Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation | Paper Citation Record

Observation b30aca0b-025d-4800-b169-8b4e06ea5eb4 · outbound

This paper cites Evidence for strong extragalactic magnetic fields from Fermi observations of TeV blazars.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Evidence for strong extragalactic magnetic fields from Fermi observations of TeV blazars

Reference 1

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Observation 175ea531-8039-4552-8703-7efa6d84ed34 · outbound

This paper cites On the Origin of Cosmic Magnetic Fields.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation On the Origin of Cosmic Magnetic Fields

Reference 2

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Observation 3396c6f7-6950-46b9-b4c3-9f047af11dac · outbound

This paper cites The First Magnetic Fields.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The First Magnetic Fields

Reference 3

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Observation c54a2aef-8691-4bda-9b1d-e92bffdd9855 · outbound

This paper cites The Cosmological Impact of Luminous TeV Blazars I: Implications of Plasma Instabilities for the Intergalactic Magnetic Field and Extragalactic Gamma-Ray Background.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The Cosmological Impact of Luminous TeV Blazars I: Implications of Plasma Instabilities for the Intergalactic Magnetic Field and Extragalactic Gamma-Ray Background

Reference 4

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Observation c6a6ce6e-5562-4b0e-898b-85c41b5e8a12 · outbound

This paper cites Magnetic fields of non-degenerate stars.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Magnetic fields of non-degenerate stars

Reference 5

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Observation 94f27dc6-8147-41e8-b6d7-3895d141ebf3 · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 6

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Observation 9e99f7c0-dc41-49c7-b34b-cd6da3cdc67b · outbound

This paper cites Relieving the Hubble tension with primordial magnetic fields.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Relieving the Hubble tension with primordial magnetic fields

Reference 7

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Observation 2f3348d7-7214-42e4-9f69-8d1c03a1adab · outbound

This paper cites Reviews of Modern Physics , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Reviews of Modern Physics , keywords =

Reference 8

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Observation 35ffe758-91f7-43d3-a60b-11c0ecf309aa · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 9

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Observation 2c012406-7773-45a0-8022-4144b9d2f73c · outbound

This paper cites , year = 1970, month = aug, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , year = 1970, month = aug, volume =

Reference 10

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Observation a04c2db9-b35a-47a9-8359-b9d242dd3882 · outbound

This paper cites II: Self-consistent Stationary Picture.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation II: Self-consistent Stationary Picture

Reference 11

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Observation 3ca3c944-00d7-42a3-8f95-044a2d93caf8 · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 12

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Observation 991ff51e-be98-41fd-ae73-1fea48a8a1af · outbound

This paper cites an unresolved cited work.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Unresolved cited work

Reference 13

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Observation ebee229f-6477-4129-9612-bfdfc2e46a2d · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 14

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Observation 1ebce45b-3428-4a10-8826-5fb02d096dee · outbound

This paper cites , year = 1966, month = sep, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , year = 1966, month = sep, volume =

Reference 15

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Observation 31d7b5f1-a6f0-4650-b894-9b65d27d30b0 · outbound

This paper cites Inefficient star formation through turbulence, magnetic fields and feedback.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Inefficient star formation through turbulence, magnetic fields and feedback

Reference 16

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Observation 5824a4f5-7178-4fa8-ad9f-b42d6e296444 · outbound

This paper cites The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations

Reference 17

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Observation 4f60b77f-b469-49c5-87a0-ffcfbb117fc7 · outbound

This paper cites Magnetic Driving of Relativistic Outflows in Active Galactic Nuclei. I. Interpretation of Parsec-Scale Accelerations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Magnetic Driving of Relativistic Outflows in Active Galactic Nuclei. I. Interpretation of Parsec-Scale Accelerations

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.528530Z

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Observation d24ed749-07d6-4be2-b6a9-30183c104991 · outbound

This paper cites Magnetic field evolution in tidal disruption events.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Magnetic field evolution in tidal disruption events

Reference 19

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Observation babb9cf9-c169-4257-be36-a5633dc7f029 · outbound

This paper cites Simulations of Magnetic Fields in Tidally-Disrupted Stars.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Simulations of Magnetic Fields in Tidally-Disrupted Stars

Reference 20

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Observation 87185c14-ddc3-43ef-a5f3-00edfa2bde75 · outbound

