scholarly journals Recent developments in no-core shell-model calculations

2009 ◽  
Vol 36 (8) ◽  
pp. 083101 ◽  
Author(s):  
Petr Navrátil ◽  
Sofia Quaglioni ◽  
Ionel Stetcu ◽  
Bruce R Barrett
2012 ◽  
Vol 387 ◽  
pp. 012016
Author(s):  
T Dytrych ◽  
K D Launey ◽  
J P Draayer ◽  
D Langr

2019 ◽  
Vol 55 (12) ◽  
Author(s):  
M. K. G. Kruse ◽  
W. E. Ormand ◽  
C. W. Johnson

2007 ◽  
Vol 16 (02) ◽  
pp. 552-560 ◽  
Author(s):  
E. CAURIER ◽  
F. NOWACKI ◽  
A. POVES

The determination of accurate nuclear matrix elements for ββ decay processes is a challenge for nuclear theory and can have a strong impact in neutrino physics. Large Scale Shell Model (LSSM) calculations are among the best tools for such determination and recent developments have allowed to extend its application domains. In particular, systematic studies of nuclear matrix elements calculations have been now undertaken in this framework for most of the ββ emitters. These calculations are crucial in the determination of the most favorable emitters in the forthcoming generation of ββ experiments. The present paper focuses on the recent advances and remaining difficulties of shell model calculations for the neutrinoless mode. Stability and predictive power of the results will be discussed.


2004 ◽  
Vol 746 ◽  
pp. 579-582 ◽  
Author(s):  
B.R. Barrett ◽  
P. Navrátil ◽  
A. Nogga ◽  
W.E. Ormand ◽  
J.P. Vary

Author(s):  
Archana Saxena ◽  
Praveen C Srivastava

Abstract We have calculated the energy spectra for neutron-rich $^{18-22}$N isotopes using the no-core shell model. To calculate the energy spectrum we have used three different $NN$ potentials: inside non-local outside Yukawa (INOY), next-to-next-to-next-leading order (N3LO) from chiral effective field theory, and charge-dependent Bonn 2000 (CDB2K). The INOY potential is a two-body interaction but also has the effect of three-body forces at short range and a non-local character present in it. The calculations have been done at $\hbar\Omega=20$ MeV, 14 MeV, and 12 MeV using INOY, N3LO, and CDB2K potentials, respectively. We have also performed shell model calculations with the YSOX interaction. The results with the INOY interaction show good agreement with the experimental data in comparison to the other three interactions. We have also shown the occupancy of different orbitals involved corresponding to the largest model space ($N_{\rm max} = 4$) in the calculations.


2006 ◽  
Vol 39 (32) ◽  
pp. 9983-9992 ◽  
Author(s):  
Bruce R Barrett ◽  
Ionel Stetcu ◽  
Petr Navrátil ◽  
James P Vary

1999 ◽  
Author(s):  
B. R. Barrett ◽  
P. Navrátil ◽  
M. J. Thoresen ◽  
W. E. Ormand

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