An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole | Paper Citation Record

Observation 74abb4a2-3259-4be2-b2ab-e018049a5718 · outbound

This paper cites The exterior region [r > R(t)] remains Schwarzschild vacuum.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole The exterior region [r > R(t)] remains Schwarzschild vacuum

Reference 1

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 2

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This paper cites [35], the system evolves toward a Schwarzschild BH with massM=h/2 ast→t d, wheret d =∞in Ref.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole [35], the system evolves toward a Schwarzschild BH with massM=h/2 ast→t d, wheret d =∞in Ref

Reference 3

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 4

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Observation 685d637d-a997-4c33-9dda-ca0f7b40ab9d · outbound

This paper cites Only the Schwarzschild BH remains att≥t d.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Only the Schwarzschild BH remains att≥t d

Reference 5

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This paper cites c9ZiMvMg0DUbBAGjp/NKq249i4s=.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole c9ZiMvMg0DUbBAGjp/NKq249i4s=

Reference 6

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Observation 8e161e60-d769-4e8d-b1ff-c5e7173881f1 · outbound

This paper cites Form(r, t), we take the simplest functionf(x) =f 0(x) in Eq.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Form(r, t), we take the simplest functionf(x) =f 0(x) in Eq

Reference 7

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 8

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This paper cites Since the EMT vanishes atX(r, t)>1, the EMT should also vanish atX(r, t) = 1.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Since the EMT vanishes atX(r, t)>1, the EMT should also vanish atX(r, t) = 1

Reference 9

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 10

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 11

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Observation 78b0cac2-350d-4bb2-a99b-4bbf58c8305d · outbound

This paper cites 9KjgRmm+HN3wAXOHAP9YIhnOIuk=.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole 9KjgRmm+HN3wAXOHAP9YIhnOIuk=

Reference 12

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This paper cites 2 showsm(r, t) atβ= 2 as a function ofr for several values oftduring a whole process of the collapse att a ≤t≤t d.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole 2 showsm(r, t) atβ= 2 as a function ofr for several values oftduring a whole process of the collapse att a ≤t≤t d

Reference 13

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 14

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This paper cites Furthermore, the above condition is satisfied asr→0.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Furthermore, the above condition is satisfied asr→0

Reference 15

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This paper cites At the negativet(t a ≤t <0), however, we have lim X→0 −κr4C hX(1−X) =−β(β+ 1) =−6,(A17) so that the SEC is violated in this limit.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole At the negativet(t a ≤t <0), however, we have lim X→0 −κr4C hX(1−X) =−β(β+ 1) =−6,(A17) so that the SEC is violated in this limit

Reference 16

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 17

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Observation 365fa6d4-570e-4932-bfc9-cd22bacc4c7b · outbound

This paper cites Bondi, Mon.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Bondi, Mon

Reference 18

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Observation 839c370b-3bad-4ba5-a262-a58c7dd166b6 · outbound

This paper cites Christodoulou, Commun.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Christodoulou, Commun

Reference 19

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This paper cites Naked Singularities in Spherically Symmetric Inhomogeneous Tolman-Bondi Dust Cloud Collapse.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Naked Singularities in Spherically Symmetric Inhomogeneous Tolman-Bondi Dust Cloud Collapse

Reference 20

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Observation 50308320-fb44-4cec-bc9d-3550c77c2a84 · outbound

This paper cites Shibata, Prog.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Shibata, Prog

Reference 21

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This paper cites Why do naked singularities form in gravitational collapse?.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Why do naked singularities form in gravitational collapse?

