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Paper Citation Record · LEDGER

Radiating black holes in general relativity need not be singular

As of 28 July 2026, this Paper Citation Record lists 31 of 31 outbound references and 1 inbound Pith citation observation for arXiv:2510.20649.

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

pith.paper-citation-record.v1
2510.20649 v2

Coverage vector

measured 31 of 31 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-18T04:32:12.428999Z

measured 32 of 32 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-07-28T06:31:03.373048+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T23:03:04.569859Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

31 of 31 outbound references displayed

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  • verified fuzzy10
  • unresolved0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 173c5b73-b4b1-4109-9157-dca8f5b70b33 · outbound

This paper cites Gravitational collapse and space-time singularities.

Radiating black holes in general relativity need not be singular Gravitational collapse and space-time singularities

Reference 1

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Observation 67f7313e-ef35-41f4-ac32-822517e58c23 · outbound

This paper cites Poisson, A Relativist’s Toolkit: The Mathematics of Black-Hole Mechanics.

Radiating black holes in general relativity need not be singular Poisson, A Relativist’s Toolkit: The Mathematics of Black-Hole Mechanics

Reference 2

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Observation a378ae4c-3d92-4bc8-b601-6c707897899c · outbound

This paper cites The Singularities of gravitational collapse and cosmology.

Radiating black holes in general relativity need not be singular The Singularities of gravitational collapse and cosmology

Reference 3

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Observation 96302b7b-116e-446d-bf40-1912025f9e1e · outbound

This paper cites an unresolved cited work.

Radiating black holes in general relativity need not be singular Unresolved cited work

Reference 4

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Observation b323996b-cd18-4eb5-bdbe-ac5274ed9dab · outbound

This paper cites Singularity Theorems and Their Consequences.

Radiating black holes in general relativity need not be singular Singularity Theorems and Their Consequences

Reference 5

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Observation 333563a4-87a3-48aa-a99c-d6a2e855e900 · outbound

This paper cites Towards a Non-singular Paradigm of Black Hole Physics.

Radiating black holes in general relativity need not be singular Towards a Non-singular Paradigm of Black Hole Physics

Reference 6

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arxiv_id, observed 2026-05-18T04:32:22.955243Z

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Observation 14b934ba-1dce-4b21-8295-4d024ab7990d · outbound

This paper cites Black hole explosions.

Radiating black holes in general relativity need not be singular Black hole explosions

Reference 7

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Observation a8d123b5-5ede-46b7-aacd-6c5f1043239a · outbound

This paper cites Particle Creation by Black Holes.

Radiating black holes in general relativity need not be singular Particle Creation by Black Holes

Reference 8

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation ecb18fef-3610-477e-91a9-d54f462f8628 · outbound

This paper cites On continued gravitational contraction.

Radiating black holes in general relativity need not be singular On continued gravitational contraction

Reference 9

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation 3030bf83-e948-48f4-ba78-dd976d788ea4 · outbound

This paper cites Israel, Event horizons in static vacuum space-times , Phys.

Radiating black holes in general relativity need not be singular Israel, Event horizons in static vacuum space-times , Phys

Reference 10

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Observation 03152fe7-3371-4437-8d4a-3d8cd73d36bd · outbound

This paper cites Geodesically complete black holes.

Radiating black holes in general relativity need not be singular Geodesically complete black holes

Reference 11

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Observation 0706d696-d3d2-4cb7-8da8-64ac716cd722 · outbound

This paper cites Event horizons in static electrovac space-times.

Radiating black holes in general relativity need not be singular Event horizons in static electrovac space-times

Reference 12

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation 71659486-5e8a-41ae-bc0e-fedc41abda16 · outbound

This paper cites Gravitational bounce.

Radiating black holes in general relativity need not be singular Gravitational bounce

Reference 13

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Observation 86c72bb1-f78f-464d-902b-d0d49fd204a6 · outbound

This paper cites Hydrostatic equilibrium and gravitational collapse of relativistic charged fluid balls.

Radiating black holes in general relativity need not be singular Hydrostatic equilibrium and gravitational collapse of relativistic charged fluid balls

Reference 14

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Observation 70830966-9ef1-47ed-8b5a-4b8081aaeb1f · outbound

This paper cites General Laws of Black-Hole Dynamics.

