Paper Citation Record · LEDGER

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation

As of 9 August 2026, this Paper Citation Record lists 56 of 56 outbound references and 3 inbound Pith citation observations for arXiv:2506.06272.

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

pith.paper-citation-record.v1
2506.06272 v2

Coverage vector

measured 56 of 56 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T06:01:07.635848Z

measured 59 of 59 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T18:54:48.018973Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T08:47:13.121897Z

Reference resolution

56 of 56 outbound references displayed

verified exact0
verified fuzzy35
unresolved20
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 193daaa1-e493-47a7-b3c9-5c010cebfefb · outbound

This paper cites K., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation K., et al

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.332975Z

Source-reported events for the cited work

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Observation c1420e95-a5ef-43e6-ae75-7e858101264e · outbound

This paper cites J., Goodwin, S.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation J., Goodwin, S

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.422341Z

Source-reported events for the cited work

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Observation 6c094077-9e60-4523-8265-9b7326658284 · outbound

This paper cites S., & Garny, M.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation S., & Garny, M

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.314930Z

Source-reported events for the cited work

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Observation d01d2c3d-f3a9-4c70-92d3-9fa0408137d8 · outbound

This paper cites Y ., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Y ., et al

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.303783Z

Source-reported events for the cited work

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Observation a83ec48d-4991-4273-a43a-953213b6b3d8 · outbound

This paper cites W., Price-Whelan, A.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation W., Price-Whelan, A

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.436716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9248465-88d1-45ad-b012-c2dc57b2763f · outbound

This paper cites 1952, MNRAS, 112, 195.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 1952, MNRAS, 112, 195

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.441277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 54cf8158-0980-40ae-b9a6-887a77cd3995 · outbound

This paper cites W., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation W., et al

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.278424Z

Source-reported events for the cited work

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Observation 4194a223-21df-4f54-940d-5929379873ef · outbound

This paper cites 2024, Dark Matter.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2024, Dark Matter

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.268360Z

Source-reported events for the cited work

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Observation 6d6f116d-accd-46ea-99c7-f4c5c3f5099a · outbound

This paper cites A., Schaller, M., Schaye, J., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation A., Schaller, M., Schaye, J., et al

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.257969Z

Source-reported events for the cited work

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Observation 8a6f2d1f-08e5-40f0-aad9-e2cf7c7e412f · outbound

This paper cites M., Fassnacht, C.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation M., Fassnacht, C

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.246875Z

Source-reported events for the cited work

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Observation cb8c5ac1-e906-4144-bd77-6b69428e2f1c · outbound

This paper cites 2025, A&A, 697, A213.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2025, A&A, 697, A213

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.236025Z

Source-reported events for the cited work

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Observation 714c817a-284e-410f-9902-7f32ff4eadcd · outbound

This paper cites 2014, Phys.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2014, Phys

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.225032Z

Source-reported events for the cited work

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Observation 137655a1-331e-4a5b-9432-2fdd0f4cd8d6 · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 13

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:08.213956Z

Source-reported events for the cited work

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Observation d00753df-3cad-475d-a74a-d2503a4fb64b · outbound

This paper cites 2025, Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2025, Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.202353Z

Source-reported events for the cited work

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Observation c7e67e35-8acd-4e29-a80f-23835552f413 · outbound

This paper cites S., Brüggen, M., Schmidt-Hoberg, K., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation S., Brüggen, M., Schmidt-Hoberg, K., et al

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.189155Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation e747a460-cd37-4e5c-ae9e-4878b7273259 · outbound

This paper cites S., Dolag, K., & Yu, H.-B.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation S., Dolag, K., & Yu, H.-B

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.177834Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 732fb124-0f6d-464c-92a0-f9c5f455efbb · outbound

This paper cites S., Kasselmann, L., Brüggen, M., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation S., Kasselmann, L., Brüggen, M., et al

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.166773Z

Source-reported events for the cited work

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Observation b6304ebe-ca39-43ca-b8be-5d5f8bab324c · outbound

This paper cites S., & Lally, J.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation S., & Lally, J

