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Paper Citation Record · LEDGER

Transport Properties of the MRI in Differentially Rotating Neutron Stars

As of 21 August 2026, this Paper Citation Record lists 100 of 101 outbound references and 0 inbound Pith citation observations for arXiv:2607.24457.

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pith.paper-citation-record.v1
2607.24457 v1

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measured 100 of 101 reference resolution

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100 of 101 outbound references displayed

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Outbound references

Observation de7822fa-4835-4fe5-9a71-5d51fec80b68 · outbound

This paper cites This ties the turbulent transport directly to the viscous-disc framework, in whichα vis is the single free parameter [19, 52, 68].

Transport Properties of the MRI in Differentially Rotating Neutron Stars This ties the turbulent transport directly to the viscous-disc framework, in whichα vis is the single free parameter [19, 52, 68]

Reference 1

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Observation 1142b423-155d-428e-988d-b99714004673 · outbound

This paper cites Let Di be the covariant derivative ofγij, with connection Γkij = 1 2 γkl(∂iγjl + ∂jγil −∂ lγij).

Transport Properties of the MRI in Differentially Rotating Neutron Stars Let Di be the covariant derivative ofγij, with connection Γkij = 1 2 γkl(∂iγjl + ∂jγil −∂ lγij)

Reference 2

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Observation 1500593e-6a43-4885-b9b1-1fb8b6d50cf2 · outbound

This paper cites j-constant.

Transport Properties of the MRI in Differentially Rotating Neutron Stars j-constant

Reference 3

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Observation f7985f00-31fa-4e5a-88ba-2853566450f4 · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Transport Properties of the MRI in Differentially Rotating Neutron Stars GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 4

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Observation c0acd3b6-4a2f-4f4d-ab88-efefecb11f1c · outbound

This paper cites Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

Reference 5

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Observation 92ac3c38-fad3-41c0-9f24-40871c94daf9 · outbound

This paper cites Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event

Reference 6

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Observation 097371ff-3ef5-4996-a328-dcc6ce510d1e · outbound

This paper cites Kilonovae.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Kilonovae

Reference 7

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Observation d22d3368-c2dd-404c-81d6-a1b883026486 · outbound

This paper cites Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case

Reference 8

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Observation fb8c4a60-9f42-48b4-a79d-07505a884740 · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 9

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Observation eb6187eb-f959-403e-9775-f422cb9f31d2 · outbound

This paper cites Theory of Core-Collapse Supernovae.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Theory of Core-Collapse Supernovae

Reference 10

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Observation 44ebbadf-ba46-444a-8691-2e1a036de8a5 · outbound

This paper cites Rembiasz, J.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Rembiasz, J

Reference 11

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Observation 33e7e0eb-7729-42f0-b4a3-c13e74790523 · outbound

This paper cites Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity

Reference 12

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Observation 86492e36-b16e-4822-866c-19c535294e2e · outbound

This paper cites Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

Reference 13

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Observation df94fa85-0561-43c8-af7b-96ea9b8fb1a0 · outbound

This paper cites Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers

Reference 14

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Observation 35cf3bd3-d109-453e-af1a-96b96af0e8c6 · outbound

This paper cites A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 15

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Observation d181d923-019e-43cc-b5ad-6ecf0d3667ea · outbound

This paper cites A magnetar formation in binary neutron star merger.

Transport Properties of the MRI in Differentially Rotating Neutron Stars A magnetar formation in binary neutron star merger

Reference 16

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Observation aab37e8b-a0ca-474c-9890-19c5f85282e9 · outbound

This paper cites Flares, jets and quasi-periodic outbursts from neutron star merger remnants.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Flares, jets and quasi-periodic outbursts from neutron star merger remnants

Reference 17

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Observation bd9c35da-d0da-4fa4-846b-74339c7139fe · outbound

This paper cites Combi and D.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Combi and D

Reference 18

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Observation 2c572692-6166-4ba0-a2f8-616a08d84127 · outbound

This paper cites On the impact of neutrinos on the launching of relativistic jets from "magnetars" produced in neutron-star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars On the impact of neutrinos on the launching of relativistic jets from "magnetars" produced in neutron-star mergers

Reference 19

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Observation 9dfaa0d9-fe23-406b-b670-982b1b6fdf92 · outbound

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Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 20

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Observation a9599650-bbe6-4da2-8bc1-ef0d708ad368 · outbound

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Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 21

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Observation 104dc2d5-ce66-434f-896c-0f4573d61311 · outbound

This paper cites Enhanced Angular Momentum Transport in Accretion Disks.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Enhanced Angular Momentum Transport in Accretion Disks

Reference 22

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Observation 75c31498-89ba-45a7-9649-84f4aca909cb · outbound

This paper cites The Magnetorotational Instability in Core Collapse Supernova Explosions.

