Published December 2019
| Version v1
Book
The 19F(p, α)16O reaction in nuclear astrophysics
Creators
- 1. Saha Institute of Nuclear Physics, Homi Bhabha National Institute, Kolkata (India)
Description
Nuclear process plays a vital role in the evolution of universe after Big Bang. At astrophysical scenario the energy released from nuclear reaction prevents the star from gravitational collapse. In this work, a crucial reaction 19F(p, α)16O which is a reaction in fourth branch of CNO cycle and the distinction between experimental data and theoretical models has been studied. Since the reaction has a controversy whether it is a direct process or compound nucleus process, H. Herndl observed that direct part is also important using the Wirzba data. The Indirect Trojan horse method can be important to study this reaction at Gamow region (27-94 KeV)
Additional details
Publishing Information
- Publisher
- Bhabha Atomic Research Centre
- Imprint Place
- Mumbai (India)
- Imprint Title
- Proceedings of the DAE-BRNS symposium on nuclear physics. V. 64
- Imprint Pagination
- 1072 p.
- Journal Page Range
- [2 p.]
Conference
- Title
- 64. DAE-BRNS symposium on nuclear physics
- Dates
- 23-27 Dec 2019
- Place
- Lucknow (India)
INIS
- Country of Publication
- India
- Country of Input or Organization
- India
- INIS RN
- 51075294
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ALPHA REACTIONS; COMPOUND NUCLEI; FLUORINE 19 TARGET; GRAVITATIONAL COLLAPSE; KEV RANGE 10-100; OXYGEN 16; PROTON REACTIONS; STAR EVOLUTION
- Descriptors DEC
- BARYON REACTIONS; CHARGED-PARTICLE REACTIONS; ENERGY RANGE; EVEN-EVEN NUCLEI; EVOLUTION; HADRON REACTIONS; ISOTOPES; KEV RANGE; LIGHT NUCLEI; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; OXYGEN ISOTOPES; STABLE ISOTOPES; TARGETS