Paper Citation Record · LEDGER

Scattering angle in a Topological Star spacetime: a self-force approach

As of 7 August 2026, this Paper Citation Record lists 79 of 79 outbound references and 4 inbound Pith citation observations for arXiv:2506.04876.

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

pith.paper-citation-record.v1
2506.04876 v1

Coverage vector

measured 79 of 79 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:39:22.596270Z

measured 83 of 83 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:32:36.523814Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-17T22:50:26.011048Z

Reference resolution

79 of 79 outbound references displayed

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External citation measurements

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Outbound references

Observation b8e536a1-b56f-41f1-95c7-9b88cd17131b · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 1

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:29.159707Z

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Observation 4af97e66-5c50-4492-82a9-38a56941d687 · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:29.050581Z

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Observation b5a3221d-994b-4817-a1d4-a01ce243fb82 · outbound

This paper cites (4.10) The associated Kretschmann invariant is (2)Kt−r = Rαβγδ Rαβγδ = r2 s (4r − 5rb)2 4r8 , (4.11) showing a geometrical role for the radius r = 5 4 rb.

Scattering angle in a Topological Star spacetime: a self-force approach (4.10) The associated Kretschmann invariant is (2)Kt−r = Rαβγδ Rαβγδ = r2 s (4r − 5rb)2 4r8 , (4.11) showing a geometrical role for the radius r = 5 4 rb

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:28.916915Z

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Observation 5cf60f81-1ccf-4b35-99fd-43a8c2fc34c1 · outbound

This paper cites (4.12) The associated Kretschmann invariant is (2)Kr−φ = [(rs + rb)r − 2rsrb]2 r8 , (4.13) showing a geometrical role for the radius r = 2rsrb (rs+rb) = 2 1 rs + 1 rb.

Scattering angle in a Topological Star spacetime: a self-force approach (4.12) The associated Kretschmann invariant is (2)Kr−φ = [(rs + rb)r − 2rsrb]2 r8 , (4.13) showing a geometrical role for the radius r = 2rsrb (rs+rb) = 2 1 rs + 1 rb

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:28.801452Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e8f6ebdf-abb5-4cbd-9314-2b521ac12692 · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:28.653838Z

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Observation e9acaf8b-c489-425e-b07d-ab8425658106 · outbound

This paper cites Let us introduce an orthonormal frame adapted to the static observers (4.16) eˆt = u = 1√−gtt ∂t , e ˆr = 1√grr ∂r , e ˆθ = 1√gθθ ∂θ , e ˆφ = 1√gφφ ∂φ , e ˆy = 1√gyy ∂y.

Scattering angle in a Topological Star spacetime: a self-force approach Let us introduce an orthonormal frame adapted to the static observers (4.16) eˆt = u = 1√−gtt ∂t , e ˆr = 1√grr ∂r , e ˆθ = 1√gθθ ∂θ , e ˆφ = 1√gφφ ∂φ , e ˆy = 1√gyy ∂y

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:28.537866Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c6071445-8d21-4d09-a1fb-8d75b97084dc · outbound

This paper cites (4.29) the transport is trivial for the θ and φ components of X and reduces to X θ(τ ) = X θ(0) and X y(τ ) = X y(0).

Scattering angle in a Topological Star spacetime: a self-force approach (4.29) the transport is trivial for the θ and φ components of X and reduces to X θ(τ ) = X θ(0) and X y(τ ) = X y(0)

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:28.395782Z

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Observation 19f79ecc-f454-4586-9bae-0f0034d51aa4 · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 8

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:28.266059Z

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Observation f3cc0d41-140f-43e6-8653-bc99900f47de · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 9

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:28.103923Z

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Observation feb5f1a8-10b2-4d9c-953a-6de7d3e18226 · outbound

This paper cites holonomy invariance.