Transport Properties of the MRI in Differentially Rotating Neutron Stars The Magnetorotational Instability in Core Collapse Supernova Explosions

Reference 23

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Observation 9271d2a7-4053-463a-9d81-856a37be2934 · outbound

This paper cites Semi-global simulations of the magneto-rotational instability in core collapse supernovae.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Semi-global simulations of the magneto-rotational instability in core collapse supernovae

Reference 24

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Observation 75965b1a-cc47-4d55-a88c-80201aa8e739 · outbound

This paper cites Mösta, C.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Mösta, C

Reference 25

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Observation 0fc42a11-41eb-49c7-aa38-31eea0f87f17 · outbound

This paper cites A global model of the magnetorotational instability in protoneutron stars.

Transport Properties of the MRI in Differentially Rotating Neutron Stars A global model of the magnetorotational instability in protoneutron stars

Reference 26

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This paper cites Magnetar formation through a convective dynamo in protoneutron stars.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Magnetar formation through a convective dynamo in protoneutron stars

Reference 27

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Observation 2d265c49-34ab-4c14-8793-19aa9252ea42 · outbound

This paper cites Viscosity and Rotation in Core-Collapse Supernovae.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Viscosity and Rotation in Core-Collapse Supernovae

Reference 28

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This paper cites Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation

Reference 29

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Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 30

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This paper cites The impact of non-dipolar magnetic fields in core-collapse supernovae.

Transport Properties of the MRI in Differentially Rotating Neutron Stars The impact of non-dipolar magnetic fields in core-collapse supernovae

Reference 31

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This paper cites Bugli, J.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Bugli, J

Reference 32

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Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 33

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Observation bb7cbef7-365c-4269-8068-25df06fff00a · outbound

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Transport Properties of the MRI in Differentially Rotating Neutron Stars Powell, B

Reference 34

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This paper cites Collapse of differentially rotating neutron stars and cosmic censorship.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Collapse of differentially rotating neutron stars and cosmic censorship

Reference 35

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Observation c2bfb55c-1875-4ea4-b3bc-24503c7b284c · outbound

This paper cites Turbulent magnetic field amplification in binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Turbulent magnetic field amplification in binary neutron star mergers

Reference 36

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This paper cites The role of turbulence and winding in the development of large-scale, strong magnetic fields in long-lived remnants of binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars The role of turbulence and winding in the development of large-scale, strong magnetic fields in long-lived remnants of binary neutron star mergers

Reference 37

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Observation de0a6e0c-9671-49c1-980e-c031386662c5 · outbound

This paper cites Aguilera-Miret, J.-E.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Aguilera-Miret, J.-E

Reference 38

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Observation 44d441e6-d2be-4dd6-8154-265cea09e5b8 · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

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source=pdf_text observed=2026-07-31T14:28:12.708072Z digest=sha256:1196f82efab8aa031851b66303a8565caa377fb51bf395ddf18c244afdc9f573

Observation 350afebc-b2ca-430d-bd77-1662314a040e · outbound

This paper cites Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.712773Z

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source=pdf_text observed=2026-07-31T14:28:12.712773Z digest=sha256:5e368148f9c386adbb6bea1fff7fb922a2d9f6335ea68108006597f42fb344e2

Observation 1a2394ba-1b63-4bed-a3ab-f0fdd6a46234 · outbound

This paper cites Shibata, S.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Shibata, S

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.718261Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.718261Z digest=sha256:9e3e4bf07f3c35446fdbf23687f6c5776b4fe3db86776b0e7ce24e8307c39bd3

