Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-12T17:35:54.178122Z
Paper Citation Record · LEDGER
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows
As of 17 August 2026, this Paper Citation Record lists 91 of 91 outbound references and 0 inbound Pith citation observations for arXiv:2411.12462.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
91 of 91 outbound references displayed
- verified exact20
- verified fuzzy28
- unresolved35
- parse uncertain0
- malformed identifier0
- metadata mismatch8
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 72673014-bd4c-4ff0-8930-46535840d326 · outbound
This paper cites & Tremaine , S.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows & Tremaine , S
Reference 1
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2ed98672-396a-439a-aee6-20a1a062a375 · outbound
This paper cites 2020 Astrophysics of Planet Formation\/ , 2nd edn.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows 2020 Astrophysics of Planet Formation\/ , 2nd edn
Reference 2
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b3f88172-cc5d-4786-b73c-a839326ddadb · outbound
This paper cites Particle-Gas Dynamics with Athena: Method and Convergence.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Particle-Gas Dynamics with Athena: Method and Convergence
Reference 3
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation 8bcb9e2f-c3cf-409f-bba7-526722d1c385 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 4
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 056757c4-c416-4f1d-a9b2-42252e58feff · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 5
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 153458ee-60fe-4fc5-9ce7-29319930688f · outbound
This paper cites Dust Settling in Magnetorotationally-Driven Turbulent Discs I: Numerical Methods and Evidence for a Vigorous Streaming Instability.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dust Settling in Magnetorotationally-Driven Turbulent Discs I: Numerical Methods and Evidence for a Vigorous Streaming Instability
Reference 6
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 31a588bb-7d6e-44a6-bd78-48a32e0a4232 · outbound
This paper cites Hydrodynamic instability in eccentric astrophysical discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Hydrodynamic instability in eccentric astrophysical discs
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:55.029398Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 962eb6b6-ddce-4e58-9024-f57557cb08a4 · outbound
This paper cites Dust distribution in protoplanetary disks - Vertical settling and radial migration.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dust distribution in protoplanetary disks - Vertical settling and radial migration
Reference 8
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:55.005276Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 11b886c5-feb5-4289-af2e-b1de47b24c8c · outbound
This paper cites FARGO3D: A new GPU-oriented MHD code.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows FARGO3D: A new GPU-oriented MHD code
Reference 9
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7d3be53a-60be-4091-bb2a-caf8459801d8 · outbound
This paper cites Puffed up Edges of Planet-opened Gaps in Protoplanetary Disks. I. hydrodynamic simulations.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Puffed up Edges of Planet-opened Gaps in Protoplanetary Disks. I. hydrodynamic simulations
Reference 10
- Resolution
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Source-reported events for the cited work
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Observation a1c09c2f-fbcb-43ed-8bc5-ae27f9aa2a8b · outbound
This paper cites Beyond Diffusion: A Generalized Mean-Field Theory of Turbulent Dust Transport in Protoplanetary Disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Beyond Diffusion: A Generalized Mean-Field Theory of Turbulent Dust Transport in Protoplanetary Disks
Reference 11
- Resolution
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Source-reported events for the cited work
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Observation 52513a86-af43-4407-9291-b18dc4421352 · outbound
This paper cites In Akademiia Nauk SSSR Doklady\/ , , vol.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows In Akademiia Nauk SSSR Doklady\/ , , vol
Reference 12
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fdd8dbf8-8f01-4a91-b7c4-33a4618aa1f2 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 13
- Resolution
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Source-reported events for the cited work
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Observation 7b900bea-d695-4b43-9e30-ff7c9686b49d · outbound
This paper cites Modeling the delivery of dust from discs to ionized winds.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Modeling the delivery of dust from discs to ionized winds
Reference 14
- Resolution
- verified exact
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Source-reported events for the cited work
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Observation 37df7a0d-6522-4c12-8c9f-801d8688076e · outbound
This paper cites , Goldreich , P.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows , Goldreich , P
Reference 15
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50205c47-affa-4ccd-8b19-390f48d106ee · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 16
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 482c0650-2050-41c1-86b1-cf357e49c3dc · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 17
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5a5b497-cd11-4319-b28f-fc7650ecb74f · outbound
This paper cites Midplane sedimentation of large solid bodies in turbulent protoplanetary discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Midplane sedimentation of large solid bodies in turbulent protoplanetary discs
Reference 18
- Resolution
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Observation 61748bff-f177-4f10-bb2f-8b5289f805c9 · outbound