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.155777Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 086ff9ea-3bb7-4dd3-b10d-6b9c53d49f7e · outbound

This paper cites 2022, A&A, 659, A24.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2022, A&A, 659, A24

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.144723Z

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Observation 837a38e6-c044-47a2-b9cc-d1cf393f221f · outbound

This paper cites P., Valentini, M., & Dolag, K.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation P., Valentini, M., & Dolag, K

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.494490Z

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Observation 0a069f38-0ed0-462f-a54d-6efdeb1d7f44 · outbound

This paper cites R., Millman, K.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation R., Millman, K

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.498396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 34394d52-fd5e-4e8f-841a-37ac64b12f21 · outbound

This paper cites W., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation W., et al

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.119157Z

Source-reported events for the cited work

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Observation 39c8285e-3657-41bb-b214-d6b83c3d77be · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 23

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:08.107718Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 557a9ae6-7014-4229-8da2-cf68c40d771a · outbound

This paper cites T., & Sarkar, S.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation T., & Sarkar, S

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.096813Z

Source-reported events for the cited work

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Observation 3d1ba0ec-625f-47bd-b218-7bb7914b728e · outbound

This paper cites Little Dark Dot.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Little Dark Dot

Reference 25

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.086048Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 3d1252b3-d30a-41b8-9f41-70dfa8b4ec0e · outbound

This paper cites D., Fall, S.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation D., Fall, S

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.074181Z

Source-reported events for the cited work

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Observation 2a53068c-af81-421c-bac7-44164ac6f451 · outbound

This paper cites D., Schaye, J., Schaller, M., & Richings, J.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation D., Schaye, J., Schaller, M., & Richings, J

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.062737Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 44850638-beea-4d8c-9392-71b001422f30 · outbound

This paper cites C., Peter, A.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation C., Peter, A

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.051026Z

Source-reported events for the cited work

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Observation f09b4938-749f-4ebf-8d97-226522e36798 · outbound

This paper cites 2020, Science, 369, 1347–1351.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2020, Science, 369, 1347–1351

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.039127Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 722bd87b-9b02-425d-8364-312ba89f1908 · outbound

This paper cites 2021, MNRAS, 507, 1662–1683.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2021, MNRAS, 507, 1662–1683

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:08.027057Z

Source-reported events for the cited work

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Observation 073196e8-5152-4690-89ca-2232fe9ff167 · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 31

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:08.015908Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation b17185b4-7929-4d57-a2d8-cedc077a019b · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.544275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 005a845e-0706-4dd0-9dca-521358751e7a · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 33

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:07.994728Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 476fe8f1-fdea-43c7-a353-20978748d35c · outbound

This paper cites O., Yang, D., & Yu, H.-B.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation O., Yang, D., & Yu, H.-B

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.976623Z

Source-reported events for the cited work

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Observation 6fc06b89-37af-4019-9c75-724081b5db78 · outbound

This paper cites F., Frenk, C.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation F., Frenk, C

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.555732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e1bc9ab5-2152-4571-8ea5-8fc8a75ac3f7 · outbound

This paper cites 2011, A&A, 532, A119.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2011, A&A, 532, A119

Reference 36

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.953451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 4f9a5586-e140-4b70-a893-77d720e19046 · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 37

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:07.941343Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 2d67cdb5-d2f6-451a-996e-cc5ef843d694 · outbound

This paper cites 2024, Digital Image Processing in Signatures of Self-Interacting Dark Matter Halo Mergers and Isolated Evolution.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2024, Digital Image Processing in Signatures of Self-Interacting Dark Matter Halo Mergers and Isolated Evolution

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.926999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 9919042c-fe96-4775-ba1d-90255900fc9f · outbound

This paper cites N., & Steinhardt, P.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation N., & Steinhardt, P

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.910799Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 0917e67d-4a8d-4ae4-9dc5-6e75aae0e1d8 · outbound

This paper cites 2024, A&A, 687, A270.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2024, A&A, 687, A270

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.898462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 2f0d09a7-ba84-4add-8b26-203406fe3b49 · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.577884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33388307-6fa9-41d2-84ac-08fc22fb8e21 · outbound

