von Zeipel, Astronomische Nachrichten 183, 345 (1910)

Reference 24

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 25

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Observation a2f0730c-8e00-49de-bd4c-ed27877b2a7a · outbound

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The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Kozai, Astron

Reference 26

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Observation b6d398d6-ea49-4828-97f1-068591359f5e · outbound

This paper cites The Lidov-Kozai Oscillation and Hugo von Zeipel.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster The Lidov-Kozai Oscillation and Hugo von Zeipel

Reference 27

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This paper cites Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation

Reference 28

Resolution
unresolved
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Unavailable: canonical work link unavailable.

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This paper cites Sesana, The Astrophysical Journal 719, 851–864 (2010).

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Sesana, The Astrophysical Journal 719, 851–864 (2010)

Reference 29

Resolution
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Source-reported events for the cited work

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Observation cca4ee76-2957-4f82-ae7e-20cc0b889bb8 · outbound

This paper cites Eccentric evolution of SMBH binaries.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Eccentric evolution of SMBH binaries

Reference 30

Resolution
verified exact
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Source-reported events for the cited work

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Observation 8d400b19-44b7-44a0-8934-a5e485d437f9 · outbound

This paper cites Evolution of growing black holes in axisymmetric galaxy cores.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Evolution of growing black holes in axisymmetric galaxy cores

Reference 31

Resolution
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Observation 3c024e79-acd3-4c1b-9acd-d7ae00ebef1f · outbound

This paper cites The Link Between Ejected Stars, Hardening and Eccentricity Growth of Super Massive Black Holes in Galactic Nuclei.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster The Link Between Ejected Stars, Hardening and Eccentricity Growth of Super Massive Black Holes in Galactic Nuclei

Reference 32

Resolution
verified exact
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Source-reported events for the cited work

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This paper cites Inward Bound: The incredible journey of massive black holes as they pair and merge; I. The effect of mass ratio in flattened rotating galactic nuclei.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Inward Bound: The incredible journey of massive black holes as they pair and merge; I. The effect of mass ratio in flattened rotating galactic nuclei

Reference 33

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This paper cites Berczik, M.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Berczik, M

Reference 34

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Source-reported events for the cited work

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This paper cites Vasiliev, F.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Vasiliev, F

Reference 35

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raw_fallback, observed 2026-08-06T17:18:56.517082Z

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=2026-08-06T17:18:47.850919Z digest=sha256:3b891fc46f6a47dc9787fb2dae43beaa0081e4f02fff8f2551e46076deda8d10

Observation b4925171-843d-4e90-a1e5-8b45dc330e5b · outbound

This paper cites Evolution of supermassive black hole binaries and tidal disruption rates in nonspherical galactic nuclei.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Evolution of supermassive black hole binaries and tidal disruption rates in nonspherical galactic nuclei

Reference 36

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:51.973193Z

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=2026-08-06T17:18:47.919501Z digest=sha256:b8160bca008bdbfbba8e397e7becda05367d93f9de5313ed4a4d4668fc0327ea

Observation e3deae81-fd9f-4848-b7b1-1ae756fb057e · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 37

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:56.472953Z

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=2026-08-06T17:18:47.970893Z digest=sha256:c5cdc2d26bd6ea79d0121c8a4ed7ffe5f8104ab60c1914b2a5f077e1080160b9

Observation 1ee0b9e9-6971-4dd2-abd1-cb406ae5a478 · outbound

This paper cites Chandrasekhar, Ellipsoidal figures of equilibrium (1969).

