Paper Citation Record · LEDGER

What happens to topological invariants (and black holes) in singularity-free theories?

As of 13 August 2026, this Paper Citation Record lists 47 of 47 outbound references and 2 inbound Pith citation observations for arXiv:2411.11450.

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

pith.paper-citation-record.v1
2411.11450 v3

Coverage vector

measured 47 of 47 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:41:00.471387Z

measured 49 of 49 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-29T05:48:54.583585Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T18:35:58.413739Z

Reference resolution

47 of 47 outbound references displayed

verified exact6
verified fuzzy8
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External citation measurements

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Outbound references

Observation aa241ad9-0541-4b52-949b-4532942ed64e · outbound

This paper cites Behavior of the Newtonian potential for ghost-free gravity and singularity-free gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Behavior of the Newtonian potential for ghost-free gravity and singularity-free gravity

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.235796Z

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Observation 61d0da63-3ff9-4832-be2f-7adda11586b9 · outbound

This paper cites On the cancellation of Newtonian singularities in higher-derivative gravity.

What happens to topological invariants (and black holes) in singularity-free theories? On the cancellation of Newtonian singularities in higher-derivative gravity

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.241433Z

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Observation 345359ea-bfb5-47c5-8b68-de2736ae08ef · outbound

This paper cites Classical properties of non-local, ghost- and singularity-free gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Classical properties of non-local, ghost- and singularity-free gravity

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.246905Z

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Observation 89f80465-5e2f-49a3-82dc-867749a3eaa7 · outbound

This paper cites The gravitational field of static p-branes in linearized ghost-free gravity.

What happens to topological invariants (and black holes) in singularity-free theories? The gravitational field of static p-branes in linearized ghost-free gravity

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.251893Z

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Observation dcbac7cf-5109-40ce-8f76-30ec2e80337d · outbound

This paper cites Effective delta sources and regularity in higher-derivative and ghost-free gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Effective delta sources and regularity in higher-derivative and ghost-free gravity

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.256789Z

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Observation f87c4ff0-4f8c-4512-900f-07de29220a92 · outbound

This paper cites Angle deficit & non-local gravitoelectromagnetism around a slowly spinning cosmic string.

What happens to topological invariants (and black holes) in singularity-free theories? Angle deficit & non-local gravitoelectromagnetism around a slowly spinning cosmic string

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-08-12T18:41:01.400110Z

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Observation ebbdbe4d-1e19-4876-845d-461959f3eb8f · outbound

This paper cites NUT charge in linearized infinite derivative gravity.

What happens to topological invariants (and black holes) in singularity-free theories? NUT charge in linearized infinite derivative gravity

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.267280Z

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Observation 2e93016a-2fa0-4707-8fcd-cfa56108e038 · outbound

This paper cites Ultrarelativistic spinning objects in non-local ghost-free gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Ultrarelativistic spinning objects in non-local ghost-free gravity

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-08-12T18:41:01.356109Z

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Observation abcd191a-01c4-47ba-8305-58da438c0056 · outbound

This paper cites Effects of Non-locality in Gravity and Quantum Theory.

What happens to topological invariants (and black holes) in singularity-free theories? Effects of Non-locality in Gravity and Quantum Theory

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.277832Z

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Observation 845bc861-0510-4ec5-afe3-ac7cefa4b3ee · outbound

This paper cites Non-locality and gravitoelectromagnetic duality.

What happens to topological invariants (and black holes) in singularity-free theories? Non-locality and gravitoelectromagnetic duality

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.283089Z

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Observation 9b5a7f4a-ead2-449b-9db0-e3f8bc85e4ab · outbound

This paper cites On the gravitational field of a massless particle,.

What happens to topological invariants (and black holes) in singularity-free theories? On the gravitational field of a massless particle,

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.630774Z

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Observation 5d368ba1-8a6c-4c3a-abde-f8db38559163 · outbound

This paper cites Q-preserving.

What happens to topological invariants (and black holes) in singularity-free theories? Q-preserving

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.646029Z

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Observation 3736edb1-d4ac-4966-ab0b-24568ef57cd0 · outbound

This paper cites Any space-time has a plane wave as a limit,.

What happens to topological invariants (and black holes) in singularity-free theories? Any space-time has a plane wave as a limit,

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.615350Z

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Observation f39a7dd8-49ac-4dc2-a923-8844a9dd46fd · outbound

This paper cites Inner-horizon instability and mass inflation in black holes,.

What happens to topological invariants (and black holes) in singularity-free theories? Inner-horizon instability and mass inflation in black holes,

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.298012Z

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Observation a32eeb79-4b2e-4092-a562-4b6c2f898fdd · outbound

This paper cites Geodesically complete black holes.

What happens to topological invariants (and black holes) in singularity-free theories? Geodesically complete black holes

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.302790Z

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Observation 9ba2461b-4b1e-4807-9111-631388280c1b · outbound

This paper cites Geodesic incompleteness of some popular regular black holes.

