Description
Welcome address; first talks on nuclear physics
Prof.
André Martin
(CERN, Geneva, Switzerland)
13/10/2008, 09:00
Normal
This welcome address will briefly present the Ettora Ma jorana Centre for Scientific Culture
of Erice, and stress the importance of quantum few-body systems at the edge of stability.
Prof.
Eduardo Garrido
(Instituto de Estructura de la Materia, CSIC, Madrid, Spain)
13/10/2008, 09:20
Talks at Critical Stability V (Erice, October 2008)
Normal
Stellar nucleosynthesis reactions are responsible for the abundances of the different
elements in the Universe. These reactions happen at very low relative energies between the
nuclei involved, and the calculation of the corresponding production rates is one
of major issues in Nuclear Astrophysics. These reactions can be of different nature (radiative
capture, rearrangement processes...)...
Prof.
Avraham Gal
(Racah Institute of Physics, Hebrew University, Jerusalem)
13/10/2008, 09:55
Talks at Critical Stability V (Erice, October 2008)
Normal
It takes two nucleons to bind a Lambda hyperon, and perhaps as many as three nucleons to bind two Lambda hyperons. In my talk I will review few-body calculations which are relevant for deciphering the onset of binding in Lambda hypernuclei and in Lambda-Lambda hypernuclei.
I will also discuss the onset of binding for Xi hyperons, stabilizing them against the free-space
conversion Xi + N...
Dr
Christian Forssén
(Chalmers University of Technology)
13/10/2008, 10:45
Talks at Critical Stability V (Erice, October 2008)
Normal
The ab initio no-core shell model (NCSM) is a well-established theoretical framework aimed at an exact description of nuclear structure starting from high precision interactions between the nucleons [1,2].
The principal foundation of the method is the use of effective interactions appropriate for the large, but finite, harmonic-oscillator model spaces employed in the calculations. These...
Prof.
Oleg O. I. Kartavtsev
(Dubna, Russia)
13/10/2008, 11:20
Talks at Critical Stability V (Erice, October 2008)
Normal
During the recent years, there is a continuous interest to the experimental and theoretical
study of the 12 C nucleus [1, 2, 3, 4]. In this respect, of special importance is the description
of the Hoyle state, which was predicted more then 50 years ago merely from the abundance
of elements in the universe. Whereas the Hoyle state is fairly well studied experimentally,
e. g., its...