This paper cites 2025, Gravothermalizing into primor- dial black holes, boson stars, and cannibal stars.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2025, Gravothermalizing into primor- dial black holes, boson stars, and cannibal stars

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.880258Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 3edc9d38-d0b8-4aed-ab8a-b483d52479e5 · outbound

This paper cites 2017, MNRAS, 467, 4719.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2017, MNRAS, 467, 4719

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.868308Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 30b6e961-9415-4fdc-b206-f9e52f9f6403 · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 44

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:07.856727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 76e17c39-296a-4dd6-b16f-32b4d232c245 · outbound

This paper cites C., Torrey, P., V ogelsberger, M., & O’Neil, S.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation C., Torrey, P., V ogelsberger, M., & O’Neil, S

Reference 45

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.845851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 1e9f7dd1-ea57-4e1f-8d10-d9345bf42c57 · outbound

This paper cites M., Brüggen, M., Schmidt-Hoberg, K., & Fischer, M.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation M., Brüggen, M., Schmidt-Hoberg, K., & Fischer, M

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.598574Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 247d9d42-d54b-4187-9c53-4a7552ea8d6f · outbound

This paper cites M., Brüggen, M., Schmidt-Hoberg, K., Fischer, M.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation M., Brüggen, M., Schmidt-Hoberg, K., Fischer, M

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.834450Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 241888ee-6d30-4a8b-854e-31862c8dea91 · outbound

This paper cites V ., Wetzel, A., & Fattahi, A.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation V ., Wetzel, A., & Fattahi, A

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.605920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ebe878fa-2175-4b26-a7f5-0fd337a70f81 · outbound

This paper cites 2005, MNRAS, 364, 1105.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2005, MNRAS, 364, 1105

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.610802Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e82c18a-695a-4772-b0c4-4a009d43b4b2 · outbound

This paper cites C., Boylan-Kolchin, M., Bullock, J.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation C., Boylan-Kolchin, M., Bullock, J

Reference 50

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.805160Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 513f0356-03bc-4f47-a618-1cabb6be7831 · outbound

This paper cites M., et al.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation M., et al

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.792617Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation db02f9da-c959-4ca9-8bc2-a94daafe7b62 · outbound

This paper cites & Yu, H.-B.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation & Yu, H.-B

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T06:01:07.621405Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7ac6416-33c0-455c-bf5a-c858781bf0ba · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 53

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:07.773336Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 8867fbaa-3cbc-4218-9966-4597909f4fa2 · outbound

This paper cites an unresolved cited work.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation Unresolved cited work

Reference 54

Resolution: unresolved; raw_fallback, observed 2026-08-07T06:01:07.761444Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation c6d83c71-9c70-4992-b6d2-080d27d4417b · outbound

This paper cites & Yu, H.-B.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation & Yu, H.-B

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T06:01:07.749791Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 7e0f63f2-bb7a-4cd3-88ad-1ec3df4f790b · outbound

This paper cites 2023, MNRAS, 526, 758–770 Article number, page 11 of 13 A&A proofs: manuscript no.

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation 2023, MNRAS, 526, 758–770 Article number, page 11 of 13 A&A proofs: manuscript no

Reference 56

Resolution: malformed identifier; raw_fallback, observed 2026-08-07T06:01:07.737070Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Pith citing papers

Observation b39326df-a453-4f8d-bdf2-94b11c6fc7af · inbound

Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses cites this paper.

Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-19T08:47:13.125730Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation b79b8252-703c-437d-b53a-ea3620260b1d · inbound

The dark fate of ultra-faint dwarfs: Gravothermal collapse in action cites this paper.

The dark fate of ultra-faint dwarfs: Gravothermal collapse in action To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-02T18:54:48.018973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e29387f7-579a-4f85-b10e-3050d931159f · inbound

Dynamical flattening of halo density cusps by Q-ball dark matter cites this paper.

Dynamical flattening of halo density cusps by Q-ball dark matter To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation

Reference 29

Resolution: unresolved; no resolver link, observed 2026-07-31T04:54:06.828298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.