Observation 96542f18-7934-4c1f-a419-7f581d443bbc · outbound

This paper cites Magnetorotational instability in relativistic hypermassive neutron stars.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Magnetorotational instability in relativistic hypermassive neutron stars

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.722975Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.722975Z digest=sha256:e2532e91f6f9115003b31399b07987794f798a47a9521a8057a4cc8f6f8728b8

Observation 0ad88d85-2c63-4da5-8279-95c06d1ca2d8 · outbound

This paper cites Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.727566Z

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source=pdf_text observed=2026-07-31T14:28:12.727566Z digest=sha256:d64686cfe3c6c970545a69aeba4dd08f2ddecf1e84521319fde8740f436f2f48

Observation d5a6b9fa-8987-49e5-b561-3bfc81d69dc4 · outbound

This paper cites Eichler, M.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Eichler, M

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.732631Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.732631Z digest=sha256:3036901e1ac909fe9fca8c50bb9954e0de1824f6fcf41f0ec12f0dac69c93308

Observation 7e3e9a9d-e962-43b3-8546-409d19beb191 · outbound

This paper cites Narayan, B.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Narayan, B

Reference 45

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.737165Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.737165Z digest=sha256:94ebd1c2e7f0099e3a7460e3677d9a310f7305a392ecb9f42f2c5b8cc3f898a0

Observation bdec8e21-efed-49ce-8358-0a99b5489988 · outbound

This paper cites The Physics of Gamma-Ray Bursts.

Transport Properties of the MRI in Differentially Rotating Neutron Stars The Physics of Gamma-Ray Bursts

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.742550Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T14:28:12.742550Z digest=sha256:f53559d5b0f2c5db86e17bfcbf3aa30edda48369d35902b1f73ec73740a69273

Observation c50c026a-000b-4fd6-a224-25d84541e09e · outbound

This paper cites The Physics of Gamma-Ray Bursts and Relativistic Jets.

Transport Properties of the MRI in Differentially Rotating Neutron Stars The Physics of Gamma-Ray Bursts and Relativistic Jets

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.747063Z

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source=pdf_text observed=2026-07-31T14:28:12.747063Z digest=sha256:f2d275eedbbfd79fa2b27123d9494f109473e199f6f05fec02abf9d1f9505ec3

Observation 5114d45f-e41a-4fb7-b69f-19fe0adb4a91 · outbound

This paper cites Jet Launching from Binary Neutron Star Mergers: Incorporating Neutrino Transport and Magnetic Fields.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Jet Launching from Binary Neutron Star Mergers: Incorporating Neutrino Transport and Magnetic Fields

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Resolution
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no resolver link, observed 2026-07-31T14:28:12.752089Z

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source=pdf_text observed=2026-07-31T14:28:12.752089Z digest=sha256:0f79a9241606dbbd00ca9a6aeacc7e34b3d9539c2f8587104d0ce1dd5b0d4f10

Observation 09d2e401-af0f-42b7-b946-94380ffbaa87 · outbound

This paper cites Gottliebet al., Large-scale evolution of seconds-long relativistic jets from black hole-neutron star mergers, As- trophys.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Gottliebet al., Large-scale evolution of seconds-long relativistic jets from black hole-neutron star mergers, As- trophys

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.757249Z

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source=pdf_text observed=2026-07-31T14:28:12.757249Z digest=sha256:bf872d1a76a8484b51444d4b1a649cb67752bf4e916f8cb48c3052fa13826c43

Observation 3c4ee4f8-fa4d-443e-9956-3b8860b7d41e · outbound

This paper cites Jetlike structures in low-mass binary neutron star merger remnants.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Jetlike structures in low-mass binary neutron star merger remnants

Reference 50

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.762446Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.762446Z digest=sha256:7c0f6aee1378ed1c6faf0e624684a57cf66c50c408f29b343990803ff74c528a

Observation 7940ded5-6b54-41f1-81f1-006ace4161fb · outbound

This paper cites General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers

Reference 51

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.769598Z

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source=pdf_text observed=2026-07-31T14:28:12.769598Z digest=sha256:016a79352455ef68de761d85a61e504547e17937ad5e455f32b82c10326260d5

