Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows | Paper Citation Record

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

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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

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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

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

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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

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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

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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

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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

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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

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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

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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

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 13

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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

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This paper cites , Goldreich , P.

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows , Goldreich , P

Reference 15

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 16

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 17

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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

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This paper cites Cambridge university press.

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Cambridge university press

Reference 19

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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

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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

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 22

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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

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 24

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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

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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

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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

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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

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This paper cites & Gouin, H.

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows & Gouin, H

Reference 29

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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

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This paper cites New York University.

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows New York University

Reference 31

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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

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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

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 34

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Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Unresolved cited work

Reference 35

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This paper cites Cambridge University Press.

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Cambridge University Press

Reference 36

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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

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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

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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

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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

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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

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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

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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

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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

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Resolution: metadata mismatch; local_arxiv, observed 2026-08-12T17:35:54.642010Z

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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

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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

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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

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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

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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

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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

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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

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Resolution: metadata mismatch; local_arxiv, observed 2026-08-12T17:35:54.534835Z

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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

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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

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Resolution: verified exact; local_arxiv, observed 2026-08-12T17:35:54.517604Z

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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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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 2026-08-17T06:30:58.91139+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.

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