Can a secluded self-interacting dark sector generate detectable gravitational waves? | Paper Citation Record

Observation e24f9ff7-a65b-4082-8924-75ca0ae0e044 · outbound

This paper cites A direct empirical proof of the existence of dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A direct empirical proof of the existence of dark matter

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Observation 01a886b9-db25-4395-886d-428b516e335d · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Planck 2018 results. VI. Cosmological parameters

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Observation 2c54e871-4bb2-4862-ba55-103374a0bbd1 · outbound

This paper cites Blumenthal, S.M.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Blumenthal, S.M

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Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.687228Z

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Observation a8080f5f-2698-40ff-a3ff-178ee8343055 · outbound

This paper cites The large-scale structure of the Universe.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The large-scale structure of the Universe

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Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.690832Z

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Observation a972e15d-732a-449d-b340-4860a94b0c3c · outbound

This paper cites Cold collapse and the core catastrophe.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cold collapse and the core catastrophe

Reference 5

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Observation 0ac65eec-e188-4d06-90b1-077fa6b56bb3 · outbound

This paper cites Moore,Evidence against dissipationless dark matter from observations of galaxy haloes, Nature 370 (1994) 629.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Moore,Evidence against dissipationless dark matter from observations of galaxy haloes, Nature 370 (1994) 629

Reference 6

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Observation cfb65b4c-d71f-408f-812d-d9cd63eee7f2 · outbound

This paper cites Observational and Theoretical Constraints on Singular Dark Matter Halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Observational and Theoretical Constraints on Singular Dark Matter Halos

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.702647Z

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Observation ee6131cc-9a06-42f1-90de-69e0888512b5 · outbound

This paper cites The unexpected diversity of dwarf galaxy rotation curves.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The unexpected diversity of dwarf galaxy rotation curves

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.706633Z

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Observation 4e810469-4a1b-49ea-92ff-88117c05d3fa · outbound

This paper cites Dark Matter Substructure in Galactic Halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Matter Substructure in Galactic Halos

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.710401Z

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Observation 2731159d-c9e2-4765-a8eb-0bbc8ad77fe2 · outbound

This paper cites Where are the missing galactic satellites?.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Where are the missing galactic satellites?

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.713858Z

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Observation c91dcda9-9e0e-412b-aca3-83a16198f202 · outbound

This paper cites The Milky Way's bright satellites as an apparent failure of LCDM.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The Milky Way's bright satellites as an apparent failure of LCDM

Reference 11

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Observation 73e0df84-2950-4e73-bcb0-009051a4b8de · outbound

This paper cites Too big to fail? The puzzling darkness of massive Milky Way subhaloes.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Too big to fail? The puzzling darkness of massive Milky Way subhaloes

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.720712Z

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Observation 8c8a0c94-c9c2-40cd-8c0a-f2d1111e775d · outbound

This paper cites A Quantitative Study of Interacting Dark Matter in Halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A Quantitative Study of Interacting Dark Matter in Halos

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.723998Z

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Observation 85403841-9ff8-4cd1-aacc-493a6416d0bd · outbound

This paper cites A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing

Reference 14

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Observation 6de79ef0-47a5-4608-bc5a-17631675dcd9 · outbound

This paper cites A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.731000Z

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Observation 086f07cc-261c-4c3d-aa47-f37ab4087b49 · outbound

This paper cites All about baryons: revisiting SIDM predictions at small halo masses.

Can a secluded self-interacting dark sector generate detectable gravitational waves? All about baryons: revisiting SIDM predictions at small halo masses

Reference 16

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Observation 8455c6bf-43df-474a-8470-7eaae2911460 · outbound

This paper cites Collisional dark matter and the structure of dark halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Collisional dark matter and the structure of dark halos

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.737706Z

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Observation f1de08ec-bb70-4042-ac23-b9e2587b4894 · outbound

This paper cites Collisional versus Collisionless Dark Matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Collisional versus Collisionless Dark Matter

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.741239Z

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Observation a69faf6e-b28d-4587-9efe-1591355b44c0 · outbound

This paper cites Constraining Self-Interacting Dark Matter with the Milky Way's dwarf spheroidals.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Constraining Self-Interacting Dark Matter with the Milky Way's dwarf spheroidals