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Chandrasekhar, Ellipsoidal figures of equilibrium (1969)

Reference 38

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:56.446126Z

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=2026-08-06T17:18:48.042779Z digest=sha256:71ac246537d09fd8e0274701504df93f890f0c1552827aff845c5d32e5bf2683

Observation 3cf6df68-63de-4b2c-9e7f-347236ae6db5 · outbound

This paper cites Close encounters of a rotating star with planets in parabolic orbits of varying inclination and the formation of Hot Jupiters.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Close encounters of a rotating star with planets in parabolic orbits of varying inclination and the formation of Hot Jupiters

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:51.728166Z

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=2026-08-06T17:18:48.084361Z digest=sha256:a9a0e2f2c627b57393176a3e513fdd94029e7d41bce79e04971eabda5501328a

Observation b12035d0-e1f3-4f16-9dbf-fc733be44afd · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 40

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:56.414916Z

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=2026-08-06T17:18:48.142791Z digest=sha256:49d4e16ef44af40ff343389031bf3b0be2ea68b91097cc09b8ae404772410665

Observation 223cd49f-cfe0-4e47-bb5f-62ef38a62338 · outbound

This paper cites The tidal disruption rate in dense galactic cusps containing a supermassive binary black hole.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster The tidal disruption rate in dense galactic cusps containing a supermassive binary black hole

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:51.476641Z

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=2026-08-06T17:18:48.205125Z digest=sha256:ad480a63fc7eeef5c1defd040813882e417395435ae01d7fbb62b058b3630703

Observation 5204df26-ffa2-46ce-9d45-3ad04fe6b652 · outbound

This paper cites Petrovich and F.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Petrovich and F

Reference 42

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:56.395029Z

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=2026-08-06T17:18:48.263290Z digest=sha256:f507c944553846b950e94ddbaffc2ec96996b135c11658f9b9a1470858608b7a

Observation b1b1c33e-4583-4faa-9844-cb908609650c · outbound

This paper cites Secular dynamics of binaries in stellar clusters I: general formulation and dependence on cluster potential.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Secular dynamics of binaries in stellar clusters I: general formulation and dependence on cluster potential

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:51.215265Z

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=2026-08-06T17:18:48.352934Z digest=sha256:9bf1e184ac8f95f6bd916b229961119ac3919ecedec86dce129b4efe048245c7

Observation 195fa8ba-495f-4aa9-a67c-50ba2710de5c · outbound

This paper cites Secular dynamics of binaries in stellar clusters II: dynamical evolution.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Secular dynamics of binaries in stellar clusters II: dynamical evolution

Reference 44

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:51.000792Z

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=2026-08-06T17:18:48.397120Z digest=sha256:fc52edc4e8ac998b586140b597d446f56dd6d32c93d9b7fb0b8e89cd97f2791d

Observation 61678453-02d7-49ef-8e1c-438db4e252a7 · outbound

This paper cites Secular dynamics of binaries in stellar clusters -- III. Doubly-averaged dynamics in the presence of general relativistic precession.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Secular dynamics of binaries in stellar clusters -- III. Doubly-averaged dynamics in the presence of general relativistic precession

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:50.757651Z

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=2026-08-06T17:18:48.452260Z digest=sha256:f9eda8c8fa02a1561d6e0a6f31ba05e6fda0b60350ec900c06756730aff75139

Observation b4d94a7d-70fa-4a3a-bb17-330fe1dd84f6 · outbound

This paper cites Masses and Scaling Relations for Nuclear Star Clusters, and their Coexistence with Central Black Holes.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Masses and Scaling Relations for Nuclear Star Clusters, and their Coexistence with Central Black Holes

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:48.510329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:48.510329Z digest=sha256:0f430a2c0c6cd77ef9230b38446cf615cacef6dfeddc03b5932c8b53bef05c94

Observation cd54eedb-648e-4878-a11d-b078667cc264 · outbound

This paper cites Young, Astrophys.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Young, Astrophys

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:56.255952Z

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=2026-08-06T17:18:48.558491Z digest=sha256:7bb4ef629fd11773dfe167d951e90f4ddd2b28fa95b2e8a6546e960f9d1c334a

Observation 84315d6a-1072-46fe-8a0b-48e5c1f1c828 · outbound

This paper cites https://en.wikipedia.org/wi ki/Orbital node#Node distinction for a graphical representation.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster https://en.wikipedia.org/wi ki/Orbital node#Node distinction for a graphical representation