Scattering angle in a Topological Star spacetime: a self-force approach holonomy invariance

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:27.904349Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6afed287-e697-4675-ae08-8302fb74a718 · outbound

This paper cites String Theory as a bridge between Gauge Theories and Quantum Gravity.

Scattering angle in a Topological Star spacetime: a self-force approach String Theory as a bridge between Gauge Theories and Quantum Gravity

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:27.780929Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 23ef3b15-8a32-42d8-853a-c342586147f9 · outbound

This paper cites Post-Newtonian Theory for Gravitational Waves.

Scattering angle in a Topological Star spacetime: a self-force approach Post-Newtonian Theory for Gravitational Waves

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:16.065256Z

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Observation 943984b8-e36c-4d7f-8320-2276b5a96442 · outbound

This paper cites On general relativistic dynamics of clas si- cal spin particles. (In German),.

Scattering angle in a Topological Star spacetime: a self-force approach On general relativistic dynamics of clas si- cal spin particles. (In German),

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:27.620102Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation cf6b3cb6-9c4c-4bb7-bfef-6f4651c8e4ea · outbound

This paper cites Gravitational Bremsstrahlung In Postlinear Fast Motion Approx- imation,.

Scattering angle in a Topological Star spacetime: a self-force approach Gravitational Bremsstrahlung In Postlinear Fast Motion Approx- imation,

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:27.470456Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7f6edace-2f01-4978-a3a9-e2f1f4db2a17 · outbound

This paper cites Gravitational Scattering Of Two Relativistic Particles In Postlinear Approxima- tion,.

Scattering angle in a Topological Star spacetime: a self-force approach Gravitational Scattering Of Two Relativistic Particles In Postlinear Approxima- tion,

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:27.324067Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation bce88c5b-fd38-4c8d-b95d-c34095f6aeb8 · outbound

This paper cites Poincar´ e-invariant gravitational ﬁeld and equations of motion of two pointlike objects: The postlinear approx- imation of general relativity,.

Scattering angle in a Topological Star spacetime: a self-force approach Poincar´ e-invariant gravitational ﬁeld and equations of motion of two pointlike objects: The postlinear approx- imation of general relativity,

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:27.159969Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e005da5f-e836-4d5d-8506-64ff3890fc92 · outbound

This paper cites Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory.

Scattering angle in a Topological Star spacetime: a self-force approach Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:16.942734Z

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Unavailable: canonical work link unavailable.

Observation 7ad5db6c-6493-4ea8-97cc-ce251182d36f · outbound

This paper cites Effective field theory approach to the gravitational two-body dynamics, at fourth post-Newtonian order and quintic in the Newton constant.

Scattering angle in a Topological Star spacetime: a self-force approach Effective field theory approach to the gravitational two-body dynamics, at fourth post-Newtonian order and quintic in the Newton constant

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.122131Z

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Unavailable: canonical work link unavailable.

Observation 779034ea-e440-4078-b044-689c2d0dc67c · outbound

This paper cites Static two-body potential at fifth post-Newtonian order.

Scattering angle in a Topological Star spacetime: a self-force approach Static two-body potential at fifth post-Newtonian order

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.250286Z

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Observation bca77a82-b557-42c4-b979-af59160529b3 · outbound

This paper cites The Effective Field Theorist's Approach to Gravitational Dynamics.

Scattering angle in a Topological Star spacetime: a self-force approach The Effective Field Theorist's Approach to Gravitational Dynamics

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.397847Z

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Unavailable: canonical work link unavailable.

Observation 93676a61-5524-4d83-976c-afc1f6c47647 · outbound

This paper cites Post-Minkowskian Effective Field Theory for Conservative Binary Dynamics.

Scattering angle in a Topological Star spacetime: a self-force approach Post-Minkowskian Effective Field Theory for Conservative Binary Dynamics

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.518972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eddedd01-9329-4dce-bcd7-615f7985e8ba · outbound

This paper cites Black Hole Binary Dynamics from the Double Copy and Effective Theory.