This paper cites A relativistic jetted outburst from a massive black hole fed by a tidally disrupted star.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A relativistic jetted outburst from a massive black hole fed by a tidally disrupted star

Reference 21

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Observation d0a4bfc6-7eb8-4e9a-8f90-b90d64f475b5 · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 22

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Observation 39204ec6-4f7e-4812-bf39-3c12226207e0 · outbound

This paper cites Producing ultra-strong magnetic fields in neutron star mergers.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Producing ultra-strong magnetic fields in neutron star mergers

Reference 23

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Observation 9c43eae2-9a27-4b68-aaf0-99bd4b06d8c9 · outbound

This paper cites Detection of microgauss coherent magnetic fields in a galaxy five billion years ago.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Detection of microgauss coherent magnetic fields in a galaxy five billion years ago

Reference 24

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Observation c0cbf40d-0e35-4a47-b500-9569aed27946 · outbound

This paper cites Planets, Stars and Stellar Systems.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Planets, Stars and Stellar Systems

Reference 25

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Observation a81d94fa-659b-42a9-8c60-ac39f65f8ebe · outbound

This paper cites Diffuse Radio Emission from Galaxy Clusters.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Diffuse Radio Emission from Galaxy Clusters

Reference 26

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Observation 301eaf42-4ba3-4f28-b23e-71859d9ebf3d · outbound

This paper cites The Astrophysics of Ultrahigh Energy Cosmic Rays.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The Astrophysics of Ultrahigh Energy Cosmic Rays

Reference 27

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Observation 8d7614cc-7f53-4622-920a-4dc9a4c24fc2 · outbound

This paper cites Hydromagnetic turbulence in computer simulations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Hydromagnetic turbulence in computer simulations

Reference 28

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Observation ac8afde9-3d4c-404b-b90f-781d01d0ec5c · outbound

This paper cites Advances in Nonlinear Dynamics , year = 2003, editor =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Advances in Nonlinear Dynamics , year = 2003, editor =

Reference 29

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Observation d68405f5-0c95-452f-923d-247d3e8381ce · outbound

This paper cites The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintained.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintained

Reference 30

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Observation 0972e7ea-ff4f-4b86-9240-f24f458d47f4 · outbound

This paper cites Computer Physics Communications , year = 1997, month = apr, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Computer Physics Communications , year = 1997, month = apr, volume =

Reference 31

Resolution: verified exact; doi, observed 2026-08-10T17:19:42.214828Z

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Observation 37efcf72-5f07-4741-b843-1352faf98678 · outbound

This paper cites Computer Physics Communications , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Computer Physics Communications , keywords =

Reference 32

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Observation 6279a792-9475-4997-9f3c-6aa95c8b0821 · outbound

This paper cites Introducing Enzo, an AMR Cosmology Application.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Introducing Enzo, an AMR Cosmology Application

Reference 33

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Observation c16ee7d4-ff38-4524-9f7e-88b2dcfb56c4 · outbound

This paper cites The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers

Reference 34

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Observation 60d633c9-9173-4e32-a976-2bd02c4f75e3 · outbound

This paper cites Enzo: An Adaptive Mesh Refinement Code for Astrophysics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Enzo: An Adaptive Mesh Refinement Code for Astrophysics

Reference 35

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Observation 57877cc5-eddb-4b55-bd3d-00dbd9ba52ec · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 36

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Observation b794db95-7ae9-41c1-a46f-7c7ef5ccff7f · outbound

This paper cites HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics

Reference 37

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Observation d7327a20-fe5c-473a-8ab3-161dc8a43f7f · outbound

This paper cites PLUTO: a Numerical Code for Computational Astrophysics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation PLUTO: a Numerical Code for Computational Astrophysics

Reference 38

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Observation 7880f3ca-589f-4dc7-a168-bf28e42ff3d8 · outbound

This paper cites Kinematic Dynamos using Constrained Transport with High Order Godunov Schemes and Adaptive Mesh Refinement.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Kinematic Dynamos using Constrained Transport with High Order Godunov Schemes and Adaptive Mesh Refinement

Reference 39

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Observation 7ed662c9-dce3-40fc-aee8-0b00d66c41b1 · outbound

This paper cites Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 40

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Observation 89a695f8-66fc-4e4b-85cd-37ab59c28d5d · outbound

