Paper Citation Record · LEDGER

Nonradial stability of topological stars

As of 18 August 2026, this Paper Citation Record lists 45 of 45 outbound references and 7 inbound Pith citation observations for arXiv:2502.04444.

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

pith.paper-citation-record.v1
2502.04444 v1

Coverage vector

measured 45 of 45 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-08T22:44:37.415261Z

measured 52 of 52 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:40:54.306583Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-17T22:50:25.826016Z

Reference resolution

45 of 45 outbound references displayed

verified exact6
verified fuzzy2
unresolved37
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Outbound references

Observation a0fad986-d8f9-4c05-b992-79ab21990cd5 · outbound

This paper cites First, we proceed by taking the limit σ → 0, which is the most interesting one for macroscopic objects.

Nonradial stability of topological stars First, we proceed by taking the limit σ → 0, which is the most interesting one for macroscopic objects

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:44:37.909703Z

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Observation 85e39198-7b45-46e3-97ab-d9e222aa9159 · outbound

This paper cites Nonradial stability of topological stars.

Nonradial stability of topological stars Nonradial stability of topological stars

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.254285Z

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Observation 0bbf4547-792f-47c8-8784-f0d5e8b78775 · outbound

This paper cites In addition, by applying the Fourier decomposition (A5) and assuming σ = 0, one notices that H4 , H5 , f− yθ decouple from the rest and can, thus, be neglected.

Nonradial stability of topological stars In addition, by applying the Fourier decomposition (A5) and assuming σ = 0, one notices that H4 , H5 , f− yθ decouple from the rest and can, thus, be neglected

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T22:44:37.898744Z

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Observation 8f8e14ce-96c9-46cc-9396-ab2aee11b55a · outbound

This paper cites an unresolved cited work.

Nonradial stability of topological stars Unresolved cited work

Reference 4

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Observation 12cd1973-7616-4dd5-b615-36e9f20bafe7 · outbound

This paper cites The information paradox: A pedagogical introduction.

Nonradial stability of topological stars The information paradox: A pedagogical introduction

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.273507Z

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Observation d03462b3-2e01-4f5e-bece-7ac94a7e7532 · outbound

This paper cites Fuzzballs and Microstate Geometries: Black-Hole Structure in String Theory.

Nonradial stability of topological stars Fuzzballs and Microstate Geometries: Black-Hole Structure in String Theory

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.278454Z

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Observation 071f96e6-4387-4f57-bfc1-e8f40c0a072c · outbound

This paper cites Snowmass White Paper: Micro- and Macro-Structure of Black Holes.

Nonradial stability of topological stars Snowmass White Paper: Micro- and Macro-Structure of Black Holes

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.281808Z

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Observation d86bcbb8-2c11-401c-a8d0-44f12dbcf5b6 · outbound

This paper cites Mergers and Typical Black Hole Microstates.

Nonradial stability of topological stars Mergers and Typical Black Hole Microstates

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:44:37.827826Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation d7f38e2e-6692-44f5-ab8d-f4948b7d8cc5 · outbound

This paper cites Smooth horizonless geometries deep inside the black-hole regime.

Nonradial stability of topological stars Smooth horizonless geometries deep inside the black-hole regime

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.289005Z

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Observation 95c66b02-f65c-4059-a884-62ba349df0a6 · outbound

This paper cites Asymptotically-flat supergravity solutions deep inside the black-hole regime.

Nonradial stability of topological stars Asymptotically-flat supergravity solutions deep inside the black-hole regime

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.292377Z

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Observation dce19542-2219-4c63-89ab-525c26a5cd6d · outbound

This paper cites Smooth Bubbling Geometries Without Supersymmetry.

Nonradial stability of topological stars Smooth Bubbling Geometries Without Supersymmetry

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.295831Z

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Observation 5a11fb8c-247f-4aad-96b2-c42ad31dd580 · outbound

This paper cites Schwarzschild-like Topological Solitons.

Nonradial stability of topological stars Schwarzschild-like Topological Solitons

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.299301Z

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Observation 38a8f059-b64e-4658-8f9a-93fa708920e2 · outbound

This paper cites an unresolved cited work.