Scattering angle in a Topological Star spacetime: a self-force approach Black Hole Binary Dynamics from the Double Copy and Effective Theory

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.633279Z

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Observation 1699cba3-a3d5-418d-a77a-495113bff72a · outbound

This paper cites Scattering Amplitudes and Conservative Binary Dynamics at ${\cal O}(G^4)$.

Scattering angle in a Topological Star spacetime: a self-force approach Scattering Amplitudes and Conservative Binary Dynamics at ${\cal O}(G^4)$

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.745414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b67b569-0d01-4965-80bf-e3bf898556e4 · outbound

This paper cites Radiative Classical Gravitational Observables at $\mathcal O(G^3)$ from Scattering Amplitudes.

Scattering angle in a Topological Star spacetime: a self-force approach Radiative Classical Gravitational Observables at $\mathcal O(G^3)$ from Scattering Amplitudes

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:17.888960Z

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Unavailable: canonical work link unavailable.

Observation e3a32d1e-3ad7-439e-a05b-3ed4edbc1bed · outbound

This paper cites The Amplitude for Classical Gravitational Scattering at Third Post-Minkowskian Order.

Scattering angle in a Topological Star spacetime: a self-force approach The Amplitude for Classical Gravitational Scattering at Third Post-Minkowskian Order

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.050861Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8a6b1fa-55af-45f7-8d0d-dfd14e48f0f8 · outbound

This paper cites Scattering Amplitudes, the Tail Effect, and Conservative Binary Dynamics at $O(G^4)$.

Scattering angle in a Topological Star spacetime: a self-force approach Scattering Amplitudes, the Tail Effect, and Conservative Binary Dynamics at $O(G^4)$

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.164404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 22d56586-d8e1-4a5f-9225-34483610769c · outbound

This paper cites Conservative Dynamics of Binary Systems at Fourth Post-Minkowskian Order in the Large-eccentricity Expansion.

Scattering angle in a Topological Star spacetime: a self-force approach Conservative Dynamics of Binary Systems at Fourth Post-Minkowskian Order in the Large-eccentricity Expansion

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.317737Z

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Unavailable: canonical work link unavailable.

Observation fd232098-227f-4318-812d-45b3e526d4fb · outbound

This paper cites Radiation Reaction and Gravitational Waves at Fourth Post-Minkowskian Order.

Scattering angle in a Topological Star spacetime: a self-force approach Radiation Reaction and Gravitational Waves at Fourth Post-Minkowskian Order

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.431749Z

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Unavailable: canonical work link unavailable.

Observation 2d7e2b43-289d-4156-9b5e-faff89a3cf41 · outbound

This paper cites Classical Observables from the Exponential Representation of the Gravitational S-Matrix.

Scattering angle in a Topological Star spacetime: a self-force approach Classical Observables from the Exponential Representation of the Gravitational S-Matrix

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.560137Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 946e82aa-e93a-4e76-8983-effa6f2ba358 · outbound

This paper cites Local-in-time Conservative Binary Dynamics at Fourth Post-Minkowskian Order.

Scattering angle in a Topological Star spacetime: a self-force approach Local-in-time Conservative Binary Dynamics at Fourth Post-Minkowskian Order

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.697767Z

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Unavailable: canonical work link unavailable.

Observation a21f6d40-8574-4a53-8655-a9caabbaedf3 · outbound

This paper cites Calabi-Yau periods for black hole scattering in classical general relativity.

Scattering angle in a Topological Star spacetime: a self-force approach Calabi-Yau periods for black hole scattering in classical general relativity

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.811928Z

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Observation ae9faf7b-6223-40de-b031-575578fe9012 · outbound

This paper cites Conservative Black Hole Scattering at Fifth Post-Minkowskian and First Self-Force Order.

Scattering angle in a Topological Star spacetime: a self-force approach Conservative Black Hole Scattering at Fifth Post-Minkowskian and First Self-Force Order

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:18.933255Z

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Observation 399d4c69-deb6-45b3-8ac2-1a999387aeaa · outbound

This paper cites Radiative contributions to gravitational scattering.