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.744503Z

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Observation df6f9bf0-3903-4d16-ab8c-5825529c5659 · outbound

This paper cites Core Formation in Dwarf Halos with Self Interacting Dark Matter: No Fine-Tuning Necessary.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Core Formation in Dwarf Halos with Self Interacting Dark Matter: No Fine-Tuning Necessary

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.747937Z

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Observation 4dc89768-2ba3-4eaa-ab12-9cd22d795958 · outbound

This paper cites Cosmological Simulations with Self-Interacting Dark Matter I: Constant Density Cores and Substructure.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cosmological Simulations with Self-Interacting Dark Matter I: Constant Density Cores and Substructure

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.751456Z

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Observation 8b8b7d42-f9a5-40bd-9957-1489d2064570 · outbound

This paper cites Cosmological Simulations with Self-Interacting Dark Matter II: Halo Shapes vs. Observations.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cosmological Simulations with Self-Interacting Dark Matter II: Halo Shapes vs. Observations

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.754765Z

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Observation d76859cf-98b9-40b8-8bc7-7600c10644ec · outbound

This paper cites Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.758341Z

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Observation 228942d2-2f8d-4f25-b05b-7c7b53100ab2 · outbound

This paper cites Dark Matter Self-interactions and Small Scale Structure.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Matter Self-interactions and Small Scale Structure

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.761671Z

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Observation e524dd08-7451-443e-ba79-5e74366d1356 · outbound

This paper cites Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.765261Z

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Observation b7f0ed05-d76f-4638-8fd2-4f80e4855818 · outbound

This paper cites Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.768818Z

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Observation 71f98f64-54ad-424e-aa16-b46fe76ce28f · outbound

This paper cites Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.772352Z

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Observation 02e5fa6c-be7f-4e38-b9b1-46e44bcf0556 · outbound

This paper cites Robertson, D.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Robertson, D

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Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.775794Z

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Observation 204563fc-a463-456d-a2f2-30cbfcd0a733 · outbound

This paper cites Observational evidence for self-interacting cold dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Observational evidence for self-interacting cold dark matter

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.778983Z

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Observation 215408fc-0d78-452f-a2c5-099d6ceb4d96 · outbound

This paper cites Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.782744Z

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Observation fa2c23ab-f08a-4539-a281-45c2c3cf3725 · outbound

This paper cites Subhaloes in Self-Interacting Galactic Dark Matter Haloes.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Subhaloes in Self-Interacting Galactic Dark Matter Haloes

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.786271Z

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Observation f4bce321-a5b4-4721-bd13-9840d0028123 · outbound

This paper cites The non-gravitational interactions of dark matter in colliding galaxy clusters.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The non-gravitational interactions of dark matter in colliding galaxy clusters

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.789831Z

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Observation 0aa45aed-d243-4eb2-8a87-85221db705b6 · outbound

This paper cites The structure and evolution of weakly self-interacting cold dark matter halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The structure and evolution of weakly self-interacting cold dark matter halos

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.793299Z

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Observation d1deed5c-0c3b-4fa5-8827-dab6f5f6718d · outbound

This paper cites Velocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Velocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.796792Z

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Observation da0a3dc5-254f-4015-8223-8d5850b54989 · outbound

This paper cites Weakly Self-Interacting Dark Matter and the Structure of Dark Halos.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Weakly Self-Interacting Dark Matter and the Structure of Dark Halos

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.800634Z

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Observation de4b6585-5236-41e0-8cff-a4be082b08f0 · outbound

This paper cites Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.803847Z

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Observation 20528d0e-f6bc-4bc4-875c-af7aaad1b4b4 · outbound

This paper cites Self-interacting hidden sector dark matter, small scale galaxy structure anomalies, and a dark force.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting hidden sector dark matter, small scale galaxy structure anomalies, and a dark force

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.807409Z

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Observation ef5df3b5-ed6e-4cfa-b2cb-04f8b0d92559 · outbound

This paper cites The Effective Theory of Self-Interacting Dark Matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The Effective Theory of Self-Interacting Dark Matter

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.810857Z

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Observation f9de5cdb-58cb-48f8-bbf6-37717ec7779c · outbound

This paper cites SIMPle Dark Matter: Self-Interactions and keV Lines.