Nonradial stability of topological stars Unresolved cited work

Reference 13

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Observation af1b530c-b666-4be2-b232-4bf8cfa478dc · outbound

This paper cites The Black Hole Information Problem.

Nonradial stability of topological stars The Black Hole Information Problem

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.306115Z

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Observation 8a00c1d5-22b2-4284-97b6-baec6030ca5f · outbound

This paper cites Four Dimensional Black Hole Microstates: From D-branes to Spacetime Foam.

Nonradial stability of topological stars Four Dimensional Black Hole Microstates: From D-branes to Spacetime Foam

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:44:37.765233Z

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Observation 9e001e96-a0b0-4929-aab8-9ea3b6666fe3 · outbound

This paper cites Themelia: the irreducible microstructure of black holes.

Nonradial stability of topological stars Themelia: the irreducible microstructure of black holes

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:44:37.749540Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e7765e12-adf8-4040-a7ec-0ccca3ea75a9 · outbound

This paper cites Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes.

Nonradial stability of topological stars Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.316568Z

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Observation 06c5ba3f-e8cb-4848-9895-471900633c7a · outbound

This paper cites Topological Stars and Black Holes.

Nonradial stability of topological stars Topological Stars and Black Holes

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.320060Z

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Observation 774e63c2-77f9-41b6-b3d9-9cc67257c4b1 · outbound

This paper cites Testing the nature of dark compact objects: a status report.

Nonradial stability of topological stars Testing the nature of dark compact objects: a status report

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.323041Z

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Observation b0a19286-5259-4124-90f3-93eca5972206 · outbound

This paper cites Imaging Topological Solitons: the Microstructure Behind the Shadow.

Nonradial stability of topological stars Imaging Topological Solitons: the Microstructure Behind the Shadow

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.326328Z

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Observation 447c673f-8927-4bee-934f-bf99d926b3e8 · outbound

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

Nonradial stability of topological stars Cavity effect in the quasinormal mode spectrum of topological stars

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.329440Z

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Observation e5b0e2a6-a72a-41d6-8296-914af686d55c · outbound

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

Nonradial stability of topological stars On the stability and deformability of top stars

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.332948Z

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Observation d7255217-6dea-4bd0-9fc9-4df336d31471 · outbound

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

Nonradial stability of topological stars Spectroscopy of magnetized black holes and topological stars

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.336685Z

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Observation ab51e3d0-5c5a-421e-925a-e8c38e2b1886 · outbound

This paper cites Non-spinning tops are stable.

Nonradial stability of topological stars Non-spinning tops are stable

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.340318Z

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Observation ffeb6d9e-c558-4895-9397-bda744c5fa4b · outbound

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

Nonradial stability of topological stars Scalar perturbations in a Top-Star spacetime

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.343982Z

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Observation f2917eaf-492b-43aa-81e8-0da273be00ef · outbound

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

Nonradial stability of topological stars Scalar waves in a Topological Star spacetime: self-force and radiative losses

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.348205Z

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Observation f6a4813f-ed98-42a9-bbac-da66b7bd7f2c · outbound

This paper cites Black Strings and p-Branes are Unstable.

Nonradial stability of topological stars Black Strings and p-Branes are Unstable

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.351899Z

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Observation 108229cc-44dd-49c2-857c-36508b298882 · outbound

This paper cites New stable phase of non-uniform charged black strings.

Nonradial stability of topological stars New stable phase of non-uniform charged black strings

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:44:37.618507Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 0d1ebda1-de4c-4668-90cb-520aa84e1649 · outbound

This paper cites Magnetic Charge Can Locally Stabilize Kaluza-Klein Bubbles.

Nonradial stability of topological stars Magnetic Charge Can Locally Stabilize Kaluza-Klein Bubbles

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:44:37.604085Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation f4b1b530-7ff9-480a-b8a1-5bbc317e4885 · outbound

This paper cites Stability of topological solitons, and black string to bubble transition.

Nonradial stability of topological stars Stability of topological solitons, and black string to bubble transition

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.361443Z

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Observation 2451209e-ce32-4149-9083-9de73e86d741 · outbound

This paper cites Echoes of ECOs: gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale.