Observation ec7f6fba-030f-4a1d-a3df-bf37e56f1024 · outbound

This paper cites Gradient sub-grid-scale model for relativistic MHD Large Eddy Simulations.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Gradient sub-grid-scale model for relativistic MHD Large Eddy Simulations

Reference 52

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.774615Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.774615Z digest=sha256:911cba3a1f47b103e2d51833ea3d440178690bc973d8e591b2e150000ccfd6cb

Observation 34962465-5975-41b8-869b-b4d4a96328c6 · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 53

Resolution
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no resolver link, observed 2026-07-31T14:28:12.779185Z

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source=pdf_text observed=2026-07-31T14:28:12.779185Z digest=sha256:0f1a0442e80d667013abfda08f61ee8808a9d3517848c46590ced8dcaf7327b8

Observation 7ce463db-2f85-42e8-97d1-802661f4384d · outbound

This paper cites The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses.

Transport Properties of the MRI in Differentially Rotating Neutron Stars The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

Reference 54

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.783818Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.783818Z digest=sha256:ad540a2fff53e6c7ce3459fc300884efca86b16753434ec50ab092230bec15cc

Observation 8514a24c-e669-4795-9bad-21182e455ab9 · outbound

This paper cites The Shakura-Sunyaev Viscosity Prescription with Variable alpha(r).

Transport Properties of the MRI in Differentially Rotating Neutron Stars The Shakura-Sunyaev Viscosity Prescription with Variable alpha(r)

Reference 55

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.789115Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T14:28:12.789115Z digest=sha256:e059eff09f01afc80af004271d91cbc440d08bf531669cb288eb40421a2e6318

Observation c2bbc7ae-c054-4c96-9dff-c050c7385153 · outbound

This paper cites Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model

Reference 56

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.794244Z

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source=pdf_text observed=2026-07-31T14:28:12.794244Z digest=sha256:132d5cc7ecddf3a5f8f6b2054a3f1426a8e20da52e3ae2099a5c33dc5c2954bd

Observation 7a4b7c28-4b18-4fd1-ade2-06b062f0f57c · outbound

This paper cites Radice and S.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Radice and S

Reference 57

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.798807Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.798807Z digest=sha256:a0d6d5d4e3cfcf9753e9672d932864b2cd9b6e72b1ec1b885f1b4ee55d35fbf5

Observation babd224b-dcb6-4066-a4f0-1d04a075308a · outbound

This paper cites Hayashi, S.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Hayashi, S

Reference 58

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.807182Z

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source=pdf_text observed=2026-07-31T14:28:12.807182Z digest=sha256:3a5a6b45cb56d3ef51021fc3270d02ac8fdbd492860908eb5a27161c85ed045f

Observation c83d5ddc-aa2a-4636-b077-ba279d852ace · outbound

This paper cites Turbulence modelling in neutron star merger simulations.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Turbulence modelling in neutron star merger simulations

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.811823Z

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source=pdf_text observed=2026-07-31T14:28:12.811823Z digest=sha256:15d12b0edb832de3188ed9d6cdf42de5b5c5a94fa04d9e6ed3d7019a308a841e

Observation 0607d643-56e9-4e9d-a9ed-46e7a87d1efa · outbound

This paper cites GR-Athena++: General-relativistic magnetohydrodynamics simulations of neutron star spacetimes.

Transport Properties of the MRI in Differentially Rotating Neutron Stars GR-Athena++: General-relativistic magnetohydrodynamics simulations of neutron star spacetimes

Reference 60

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.816445Z

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source=pdf_text observed=2026-07-31T14:28:12.816445Z digest=sha256:b9d7a123e55635005fa15a15c0c8e210151c8043436ce3e9d450ce85ef83d3f2

Observation b80bc198-ed01-4c04-bab5-7ec1edc83c34 · outbound

This paper cites GRAthena++: puncture evolutions on vertex-centered oct-tree AMR.

Transport Properties of the MRI in Differentially Rotating Neutron Stars GRAthena++: puncture evolutions on vertex-centered oct-tree AMR

Reference 61

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.821600Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.821600Z digest=sha256:044fd6759fbdce4baea755dd5104526af35173bb5f31fa71f3a0b37eb0692a67

Observation eedd2fa8-2bc2-467f-b33b-ca50adf8863f · outbound

This paper cites GR-Athena++: magnetohydrodynamical evolution with dynamical space-time.

