Abstract
The lectures are primarily addressed to Ph.D. students in Theoretical Nuclear and Hadronic Physics. Participation of experimentalists and post-docs is also encouraged. The goal of the lectures is to provide a pedagogical introduction to the basic concepts and tools needed for research in nuclear structure and nuclear reactions. The ingredients of modern theories suited to investigate the behavior of normal to exotic nuclei will be presented. A part of the lectures will also illustrate how nuclear properties evolve when heating nuclei and, more generally, the response of nuclear matter in several conditions of density and temperature, as encountered in compact stellar objects.

Organizers
Francesco Becattini (University of Firenze) - Ignazio Bombaci (University of Pisa) - Angela Bonaccorso (INFN - Pisa) - Giampaolo Co (Unisalento - Lecce) - Maria Colonna (INFN - LNS) - Gianni Salmè (INFN - Roma1) - Elena Santopinto (INFN - Genova) - Enrico Vigezzi (INFN - Milano)

Website
http://poincare.unisalento.it/ggi/




Lecturers


Michele Viviani (Pisa),Luigi Coraggio, (Napoli):
From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei.

Dario Vretenar (Zagreb, Croatia):
Many-body methods: from normal to exotic nuclei.

Francesca Gulminelli (Caen, France):
Thermal properties of nuclear systems.

Carlos Bertulani (Commerce, Texas, USA):
Nuclear structure information from peripheral reactions.

Fridolin Weber (San Diego, CA, USA)
Physics of Neutron Stars .


Talks

Date	Speaker	Title	Type	Useful Links
Feb 24, 2014 - 10:00	Michele Viviani	From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei. I	Lecture		Slides
Feb 24, 2014 - 14:00	Dario Vretenar	Many-body methods: from normal to exotic nuclei. I	Lecture		Slides
Feb 25, 2014 - 10:00	Michele Viviani	From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei. II	Lecture
Feb 25, 2014 - 14:00	Dario Vretenar	Many-body methods: from normal to exotic nuclei. II	Lecture
Feb 26, 2014 - 10:00	Michele Viviani	From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei. III	Lecture
Feb 26, 2014 - 11:00	Luigi Coraggio	From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei. III	Lecture		Slides
Feb 26, 2014 - 14:00	Dario Vretenar	Many-body methods: from normal to exotic nuclei. III	Lecture
Feb 27, 2014 - 11:00	Dario Vretenar	Many-body methods: from normal to exotic nuclei. IV	Lecture
Feb 27, 2014 - 11:00	Francesca Gulminelli	Thermal properties of nuclear systems. I	Lecture		Slides
Feb 27, 2014 - 14:00	Luigi Coraggio	From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei. IV	Lecture
Feb 28, 2014 - 10:00	Francesca Gulminelli	Thermal properties of nuclear systems. II	Lecture
Feb 28, 2014 - 11:00	Dario Vretenar	Many-body methods: from normal to exotic nuclei. V	Lecture
Feb 28, 2014 - 14:00	Luigi Coraggio	From nucleon-nucleon to nucleon-nucleus interactions: from light to heavy nuclei. V	Lecture
Mar 03, 2014 - 09:00	Francesca Gulminelli	Thermal properties of nuclear systems. III	Lecture
Mar 03, 2014 - 11:00	Carlos Bertulani	Nuclear structure information from peripheral reactions. I	Lecture		Slides
Mar 03, 2014 - 14:00	Fridolin Weber	Physics of Neutron Stars. I	Lecture		Slides
Mar 04, 2014 - 09:00	Fridolin Weber	Physics of Neutron Stars. II	Lecture		Slides
Mar 04, 2014 - 11:00	Francesca Gulminelli	Thermal properties of nuclear systems. IV	Lecture
Mar 04, 2014 - 14:00	Carlos Bertulani	Nuclear structure information from peripheral reactions. II	Lecture
Mar 05, 2014 - 10:00	Carlos Bertulani	Nuclear structure information from peripheral reactions. III	Lecture
Mar 05, 2014 - 14:00	Fridolin Weber	Physics of Neutron Stars. III	Lecture
Mar 05, 2014 - 16:00	Massimiliano Razzano	High-energy pulsars in the Fermi era	Seminar	Abstract High-energy pulsars in the Fermi era In its first five years of operations, the Fermi Gamma-ray Space Telescope has revolutionized our view of the gamma-ray Universe. Thanks to its unprecedented performance, Fermi has detected about two thousand sources and unveiled new classes of gamma-ray emitters. In particular, pulsars are the main contributors to the gamma-ray source population in our Galaxy and are relevant not only to Astrophysics. In fact, they are excellent natural laboratories to probe the laws of Physics under extreme conditions, e.g. of gravity and elecromagnetic fields. I will review the recent Fermi results on pulsars and how they are helping us to understand the physics of neutron stars and their magnetospheres.
Mar 06, 2014 - 10:00	Fridolin Weber	Physics of Neutron Stars. IV	Lecture
Mar 06, 2014 - 14:00	Carlos Bertulani	Nuclear structure information from peripheral reactions. IV	Lecture
Mar 07, 2014 - 09:00	Carlos Bertulani	Nuclear structure information from peripheral reactions. V	Lecture
Mar 07, 2014 - 11:00	Fridolin Weber	Physics of Neutron Stars. V	Lecture