Scattering angle in a Topological Star spacetime: a self-force approach Radiative contributions to gravitational scattering

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.051430Z

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Observation 6fedc03c-46a3-4eb2-88bd-cee294a7d42b · outbound

This paper cites Radiated momentum and radiation-reaction in gravitational two-body scattering including time-asymmetric effects.

Scattering angle in a Topological Star spacetime: a self-force approach Radiated momentum and radiation-reaction in gravitational two-body scattering including time-asymmetric effects

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.161087Z

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Observation cd675708-8d07-43b3-b322-24e64755bf67 · outbound

This paper cites Black Hole Quasinormal Modes and Seiberg-Witten Theory.

Scattering angle in a Topological Star spacetime: a self-force approach Black Hole Quasinormal Modes and Seiberg-Witten Theory

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.269211Z

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Unavailable: canonical work link unavailable.

Observation 504cd4d1-0bd0-4544-97b1-a4ef06202593 · outbound

This paper cites QNMs of branes, BHs and fuzzballs from quantum SW geometries,.

Scattering angle in a Topological Star spacetime: a self-force approach QNMs of branes, BHs and fuzzballs from quantum SW geometries,

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.384494Z

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Unavailable: canonical work link unavailable.

Observation 775c54a1-8f08-4a0c-80f2-517663e87f6b · outbound

This paper cites More on the SW-QNM correspondence.

Scattering angle in a Topological Star spacetime: a self-force approach More on the SW-QNM correspondence

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.491982Z

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Observation 0033416a-badc-4761-898b-6f6f60a9a0d6 · outbound

This paper cites Exact solution of Kerr black hole perturbations via CFT$_2$ and instanton counting. Greybody factor, Quasinormal modes and Love numbers.

Scattering angle in a Topological Star spacetime: a self-force approach Exact solution of Kerr black hole perturbations via CFT$_2$ and instanton counting. Greybody factor, Quasinormal modes and Love numbers

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.583638Z

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Unavailable: canonical work link unavailable.

Observation 06426969-eff0-44d4-b38e-4da90d2dfd6e · outbound

This paper cites Irregular Liouville correlators and connection formulae for Heun functions.

Scattering angle in a Topological Star spacetime: a self-force approach Irregular Liouville correlators and connection formulae for Heun functions

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.735879Z

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Unavailable: canonical work link unavailable.

Observation 3fef28cd-e214-4cf2-9bd3-83eebd00a6aa · outbound

This paper cites 2-charge circular fuzz-balls and their perturbations.

Scattering angle in a Topological Star spacetime: a self-force approach 2-charge circular fuzz-balls and their perturbations

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.846458Z

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Unavailable: canonical work link unavailable.

Observation f99a2182-791e-4c3b-8fc3-53c50973346c · outbound

This paper cites CFT description of BH's and ECO's: QNMs, superradiance, echoes and tidal responses.

Scattering angle in a Topological Star spacetime: a self-force approach CFT description of BH's and ECO's: QNMs, superradiance, echoes and tidal responses

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:19.959126Z

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Observation 8d333a3f-d853-4157-8127-51bd1097e620 · outbound

This paper cites Black Hole Perturbation Theory Meets CFT$_2$: Kerr Compton Amplitudes from Nekrasov-Shatashvili Functions.

Scattering angle in a Topological Star spacetime: a self-force approach Black Hole Perturbation Theory Meets CFT$_2$: Kerr Compton Amplitudes from Nekrasov-Shatashvili Functions

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.071876Z

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Unavailable: canonical work link unavailable.

Observation ddf41628-eb19-466b-8b96-5278ae17119a · outbound

This paper cites Tidal resonances for fuzzballs.

Scattering angle in a Topological Star spacetime: a self-force approach Tidal resonances for fuzzballs

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.166092Z

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Unavailable: canonical work link unavailable.