Can a secluded self-interacting dark sector generate detectable gravitational waves? SIMPle Dark Matter: Self-Interactions and keV Lines

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.815122Z

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Observation 83065af8-e46d-4beb-aea6-8257b81290c6 · outbound

This paper cites Tight bonds between sterile neutrinos and dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Tight bonds between sterile neutrinos and dark matter

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.818758Z

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Observation b3aeb153-674f-4523-98c2-5171d1785bd8 · outbound

This paper cites Dark Matter Self-Interactions and Light Force Carriers.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Matter Self-Interactions and Light Force Carriers

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.822096Z

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Observation 7cbc51f6-0759-4b9f-bce4-96111b46a443 · outbound

This paper cites Asymmetric dark matter with a spontaneously broken $U(1)'$: self-interaction and gravitational waves.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Asymmetric dark matter with a spontaneously broken $U(1)'$: self-interaction and gravitational waves

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.825654Z

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Observation 4753cb31-1c76-4d39-b0f1-1e5524508d65 · outbound

This paper cites Self-interacting dark matter with a stable vector mediator.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting dark matter with a stable vector mediator

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.829208Z

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Observation 297595f6-8a5b-48d8-8309-1bb28afa9c68 · outbound

This paper cites Halo Shape and Relic Density Exclusions of Sommerfeld-Enhanced Dark Matter Explanations of Cosmic Ray Excesses.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Halo Shape and Relic Density Exclusions of Sommerfeld-Enhanced Dark Matter Explanations of Cosmic Ray Excesses

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.832973Z

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Observation 8c7d291e-7055-47ce-b9b2-1d4d847fb04c · outbound

This paper cites Hidden Charged Dark Matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Hidden Charged Dark Matter

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.836636Z

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Observation 39c863ca-aa9a-4265-8b73-c1d10bcca88d · outbound

This paper cites Diurnal modulation signal from dissipative hidden sector dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Diurnal modulation signal from dissipative hidden sector dark matter

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.840401Z

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Observation ee2021d8-40c7-4660-a303-5aaa4e2776fe · outbound

This paper cites Dissipative hidden sector dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dissipative hidden sector dark matter

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.844033Z

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Observation fd52a69d-0eb7-471f-9fc8-4035ed259e7d · outbound

This paper cites Solving the small-scale structure puzzles with dissipative dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Solving the small-scale structure puzzles with dissipative dark matter

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.847593Z

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Observation 1ef1931c-0b0e-43c0-91ea-797a961ad4f9 · outbound

This paper cites Self-interacting dark matter and cosmology of a light scalar mediator.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting dark matter and cosmology of a light scalar mediator

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.850946Z

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Observation 3a0a79b9-73a1-45b2-a142-f216e88fca63 · outbound

This paper cites Self-interacting dark matter with a vector mediator: kinetic mixing with U(1)$_{(B-L)_3}$ gauge boson.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting dark matter with a vector mediator: kinetic mixing with U(1)$_{(B-L)_3}$ gauge boson

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.854485Z

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Observation fe409658-8fac-4cd7-a5d6-fd2823570ef3 · outbound

This paper cites Self-interacting dark matter and muon $g-2$ in a gauged U$(1)_{L_{\mu} - L_{\tau}}$ model.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting dark matter and muon $g-2$ in a gauged U$(1)_{L_{\mu} - L_{\tau}}$ model

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.857835Z

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Observation d3e14dad-5d0c-4c81-84a2-e1c0cd93c369 · outbound

This paper cites Unification of the Standard Model and Dark Matter Sectors in [SU(5)$\times$U(1)]$^4$.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Unification of the Standard Model and Dark Matter Sectors in [SU(5)$\times$U(1)]$^4$

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.861339Z

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Observation 1da82483-5e5a-434c-b99c-bec848937dc4 · outbound

This paper cites Unification for the Darkly Charged Dark Matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Unification for the Darkly Charged Dark Matter

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.864814Z

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Observation 284ee23a-3f15-407b-87ba-8a2bdcb2de56 · outbound

This paper cites Maximally self-interacting dark matter: models and predictions.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Maximally self-interacting dark matter: models and predictions

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.868350Z

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Observation 5effa59f-4204-40f3-8105-f13ce23c9413 · outbound

This paper cites View FImP Miracle (by Scale Invariance) $\acute{\rm a}$ $\rm la$ Self-interaction.