Reference 48

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:55.987835Z

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=2026-08-06T17:18:48.611384Z digest=sha256:90bdcc9843aedab19c4562b4c1abf5cec26babc27c410041b9f9787c61fad7c5

Observation 480eab13-d426-492e-88c1-8e98602d060d · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 49

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:55.764035Z

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=2026-08-06T17:18:48.646197Z digest=sha256:924aea4f4856af574d5bfacc35fd5a9d8038a4cb89e5f155cbb32c6d4ee43b05

Observation b156c72a-d987-4f2b-82cb-b9b56fece5b8 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 50

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:55.521553Z

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=2026-08-06T17:18:48.703274Z digest=sha256:b388fe193590191f1531238f6cbdf20b674ab5c216406c65ae3f571453a75f15

Observation 95c91c41-a12e-4325-8a6a-f3dc7406b003 · outbound

This paper cites Merritt, Dynamics and Evolution of Galactic Nuclei (2013).

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Merritt, Dynamics and Evolution of Galactic Nuclei (2013)

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:55.313460Z

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=2026-08-06T17:18:48.752164Z digest=sha256:ee46a903bdb295ae49e7f58e8d7fd306ef581c3915e9f9de52f85340a2b8493f

Observation d3530375-bc16-4ee4-9da1-23cf1cca80e0 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 52

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:55.187622Z

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=2026-08-06T17:18:48.814073Z digest=sha256:6b9acd1a17b72449067da46b24cf50618bd96682463601fe67b587e6bdfec00d

Observation 1187b160-1d34-470a-a269-615b8a5973b5 · outbound

This paper cites In the former case we use κ, while in the latter case we show explicitly ( ±) in all appropriate equations.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster In the former case we use κ, while in the latter case we show explicitly ( ±) in all appropriate equations

Reference 53

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:55.014163Z

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=2026-08-06T17:18:48.860190Z digest=sha256:77716158a774de39f1885323e3c90ccaf0f7e08998dd5d9a837187c3fe3dbca2

Observation bfce1157-9178-455e-8751-d92333286965 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 54

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:54.823795Z

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=2026-08-06T17:18:48.917030Z digest=sha256:5266e1894c4055578038c9cb56643860591570420d59c7a5c1748438fe9f6136

Observation 6d56f125-6798-4991-b372-ae567cdbd436 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 55

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:54.675123Z

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=2026-08-06T17:18:48.963974Z digest=sha256:d5ef3aaa6cdf3ee6b2cb42e26e1b10f948444f18862998bdeaca56a5b8a558c8

Observation 99d57969-05e2-4314-85e8-de354d9bcb08 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 56

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:54.431928Z

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=2026-08-06T17:18:49.043983Z digest=sha256:de9d9b434a43fbbdc3e8587178204a8f654037a7ddeafab288b6aaf70c0d5aff

Observation f9c60a94-ed28-482e-9eba-42bd70d24086 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 57

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:54.162146Z

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=2026-08-06T17:18:49.152444Z digest=sha256:392cd77be3402ad31ea3bdb3781f9644a53fcd0f9fef42adf90474874c344b20

Observation c969c0ac-18ab-4d2d-b10e-66014d6e0467 · outbound

This paper cites Cutler, D.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Cutler, D

Reference 58

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:54.024942Z

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=2026-08-06T17:18:49.245170Z digest=sha256:abdd20491f8575b1287590883393f781719c91a02838aa512f5bf490cd332d14

Observation 7d7fb2cb-66a6-4b5e-a6f4-90f2fc7f850f · outbound

This paper cites Evolution of the Carter constant for inspirals into a black hole: effect of the black hole quadrupole.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Evolution of the Carter constant for inspirals into a black hole: effect of the black hole quadrupole

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:49.339382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:49.339382Z digest=sha256:873822e5deb82d27a894d4536d106a28249083ac6b42333c07441ad5a86533d7