This paper cites Cambridge university press.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Cambridge university press
Reference 19
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e7ee4b93-da1a-48d5-94b3-b1f539e354f3 · outbound
This paper cites Dynamics of dust grains in turbulent molecular clouds. Conditions for decoupling and limits of different numerical implementations.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dynamics of dust grains in turbulent molecular clouds. Conditions for decoupling and limits of different numerical implementations
Reference 20
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 3a359a06-5697-4c22-bcb0-88bca7ef84c0 · outbound
This paper cites Journal of Atmospheric Sciences 20 (3), 201--208.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Journal of Atmospheric Sciences 20 (3), 201--208
Reference 21
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 30c57407-9cdd-4289-b1e2-8ae8f6eecb2f · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 22
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d49119ba-f2d5-4668-bbfb-09287ef48fe3 · outbound
This paper cites , Morfill , G.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows , Morfill , G
Reference 23
- Resolution
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Source-reported events for the cited work
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Observation 7171a0fd-e065-4749-9521-7c93272a841c · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 24
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6912b2ac-940a-4748-a252-706a72f3eda7 · outbound
This paper cites 1924 On the Resistance Experienced by Spheres in their Motion through Gases.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows 1924 On the Resistance Experienced by Spheres in their Motion through Gases
Reference 25
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation fc73b3d5-905e-40fa-9c07-88cc86e89fe2 · outbound
This paper cites Radiation Hydrodynamical Turbulence In Protoplanetary Disks: Numerical Models and Observational Constraints.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Radiation Hydrodynamical Turbulence In Protoplanetary Disks: Numerical Models and Observational Constraints
Reference 26
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28a8f389-37a2-4da3-9a14-3b61eadc7bd0 · outbound
This paper cites 2014 On multiphase turbulence models for collisional fluid–particle flows.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows 2014 On multiphase turbulence models for collisional fluid–particle flows
Reference 27
- Resolution
- verified fuzzy
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 0f4a1912-5d66-41d5-9ee8-dabab2435233 · outbound
This paper cites Dust settling in local simulations of turbulent protoplanetary disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dust settling in local simulations of turbulent protoplanetary disks
Reference 28
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 47224f41-cd3c-485a-be79-3befe46d1313 · outbound
This paper cites & Gouin, H.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows & Gouin, H
Reference 29
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f8d3ab40-5f12-47d8-8481-50b5148cd4d9 · outbound
This paper cites & Tremaine , S.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows & Tremaine , S
Reference 30
- Resolution
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Source-reported events for the cited work
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Observation 58bfb71c-c27a-41de-8852-22cccb092bf3 · outbound
This paper cites New York University.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows New York University
Reference 31
- Resolution
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Observation e3cc90ce-32de-4a8d-b277-a50493504b22 · outbound
This paper cites Communications on pure and applied mathematics 2 (4), 331--407.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Communications on pure and applied mathematics 2 (4), 331--407
Reference 32
- Resolution
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Observation b8485d0f-8637-4420-896e-fc49fbf2ac73 · outbound
This paper cites SIAM review 25 (1), 35--61.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows SIAM review 25 (1), 35--61
Reference 33
- Resolution
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Source-reported events for the cited work
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Observation 33b4942a-4ec0-4ac7-8459-d854c465f10d · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 34
- Resolution
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Source-reported events for the cited work
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Observation 16ef0f2d-cebf-4845-9c56-cfb772d93f2a · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 35
- Resolution
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Source-reported events for the cited work
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Observation 9290ccbc-aa85-48de-a77e-5e4f232b820b · outbound
This paper cites Cambridge University Press.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Cambridge University Press
Reference 36
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 431ab8a3-2e35-4fbe-8896-d419248f9640 · outbound
This paper cites & Chibbaro, Sergio 2019 A lagrangian probability-density-function model for collisional turbulent fluid–particle flows.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows & Chibbaro, Sergio 2019 A lagrangian probability-density-function model for collisional turbulent fluid–particle flows
Reference 37
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5c856b12-1d95-4b0c-a655-18357c646ace · outbound
This paper cites & Chibbaro, Sergio 2021 A Lagrangian probability-density-function model for turbulent particle-laden channel flow in the dense regime.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows & Chibbaro, Sergio 2021 A Lagrangian probability-density-function model for turbulent particle-laden channel flow in the dense regime
