DEL ZANNA, LUCA

DEL ZANNA, LUCA  

Fisica e Astronomia  

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Risultati 1 - 20 di 124 (tempo di esecuzione: 0.05 secondi).
Titolo Data di pubblicazione Autore(i) File
2D relativistic MHD simulations of PWNe: Preliminary results 2004 E. Amato;L. Del Zanna;N. Bucciantini
3D Relativistic MHD Simulations of Pulsar Bow Shock Nebulae 2020 Bucciantini N.; Olmi B.; Del Zanna L.
A constrained transport method for the solution of the resistive relativistic MHD equations 2019 Mignone, A; Mattia, G; Bodo, G; Del Zanna, L
A fourth-order accurate finite volume scheme for resistive relativistic MHD 2024 Mignone, A.; Berta, V.; Rossazza, M.; Bugli, M.; Mattia, G.; Del Zanna, L.; Pareschi, L.
A fully covariant mean-field dynamo closure for numerical 3 + 1 resistive GRMHD 2013 Bucciantini, N.; Del Zanna, L.
A GPU-Accelerated Modern Fortran Version of the ECHO Code for Relativistic Magnetohydrodynamics 2024 Del Zanna, Luca; Landi, Simone; Serafini, Lorenzo; Bugli, Matteo; Papini, Emanuele
A perturbative approach to the hydrodynamics of heavy ion collisions 2014 S. Floerchinger; U.A. Wiedemann; A. Beraudo; L. Del Zanna; G. Inghirami; V. Rolando
A simple and efficient high-resolution shock-capturing method for relativistic fluid dynamics 2003 N. Bucciantini; L. Del Zanna
A steady flow model for quiescent prominences 1996 L. DEL ZANNA; A. HOOD
A study of vorticity formation in high energy nuclear collisions 2015 Becattini, F.; Inghirami, G.; Rolando, V.; Beraudo, A.; Del Zanna, L.; De Pace, A.; Nardi, M.; Pagliara, G.; Chandra, V.
A third order shock-capturing code for relativistic 3-D MHD 2003 L. Del Zanna; N. Bucciantini; P. Londrillo
Activation of MHD reconnection on ideal timescales 2017 Landi, S.; Papini, E.; Del Zanna, L.; Tenerani, A.; Pucci, F.
Amplification of magnetic fields in accretion discs by GRMHD dynamo 2020 Tomei N.; Del Zanna L.; Bugli M.; Bucciantini N.
An efficient shock-capturing central-type scheme for multidimensional relativistic flows - I. Hydrodynamics 2002 L. DEL ZANNA; N. BUCCIANTINI
An efficient shock-capturing central-type scheme for multidimensional relativistic flows. II. Magnetohydrodynamics 2003 L. DEL ZANNA; N. BUCCIANTINI; P. LONDRILLO
An MHD model for solar coronal plumes 1997 L. DEL ZANNA; A. HOOD; A. LONGBOTTOM
Are GRMHD Mean-Field Dynamo Models of Thick Accretion Disks SANE? 2021 Niccolò Tomei; Luca Del Zanna; Matteo Bugli; Niccolo' Bucciantini
Axially symmetric relativistic MHD simulations of Pulsar Wind Nebulae in Supernova Remnants 2004 L. DEL ZANNA; E. AMATO; N. BUCCIANTINI
Axisymmetric equilibrium models for magnetised neutron stars in scalar-tensor theories 2020 Soldateschi J.; Bucciantini N.; Del Zanna L.
Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition 2014 Pili, A. G.; Bucciantini, N.; Del Zanna, L.