Nuclear physics midterm plan at LNS

Author:

Agodi C.,Cappuzzello F.,Cardella G.,Cirrone G. A. P.,De Filippo E.,Di Pietro A.,Gargano A.,La Cognata M.,Mascali D.,Milluzzo G.,Nania R.,Petringa G.,Pidatella A.,Pirrone S.,Pizzone R. G.,Rapisarda G. G.,Sergi M. L.,Tudisco S.,Valiente-Dobón J. J.,Vardaci E.,Abramczyk H.,Acosta L.,Adsley P.,Amaducci S.,Banerjee T.,Batani D.,Bellone J.,Bertulani C.,Biri S.,Bogachev A.,Bonanno A.,Bonasera A.,Borcea C.,Borghesi M.,Bortolussi S.,Boscolo D.,Brischetto G. A.,Burrello S.,Busso M.,Calabrese S.,Calinescu S.,Calvo D.,Capirossi V.,Carbone D.,Cardinali A.,Casini G.,Catalano R.,Cavallaro M.,Ceccuzzi S.,Celona L.,Cherubini S.,Chieffi A.,Ciraldo I.,Ciullo G.,Colonna M.,Cosentino L.,Cuttone G.,D’Agata G.,De Gregorio G.,Degl’Innocenti S.,Delaunay F.,Di Donato L.,Di Nitto A.,Dickel T.,Doria D.,Ducret J. E.,Durante M.,Esposito J.,Farrokhi F.,Fernandez Garcia J. P.,Figuera P.,Fisichella M.,Fulop Z.,Galatá A.,Galaviz Redondo D.,Gambacurta D.,Gammino S.,Geraci E.,Gizzi L.,Gnoffo B.,Groppi F.,Guardo G. L.,Guarrera M.,Hayakawa S.,Horst F.,Hou S. Q.,Jarota A.,José J.,Kar S.,Karpov A.,Kierzkowska-Pawlak H.,Kiss G. G.,Knyazheva G.,Koivisto H.,Koop B.,Kozulin E.,Kumar D.,Kurmanova A.,La Rana G.,Labate L.,Lamia L.,Lanza E. G.,Lay J. A.,Lattuada D.,Lenske H.,Limongi M.,Lipoglavsek M.,Lombardo I.,Mairani A.,Manetti S.,Marafini M.,Marcucci L.,Margarone D.,Martorana N. S.,Maunoury L.,Mauro G. S.,Mazzaglia M.,Mein S.,Mengoni A.,Milin M.,Mishra B.,Mou L.,Mrazek J.,Nadtochy P.,Naselli E.,Nicolai P.,Novikov K.,Oliva A. A.,Pagano A.,Pagano E. V.,Palmerini S.,Papa M.,Parodi K.,Patera V.,Pellumaj J.,Petrone C.,Piantelli S.,Pierroutsakou D.,Pinna F.,Politi G.,Postuma I.,Prajapati P.,Prada Moroni P. G.,Pupillo G.,Raffestin D.,Racz R.,Reidel C.-A.,Rifuggiato D.,Risitano F.,Rizzo F.,Roca Maza X.,Romano S.,Roso L.,Rotaru F.,Russo A. D.,Russotto P.,Saiko V.,Santonocito D.,Santopinto E.,Sarri G.,Sartirana D.,Schuy C.,Sgouros O.,Simonucci S.,Sorbello G.,Soukeras V.,Spartá R.,Spatafora A.,Stanoiu M.,Taioli S.,Tessonnier T.,Thirolf P.,Tognelli E.,Torresi D.,Torrisi G.,Trache L.,Traini G.,Trimarchi M.,Tsikata S.,Tumino A.,Tyczkowski J.,Yamaguchi H.,Vercesi V.,Vidana I.,Volpe L.,Weber U.

Abstract

AbstractThe next years will see the completion of several new facilities at Istituto Nazionale di Fisica Nucleare – Laboratori Nazionali del Sud (LNS) opening up new possibilities in the fields of nuclear structure, nuclear dynamics, nuclear astrophysics and applications. These include a new line for high-intensity cyclotron beams, a new facility for in-flight production of radioactive ion beams, the PANDORA plasma trap for multidisciplinary studies and a high-power laser for basic science and applied physics. The nuclear physics community has organized a workshop to discuss the new physics opportunities that will be possible in the middle term (5–7 years) by employing state-of-the-art detection systems. A detailed discussion of the outcome from the workshop is presented in this report.

Funder

Università degli Studi di Catania

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy,Fluid Flow and Transfer Processes

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