Reference 38
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d557ca80-a087-4112-9650-8e4e70661fa8 · outbound
This paper cites On the settling of small grains in dusty discs: analysis and formulas.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows On the settling of small grains in dusty discs: analysis and formulas
Reference 39
- Resolution
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Observation 6d05a942-ad59-4643-809d-b5275d879ee9 · outbound
This paper cites Dusty gas with SPH - I. Algorithm and test suite.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dusty gas with SPH - I. Algorithm and test suite
Reference 40
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation da90e410-bc3c-419e-b543-45dafe05e7b9 · outbound
This paper cites Dusty gas with SPH - II. Implicit timestepping and astrophysical drag regimes.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dusty gas with SPH - II. Implicit timestepping and astrophysical drag regimes
Reference 41
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2cdbd8b4-333b-4efb-a057-e91fe8dcac1e · outbound
This paper cites Dusty gas with one fluid.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dusty gas with one fluid
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:53.934105Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9c58ac2e-a3d1-45a3-98a6-16294a76247e · outbound
This paper cites Thermal hysteresis and front propagation in dense planetary rings.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Thermal hysteresis and front propagation in dense planetary rings
Reference 43
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 30a153d5-647f-4b6c-9f52-dac3e98aaab3 · outbound
This paper cites Dense planetary rings and the viscous overstability.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dense planetary rings and the viscous overstability
Reference 44
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-12T17:35:54.642010Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 176b67ca-737c-49d0-b907-952e97f1b62f · outbound
This paper cites Local models of astrophysical discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Local models of astrophysical discs
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.615644Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 7d4da0e9-d65f-4f11-92d0-4531a8354484 · outbound
This paper cites Hydro-, Magnetohydro-, and Dust-Gas Dynamics of Protoplanetary Disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Hydro-, Magnetohydro-, and Dust-Gas Dynamics of Protoplanetary Disks
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:53.955044Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 95ba64e7-920e-4315-9d5c-ab6d288e3970 · outbound
This paper cites Journal of statistical Physics 83 , 1021--1065.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Journal of statistical Physics 83 , 1021--1065
Reference 47
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.533288Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a08b3eb2-2f8b-4963-a2ca-fb2d48178d13 · outbound
This paper cites Dust settling against hydrodynamic turbulence in protoplanetary discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dust settling against hydrodynamic turbulence in protoplanetary discs
Reference 48
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-12T17:35:54.582242Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a2edbf27-aa70-4e50-b09d-a963d56f5b05 · outbound
This paper cites Cooling Requirements for the Vertical Shear Instability in Protoplanetary Disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Cooling Requirements for the Vertical Shear Instability in Protoplanetary Disks
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:53.969613Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4fb43e42-2686-48f2-b369-9233605afca2 · outbound
This paper cites A thermodynamic view of dusty protoplanetary disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows A thermodynamic view of dusty protoplanetary disks
Reference 50
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.552759Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2322809e-e037-4257-8fcc-fff9110b6fa5 · outbound
This paper cites Importance of magnetic fields in highly eccentric discs with applications to tidal disruption events.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Importance of magnetic fields in highly eccentric discs with applications to tidal disruption events
Reference 51
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-12T17:35:54.534835Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2a972a73-7f30-40d1-a5f2-1d632872a5c5 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 52
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T17:35:55.515711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ed907ae5-f9b6-407f-855a-651bf8d16f42 · outbound
This paper cites A Particle Module for the PLUTO Code: III -- Dust.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows A Particle Module for the PLUTO Code: III -- Dust
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.517604Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 832ef125-a406-4686-8122-805dee6bfbb8 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 54
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T17:35:55.498801Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 1ec1f3f0-358c-44d2-9f92-73e4655134e9 · outbound
This paper cites Progress in Energy and Combustion Science 50 , 1--62.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Progress in Energy and Combustion Science 50 , 1--62
Reference 55
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.478905Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 442c60de-e632-4c2e-9ef4-55345e57adb7 · outbound
This paper cites Physics Reports 665 (2016) , 1--122.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Physics Reports 665 (2016) , 1--122
