Arcetri High Energy Group 
Reserch Fields
The Group
The high-energy astrophysics group in Arcetri, was founded by F.Pacini, and is one of the leading italian reserch group in the field of non-thermal particle acceleration, cosmic rays, relativistic fluid dynamics, and supernova remnants. The group is mostly involved in theroretical modellign of astrophysical objects and processes, with a focus on numerical simulations. The various are involved in various projects at the national and internationa level, ranging from theoretical investigation of key astrophysical process to the developement of rthe science for the next generation gamma and X-ray telescopes. The group has a long standing collaboration with the Universita' di Firenze, and the local plasma physics group.
Ongoing Projects - Grants
ASI-INAF 2017: Attività di Studio per la comunità scientifica di Astrofisica delle Alte Energie e Fisica Astroparticellare
CTA-SKA project 2016: Probing particle acceleration and gamma-ray propagation with CTA and its precursor
PRIN 2015: Multi-scale Simulations of High-Energy Astrophysical Plasmas
CIPE 2016: High performance data network
Recent Papers
On the origin of jet-like features in bow shock pulsar wind nebulaeOlmi, B.; Bucciantini, N.
Accepted in MNRAS
Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: emission and polarization
Olmi, B.; Bucciantini, N.
MNRAS 488, 5690
The dust content of the Crab Nebula
De Looze, I.; Barlow, M. J.; Bandiera, R. et al.
MNRAS 488, 164
Exploring particle escape in supernova remnants through gamma rays
Celli, S.; Morlino, G.; Gabici, S.; Aharonian, F.
Accepted in MNRAS