Reference 22

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This paper cites Gravitational collapse of barotropic spherical fluids.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Gravitational collapse of barotropic spherical fluids

Reference 23

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This paper cites Black hole formation in perfect fluid collapse.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Black hole formation in perfect fluid collapse

Reference 24

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Observation bc99435a-7000-4fdd-9c8c-574a59fc3c31 · outbound

This paper cites Generalized Lemaitre-Tolman-Bondi Solutions with Pressure.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Generalized Lemaitre-Tolman-Bondi Solutions with Pressure

Reference 25

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This paper cites Strong curvature naked singularities in spherically symmetric perfect fluid collapse.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Strong curvature naked singularities in spherically symmetric perfect fluid collapse

Reference 26

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This paper cites Towards consistent black-to-white hole bounces from matter collapse.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Towards consistent black-to-white hole bounces from matter collapse

Reference 27

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This paper cites Recent developments in gravitational collapse and spacetime singularities.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Recent developments in gravitational collapse and spacetime singularities

Reference 28

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Observation 1d351893-bc38-4b04-974a-4b8fb908a43f · outbound

This paper cites Quantum gravitational collapse: non-singularity and non-locality.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Quantum gravitational collapse: non-singularity and non-locality

Reference 29

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This paper cites Schrodinger formalism, black hole horizons and singularity behavior.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Schrodinger formalism, black hole horizons and singularity behavior

Reference 30

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This paper cites Singularity avoidance for collapsing quantum dust in the Lemaitre-Tolman-Bondi model.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Singularity avoidance for collapsing quantum dust in the Lemaitre-Tolman-Bondi model

Reference 31

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This paper cites Black hole singularity resolution via the modified Raychaudhuri equation in loop quantum gravity.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Black hole singularity resolution via the modified Raychaudhuri equation in loop quantum gravity

Reference 32

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This paper cites Quantum Oppenheimer-Snyder model.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Quantum Oppenheimer-Snyder model

Reference 33

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This paper cites Black hole collapse and bounce in effective loop quantum gravity.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Black hole collapse and bounce in effective loop quantum gravity

Reference 34

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This paper cites Quantum gravity of dust collapse: shock waves from black holes.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Quantum gravity of dust collapse: shock waves from black holes

Reference 35

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This paper cites On the fate of quantum black holes.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole On the fate of quantum black holes

Reference 36

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This paper cites Configurational entropy of black hole quantum cores.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Configurational entropy of black hole quantum cores

Reference 37

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This paper cites Gravitational collapse in effective loop quantum gravity: beyond marginally bound configurations.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Gravitational collapse in effective loop quantum gravity: beyond marginally bound configurations

Reference 38

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This paper cites On gravitational collapse and integrable singularities.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole On gravitational collapse and integrable singularities

Reference 39

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Observation 2aca7f79-b1e7-4eed-8059-fb6cc233aa0b · outbound

This paper cites Penrose, Phys.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Penrose, Phys

Reference 40

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Observation 328ce03e-a175-4aa6-9483-5028a6a70f25 · outbound

This paper cites First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

Reference 41

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Observation 4777475e-b04f-454e-9326-be6e8453e0f9 · outbound

This paper cites First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

Reference 42

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Observation 5db5a79d-6000-437b-a9af-ed86922be574 · outbound

This paper cites Poisson and W.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Poisson and W

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.377341Z

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This paper cites Poisson and W.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Poisson and W

Reference 44

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Observation 5c639665-fa33-4263-b1d7-fba6cfd51d12 · outbound

This paper cites Penrose, Riv.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Penrose, Riv

Reference 45

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Observation 174cf12f-fb2a-445e-9f4e-005cf636f182 · outbound

This paper cites Penrose, inGeneral Relativity: An Einstein Cente- nary Survey, edited by S.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Penrose, inGeneral Relativity: An Einstein Cente- nary Survey, edited by S

Reference 46

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.365767Z

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An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 47

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Observation 694eab22-4310-427f-b6b1-c18e77a222d4 · outbound

This paper cites Ovalle, Phys.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Ovalle, Phys

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.352221Z

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Observation e1eb82ca-5f83-4b1d-b534-5959384b57e1 · outbound

This paper cites Interior Dynamics of Regular Schwarzschild Black Holes.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Interior Dynamics of Regular Schwarzschild Black Holes

Reference 49

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Observation 4d131080-25ff-4799-99b7-4c08c411eaad · outbound