Reference 56
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.466190Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation aa43e1d9-06cd-4f0d-a9f2-85dda9aa880b · outbound
This paper cites Physics of Fluids 26 (11), 113303.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Physics of Fluids 26 (11), 113303
Reference 57
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.448163Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 837a131a-f05f-4f66-9098-bf6111f0c63e · outbound
This paper cites The dynamics of discrete particles in turbulent flows: open issues and current challenges in statistical modeling.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows The dynamics of discrete particles in turbulent flows: open issues and current challenges in statistical modeling
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.493882Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 4925a004-6b5f-46b6-b8e6-09f6f119ee64 · outbound
This paper cites Physics Reports 352 (1), 1--214.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Physics Reports 352 (1), 1--214
Reference 59
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.434016Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation dc70f1d5-b803-424b-91fb-abcda0b53d42 · outbound
This paper cites Physics of fluids 16 (7), 2419--2431.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Physics of fluids 16 (7), 2419--2431
Reference 60
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.414666Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ae51a90b-056b-407e-b051-0ef19e2002c2 · outbound
This paper cites Linear and nonlinear evolution of the vertical shear instability in accretion discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Linear and nonlinear evolution of the vertical shear instability in accretion discs
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.031417Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4e98218b-524d-4b99-b838-601c7844e747 · outbound
This paper cites On the dynamics of magnetorotational turbulent stresses.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows On the dynamics of magnetorotational turbulent stresses
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.462574Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e3833999-9bfe-4d56-b831-998b45304169 · outbound
This paper cites Local and global dynamics of eccentric astrophysical discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Local and global dynamics of eccentric astrophysical discs
Reference 63
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.446244Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 24d099b8-2101-4f7a-afd6-18beefcb2a96 · outbound
This paper cites Hydrodynamic instability in warped astrophysical discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Hydrodynamic instability in warped astrophysical discs
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.045061Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8f16ba6c-dc66-4d93-bb20-f13e316d6410 · outbound
This paper cites Local and global dynamics of warped astrophysical discs.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Local and global dynamics of warped astrophysical discs
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.049184Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 825f0ecf-9e76-400f-afd9-4a70459c6f02 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 66
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T17:35:55.394767Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 86a27330-50bd-4bfb-ae32-2fa3d9d5f8f6 · outbound
This paper cites Closed-form expressions for particle relative velocities induced by turbulence.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Closed-form expressions for particle relative velocities induced by turbulence
Reference 67
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.394038Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a301516c-659c-404a-aa21-cce730359bbc · outbound
This paper cites Catching drifting pebbles II. A stochastic equation of motions for pebbles.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Catching drifting pebbles II. A stochastic equation of motions for pebbles
Reference 68
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.372579Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 480f2631-3b90-467a-9da0-4fafe442cbd4 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 69
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T17:35:55.374301Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f8c72c47-3e3c-478d-9a34-cdf75f609a48 · outbound
This paper cites The Local Instability of Steady Astrophysical Flows with non Circular Streamlines with Application to Differentially Rotating Disks with Free Eccentricity.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows The Local Instability of Steady Astrophysical Flows with non Circular Streamlines with Application to Differentially Rotating Disks with Free Eccentricity
Reference 70
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.353141Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e59905d2-315c-4017-99c1-33bcd8f1554b · outbound
This paper cites , Chibbaro, S.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows , Chibbaro, S
Reference 71
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.355587Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 4e5066a8-11e9-48c9-a1c5-fe167923e704 · outbound
This paper cites 1985 Pdf methods for turbulent reactive flows.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows 1985 Pdf methods for turbulent reactive flows
Reference 72
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.338140Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation cf4480c6-a603-4e8c-82b3-83a354dc2e18 · outbound
This paper cites The Physics of fluids 30 (8), 2374--2379.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows The Physics of fluids 30 (8), 2374--2379
Reference 73