Can a secluded self-interacting dark sector generate detectable gravitational waves? View FImP Miracle (by Scale Invariance) $\acute{\rm a}$ $\rm la$ Self-interaction

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.872187Z

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Observation a3f08bcc-ddf1-4959-997e-118cb7965782 · outbound

This paper cites Protophobic Light Vector Boson as a Mediator to the Dark Sector.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Protophobic Light Vector Boson as a Mediator to the Dark Sector

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.875673Z

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Observation bea04269-bb3e-4c70-9b69-a37561d91edc · outbound

This paper cites $\nu \Lambda$MDM: A Model for Sterile Neutrino and Dark Matter Reconciles Cosmological and Neutrino Oscillation Data after BICEP2.

Can a secluded self-interacting dark sector generate detectable gravitational waves? $\nu \Lambda$MDM: A Model for Sterile Neutrino and Dark Matter Reconciles Cosmological and Neutrino Oscillation Data after BICEP2

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.879133Z

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Observation f536486e-2960-4916-b2df-49c5226679e8 · outbound

This paper cites Self-interacting scalar dark matter with local $Z_{3}$ symmetry.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting scalar dark matter with local $Z_{3}$ symmetry

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.882717Z

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Observation 3cbe5f18-34e8-48d2-90a6-3616d8b26c15 · outbound

This paper cites Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.886072Z

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Observation ea2b5e8d-aff7-4e2b-a8ef-bafa8eff0332 · outbound

This paper cites Inception of Self-Interacting Dark Matter with Dark Charge Conjugation Symmetry.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Inception of Self-Interacting Dark Matter with Dark Charge Conjugation Symmetry

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.889459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95871d9a-e889-47fa-9652-d2e3ea3a2ed6 · outbound

This paper cites Self-Scattering for Dark Matter with an Excited State.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-Scattering for Dark Matter with an Excited State

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.893167Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6317f272-3076-4205-8c5a-3a49f7482136 · outbound

This paper cites Resonant Dark Forces and Small Scale Structure.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Resonant Dark Forces and Small Scale Structure

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.896543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation add026aa-6d4f-4110-b3a9-e5ccaafee456 · outbound

This paper cites Beyond Collisionless Dark Matter: Particle Physics Dynamics for Dark Matter Halo Structure.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Beyond Collisionless Dark Matter: Particle Physics Dynamics for Dark Matter Halo Structure

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.900324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3ebda60-63b2-42c0-8d44-f76c7e200bd6 · outbound

This paper cites Is dark matter with long-range interactions a solution to all small-scale problems of \Lambda CDM cosmology?.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Is dark matter with long-range interactions a solution to all small-scale problems of \Lambda CDM cosmology?

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.903856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3c57207-c041-4133-a80f-8df400345848 · outbound

This paper cites Higgs exotic decays in general NMSSM with self-interacting dark matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Higgs exotic decays in general NMSSM with self-interacting dark matter

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.907420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b37a9cc-0d7e-4629-9fcb-d32f767a7052 · outbound

This paper cites Updated BBN constraints on electromagnetic decays of MeV-scale particles.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Updated BBN constraints on electromagnetic decays of MeV-scale particles

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.910942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ce89b31-570f-4e5e-a4ce-e9fe1bd325f5 · outbound

This paper cites BBN constraints on MeV-scale dark sectors. Part II. Electromagnetic decays.

