Published November 20, 2012 | Version v1
Journal article Metadata-only

Towards a study of the 22Ne(p,γ)23Na reaction at LUNA

Creators

  • 1. Helmholtz Zentrum Dresden-Rossendorf, Dresden (Germany)
  • 2. Dipartimento di fisica, Università di Padova, and INFN Sezione di Padova, Padova (Italy)
  • 3. Dipartimento di fisica, Università di Genova, and INFN Sezione di Genova, Genova (Italy)

Description

The 22Ne(p,γ)23Na reaction is a part of the hydrogen burning NeNa cycle. In second-generation stars hydrogen burning may proceed via this cycle. The rate of the 22Ne(p,γ)23Na reaction depends on the strength of several resonances in the energy range of the LUNA 400 kV accelerator which have never been observed in direct experiments. A related study is under preparation at LUNA.

Additional details

Identifiers

DOI
10.1063/1.4768510;

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1498
Journal Issue
1
Journal Page Range
p. 314-318
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Carpathian summer school of physics 2012
Dates
24 Jun - 7 Jul 2012
Place
Sinaia (Romania)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
44034903
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ASTROPHYSICS; CAPTURE; HYDROGEN BURNING; NEON 22 TARGET; NUCLEAR REACTION KINETICS; NUCLEOSYNTHESIS; PROTON REACTIONS; PROTONS; SODIUM 23; STARS
Descriptors DEC
BARYON REACTIONS; BARYONS; CHARGED-PARTICLE REACTIONS; ELEMENTARY PARTICLES; FERMIONS; HADRON REACTIONS; HADRONS; ISOTOPES; KINETICS; LIGHT NUCLEI; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; NUCLEONS; ODD-EVEN NUCLEI; PHYSICS; REACTION KINETICS; SODIUM ISOTOPES; STABLE ISOTOPES; STAR BURNING; SYNTHESIS; TARGETS

Optional Information

Notes
(c) 2012 American Institute of Physics
Collaborations
LUNA Collaboration