Published November 24, 2010
| Version v1
Journal article
Shell Model Two Body Matrix Elements Calculations for the Neutrinoless Double Beta Decay of 48Ca
Creators
- 1. Horia Hulubei National Institute for Physics and Nuclear Engineering (IFIN-HH) 407 Atomistilor, Magurele-Bucharest 077125 (Romania)
Description
In this paper we present two Shell Model approaches for computing the two-body matrix elements involved in the neutrinoless double beta decay of 48Ca. One of the methods involves integration of the radial part over the momentum space, while the other only requires computations in the coordinate space. This has an influence in the complexity of the numerical approach and the necessary computation time. We will explain how this reflects into the obtained results, pointing out the advantages and the limitations of each method.
Additional details
Identifiers
- DOI
- 10.1063/1.3527234;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1304
- Journal Issue
- 1
- Journal Page Range
- p. 406-410
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- From nuclei to stars
- Acronym
- Carpathian summer school of physics - Exotic nuclei and nuclear/particle astrophysics (III)
- Dates
- 20 Jun - 3 Jul 2010
- Place
- Sinaia (Romania)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42099762
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CALCIUM 48; CALCULATION METHODS; DOUBLE BETA DECAY; MATRIX ELEMENTS; NEUTRINOS; NUCLEONS; SHELL MODELS; TWO-BODY PROBLEM; WAVE FUNCTIONS
- Descriptors DEC
- ALKALINE EARTH ISOTOPES; BARYONS; BETA DECAY; BETA-MINUS DECAY; CALCIUM ISOTOPES; DECAY; ELEMENTARY PARTICLES; EVEN-EVEN NUCLEI; FERMIONS; FUNCTIONS; HADRONS; INTERMEDIATE MASS NUCLEI; ISOTOPES; LEPTONS; MANY-BODY PROBLEM; MASSLESS PARTICLES; MATHEMATICAL MODELS; NUCLEAR DECAY; NUCLEAR MODELS; NUCLEI; STABLE ISOTOPES
Optional Information
- Notes
- (c) 2010 American Institute of Physics