Can a secluded self-interacting dark sector generate detectable gravitational waves? BBN constraints on MeV-scale dark sectors. Part II. Electromagnetic decays

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.914477Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d003e909-0cde-4a06-8c88-4dec675ecb10 · outbound

This paper cites Cosmological Constraints on Dark Scalar.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cosmological Constraints on Dark Scalar

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.917878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09cdfc64-f5f0-4864-b66f-3ea8c9881c39 · outbound

This paper cites Hubble Tension and Cosmological Imprints of $U(1)_X$ Gauge Symmetry: $U(1)_{B_3-3 L_i}$ as a case study.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Hubble Tension and Cosmological Imprints of $U(1)_X$ Gauge Symmetry: $U(1)_{B_3-3 L_i}$ as a case study

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.921401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 36b43c14-d2bf-4899-906a-6f0987d886f6 · outbound

This paper cites The $N_{\rm eff}$ at CMB challenges $U(1)_X$ light gauge boson scenarios.

Can a secluded self-interacting dark sector generate detectable gravitational waves? The $N_{\rm eff}$ at CMB challenges $U(1)_X$ light gauge boson scenarios

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.925062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c745a7b-8c43-4659-aa7b-0d846c06b347 · outbound

This paper cites Revisiting Supernova 1987A Constraints on Dark Photons.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Revisiting Supernova 1987A Constraints on Dark Photons

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.929009Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6ba12ac-d7ce-4743-b950-a516f14d4ca6 · outbound

This paper cites Cooling the Shock: New Supernova Constraints on Dark Photons.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cooling the Shock: New Supernova Constraints on Dark Photons

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.932722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7805547-0a22-450a-bea4-9cbf477cb28c · outbound

This paper cites Direct Detection Signatures of Self-Interacting Dark Matter with a Light Mediator.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Direct Detection Signatures of Self-Interacting Dark Matter with a Light Mediator

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.936611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bb9276cf-ae5d-4152-9ba9-3ac317067b92 · outbound

This paper cites KOTO vs. NA62 Dark Scalar Searches.

Can a secluded self-interacting dark sector generate detectable gravitational waves? KOTO vs. NA62 Dark Scalar Searches

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.940294Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a485591c-36fa-42f3-86db-031058c212bb · outbound

This paper cites Asymmetric Dark Matter and Dark Radiation.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Asymmetric Dark Matter and Dark Radiation

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.943828Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d6b4efb-4736-4209-90ff-1997bfb71f2b · outbound

This paper cites Gravitational waves from dark first order phase transitions and dark photons.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Gravitational waves from dark first order phase transitions and dark photons

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.947890Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c498a650-85a4-48b7-b564-e3b01b306c18 · outbound

This paper cites NANOGrav results and Dark First Order Phase Transitions.

Can a secluded self-interacting dark sector generate detectable gravitational waves? NANOGrav results and Dark First Order Phase Transitions

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.951677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88c6ca0a-e6ce-4824-9416-52d56eed5e2a · outbound

This paper cites Dark Matter production from relativistic bubble walls.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Matter production from relativistic bubble walls

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.955314Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b5b557d-40fb-464a-8581-be1c8afb6509 · outbound

This paper cites Ultra-relativistic bubbles from the simplest Higgs portal and their cosmological consequences.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Ultra-relativistic bubbles from the simplest Higgs portal and their cosmological consequences

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.959081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f1cff9c-d167-4ac5-97a8-a25fe0697c5e · outbound

This paper cites Dark Quark Nuggets.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Quark Nuggets

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.962898Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7efc2e7-b0a3-4e3f-a33c-9096c2fcafbe · outbound

This paper cites Dark, Cold, and Noisy: Constraining Secluded Hidden Sectors with Gravitational Waves.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark, Cold, and Noisy: Constraining Secluded Hidden Sectors with Gravitational Waves

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.966774Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a6d2d38-9334-420f-87c5-9b710ab1486c · outbound

This paper cites A two-component vector WIMP -- fermion FIMP dark matter model with an extended seesaw mechanism.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A two-component vector WIMP -- fermion FIMP dark matter model with an extended seesaw mechanism

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.970660Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4db5a42f-6be8-4a7c-910b-11f83eb6580a · outbound

This paper cites A Two-Component Dark Matter Model and its Associated Gravitational Waves.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A Two-Component Dark Matter Model and its Associated Gravitational Waves

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.974327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ed1feb9-2f00-404e-998d-e9c3a033df2f · outbound

This paper cites Sensitivity to Dark Sector Scales from Gravitational Wave Signatures.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Sensitivity to Dark Sector Scales from Gravitational Wave Signatures