Observation dcac4db0-22f1-41ee-a3c4-4726f58859b0 · outbound

This paper cites Perturbative Approach to an orbital evolution around a Supermassive black hole.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Perturbative Approach to an orbital evolution around a Supermassive black hole

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:49.451524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:49.451524Z digest=sha256:4e2f0b633cacbc8de19a363c6cc8bccc92c885abe7e45ac7625f64f36c80a2a8

Observation f316d218-7877-4591-b10a-91a61e336be1 · outbound

This paper cites Orbits Around Black Holes in Triaxial Nuclei.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Orbits Around Black Holes in Triaxial Nuclei

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:49.577086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:49.577086Z digest=sha256:7879fe9d308f86e9b676f3fe41482d4eee1281bd88eff60f3d90da091021ca83

Observation fbd17e42-91d5-4f06-8214-10f7f62cec01 · outbound

This paper cites Thus, contrary to our case small values of 28 ǫ can only be obtained for i0 ≈π/2.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Thus, contrary to our case small values of 28 ǫ can only be obtained for i0 ≈π/2

Reference 62

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:53.907332Z

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=2026-08-06T17:18:49.671366Z digest=sha256:21c94d18fa21bba6e2911b3f95b98f445e772684c6ec75083948bd4e6ede161b

Observation 2eafd6af-fb0b-4351-be09-f2a13adf7c6c · outbound

This paper cites Tomar, C.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Tomar, C

Reference 63

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T17:18:53.682935Z

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=2026-08-06T17:18:49.771723Z digest=sha256:d0d7dd341b04fbd4473a1472bf030d046b16b5c5c149197ea5edfa2c359cc2b4

Observation cd763804-9bb3-4e4f-8284-7bb3f34f37f9 · outbound

This paper cites Inspiralling compact binaries in quasi-elliptical orbits: The complete third post-Newtonian energy flux.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Inspiralling compact binaries in quasi-elliptical orbits: The complete third post-Newtonian energy flux

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:49.904667Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:49.904667Z digest=sha256:ea61d9d3879a06e6a566563c64726fddb829e7a7cb6b403fa4fdcef2777aa36a

Observation 8613f1d5-696b-4c27-8e6f-0d3adc98507d · outbound

This paper cites Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:50.024838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:50.024838Z digest=sha256:581538c5145f82af87601517ea16e5ebe7539e80d7a8502936b3300a5adb4c0b

Observation dfcfbd6a-b5bb-4fd4-aadf-6870b35375a3 · outbound

This paper cites an unresolved cited work.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Unresolved cited work

Reference 66

Resolution
unresolved
raw_fallback, observed 2026-08-06T17:18:53.408326Z

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=2026-08-06T17:18:50.148153Z digest=sha256:63ad3fd4fc8dcbb16c8194c9c44d003c2d181f1517474c9448309fba5f16b38d

Observation 97cef153-9726-411a-9f80-33555a3d062f · outbound

This paper cites Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:50.238102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:50.238102Z digest=sha256:bd5e18841d4fcc2c27eea6b31a9a77a3c2f2b13b16e3506118c8ed8d14e6b4fe

Observation fdae8f54-a974-4d82-917d-869ae82134aa · outbound

This paper cites On the evolution of a twisted thin accretion disc in eccentric inclined supermassive binary black holes.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster On the evolution of a twisted thin accretion disc in eccentric inclined supermassive binary black holes

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:50.361705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:50.361705Z digest=sha256:835a7319519180599f836e9be23b093988509d4fa58b8aa5ad01534d54fc5a64

Observation 8b0291b5-efbd-4793-86ac-65530d3db9a2 · outbound

This paper cites Binney and S.

The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster Binney and S

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-06T17:18:50.507321Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:18:50.507321Z digest=sha256:fc368f104d0b1c107b1b1e0e98c1b9bf82723b025611a65521fa98cb2e85ebc8

Pith citing papers

No inbound Pith citation observations are available.