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Physical Review D

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Neutron star evolution with the Bemfica-Disconzi-Noronha-Kovtun viscous hydrodynamics framework

Harry L. H. Shum1,2, Fernando Abalos3,4, Yago Bea5, Miguel Bezares1,2, Pau Figueras6, and Carlos Palenzuela3,4

  • 1Nottingham Centre of Gravity, University of Nottingham, Nottingham NG7 2RD, United Kingdom
  • 2School of Mathematical Sciences, University of Nottingham, Nottingham, NG7 2RD, United Kingdom
  • 3Departament de Física, Universitat de les Illes Balears, Palma de Mallorca, E-07122, Spain
  • 4Institute of Applied Computing and Community Code (IAC3), Universitat de les Illes Balears, Palma de Mallorca, E-07122, Spain
  • 5Departament de Física Quàntica i Astrofísica and Institut de Ciències del Cosmos (ICC), Universitat de Barcelona, Martí i Franquès 1, ES-08028, Barcelona, Spain
  • 6School of Mathematical Sciences, Queen Mary University of London, Mile End Road, London E1 4NS, United Kingdom

Axial oscillations of viscous neutron stars

Sofía Bussières, Jaime Redondo-Yuste, José Javier Ortega Gómez, and Vitor Cardoso

Phys. Rev. D 114 044012 (2026)

Subgrid modeling for relativistic magnetohydrodynamics with machine learning

William Cook and Sebastiano Bernuzzi

Phys. Rev. D 114 063010 (2026)

Solving Bemfica-Disconzi-Noronha-Kovtun diffusion using physics-informed neural networks

Vicente Chomalí-Castro, Nick Clarisse, Nicki Mullins, and Jorge Noronha

Phys. Rev. D 114 076013 (2026)

Finite-volume scheme for first-order viscoresistive relativistic magnetohydrodynamics

Ruben Lier, Jay Armas, and Oliver Porth

Phys. Rev. D 114 083046 (2026)

Radial oscillations of viscous stars

Lennox S. Keeble and Jaime Redondo-Yuste

Phys. Rev. D 113 124058 (2026)

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