What happens to topological invariants (and black holes) in singularity-free theories? Geodesic incompleteness of some popular regular black holes

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.307674Z

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Observation fc8611cf-84ac-4bda-ba64-714ec761218a · outbound

This paper cites Mass-gap for black hole formation in higher derivative and ghost free gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Mass-gap for black hole formation in higher derivative and ghost free gravity

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.312541Z

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Observation 94f1d010-158b-4726-8fb6-56d160240e9e · outbound

This paper cites Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$.

What happens to topological invariants (and black holes) in singularity-free theories? Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.317984Z

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Observation 9f50b1d4-f85c-4619-a73a-4901e6a9ee33 · outbound

This paper cites Non-singular general relativistic grav- itational collapse,.

What happens to topological invariants (and black holes) in singularity-free theories? Non-singular general relativistic grav- itational collapse,

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.582506Z

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Observation 634f6d13-2f18-4616-b44f-b1dfb5926dfd · outbound

This paper cites Vacuum non-singular black hole,.

What happens to topological invariants (and black holes) in singularity-free theories? Vacuum non-singular black hole,

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.564921Z

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Observation 6220b908-403a-400f-a27e-2e47637cc20c · outbound

This paper cites Formation and evaporation of regular black holes,.

What happens to topological invariants (and black holes) in singularity-free theories? Formation and evaporation of regular black holes,

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.334650Z

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Observation eb96e8eb-4d22-447b-b049-0e669656237c · outbound

This paper cites Notes on non-singular models of black holes.

What happens to topological invariants (and black holes) in singularity-free theories? Notes on non-singular models of black holes

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.339773Z

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Observation e1d3b7b2-4b8b-4e34-99b1-600c0a9a71ed · outbound

This paper cites Note on black holes with kilometer-scale ultraviolet regulators.

What happens to topological invariants (and black holes) in singularity-free theories? Note on black holes with kilometer-scale ultraviolet regulators

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.346020Z

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Observation 2a34b8db-1441-4bc0-8d5a-e2a988f9005b · outbound

This paper cites Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics.

What happens to topological invariants (and black holes) in singularity-free theories? Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.351161Z

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Observation 2f39a584-9549-4264-b281-82598915f0e2 · outbound

This paper cites New Regular Black Hole Solution from Nonlinear Electrodynamics.

What happens to topological invariants (and black holes) in singularity-free theories? New Regular Black Hole Solution from Nonlinear Electrodynamics

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.356274Z

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Observation c927e01b-4c47-4c93-8e80-3e84228956fd · outbound

This paper cites Regular electrically charged structures in Nonlinear Electrodynamics coupled to General Relativity.

What happens to topological invariants (and black holes) in singularity-free theories? Regular electrically charged structures in Nonlinear Electrodynamics coupled to General Relativity

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.361253Z

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Observation c7994ec5-2cb5-403d-8f37-f18c5f1f27e9 · outbound

This paper cites Regular Magnetic Black Holes and Monopoles from Nonlinear Electrodynamics.

What happens to topological invariants (and black holes) in singularity-free theories? Regular Magnetic Black Holes and Monopoles from Nonlinear Electrodynamics

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.365976Z

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Observation 1d277c7e-5eed-4f39-9fc6-d5634fbc9638 · outbound

This paper cites Nonperturbative evolution equation for quantum gravity,.

What happens to topological invariants (and black holes) in singularity-free theories? Nonperturbative evolution equation for quantum gravity,

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.371865Z

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Observation 385c4fe0-090b-4445-94c2-a6ec1b0f3479 · outbound

This paper cites Renormalization group improved black hole spacetimes.

What happens to topological invariants (and black holes) in singularity-free theories? Renormalization group improved black hole spacetimes

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.376246Z

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Observation 8b4ab823-5a92-4c95-9789-929250fab66e · outbound

This paper cites Dynamical renormalization of black-hole spacetimes.

What happens to topological invariants (and black holes) in singularity-free theories? Dynamical renormalization of black-hole spacetimes

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.381065Z

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Observation 2ab2aa46-ee38-4052-bec6-2de9bdeb1da8 · outbound

This paper cites Resolving Spacetime Singularities within Asymptotic Safety.

What happens to topological invariants (and black holes) in singularity-free theories? Resolving Spacetime Singularities within Asymptotic Safety

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.386183Z

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Observation 21a96f1d-d83e-46f5-ad13-addf1e07bd61 · outbound

This paper cites Regular black hole from a confined spin connection in Poincare gauge gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Regular black hole from a confined spin connection in Poincare gauge gravity

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.391313Z

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Observation d644f8ea-f3bb-4ffa-9314-dade424f287d · outbound

This paper cites A new type of nonsingular black-hole solution in general relativity.

What happens to topological invariants (and black holes) in singularity-free theories? A new type of nonsingular black-hole solution in general relativity

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.396372Z

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Observation c33dfdcf-55ee-45c6-98d9-568fb5c67f45 · outbound

This paper cites Black-bounce to traversable wormhole.

