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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

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

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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Observation 342c08bb-4ddc-41f4-b091-6b050249684f · outbound

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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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Observation cee1c02a-4afc-446f-b644-bc8f251c5549 · outbound

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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
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Unavailable: canonical work link unavailable.

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Observation bcd1dcda-c876-443a-afc9-7422c803b3d4 · outbound

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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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
local_arxiv, observed 2026-08-06T17:18:52.601943Z

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
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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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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Observation ab8c0215-a156-4007-8cd2-0b3c4be73a78 · outbound

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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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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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

Resolution
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Source-reported events for the cited work

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Observation 07f441fe-ac17-4b5d-b870-cf84e9467b39 · outbound

This paper cites Vasiliev, F.

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

Reference 35

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:47.850919Z digest=sha256:8608a9244e454083e6ffb22fc14d45fdd7421a685ecf0dc2f1a9398352109b07

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:47.919501Z digest=sha256:fcd5f5673168faddd3675a01e07538dca78a045d39c0eff8ae4db661edd3bc0a

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:47.970893Z digest=sha256:176b704221ba0774199eb7b6924e4d46eb4a67d8afd5899f505d1c01e97bfc54

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.042779Z digest=sha256:1563a61196911c7dac960ed6d64e7435b79a939f5e5d02a3d699434b846d6e9b

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.084361Z digest=sha256:6d8191fd64939546ae7c8c32803822c3810d71bd81168b40d6cee8d066da0ae7

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.142791Z digest=sha256:5a1e8c4da9015ff6f7b3266fbbba25c43cc13c028dbf13a66477ffafb6674e6e

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.205125Z digest=sha256:b9b43d27eb68aebe3a49e070b81938bb3faa48542691b919cc21fc33b2afdc78

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.263290Z digest=sha256:49defc7b6df1385ed30ced8dacd7c0b10e42865474dd33db8bcc3671634fabe0

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.352934Z digest=sha256:96e907461b113b2dc959f23db61757244550fa06fe3454d07e10e60715d63048

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.397120Z digest=sha256:1126a8fba90c71f4528ccb0077bca9d661691220c6b48f7d3fe4ce9307778de5

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.452260Z digest=sha256:65694f12cc1b2665de80701213d4c16c9e62934238d7b51d0f48f4d3c7611b4a

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.558491Z digest=sha256:fc8fd57cea727db55bb076779c6d37cfaa11b61e866a889003e457d4d05181f9

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.611384Z digest=sha256:5b4697615ba025f2bcbfc85e90c85cc1106b19a61a72988df37bd3cbab7f6fd9

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.646197Z digest=sha256:1c2b44125d68673ffc46314f3fd2275aadddfbd0891f13cb88b70c450a105422

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.703274Z digest=sha256:d7e39c055eee0a4202ffa86f9c093b8a602d36d5f4597b7408de091f39b71c79

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.752164Z digest=sha256:15a1ced3175f8cd94640a3729f21cd50a498cd58c3e8142fe74f6137a6d0f8ef

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.814073Z digest=sha256:30c06dcf466f0ba81ae8c2139ae761e801fe9f7a295d81d2d6995bbb079b2311

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.860190Z digest=sha256:d93feb693f8b53a7108f40b65a52fa45462c302803b71cf6fda0f96d17cde826

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.917030Z digest=sha256:67b71ed409ba1174f3bcd79ca532b768d6ec482202e41088fddb8b194e7420b9

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:48.963974Z digest=sha256:871cd780026682752f565f491926a301f61aae56cb61ec89ee0cccb21004b5f5

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:49.043983Z digest=sha256:f84f06fb3b5528de501041aa780eae4eb60ca19c3cc06ef0654a5aa3109012c7

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:49.152444Z digest=sha256:0f4039dd7097c420b10a68bd074afaa3c3be4606e808bc40d9a3f036811f08ee

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:49.245170Z digest=sha256:86ad646c3510b9e15596a9e4efb668a6e72efe3d51578c6247b0b7989db9df99

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:49.671366Z digest=sha256:e08e5f8aae38600fde73dbf37d1fbe6f0baeb370b7bc16e5df791f1aa31caff2

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:49.771723Z digest=sha256:c3095239d1cf967888c7e6ad30ad54d26d38d17d1cb7d176dcc6ee35b1ec3d67

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-06T17:18:50.148153Z digest=sha256:14d5ab1eb38ca93edc38f8c0118b869d7b21f5637dc1419de466a978a42b4e1a

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.