Fragmentation of relativistic nuclei in peripheral interactions in nuclear track emulsion
Journal Article
·
· Physics of Atomic Nuclei
- Joint Institute for Nuclear Research (Russian Federation)
- Russian Academy of Sciences, Lebedev Institute of Physics (Russian Federation)
- Institute of Space Sciences (Romania)
- Institute of Physics (Armenia)
- Bulgarian Academy of Sciences, Institute of Nuclear Research and NuclearEnergy (Bulgaria)
The technique of nuclear track emulsions is used to explore the fragmentation of light relativistic nuclei down to the most peripheral interactions: nuclear 'white' stars. A complete pattern of the relativistic dissociation of a 8B nucleus with target fragment accompaniment is presented. Relativistic dissociation {sup 9}Be {yields} 2{alpha} is explored using significant statistics, and a relative contribution of {sup 8}Be decays from 0+ and 2+ states is established. Target fragment accompaniments are shown for relativistic fragmentation {sup 14}N {yields} 3He +H and {sup 22}Ne {yields} 5He. The leading role of the electromagnetic dissociation on heavy nuclei with respect to breakups on target protons is demonstrated in all these cases. It is possible to conclude that the peripheral dissociation of relativistic nuclei in nuclear track emulsion is a unique tool to study many-body systems composed of the lightest nuclei and nucleons in the energy scale relevant for nuclear astrophysics.
- OSTI ID:
- 21404705
- Journal Information:
- Physics of Atomic Nuclei, Journal Name: Physics of Atomic Nuclei Journal Issue: 9 Vol. 71; ISSN 1063-7788; ISSN PANUEO
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
79 ASTRONOMY AND ASTROPHYSICS
ALKALINE EARTH ISOTOPES
ALPHA DECAY RADIOISOTOPES
ASTROPHYSICS
BARYONS
BERYLLIUM 8
BERYLLIUM 9
BERYLLIUM ISOTOPES
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BORON 8
BORON ISOTOPES
COLLOIDS
DECAY
DISPERSIONS
DISSOCIATION
DWARF STARS
ELEMENTARY PARTICLES
EMULSIONS
ENERGY RANGE
EVEN-EVEN NUCLEI
EVEN-ODD NUCLEI
FERMIONS
FRAGMENTATION
HADRONS
HEAVY NUCLEI
HELIUM 3
HELIUM 5
HELIUM ISOTOPES
ISOTOPES
LIGHT NUCLEI
MANY-BODY PROBLEM
MILLISECONDS LIVING RADIOISOTOPES
NEON 22
NEON ISOTOPES
NITROGEN 14
NITROGEN ISOTOPES
NUCLEI
NUCLEONS
ODD-ODD NUCLEI
PARTICLE DECAY
PARTICLE TRACKS
PHYSICS
PROTONS
RADIOISOTOPES
RELATIVISTIC RANGE
STABLE ISOTOPES
STARS
WHITE DWARF STARS
79 ASTRONOMY AND ASTROPHYSICS
ALKALINE EARTH ISOTOPES
ALPHA DECAY RADIOISOTOPES
ASTROPHYSICS
BARYONS
BERYLLIUM 8
BERYLLIUM 9
BERYLLIUM ISOTOPES
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BORON 8
BORON ISOTOPES
COLLOIDS
DECAY
DISPERSIONS
DISSOCIATION
DWARF STARS
ELEMENTARY PARTICLES
EMULSIONS
ENERGY RANGE
EVEN-EVEN NUCLEI
EVEN-ODD NUCLEI
FERMIONS
FRAGMENTATION
HADRONS
HEAVY NUCLEI
HELIUM 3
HELIUM 5
HELIUM ISOTOPES
ISOTOPES
LIGHT NUCLEI
MANY-BODY PROBLEM
MILLISECONDS LIVING RADIOISOTOPES
NEON 22
NEON ISOTOPES
NITROGEN 14
NITROGEN ISOTOPES
NUCLEI
NUCLEONS
ODD-ODD NUCLEI
PARTICLE DECAY
PARTICLE TRACKS
PHYSICS
PROTONS
RADIOISOTOPES
RELATIVISTIC RANGE
STABLE ISOTOPES
STARS
WHITE DWARF STARS