This paper cites GADGET: A code for collisionless and gasdynamical cosmological simulations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation GADGET: A code for collisionless and gasdynamical cosmological simulations

Reference 41

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Observation a1b05a4d-4a1c-4060-b783-d02906d3f1a5 · outbound

This paper cites Journal of Computational Physics , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Journal of Computational Physics , keywords =

Reference 42

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Observation 3b3f6629-0507-43fc-bec3-289e2c6945f7 · outbound

This paper cites An Approximate Riemann Solver for Magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation An Approximate Riemann Solver for Magnetohydrodynamics

Reference 43

Resolution: verified exact; doi, observed 2026-08-10T17:19:42.146454Z

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Observation 488717fa-cbd7-41f4-8c2e-cd770fbd7f28 · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 44

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Observation 5c363acf-cc5e-47e8-94ec-18f177149290 · outbound

This paper cites A Constrained Transport Scheme for MHD on Unstructured Static and Moving Meshes.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A Constrained Transport Scheme for MHD on Unstructured Static and Moving Meshes

Reference 45

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Observation c3093f51-61ca-4055-9de3-2e464075ba44 · outbound

This paper cites A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics

Reference 46

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Observation acb96eb7-f463-4284-a97c-fb647b58ef17 · outbound

This paper cites Cosmological AMR MHD with Enzo.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Cosmological AMR MHD with Enzo

Reference 47

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Observation b4ba716f-a69b-43cd-afce-98daf065e328 · outbound

This paper cites A Second-Order Unsplit Godunov Scheme for Cell-Centered MHD: the CTU-GLM scheme.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A Second-Order Unsplit Godunov Scheme for Cell-Centered MHD: the CTU-GLM scheme

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.712170Z

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Observation 85c869b7-bbfb-4d94-9f92-c1ff64722324 · outbound

This paper cites An Intercomparison Between Divergence-Cleaning and Staggered Mesh Formulations for Numerical Magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation An Intercomparison Between Divergence-Cleaning and Staggered Mesh Formulations for Numerical Magnetohydrodynamics

Reference 49

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Observation 5af72d7e-a5fc-49f0-a8d2-3e726b6cc47e · outbound

This paper cites Waagan and C.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Waagan and C

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.725089Z

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Observation e3891fba-f256-4ec4-9f98-daf4a37b5603 · outbound

This paper cites High-order conservative finite difference GLM-MHD schemes for cell-centered MHD.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation High-order conservative finite difference GLM-MHD schemes for cell-centered MHD

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.730317Z

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Observation d2a123e0-abb0-45dd-8818-a7358c69982b · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 52

Resolution: verified exact; doi, observed 2026-08-10T17:19:42.107654Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation b87bf451-a00c-4c37-ad5f-2bb29abaf04f · outbound

This paper cites Journal of Computational Physics , year = 1999, month = mar, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Journal of Computational Physics , year = 1999, month = mar, volume =

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.740593Z

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Observation 388b07d1-788b-45be-870c-60809cd69606 · outbound

This paper cites Relativistic MHD with Adaptive Mesh Refinement.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Relativistic MHD with Adaptive Mesh Refinement

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.749990Z

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Observation edddc148-2c99-4963-9a79-662e98e2b215 · outbound

This paper cites Self-gravitational Magnetohydrodynamics with Adaptive Mesh Refinement for Protostellar Collapse.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Self-gravitational Magnetohydrodynamics with Adaptive Mesh Refinement for Protostellar Collapse

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.755715Z

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Observation 5170ac70-2b4d-4cad-bc37-ac4cc28a1962 · outbound

This paper cites The PLUTO Code for Adaptive Mesh Computations in Astrophysical Fluid Dynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The PLUTO Code for Adaptive Mesh Computations in Astrophysical Fluid Dynamics

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.760986Z

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Observation c8cec4ed-e720-4bbe-891c-ea44883344ea · outbound

This paper cites Journal of Computational Physics , year = 2012, month = feb, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Journal of Computational Physics , year = 2012, month = feb, volume =

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.766971Z

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Observation 3cc72853-29e5-43ea-a588-49fe30f38f34 · outbound

This paper cites Journal of Computational Physics , year = 2000, month = jul, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Journal of Computational Physics , year = 2000, month = jul, volume =

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.771757Z

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Observation 787c5f3a-4b7d-4b8f-b8ef-7c3545bd7fa5 · outbound

