Erratum to: A study of vorticity formation in high energy nuclear collisions

Autor: F. Becattini, G. Inghirami, V. Rolando, A. Beraudo, L. Del Zanna, A. De Pace, M. Nardi, G. Pagliara, V. Chandra

Publikováno v: European Physical Journal C: Particles and Fields, Vol 78, Iss 5, Pp 1-4 (2018)

Due to an oversight of ours in proofreading and a communication problem with the publisher, the figures published in F. Becattini et al. Eur. Phys. J. C (2015) 75: 406 were not correct. This Erratum contains the correct figures as in arXiv 1501.04468

Externí odkaz: https://doaj.org/article/dc0f51a98f494a5c9c1094e523ecc006

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

Systematic construction of upwind constrained transport schemes for MHD

Autor: Andrea Mignone, L. Del Zanna

The constrained transport (CT) method reflects the state of the art numerical technique for preserving the divergence-free condition of magnetic field to machine accuracy in multi-dimensional MHD simulations performed with Godunov-type, or upwind, co

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96cf8502bcba3b3c0bc94ccb903f9870
http://hdl.handle.net/2318/1766300

General relativistic magnetohydrodynamic dynamo in thick accretion disks: fully nonlinear simulations

Autor: L. Del Zanna, Niccolò Tomei, Niccolò Bucciantini, Matteo Bugli

Publikováno v: Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 491 (2), pp.2346-2359. ⟨10.1093/mnras/stz3146⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 491 (2), pp.2346-2359. ⟨10.1093/mnras/stz3146⟩

The recent imaging of the M87 black hole at millimeter wavelengths by the Event Horizon Telescope (EHT) collaboration has triggered a renewed interest in numerical models for the accretion of magnetized plasma in the regime of general relativistic ma

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bab280923753a2186d3dc945eacad582
https://hal.archives-ouvertes.fr/hal-02432596

Papaloizou–Pringle instability suppression by the magnetorotational instability in relativistic accretion discs

Autor: Pedro J. Montero, Ewald Müller, Niccolò Bucciantini, L. Del Zanna, Jérôme Guilet, Matteo Bugli

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Monthly Notices of the Royal Astronomical Society, 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Mon.Not.Roy.Astron.Soc., 2018, 475, pp.108. 〈10.1093/mnras/stx3158〉

Geometrically thick tori with constant specific angular momentum have been widely used in the last decades to construct numerical models of accretion flows onto black holes. Such discs are prone to a global non-axisymmetric hydrodynamic instability,

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97a1486c35061c87e67fd0c776a3663d
https://doi.org/10.1093/mnras/stx3158