Observation b5a92547-1a74-4a18-8a42-7d40ae9de781 · outbound

This paper cites Resumming Post-Minkowskian and Post-Newtonian gravitational waveform expansions.

Scattering angle in a Topological Star spacetime: a self-force approach Resumming Post-Minkowskian and Post-Newtonian gravitational waveform expansions

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.250471Z

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Unavailable: canonical work link unavailable.

Observation 3ba820cd-7995-49c0-832b-0c3ac0a4ba15 · outbound

This paper cites Topological Stars and Black Holes.

Scattering angle in a Topological Star spacetime: a self-force approach Topological Stars and Black Holes

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.355445Z

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Unavailable: canonical work link unavailable.

Observation b8c5479c-0549-42ea-b403-e7239882095c · outbound

This paper cites Cavity effect in the quasinormal mode spectrum of topological stars.

Scattering angle in a Topological Star spacetime: a self-force approach Cavity effect in the quasinormal mode spectrum of topological stars

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.470978Z

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Unavailable: canonical work link unavailable.

Observation 88e0c134-b7b0-433c-a01f-628f13537e88 · outbound

This paper cites On the stability and deformability of top stars.

Scattering angle in a Topological Star spacetime: a self-force approach On the stability and deformability of top stars

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.556913Z

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Unavailable: canonical work link unavailable.

Observation 983379f7-61fe-4d4d-9f9f-98ec4883a3c2 · outbound

This paper cites Charge (in)stability and superradiance of Topological Stars.

Scattering angle in a Topological Star spacetime: a self-force approach Charge (in)stability and superradiance of Topological Stars

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.671348Z

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Unavailable: canonical work link unavailable.

Observation 93496f53-e210-4175-af50-3e8483362598 · outbound

This paper cites Spectroscopy of magnetized black holes and topological stars.

Scattering angle in a Topological Star spacetime: a self-force approach Spectroscopy of magnetized black holes and topological stars

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.728570Z

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Unavailable: canonical work link unavailable.

Observation bcbc528f-d908-4fad-960e-f18b770b6ccf · outbound

This paper cites Non-spinning tops are stable.

Scattering angle in a Topological Star spacetime: a self-force approach Non-spinning tops are stable

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.784612Z

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Unavailable: canonical work link unavailable.

Observation 7ea8b35e-06c5-4159-b750-60485488c6f9 · outbound

This paper cites Scalar waves from unbound orbits in a TS spacetime: PN reconstruction of the field and radiation losses in a self-force approach.

Scattering angle in a Topological Star spacetime: a self-force approach Scalar waves from unbound orbits in a TS spacetime: PN reconstruction of the field and radiation losses in a self-force approach

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.848449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d707255-8d0e-4191-bc41-acc5eebdc152 · outbound

This paper cites Scalar perturbations in a Top-Star spacetime.

Scattering angle in a Topological Star spacetime: a self-force approach Scalar perturbations in a Top-Star spacetime

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.924686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 30b77b28-e9db-4314-b003-af7449623518 · outbound

This paper cites Scalar waves in a Topological Star spacetime: self-force and radiative losses.

Scattering angle in a Topological Star spacetime: a self-force approach Scalar waves in a Topological Star spacetime: self-force and radiative losses

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:21.005116Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b45565c-bc6b-478d-9517-53a84f6c912b · outbound

This paper cites Nonradial stability of topological stars.

Scattering angle in a Topological Star spacetime: a self-force approach Nonradial stability of topological stars

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:21.064249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 457c89b4-408a-42de-b46d-3a51384a5149 · outbound

This paper cites On the Papapetrou field in vacuum.

Scattering angle in a Topological Star spacetime: a self-force approach On the Papapetrou field in vacuum

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-07T10:39:23.374641Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8bc21891-cbcb-44c9-bd81-0189922cdb30 · outbound

This paper cites Sur la radiation gravitationnelle,.