Radiating black holes in general relativity need not be singular General Laws of Black-Hole Dynamics

Reference 15

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Observation 665df536-5b9c-4c2f-8585-0bd6c18136f7 · outbound

This paper cites Isolated and dynamical horizons and their applications.

Radiating black holes in general relativity need not be singular Isolated and dynamical horizons and their applications

Reference 16

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Observation 9946a6c9-5bde-44a9-9758-337f8579fb1f · outbound

This paper cites Evaporation of near-extremal Reissner-Nordstrom black holes.

Radiating black holes in general relativity need not be singular Evaporation of near-extremal Reissner-Nordstrom black holes

Reference 17

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Observation 9af58537-0190-46c6-96cc-d4314234ce47 · outbound

This paper cites Formation and Evaporation of Charged Black Holes.

Radiating black holes in general relativity need not be singular Formation and Evaporation of Charged Black Holes

Reference 18

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Observation 9d287c56-fc2d-4051-a1e7-4c06a5a801e5 · outbound

This paper cites Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime.

Radiating black holes in general relativity need not be singular Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime

Reference 19

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Observation 66795082-c2e6-4d12-b414-efbc8c5d0235 · outbound

This paper cites On the viability of regular black holes.

Radiating black holes in general relativity need not be singular On the viability of regular black holes

Reference 20

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Observation 06aa7efb-a695-4e6c-8972-cf5a2e73eff9 · outbound

This paper cites Black hole inner horizon evaporation in semiclassical gravity.

Radiating black holes in general relativity need not be singular Black hole inner horizon evaporation in semiclassical gravity

Reference 21

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Observation f75ae056-b2e9-489a-af54-99166e48c518 · outbound

This paper cites Classical mass inflation vs semiclassical inner horizon inflation.

Radiating black holes in general relativity need not be singular Classical mass inflation vs semiclassical inner horizon inflation

Reference 22

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Observation 0b6e9815-d94b-414d-a403-21fcff8d1829 · outbound

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

Radiating black holes in general relativity need not be singular Inner-horizon instability and mass inflation in black holes

Reference 23

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Observation 39d1f3bc-0774-40f4-a66c-6b7b098e773c · outbound

This paper cites Internal structure of black holes.

Radiating black holes in general relativity need not be singular Internal structure of black holes

Reference 24

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Observation cb9a0f25-03fa-46bb-b269-03b7200a2b5f · outbound

This paper cites Mass inflation without Cauchy horizons.

Radiating black holes in general relativity need not be singular Mass inflation without Cauchy horizons

Reference 25

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Observation a8c4d148-bcae-4d9a-916b-f6f0318b41ee · outbound

This paper cites Semiclassical evolution of a dynamically formed spherical black hole with an inner horizon.

Radiating black holes in general relativity need not be singular Semiclassical evolution of a dynamically formed spherical black hole with an inner horizon

Reference 26

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation 5c018456-a07a-4a49-ba8b-4dc71798d829 · outbound

This paper cites The disinformation problem for black holes (conference version).

Radiating black holes in general relativity need not be singular The disinformation problem for black holes (conference version)

Reference 27

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation 31ac55d4-fa24-430a-943d-65fe7f72d7a7 · outbound

This paper cites The information paradox: A pedagogical introduction.

Radiating black holes in general relativity need not be singular The information paradox: A pedagogical introduction

Reference 28

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation 1d02957e-7a65-4a25-ab08-f523fd6a1456 · outbound

This paper cites The entropy of hawking radiation.

Radiating black holes in general relativity need not be singular The entropy of hawking radiation

Reference 29

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Observation abc76aab-d81a-4074-89a5-6f4a11ac86f5 · outbound

This paper cites On the assumptions leading to the information loss paradox.

Radiating black holes in general relativity need not be singular On the assumptions leading to the information loss paradox

Reference 30

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Radiating black holes in general relativity need not be singular Can black holes evaporate past extremality?

Reference 31

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No event found in the named queried sources as of 2026-07-28T06:31:03.373048+00:00.

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Pith citing papers

Observation bcb5a9fb-8073-4450-b849-8219c968f1fc · inbound

Semiclassical regularity of compact trapped regions: From dynamical horizons to inner extremality cites this paper.

Semiclassical regularity of compact trapped regions: From dynamical horizons to inner extremality Radiating black holes in general relativity need not be singular

Reference 40

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no resolver link, observed 2026-07-11T23:03:04.569859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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