📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

Alpha-induced reactions in nuclear astrophysics

Lead Research Organisation: University of York
Department Name: Physics

Abstract

Studying the 15N(a,g) and 17O(a,n) reactions using direct and indirect techniques to better understand nucleosynthesis in AGB and massive stars.

People

ORCID iD

Publications

10 25 50

publication icon
Frost-Schenk J (2018) Cycling the hot CNO: a teaching methodology in Physics Education

publication icon
Turturica G (2019) Investigation of Compton scattering for gamma beam intensity measurements and perspectives at ELI-NP in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

publication icon
Frost-Schenk J (2022) The impact of 17O + a reaction rate uncertainties on the s-process in rotating massive stars in Monthly Notices of the Royal Astronomical Society

Studentship Projects

Project Reference Relationship Related To Start End Student Name
ST/N50452X/1 30/09/2015 30/03/2021
1799912 Studentship ST/N50452X/1 31/03/2016 30/11/2019
 
Description The findings comprise of two key experimental outcomes:
- A measurement of 15N + 4He occurred for the study of 19F abundances. The first directly measured measurement of the direct capture cross-section occurred using DRAGON, utilising a windowless He gas target and 15N beam. The work was intended to help explain galactic spectra.
- Measurement of 21Ne occurred at TUNL (Triangle Universities Nuclear Laboratory) utilising a neutron transfer process. The measurement has helped restrain the ratio of what happens after 17O reacts with an alpha particle; whether it proceeds by emitting a neutron or gamma. This work has further improved the understanding of 16O as a neutron poison, which is useful in stellar models. The reaction has also obtained information on states in 21Ne.
I have also been involved in outreach, including publication based on these activities, and it is hoped that this component of the work has had a positive impact on those considering studying physics.
Exploitation Route There have already been 3 further measurements based on this work.
Sectors Other