Scattering angle in a Topological Star spacetime: a self-force approach Sur la radiation gravitationnelle,

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:26.998564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 113290eb-9267-4042-840e-b14df6d165e2 · outbound

This paper cites Introduction d’un tenseur du quatri` eme ordre ,.

Scattering angle in a Topological Star spacetime: a self-force approach Introduction d’un tenseur du quatri` eme ordre ,

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:26.828881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c54c93d0-5da6-46f5-8640-0881baebe320 · outbound

This paper cites Les ´ etats de radiation et le probl` eme de l’´ energie en relativit´ e g´ en´ erale,.

Scattering angle in a Topological Star spacetime: a self-force approach Les ´ etats de radiation et le probl` eme de l’´ energie en relativit´ e g´ en´ erale,

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:26.651885Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2a2df533-ee7b-46b5-b2df-deea78d211a8 · outbound

This paper cites La radiation gravitationnelle,.

Scattering angle in a Topological Star spacetime: a self-force approach La radiation gravitationnelle,

Reference 59

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:26.523891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8f2a6eeb-efeb-4050-bbeb-22448c467128 · outbound

This paper cites On the Bel-Robinson tensor,.

Scattering angle in a Topological Star spacetime: a self-force approach On the Bel-Robinson tensor,

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:26.377021Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c4b1c5e0-7a03-4a6a-9985-a3050cbcff72 · outbound

This paper cites Black hole in a uniform magnetic ﬁeld,.

Scattering angle in a Topological Star spacetime: a self-force approach Black hole in a uniform magnetic ﬁeld,

Reference 61

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:26.200071Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 87d0625d-625e-445b-8f9e-7057e48fe4ca · outbound

This paper cites Consequences of a Killing symmetry in spacetime's local structure.

Scattering angle in a Topological Star spacetime: a self-force approach Consequences of a Killing symmetry in spacetime's local structure

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-07T10:39:23.223776Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation b4c86470-9909-418c-ad44-2b9b702e5e2f · outbound

This paper cites Stationary Solutions, Energy and the Bel- Robinson Tensor,.

Scattering angle in a Topological Star spacetime: a self-force approach Stationary Solutions, Energy and the Bel- Robinson Tensor,

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:25.988169Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation dbdd0b34-33f1-4e55-bc85-f3cbb2c29f78 · outbound

This paper cites The Bel- Robinson tensor for the collision of gravitational plane waves,.

Scattering angle in a Topological Star spacetime: a self-force approach The Bel- Robinson tensor for the collision of gravitational plane waves,

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:25.800119Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 9117aedb-9ce9-4c50-a884-a8446b5de2ff · outbound

This paper cites Gravitational Superenergy Tensor.

Scattering angle in a Topological Star spacetime: a self-force approach Gravitational Superenergy Tensor

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-08-07T10:39:23.081887Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f2db592d-5b8c-472f-a3e7-d49679165ebf · outbound

This paper cites Some Prop- erties of the Bel and Bel-Robinson Tensors,.

Scattering angle in a Topological Star spacetime: a self-force approach Some Prop- erties of the Bel and Bel-Robinson Tensors,

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:25.652322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 22063bb2-285f-4153-9e95-8cdb6741e6da · outbound

This paper cites Positivity properties of the Bel-Robin son tensor,.

Scattering angle in a Topological Star spacetime: a self-force approach Positivity properties of the Bel-Robin son tensor,

Reference 67

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:25.485794Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a51f0e35-6ef2-4520-abe7-4025f4b9a2b7 · outbound

This paper cites The gravitoelectromagnetic stress-energy tensor.

Scattering angle in a Topological Star spacetime: a self-force approach The gravitoelectromagnetic stress-energy tensor

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-07T10:39:22.902053Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 15c5672f-e0dd-4aa0-b028-aaed13c4e26a · outbound

This paper cites Super-energy tensors.