Nonradial stability of topological stars Echoes of ECOs: gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.364859Z

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Observation 1da216c3-74a3-46ec-acce-3c280eb36d4e · outbound

This paper cites Is the gravitational-wave ringdown a probe of the event horizon?.

Nonradial stability of topological stars Is the gravitational-wave ringdown a probe of the event horizon?

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.368403Z

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Observation 377ed646-4488-4253-b393-e7f5ab6161d0 · outbound

This paper cites Tests for the existence of horizons through gravitational wave echoes.

Nonradial stability of topological stars Tests for the existence of horizons through gravitational wave echoes

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.371984Z

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Observation 37922ee0-2c8c-4a67-951f-ad7768c79dd3 · outbound

This paper cites Topological Stars, Black holes and Generalized Charged Weyl Solutions.

Nonradial stability of topological stars Topological Stars, Black holes and Generalized Charged Weyl Solutions

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.375694Z

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Observation ca5c4b5b-dc3a-410f-91ee-f3b4d93937f8 · outbound

This paper cites Motion of charged particles around a magnetic black hole/topological star with a compact extra dimension.

Nonradial stability of topological stars Motion of charged particles around a magnetic black hole/topological star with a compact extra dimension

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-08-08T22:44:37.539641Z

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Observation 0e301cf1-991a-49f3-a3c0-c32f10947db9 · outbound

This paper cites Light rings as observational evidence for event horizons: long-lived modes, ergoregions and nonlinear instabilities of ultracompact objects.

Nonradial stability of topological stars Light rings as observational evidence for event horizons: long-lived modes, ergoregions and nonlinear instabilities of ultracompact objects

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.382859Z

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Observation 1d4e238a-3f31-43fd-a63a-e2319dfe1f38 · outbound

This paper cites Gravitoelectromagnetic coupled perturbations and quasinormal modes of a charged black hole with scalar hair.

Nonradial stability of topological stars Gravitoelectromagnetic coupled perturbations and quasinormal modes of a charged black hole with scalar hair

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.386495Z

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Observation edeb72aa-6821-4153-8944-dfda04fbad39 · outbound

This paper cites Quasinormal modes of a charged black hole with scalar hair.

Nonradial stability of topological stars Quasinormal modes of a charged black hole with scalar hair

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.389659Z

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Observation 6e4fef3e-d01c-420b-adec-7d3d704e8ff0 · outbound

This paper cites Black Hole Perturbations and Electric-Magnetic Duality.

Nonradial stability of topological stars Black Hole Perturbations and Electric-Magnetic Duality

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.392742Z

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Observation ac5ba907-94fc-4045-9bcd-abac63e04998 · outbound

This paper cites Advanced Methods in Black-Hole Perturbation Theory.

Nonradial stability of topological stars Advanced Methods in Black-Hole Perturbation Theory

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.396034Z

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Observation a5a25c7c-4606-4eda-94c7-74ee37e84b6a · outbound

This paper cites Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric.

Nonradial stability of topological stars Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.399450Z

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Observation 017f2009-b9d6-4546-87cb-8a7703cfe517 · outbound

This paper cites an unresolved cited work.

Nonradial stability of topological stars Unresolved cited work

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.403217Z

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Observation 1e5fd6f3-3ca0-425e-b0b6-b1b7b9ac2c87 · outbound

This paper cites Light ring stability in ultra-compact objects.

Nonradial stability of topological stars Light ring stability in ultra-compact objects

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.406810Z

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Observation 5f2abab9-23aa-48f8-97b9-65ddac589bf9 · outbound

This paper cites Instability of supersymmetric microstate geometries.

Nonradial stability of topological stars Instability of supersymmetric microstate geometries

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.411532Z

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Observation ffdd66f9-b2f6-440e-9b94-25decccc9e3f · outbound

This paper cites Slowly Decaying Waves on Spherically Symmetric Spacetimes and an Instability of Ultracompact Neutron Stars.

Nonradial stability of topological stars Slowly Decaying Waves on Spherically Symmetric Spacetimes and an Instability of Ultracompact Neutron Stars

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.415261Z

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Pith citing papers

Observation 85e39198-7b45-46e3-97ab-d9e222aa9159 · inbound