DATA: 02-02-2017

Seminario dr.ssa Martina Cardillo Cosmic-­‐Rays are very high energy particles, mainly rotons, that from their sources to Earth with a power-­law spectral distribution, energy of about 10^20 eV. Despite the great amount of data collected from their discovery (in 1912), we are not yet able to understand one of the most important issue: what is CR's origin Where are they accelerated? The best candidate as sources for the part of CR's spectrum up to energy of about 10^15 eV) are Supernova Remnants but there is the lack of a direct of CR's acceleration in theirshocks. Our work is focused on this topic. Our aim is a better understanding of the connectionbetween SNR and Galactic CRs through the development of realistic models that can explain experimental data from gamma-ray satellites and particle detectors. So far, the only thing that can be considered as certain is that, for the high-­energy astrophysics, “this is a tricky situation”


09-12-2019: Visita ai laboratori della Sezione INFN di Trieste da parte di studenti del Liceo Scientifico dell' IIS Cattaneo-Dall'Aglio di Castelnovo ne' Monti (RE)
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06-12-2019: From kaonic atoms to strangeness in neutron stars
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05-12-2019: A scuola di radioattivita'
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04-12-2019: Nuclei per l'ambiente
04-12-2019: A. Melchiorri - A crisis in lalalambda land?
02-12-2019: MariX: Conceptual Design Report of a Multi-disciplinary Advanced Research Infrastructure for the generation and application of X-rays
28-11-2019: Quantum Optical Control of Levitated Solids: a novel probe for the gravity-quantum interface





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