Published December 2019 | Version v1
Book

The 19F(p, α)16O reaction in nuclear astrophysics

  • 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)

Part of:
Proceedings of the DAE-BRNS symposium on nuclear physics. V. 64

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)

Optional Information