Scattering angle in a Topological Star spacetime: a self-force approach Super-energy tensors

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:21.927941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45802e1b-e168-42a6-8d5e-605ec2263ead · outbound

This paper cites Electromagnetic - Like Boost Transformations of Weyl and Minimal Super- Energy Observers in Black Hole Spacetimes,.

Scattering angle in a Topological Star spacetime: a self-force approach Electromagnetic - Like Boost Transformations of Weyl and Minimal Super- Energy Observers in Black Hole Spacetimes,

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:25.306854Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7fd97bb4-af83-45a9-a767-afc5f72da098 · outbound

This paper cites Gravi- tation,.

Scattering angle in a Topological Star spacetime: a self-force approach Gravi- tation,

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:22.027516Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6d770ec-d34f-4390-aa6d-aabc77541c9e · outbound

This paper cites Geometric transport along circular orbits in stationary axisymmetric spacetimes.

Scattering angle in a Topological Star spacetime: a self-force approach Geometric transport along circular orbits in stationary axisymmetric spacetimes

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:22.095662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e75a61d-99f4-4da0-b4a2-15951896efb6 · outbound

This paper cites Gravitational scattering of two black holes at the fourth post-Newtonian approximation.

Scattering angle in a Topological Star spacetime: a self-force approach Gravitational scattering of two black holes at the fourth post-Newtonian approximation

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:22.138747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0438350f-d0f0-4c59-931a-98e68dc34157 · outbound

This paper cites Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model.

Scattering angle in a Topological Star spacetime: a self-force approach Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:22.223551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf10da14-b7bb-4ed8-a178-3c2c978d30cb · outbound

This paper cites Post-Minkowskian self-force in the low-velocity limit: scalar field scattering.

Scattering angle in a Topological Star spacetime: a self-force approach Post-Minkowskian self-force in the low-velocity limit: scalar field scattering

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:22.303012Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f08fc67-456b-4524-a041-17a9fa6cf812 · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 76

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:25.114347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2380b93c-e4eb-4a3a-a213-c20dda2f4d8b · outbound

This paper cites an unresolved cited work.

Scattering angle in a Topological Star spacetime: a self-force approach Unresolved cited work

Reference 77

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:39:24.919285Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a1dea767-57b8-4eaa-a7d3-0b091bff72aa · outbound

This paper cites TS plus α → 0 is not Schwarzschild.

Scattering angle in a Topological Star spacetime: a self-force approach TS plus α → 0 is not Schwarzschild

Reference 78

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:24.739322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c782d87c-1e6d-415f-b6ea-5fb54f9dcd00 · outbound

This paper cites Damour for raising this issue.

Scattering angle in a Topological Star spacetime: a self-force approach Damour for raising this issue

Reference 79

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:39:24.535767Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Pith citing papers

Observation 4f8157cc-c7bd-4777-90c8-09fa7d0b8b12 · inbound

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit cites this paper.

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit Scattering angle in a Topological Star spacetime: a self-force approach

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T00:32:36.523814Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 272475c7-c402-4497-9257-9a0a041a46cf · inbound

Gravitational Atoms from Topological Stars cites this paper.

Gravitational Atoms from Topological Stars Scattering angle in a Topological Star spacetime: a self-force approach

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:50:26.012929Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 0f33a17e-074a-44eb-ba49-30032331f7f2 · inbound

"Waveforms" at the Horizon cites this paper.

"Waveforms" at the Horizon Scattering angle in a Topological Star spacetime: a self-force approach

Reference 115

Resolution: unresolved; no resolver link, observed 2026-08-03T04:12:13.781206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bcad9721-3afe-4da5-a34a-f9b0b050d54f · inbound

The radial action for massive particles in spherically symmetric geometries: Exact resummation at any PM order cites this paper.

The radial action for massive particles in spherically symmetric geometries: Exact resummation at any PM order Scattering angle in a Topological Star spacetime: a self-force approach

Reference 22

Resolution: malformed identifier; no resolver link, observed 2026-08-02T01:05:57.282863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.