Transport Properties of the MRI in Differentially Rotating Neutron Stars GR-Athena++: magnetohydrodynamical evolution with dynamical space-time

Reference 62

Resolution
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no resolver link, observed 2026-07-31T14:28:12.826748Z

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source=pdf_text observed=2026-07-31T14:28:12.826748Z digest=sha256:515587ef6b5d5628e3b1f2977dc78eb147424810f2b8cec4998bdc6e9638990e

Observation 4f3afdeb-2949-4a39-ba71-19a1558ea003 · outbound

This paper cites Daszuta, S.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Daszuta, S

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no resolver link, observed 2026-07-31T14:28:12.831628Z

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source=pdf_text observed=2026-07-31T14:28:12.831628Z digest=sha256:322bb44ed0bc202b6c00f71664791e57bc5512c0fe9808832380135ddfd1736e

Observation 3619cbe0-a696-4bcc-ad89-da9be4411149 · outbound

This paper cites General relativistic magnetohydrodynamics simulations for binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars General relativistic magnetohydrodynamics simulations for binary neutron star mergers

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-07-31T14:30:53.694193Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-31T14:28:12.837726Z digest=sha256:bc04ae98a7e9cd381f5416d293de8de468eaa8af1e2cf412c562cd968c59f777

Observation f3226d7a-77fd-46a2-92ac-fc81b2ab389d · outbound

This paper cites General-Relativistic Magnetohydrodynamic Equations: the bare essential.

Transport Properties of the MRI in Differentially Rotating Neutron Stars General-Relativistic Magnetohydrodynamic Equations: the bare essential

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source=pdf_text observed=2026-07-31T14:28:12.842704Z digest=sha256:d07a8f0eb4dc1db0129628cf2d295e39ce3b841b668250a914aec3f33b7d733d

Observation c967d10f-8e67-407f-894f-df6e13a2167f · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 66

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source=pdf_text observed=2026-07-31T14:28:12.848324Z digest=sha256:b802cc2d4dd41b749077fda93aa1a4c98541105dba4331bfd2380ce9349761a0

Observation 57de2109-305a-4431-aad3-16f26e2b6cd3 · outbound

This paper cites Rezzolla and O.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Rezzolla and O

Reference 67

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source=pdf_text observed=2026-07-31T14:28:12.854532Z digest=sha256:0db6b1ed7a82b825b698d66a57f11c2aa7c9fc22bfb8c578b343c8b0f9612516

Observation ca3eb1fe-013b-45a2-b31d-d320a96162f3 · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 68

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unresolved
no resolver link, observed 2026-07-31T14:28:12.863478Z

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source=pdf_text observed=2026-07-31T14:28:12.863478Z digest=sha256:1c2a8de92667e53fab574472a2ee50bf62a2f695f48a241bcc8ad3424fb25bb3

Observation 2425da85-973b-43c2-a747-5df7a7f36e8c · outbound

This paper cites Turbulence in Magnetised Neutron Stars.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Turbulence in Magnetised Neutron Stars

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.869935Z

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source=pdf_text observed=2026-07-31T14:28:12.869935Z digest=sha256:94163a31096e98900fcfaf8fde8660647cd85223e4b570534b9cd345da5ad9d9

Observation d8edbee3-0b0f-4c5e-8fc9-8f54ed0389b3 · outbound

This paper cites Rotating Stars in Relativity.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Rotating Stars in Relativity

Reference 70

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.876647Z

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source=pdf_text observed=2026-07-31T14:28:12.876647Z digest=sha256:5e76a6f126f509450aa5aed80b79aa184075e03a2cff2042af9953f040c5974d

Observation 0f49121f-ad68-4e62-95ba-da6ce64dcb91 · outbound

This paper cites Frank, A.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Frank, A

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.881730Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.881730Z digest=sha256:619cbb0195e714f254bc2e4f6d5d33e334b2938d9eda832e86ea0e992e83c9c5