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.317371Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 11ce3f7e-7027-4b78-9c36-2dc0c1094b75 · outbound
This paper cites 2000 Turbulent Flows\/.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows 2000 Turbulent Flows\/
Reference 74
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.300477Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 77842790-0a85-42be-a93b-efa5bb7c2448 · outbound
This paper cites Physics of Fluids 14 (7), 2360--2375.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Physics of Fluids 14 (7), 2360--2375
Reference 75
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.283281Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 760ab408-0adb-4fb8-afb2-9a31fb58b58c · outbound
This paper cites Journal of computational physics 43 (2), 357--372.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Journal of computational physics 43 (2), 357--372
Reference 76
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.264116Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 285f97f1-3c7a-4151-9758-3b0304ba2c0b · outbound
This paper cites Physics of Fluids A: Fluid Dynamics 3 (6), 1577--1586.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Physics of Fluids A: Fluid Dynamics 3 (6), 1577--1586
Reference 77
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.245283Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 28a6b178-0bb8-48a5-acb2-a6b62a84e398 · outbound
This paper cites Wavelike nature of the vertical shear instability in global protoplanetary disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Wavelike nature of the vertical shear instability in global protoplanetary disks
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T17:35:54.333242Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation b599712a-f756-4967-a8a3-67ec9a8c7802 · outbound
This paper cites Dust Evolution in Protoplanetary Disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Dust Evolution in Protoplanetary Disks
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.123755Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 601bcb9a-a9dc-40f5-8ac2-4b38e882767c · outbound
This paper cites Geophysics 51 (10), 1954--1966.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Geophysics 51 (10), 1954--1966
Reference 80
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.229578Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8351668d-c245-4d60-b1e8-71e432de38b3 · outbound
This paper cites Journal of fluid mechanics 180 , 529--556.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Journal of fluid mechanics 180 , 529--556
Reference 81
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.210429Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation af983e4d-8c08-4e9b-bbc6-7fe53826d0c5 · outbound
This paper cites Shock waves 4 , 25--34.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Shock waves 4 , 25--34
Reference 82
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.191638Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 9d05100c-c756-485d-9321-d58246b89447 · outbound
This paper cites In 16th aiaa computational fluid dynamics conference\/ , p.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows In 16th aiaa computational fluid dynamics conference\/ , p
Reference 83
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.171093Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 693f3627-f274-42b3-b6d3-68bc62de9785 · outbound
This paper cites an unresolved cited work.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work
Reference 84
- Resolution
- unresolved
- raw_fallback, observed 2026-08-12T17:35:55.150104Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6b639417-ce6a-4278-8cee-9d7ac820ecb1 · outbound
This paper cites 1985 The moments of the multivariate normal.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows 1985 The moments of the multivariate normal
Reference 85
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T17:35:55.131215Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f6b2bec0-629d-4d82-af77-83e2fdf77d9a · outbound
This paper cites Integration of Particle-Gas Systems with Stiff Mutual Drag Interaction.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Integration of Particle-Gas Systems with Stiff Mutual Drag Interaction
Reference 86
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-12T17:35:54.303473Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6b75a790-6cb1-412a-a217-623f5378b504 · outbound
This paper cites Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.155875Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d9bce29-aab6-4774-a620-098859a41f72 · outbound
This paper cites Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Particle Stirring in Turbulent Gas Disks: Including Orbital Oscillations
Reference 88
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.162253Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1273af2-359a-418e-9cd8-67980635fbb6 · outbound
This paper cites Particle Concentration At Planet Induced Gap Edges and Vortices: I. Inviscid 3-D Hydro Disks.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Particle Concentration At Planet Induced Gap Edges and Vortices: I. Inviscid 3-D Hydro Disks
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.167071Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7ebd8089-956c-42b3-9c83-61e12c739621 · outbound
This paper cites , " * write output.state after.block = add.period write newline.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows , " * write output.state after.block = add.period write newline
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.172824Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 44efa19e-fc4c-4627-8ed2-99e4f8c76ae5 · outbound
This paper cites write newline.
Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows write newline
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:35:54.178122Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.