This paper cites Philosophical Transactions of the Royal Society of London Series I , year = 1865, month = jan, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Philosophical Transactions of the Royal Society of London Series I , year = 1865, month = jan, volume =

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.776540Z

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Observation 6cadb6b1-907e-4e40-9beb-92887469581c · outbound

This paper cites On the forces, stresses, and fluxes of energy in the electromagnetic field.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation On the forces, stresses, and fluxes of energy in the electromagnetic field

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.781381Z

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Observation 403874df-3469-4a1a-8135-a528eb44487d · outbound

This paper cites Journal of Computational Physics , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Journal of Computational Physics , keywords =

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.786601Z

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Observation 041c745c-db71-4acd-b296-01df38beeb57 · outbound

This paper cites Frontiers in Astronomy and Space Sciences , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Frontiers in Astronomy and Space Sciences , keywords =

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.792662Z

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Observation da80cc66-079e-4704-ad9b-92fd174514a3 · outbound

This paper cites Improving divergence cleaning in cosmological SPMHD simulations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Improving divergence cleaning in cosmological SPMHD simulations

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.797902Z

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Observation fb0d0c94-6f06-4963-b21a-67a83ebdf64e · outbound

This paper cites Astrophysical Smooth Particle Hydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Astrophysical Smooth Particle Hydrodynamics

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.803591Z

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Observation c568bd3d-f70d-4429-9a0d-94e6403b2538 · outbound

This paper cites Reports on Progress in Physics , year = 2005, month = aug, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Reports on Progress in Physics , year = 2005, month = aug, volume =

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.809924Z

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Observation 440c53a1-30ea-4ee6-ae94-564b10d388a3 · outbound

This paper cites A Constrained-Gradient Method to Control Divergence Errors in Numerical MHD.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A Constrained-Gradient Method to Control Divergence Errors in Numerical MHD

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.815245Z

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Observation 13c0ce65-c64f-4c2f-b30f-d0158f559fed · outbound

This paper cites Smoothed Particle Magnetohydrodynamics: A State of the Union.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Smoothed Particle Magnetohydrodynamics: A State of the Union

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Resolution: metadata mismatch; local_arxiv, observed 2026-08-10T17:19:42.064142Z

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Observation baf25cc9-4f13-47c3-ae4b-f29313e1289c · outbound

This paper cites Journal of Computational Physics , year = 1995, month = jan, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Journal of Computational Physics , year = 1995, month = jan, volume =

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.836229Z

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Observation 7ba9e3db-3734-4503-86f4-10285bf56dd4 · outbound

This paper cites , year = 1994, month = jan, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , year = 1994, month = jan, volume =

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.841345Z

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Observation 1db6a601-ee73-4b71-adad-9e58152170de · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 72

Resolution: verified exact; doi, observed 2026-08-10T17:19:42.040053Z

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Observation 260e9021-ad40-4c46-8e4f-d995b63eddfa · outbound

This paper cites Minimizing Dispersive Errors in Smoothed Particle Magnetohydrodynamics for Strongly Magnetized Medium.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Minimizing Dispersive Errors in Smoothed Particle Magnetohydrodynamics for Strongly Magnetized Medium

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.850921Z

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Observation 828fe441-0370-4973-ad7b-51b2e00ba6f8 · outbound

This paper cites American Journal of Physics , year = 1970, month = apr, volume =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation American Journal of Physics , year = 1970, month = apr, volume =

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Resolution: verified exact; doi, observed 2026-08-10T17:19:42.022239Z

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Observation 4f86bb87-12dd-4991-ad81-81b98f6af290 · outbound

This paper cites Reviews of Geophysics and Space Physics , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Reviews of Geophysics and Space Physics , keywords =

Reference 75

Resolution: verified exact; doi, observed 2026-08-10T17:19:42.005360Z

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Observation c746c5f3-a27a-4f22-bd8e-d9a9672ca32d · outbound

This paper cites A Vector Potential implementation for Smoothed Particle Magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A Vector Potential implementation for Smoothed Particle Magnetohydrodynamics

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Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.873967Z

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Observation d7010c38-39f2-4489-9c2b-53018d75ffa9 · outbound

This paper cites An Integral-based Approach for the Vector Potential in Smoothed Particle Magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation An Integral-based Approach for the Vector Potential in Smoothed Particle Magnetohydrodynamics