Observation 9efbf913-9712-42f0-b69b-802324ce1e59 · outbound

This paper cites Relativistic Magnetohydrodynamics In Dynamical Spacetimes: Numerical Methods And Tests.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Relativistic Magnetohydrodynamics In Dynamical Spacetimes: Numerical Methods And Tests

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.887380Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.887380Z digest=sha256:c08dc6a775842de48ad1f6b58bc7e3caf1ab2473f3d2d99c122260aeb5bb4eef

Observation d8d00e78-7405-4881-b915-c42d3ab04f63 · outbound

This paper cites Dependence of inner accretion disk stress on parameters: the Schwarzschild case.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Dependence of inner accretion disk stress on parameters: the Schwarzschild case

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.892968Z

Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.892968Z digest=sha256:381e2878949677dff67ed32ab0f5545aae463f470fbae23a813d4ffe9dce993b

Observation 5dbdba12-c48c-4469-bedc-274245ed57a6 · outbound

This paper cites Assessing Quantitative Results in Accretion Simulations: From Local to Global.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Assessing Quantitative Results in Accretion Simulations: From Local to Global

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.901359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T14:28:12.901359Z digest=sha256:3b00ead90665d6af8ae12ff8398b4c2e0590de4eaf8e99e287dd823c27b1affa

Observation 85d7c9dd-b66d-4e1a-9710-ff7363b1beb0 · outbound

This paper cites Testing Convergence for Global Accretion Disks.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Testing Convergence for Global Accretion Disks

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.906620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T14:28:12.906620Z digest=sha256:58ae9942993f7a40e485f1d274fccc3d94da82af3ea7f297b053dcd742180e76

Observation c1c0554a-9203-4d17-9a6b-f441b3990ece · outbound

This paper cites Termination of the magnetorotational instability via parasitic instabilities in core-collapse supernovae.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Termination of the magnetorotational instability via parasitic instabilities in core-collapse supernovae

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.912528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T14:28:12.912528Z digest=sha256:19df22f22370ba8ca99dc417b08e3ee52bb87972249c28bf6748d0f08104b463

Observation 2990b55e-1b0f-48fc-894f-84680a4fc4b2 · outbound

This paper cites Miravet-Tenés, M.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Miravet-Tenés, M

Reference 77

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.922450Z

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source=pdf_text observed=2026-07-31T14:28:12.922450Z digest=sha256:accb0fb14cede6f41d993bc85cfb775d6a6617a395cf6f068c6d4ca22da8bdad

Observation 4f4f391e-7acc-4d11-a55d-a76a8216baec · outbound

This paper cites Sagaut and C.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Sagaut and C

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Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:12.927561Z

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source=pdf_text observed=2026-07-31T14:28:12.927561Z digest=sha256:5009aa45bdb9eecb2ed3677a92c5656b5d264899d1d23e276e4c7e74a576d7f5

Observation 53a07439-9e84-4e53-b32b-cc80872e01d2 · outbound

This paper cites GRMHD large eddy simulations with gradient subgrid-scale model.

Transport Properties of the MRI in Differentially Rotating Neutron Stars GRMHD large eddy simulations with gradient subgrid-scale model

Reference 79

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source=pdf_text observed=2026-07-31T14:28:12.934165Z digest=sha256:ef80e8aeb1d99ca8f0db9052c89a585e0199ec6c6b1fbddacab169aa6354c00d

Observation 0fa7d01f-eccf-4ec0-a55d-e2d549a9f52b · outbound

This paper cites Universality of the turbulent magnetic field in hypermassive neutron stars produced by binary mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Universality of the turbulent magnetic field in hypermassive neutron stars produced by binary mergers

Reference 80

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source=pdf_text observed=2026-07-31T14:28:12.939397Z digest=sha256:c0d44e34e27356065eb08698f1f1a3cc89000d3cbf67cd03b6ff9374b9cd20a3

Observation 83403343-e42e-47e0-be54-b3b7f631f072 · outbound

This paper cites Large Eddy Simulations of Magnetized Mergers of Black Holes and Neutron Stars.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Large Eddy Simulations of Magnetized Mergers of Black Holes and Neutron Stars