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.977995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c3915b7-b7bf-4b90-b7c3-7698f2c24c5d · outbound

This paper cites Hearing without seeing: gravitational waves from hot and cold hidden sectors.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Hearing without seeing: gravitational waves from hot and cold hidden sectors

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.981939Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ff0844d5-4afa-44a7-8a0f-7930e7de6325 · outbound

This paper cites Electroweak Phase Transition with an SU(2) Dark Sector.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Electroweak Phase Transition with an SU(2) Dark Sector

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.985386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1165d42e-e7a5-4485-9166-4da6ce244775 · outbound

This paper cites Self-interacting dark matter implied by nano-Hertz gravitational waves.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Self-interacting dark matter implied by nano-Hertz gravitational waves

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.989469Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 874de430-c311-40b7-ba72-274a2ff3e987 · outbound

This paper cites Gravitational waves from first order electroweak phase transition in models with the $U(1)_X^{}$ gauge symmetry.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Gravitational waves from first order electroweak phase transition in models with the $U(1)_X^{}$ gauge symmetry

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.992986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2f00dc71-42f9-4dc9-9445-bf27abb22d73 · outbound

This paper cites Explore Inert Dark Matter Blind Spots with Gravitational Wave Signatures.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Explore Inert Dark Matter Blind Spots with Gravitational Wave Signatures

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.996333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b4ec068e-8308-4647-9407-e529ede130ac · outbound

This paper cites Hearing the signals of dark sectors with gravitational wave detectors.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Hearing the signals of dark sectors with gravitational wave detectors

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.999955Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95c329c2-2058-4343-9dbb-c208e554e1eb · outbound

This paper cites Whispers from the dark side: Confronting light new physics with NANOGrav data.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Whispers from the dark side: Confronting light new physics with NANOGrav data

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.003705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68796912-2bad-4e3d-97c0-bbd656d9b268 · outbound

This paper cites Gravitational Waves From a Dark (Twin) Phase Transition.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Gravitational Waves From a Dark (Twin) Phase Transition

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.007224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 47778696-920c-4f4e-af5e-4ecde17422ff · outbound

This paper cites Gravitational Waves From SU(N) Glueball Dark Matter.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Gravitational Waves From SU(N) Glueball Dark Matter

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.011068Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c3eca19-e506-4d75-bcd4-bf3b3387e9a7 · outbound

This paper cites Gravitational wave from dark sector with dark pion.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Gravitational wave from dark sector with dark pion

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.014807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c39d5fb-3d2f-40ad-a1ca-4d660af8300a · outbound

This paper cites A hidden self-interacting dark matter sector with first order cosmological phase transition and gravitational wave.

Can a secluded self-interacting dark sector generate detectable gravitational waves? A hidden self-interacting dark matter sector with first order cosmological phase transition and gravitational wave

Reference 95

Resolution: verified exact; local_arxiv, observed 2026-08-08T23:34:36.390205Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c81fdd01-5ef7-44f3-ba43-45d1ab004f47 · outbound

This paper cites Cosmological phase transitions, gravitational waves and self-interacting dark matter in the singlet extension of MSSM.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Cosmological phase transitions, gravitational waves and self-interacting dark matter in the singlet extension of MSSM

Reference 96

Resolution: verified exact; local_arxiv, observed 2026-08-08T23:34:36.375327Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 275f923e-3cd7-4b00-93ff-d045d72fedd2 · outbound

This paper cites Witten,Cosmic Separation of Phases, Phys.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Witten,Cosmic Separation of Phases, Phys

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.025897Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b11583c3-fb09-40a9-ae95-08e2d4607e73 · outbound

This paper cites Dark Chiral Phase Transition Driven by Chemical Potential and its Gravitational Wave Test.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Chiral Phase Transition Driven by Chemical Potential and its Gravitational Wave Test

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.029123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d67c97e4-e68b-4316-9053-d6b5ab9f2ab3 · outbound

This paper cites Costa, J.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Costa, J

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.033071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4868b6e-e3fa-4c66-8285-99940621932e · outbound

This paper cites Supercooled phase transitions in conformal dark sectors explain NANOGrav data.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Supercooled phase transitions in conformal dark sectors explain NANOGrav data

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:35.036451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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