Reference 79

Resolution: metadata mismatch; local_arxiv, observed 2026-08-10T17:19:41.989799Z

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Observation 2614dfa1-a9e6-406e-9eee-eb16e1a2b7da · outbound

This paper cites Magnetorotational instability with smoothed particle hydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Magnetorotational instability with smoothed particle hydrodynamics

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.885543Z

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Observation 664570f5-ff7c-4e00-9af5-486869db6a86 · outbound

This paper cites A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.892500Z

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Observation ffb6f4d0-aca3-446b-9a0e-fc21ba4bd94f · outbound

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Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.900171Z

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Observation d4b6dd48-dd84-451d-af34-2fb23b0c7d01 · outbound

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Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.906396Z

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Observation 5402e63d-33e7-41a7-985c-de3414bc712c · outbound

This paper cites Cosmological Simulations of Galaxy Formation.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Cosmological Simulations of Galaxy Formation

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.913231Z

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Observation 78f21618-2618-4b40-ad65-eea087ff6df7 · outbound

This paper cites Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges.

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Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.918721Z

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Observation cf26b3bc-df04-4fe2-88c9-240c14af3788 · outbound

This paper cites Theoretical Challenges in Galaxy Formation.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Theoretical Challenges in Galaxy Formation

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.924733Z

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Observation 5f569694-dbf6-48ee-a670-7747e0627854 · outbound

This paper cites Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.930647Z

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Observation ddcf87b0-da91-4af2-8aec-40436c8dca1b · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.940806Z

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Observation b172207f-bc0e-492e-b02d-5eee06fb4062 · outbound

This paper cites Spin-driven jet feedback in idealised simulations of galaxy groups and clusters.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Spin-driven jet feedback in idealised simulations of galaxy groups and clusters

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.946394Z

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Observation f63678dc-856b-47dd-9d3a-6c3ce8c0a85b · outbound

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Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The multiphase circumgalactic medium traced by low metal ions in EAGLE zoom simulations

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.952116Z

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Observation b12cf5ec-f6da-49f5-959c-ea61083637eb · outbound

This paper cites The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.957610Z

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Observation 89ffc935-df89-41a8-b560-97919fd56b2c · outbound

This paper cites The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.963208Z

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Observation f13919e7-7236-491e-ad23-3dbc1c854c84 · outbound

This paper cites Relativistic SZ temperatures and hydrostatic mass bias for massive clusters in the FLAMINGO simulations.

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Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.968447Z

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Observation 5fb8fc7c-e2be-4a4a-b990-734103b583e9 · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.973485Z

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Observation 920ba377-262a-4fea-8a4a-c3563c9b4fba · outbound

This paper cites The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters.

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Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.977735Z

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Observation 1a6bd224-0207-4e41-b590-b663c20dbc3c · outbound

This paper cites Gradient Particle Magnetohydrodynamics.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Gradient Particle Magnetohydrodynamics

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.982032Z

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Observation 08e8a271-de0b-4444-b009-f8578650eff0 · outbound

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Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.987345Z

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Observation fd666878-a68c-4637-9114-2770d304d10e · outbound

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Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.992555Z

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Observation 8a9fcf86-c801-4e01-9167-ee41268ffef9 · outbound

This paper cites Numerical Modeling of Space Plasma Flows (ASTRONUM2012) , year = 2013, editor =.

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Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:40.005791Z

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Observation fdcda102-882f-4be1-87ae-231437d5a0a1 · outbound

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Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:40.010911Z

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Observation b6d4e41a-888f-46d2-844d-76578f806110 · outbound

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Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation SWIFT: Maintaining weak-scalability with a dynamic range of $10^4$ in time-step size to harness extreme adaptivity

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Resolution: metadata mismatch; local_arxiv, observed 2026-08-10T17:19:41.950202Z

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Observation e496b0b6-3fae-41d6-a458-05219be4e0eb · outbound

This paper cites Proceedings of the Platform for Advanced Scientific Computing Conference , year = 2016, month = jun, eid =.

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Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:40.023054Z

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Observation 11514370-2495-4da7-bcaa-06dfd23930c1 · outbound

This paper cites , keywords =.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation , keywords =

Reference 105

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:40.029975Z

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Observation f0d9320f-b95b-4e09-8680-66489f970c44 · outbound

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