This paper cites OnSchwarzschildblackholesingularityformation.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole OnSchwarzschildblackholesingularityformation

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-07-10T13:27:05.984594Z

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Observation 09eda059-56aa-44ea-981a-e8afeba46948 · outbound

This paper cites Aoki and J.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Aoki and J

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.357491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 2f69203d-dd45-424f-8401-01b14572338a · outbound

This paper cites Casadio, A.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Casadio, A

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.345629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 304e7bd6-59ef-495d-8b56-792559e70064 · outbound

This paper cites Casadio, A.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Casadio, A

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.347877Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 36964c16-605a-486f-8972-2205c29e3d82 · outbound

This paper cites Space-Times with Integrable Singularity.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Space-Times with Integrable Singularity

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:05.969382Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation b572b970-06e9-4be1-a222-d355bff8c7b3 · outbound

This paper cites Ovalle, Phys.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Ovalle, Phys

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.349817Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation b48c5fb7-c369-42e8-bbab-b6fe9b0428cb · outbound

This paper cites Arrechea, S.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Arrechea, S

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.355188Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 8163e120-a8d9-4834-818c-0dd9c17dae67 · outbound

This paper cites Schwarzschild, Sitzungsber.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Schwarzschild, Sitzungsber

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.375620Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 86361e1b-56e1-407a-a615-cf441bebf2f7 · outbound

This paper cites Charge Conservation, Entropy Current, and Gravitation.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Charge Conservation, Entropy Current, and Gravitation

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:06.007844Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation c3dc2612-881c-4309-b2d0-5c6b79a668d7 · outbound

This paper cites Conserved non-Noether charge in general relativity: Physical definition vs. Noether's 2nd theorem.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Conserved non-Noether charge in general relativity: Physical definition vs. Noether's 2nd theorem

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:05.972302Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 6133257c-d8d5-4cd8-88b0-1cec90a95a93 · outbound

This paper cites Conserved charges in general relativity.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Conserved charges in general relativity

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:05.999641Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation d2657aae-5ef6-4e3a-a142-fe11bb3085e7 · outbound

This paper cites Generic Naked Singularities in Vaidya Spacetimes.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Generic Naked Singularities in Vaidya Spacetimes

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:06.010419Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation a3488fe5-b462-4960-afbd-cd5714153a28 · outbound

This paper cites Trapped surfaces in Oppenheimer-Snyder black holes.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Trapped surfaces in Oppenheimer-Snyder black holes

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:06.029404Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation d8ed060d-e29c-468f-89b5-0e43da247c95 · outbound

This paper cites Plebanski, Acta Phys.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Plebanski, Acta Phys

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-07-10T13:27:06.351989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation b468632d-83ae-4722-8c61-4f2584d6d1f5 · outbound

This paper cites an unresolved cited work.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Unresolved cited work

Reference 64

Resolution: unresolved; raw_fallback, observed 2026-07-10T13:27:06.350107Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 45cb1b09-e12b-4e94-81f4-b6918c4ec1a1 · outbound

This paper cites Classical and semi-classical energy conditions.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Classical and semi-classical energy conditions

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:05.981783Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation fb419e7f-0cd7-4b54-95ca-09e737902f14 · outbound

This paper cites Energy conditions in arbitrary dimensions.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Energy conditions in arbitrary dimensions

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:06.001149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 1f2d44e5-a86c-4779-a30f-9780381b92f9 · outbound

This paper cites Criteria for energy conditions.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Criteria for energy conditions

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:06.021122Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 9176d720-abf7-4655-97f7-e79c82365717 · outbound

This paper cites Energy conditions in static, spherically symmetric spacetimes and effective geometries.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Energy conditions in static, spherically symmetric spacetimes and effective geometries

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:05.990500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation e5b93f47-09ea-4aa7-88d0-de91d745b922 · outbound

This paper cites Families of regular spacetimes and energy conditions.

An analytic model for a total process of gravitational collapse: From star to Schwarzschild black hole Families of regular spacetimes and energy conditions

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-07-10T13:27:05.998560Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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