Published December 1984
| Version v1
Journal article
Deuterium and helium 3 production by supernovae of the first generation
Creators
- 1. AN SSSR, Moscow. Inst. Geokhimii i Analiticheskoj Khimii
Description
Possibility of deuterium and helium 3 synthesis in supernovae of the first generation is Under discussion. Consideration is performed in the frameWork of the model, according to Which powerfUl shock wave occUrring in sUpernovae explosion leads to collective particle acceleration up to relativistic energies. Interaction of particles with atomic nuclei of substance of supernoval shells leads to formation of light and anomalous isotopes. The highest contribution to deuterium and helium 3 synthesis is made at the expense of nuclear reaction: H(p, rho+/D, 4He (pd)3He, 4He(p2p)3T, 4He(p, pn)3He, 4He(p, pd)), and 4He(p, 2pn)SD
Additional details
Additional titles
- Original title (Russian)
- Образование дейтерия и гелия-3 сверхновыми первого поколения
Publishing Information
- Journal Title
- Zh. Ehksp. Teor. Fiz.
- Journal Volume
- 48
- Journal Issue
- 11
- Series
- Zh. Ehksp. Teor. Fiz.
- Journal Page Range
- 2080-2082
- ISSN
- 0044-4510
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 16066013
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DEUTERIUM; EXCITATION FUNCTIONS; HELIUM 3; HELIUM 4 TARGET; HYDROGEN 1 TARGET; NUCLEOSYNTHESIS; PROTON REACTIONS; SHOCK WAVES; SUPERNOVAE
- Descriptors DEC
- BARYON REACTIONS; BINARY STARS; ERUPTIVE VARIABLE STARS; EVEN-ODD NUCLEI; HADRON REACTIONS; HELIUM ISOTOPES; HYDROGEN ISOTOPES; ISOTOPES; LIGHT NUCLEI; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; ODD-ODD NUCLEI; STABLE ISOTOPES; STARS; SYNTHESIS; TARGETS; VARIABLE STARS
Optional Information
- Notes
- For English translation see the journal Soviet Physics - JETP (USA).