Reference 81

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source=pdf_text observed=2026-07-31T14:28:12.947615Z digest=sha256:31a43ac54bd5cf27207bc36e81d2bc67d692deb16f5a0daef7dec7d5e4510e5e

Observation b153cbe5-b917-4a42-9919-935ad71bb8b7 · outbound

This paper cites Long-term evolution of neutron-star merger remnants in general relativistic resistive-magnetohydrodynamics with a mean-field dynamo term.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Long-term evolution of neutron-star merger remnants in general relativistic resistive-magnetohydrodynamics with a mean-field dynamo term

Reference 82

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source=pdf_text observed=2026-07-31T14:28:12.953062Z digest=sha256:fada1e3cc24305130c1f25eb48f133397d4f7002af6a85e0c286b96e15ef4ae8

Observation 16e3039c-9262-4227-8124-c1b425a98696 · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 83

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Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:12.959713Z digest=sha256:63e00d6e9e42085643bd2e3799ced5e55cd33269479735374cf122973a593b88

Observation 57722772-acf0-495d-a761-82fee96b7c89 · outbound

This paper cites Kato and J.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Kato and J

Reference 84

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source=pdf_text observed=2026-07-31T14:28:12.965755Z digest=sha256:c3bc1d4d53363ffb09494d0889f6f49ef537d20a2d4a6e420c21d2dbde22890e

Observation 149099c9-35f1-4b29-b89a-a9a1eb67412e · outbound

This paper cites Prandtl,Report on Investigation of Developed Turbu- lence, Tech.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Prandtl,Report on Investigation of Developed Turbu- lence, Tech

Reference 85

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source=pdf_text observed=2026-07-31T14:28:12.972554Z digest=sha256:277b048eb707dceed0e2be6b913c7dfe8d26be59357344cfbb77c3f437d33a39

Observation c6c53ce3-0002-4df5-b4a1-fdb1e07b7d5f · outbound

This paper cites Astrophysical magnetic fields and nonlinear dynamo theory.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Astrophysical magnetic fields and nonlinear dynamo theory

Reference 86

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source=pdf_text observed=2026-07-31T14:28:12.978861Z digest=sha256:ea72c80555cd217f6d1601367d0c8268bc4c68679e15f68f0ac633f9227cb897

Observation 25f5ce28-ec32-44c0-b113-eff9282f8f6b · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 87

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no resolver link, observed 2026-07-31T14:28:12.984872Z

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source=pdf_text observed=2026-07-31T14:28:12.984872Z digest=sha256:cfd659cf7b24ccd16f2e8aae5b3e104fd0afa42058275e4a51589a2cc0eb0cd2

Observation 01f0948e-a935-4642-958c-07e661126077 · outbound

This paper cites Krause and K.-H.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Krause and K.-H

Reference 88

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no resolver link, observed 2026-07-31T14:28:12.990610Z

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source=pdf_text observed=2026-07-31T14:28:12.990610Z digest=sha256:e4ac405931c3fe0a2a1165f198385f5bd8819b4b269ef3b9ba3b31ce84f7d5d9

Observation 29c3ec09-53b5-4932-b303-75c122313b1b · outbound

This paper cites Impact of a mean field dynamo on neutron star mergers leading to magnetar remnants.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Impact of a mean field dynamo on neutron star mergers leading to magnetar remnants

Reference 89

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source=pdf_text observed=2026-07-31T14:28:12.996066Z digest=sha256:5c5f5506ca64f70fe6bd396fd26c235997c21090aa7f50c37cebc42e4e6e92e6

Observation b64b57bb-5b43-415c-94a7-f37bf390a394 · outbound

This paper cites Smagorinsky, General circulation experiments with the primitive equations.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Smagorinsky, General circulation experiments with the primitive equations

Reference 90

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source=pdf_text observed=2026-07-31T14:28:13.001520Z digest=sha256:c61f78b7aa9eabc44d8ed6a5231d4524bb41f45d277090f2ee0389712fa1a7f0

Observation f5e82b43-c29f-4c21-bb16-28346de94c73 · outbound

This paper cites Hanauske, K.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Hanauske, K

Reference 91

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source=pdf_text observed=2026-07-31T14:28:13.007792Z digest=sha256:f7e59cd99b21b388e76fad7f7b686f435065c98509024a17749974bd41aa8239