What happens to topological invariants (and black holes) in singularity-free theories? Black-bounce to traversable wormhole

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.401780Z

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Observation 119a4319-f124-450b-98cd-b1190afde8a5 · outbound

This paper cites Non-singular "Gauss'' black hole from non-locality.

What happens to topological invariants (and black holes) in singularity-free theories? Non-singular "Gauss'' black hole from non-locality

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-08-12T18:41:00.696710Z

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Observation c9622ceb-0465-4c38-aa5a-9801962f4318 · outbound

This paper cites Diffeomorphism-invariant observables and their nonlocal algebra.

What happens to topological invariants (and black holes) in singularity-free theories? Diffeomorphism-invariant observables and their nonlocal algebra

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.412048Z

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Observation 62a17bee-01c1-4599-8146-4587560c7388 · outbound

This paper cites Quantum scattering on a delta potential in ghost-free theory.

What happens to topological invariants (and black holes) in singularity-free theories? Quantum scattering on a delta potential in ghost-free theory

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-08-12T18:41:00.652917Z

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Observation 3b347d49-0db7-4957-a685-f256f86d6d2b · outbound

This paper cites Probing the vacuum fluctuations in scalar ghost-free theories.

What happens to topological invariants (and black holes) in singularity-free theories? Probing the vacuum fluctuations in scalar ghost-free theories

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-08-12T18:41:00.629117Z

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Observation 32ac719c-ca79-4138-8417-72e0b0995983 · outbound

This paper cites Action principle selection of regular black holes.

What happens to topological invariants (and black holes) in singularity-free theories? Action principle selection of regular black holes

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.427808Z

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Observation 2f579017-3566-4daf-880c-c0755291bf73 · outbound

This paper cites Sifting quantum black holes through the principle of least action.

What happens to topological invariants (and black holes) in singularity-free theories? Sifting quantum black holes through the principle of least action

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.432890Z

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Observation baa15fe3-7401-4c55-b78a-2c49b3a812b8 · outbound

This paper cites Suppression of spacetime singularities in quantum gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Suppression of spacetime singularities in quantum gravity

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.438598Z

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Observation b1858125-1edc-4b26-b054-d98c01917f56 · outbound

This paper cites A non-local way around the no-global-symmetries conjecture in quantum gravity?.

What happens to topological invariants (and black holes) in singularity-free theories? A non-local way around the no-global-symmetries conjecture in quantum gravity?

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.444229Z

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Observation cb744c86-acb5-47f5-8f4a-058b4b793d64 · outbound

This paper cites Regular Black Holes From Pure Gravity.

What happens to topological invariants (and black holes) in singularity-free theories? Regular Black Holes From Pure Gravity

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T18:41:00.449822Z

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Observation 3cdb7af4-7b6f-442b-b738-f1e8873d6a17 · outbound

This paper cites Shift of an electron interference pat- tern by enclosed magnetic flux,.

What happens to topological invariants (and black holes) in singularity-free theories? Shift of an electron interference pat- tern by enclosed magnetic flux,

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.547314Z

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Observation 8b92bab1-03c7-41c2-b91a-f22d049171e4 · outbound

This paper cites Observation of Aharonov–Bohm ef- fect by electron holography,.

What happens to topological invariants (and black holes) in singularity-free theories? Observation of Aharonov–Bohm ef- fect by electron holography,

Reference 45

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.527931Z

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Observation 63e8e8fb-2c61-4987-918f-5ca224d908c6 · outbound

This paper cites Synthesis and Observation of Non-Abelian Gauge Fields in Real Space.

What happens to topological invariants (and black holes) in singularity-free theories? Synthesis and Observation of Non-Abelian Gauge Fields in Real Space

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-12T18:41:00.522291Z

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Observation cedf0cf6-342d-423a-a260-3b5aac50e6ae · outbound

This paper cites Observation of a gravitational Aharonov–Bohm effect,.

What happens to topological invariants (and black holes) in singularity-free theories? Observation of a gravitational Aharonov–Bohm effect,

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:41:01.510621Z

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Pith citing papers

Observation 9bc57efe-2b9d-44c8-8d7e-8db61c900783 · inbound

Carr criterion and mass gaps in non-singular primordial black hole formation cites this paper.

Carr criterion and mass gaps in non-singular primordial black hole formation What happens to topological invariants (and black holes) in singularity-free theories?

Reference 67

Resolution: verified exact; arxiv_id, observed 2026-06-29T05:53:09.009847Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation b9751b16-6a35-4c60-846c-096046377f4a · inbound

On the Meaning of Localization in Non-Local Quantum Field Theory and On the Limits of a Space-Time Description and the Physical Meaning of Phase Space in a Nonlocal Continuum cites this paper.

On the Meaning of Localization in Non-Local Quantum Field Theory and On the Limits of a Space-Time Description and the Physical Meaning of Phase Space in a Nonlocal Continuum What happens to topological invariants (and black holes) in singularity-free theories?

Reference 115

Resolution: verified exact; arxiv_id, observed 2026-07-01T18:35:58.415191Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.