Observation 9590a51f-68d0-41a6-aaf9-863b90d5df2a · outbound

This paper cites Ury¯ u, A.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Ury¯ u, A

Reference 92

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verified exact
doi, observed 2026-07-31T14:30:53.420328Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-31T14:28:13.012629Z digest=sha256:0246e3ea31e82f841c5df85c4c99c58ebebdef8e58ca9812a05e4785fdf2fd6b

Observation 55697e2b-d709-463e-af51-45967e2a000a · outbound

This paper cites Masking equation of state effects in binary neutron star mergers.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Masking equation of state effects in binary neutron star mergers

Reference 93

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source=pdf_text observed=2026-07-31T14:28:13.019307Z digest=sha256:dea11e52eb379706a260f6bb502b961b8655e0cc2858a60c26430f611b599eff

Observation ca0a9a2e-33c0-41ad-ae03-cb8c5dde36d6 · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 94

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source=pdf_text observed=2026-07-31T14:28:13.026433Z digest=sha256:ac971ceb09188ffeb998f6748e24c070e045abf4acab0490219dce07bc567c7c

Observation c01b920b-0b02-4082-8b58-0e894a98771a · outbound

This paper cites An Extension of the Athena++ Code Framework for GRMHD Based on Advanced Riemann Solvers and Staggered-Mesh Constrained Transport.

Transport Properties of the MRI in Differentially Rotating Neutron Stars An Extension of the Athena++ Code Framework for GRMHD Based on Advanced Riemann Solvers and Staggered-Mesh Constrained Transport

Reference 95

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Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:13.031870Z digest=sha256:d5d8e29fc612e8ac8ccd8bdee7d4cb0778ef0759a0fba24a0dbd637875d1c188

Observation ac98fe9a-43a5-4e37-94e0-b11936ac83fb · outbound

This paper cites an unresolved cited work.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Unresolved cited work

Reference 96

Resolution
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no resolver link, observed 2026-07-31T14:28:13.038143Z

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source=pdf_text observed=2026-07-31T14:28:13.038143Z digest=sha256:f474e1539549152614568cccc2edb53c87678d47f866f611a206b1db22a43e9f

Observation fcb17d0d-fcc6-4e50-84ac-813c52f42aa6 · outbound

This paper cites Giacomazzo and L.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Giacomazzo and L

Reference 97

Resolution
unresolved
no resolver link, observed 2026-07-31T14:28:13.056147Z

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source=pdf_text observed=2026-07-31T14:28:13.056147Z digest=sha256:806f21649e72da1bf4958288a7fda11e826c41c802387638132c0cc6e9cb810f

Observation 33314d9f-8e44-44be-ab1e-9b5d75294469 · outbound

This paper cites General relativistic viscous hydrodynamics of differentially rotating neutron stars.

Transport Properties of the MRI in Differentially Rotating Neutron Stars General relativistic viscous hydrodynamics of differentially rotating neutron stars

Reference 98

Resolution
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no resolver link, observed 2026-07-31T14:28:13.065394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T14:28:13.065394Z digest=sha256:0652a98982c42754d715323f60cbe6291f200af9b524d2ff495d47170880e265

Observation dd2570b1-6b84-4ddb-84fd-f3a9906f5c96 · outbound

This paper cites Delayed jet launching in binary neutron star mergers with realistic initial magnetic fields.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Delayed jet launching in binary neutron star mergers with realistic initial magnetic fields

Reference 99

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Source-reported events for the cited work

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source=pdf_text observed=2026-07-31T14:28:13.078424Z digest=sha256:21b5cd1d98746d2d2362bcfb53f80a1ba60e609c976d9bf67aef36d87b3f4673

Observation c385f702-1a45-4a9b-9e4b-febc5958cee3 · outbound

This paper cites Bamber, A.

Transport Properties of the MRI in Differentially Rotating Neutron Stars Bamber, A

Reference 100

Resolution
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source=pdf_text observed=2026-07-31T14:28:13.085029Z digest=sha256:18f0e192b1170621919633ac31c3712a538ee8b2a4bdfab96b3f9e769aff93a2

Pith citing papers

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