Slide 1An overview of the S1105 experiment at TRIUMF. 1 Martin Jones The University of Liverpool Email: [email protected] Slide 2 Overview. Martin Jones – Tigress experiment…

Slide 1Nucleus-Nucleus 2012San Antonio (TX) 18 F+p  15 O +  @ CRIB 1 Slide 2 Astrophysical motivations  Gamma-ray emission of energy 511 keV from novae is dominated…

Slide 1 Hydrogen burning under extreme conditions Scenarios: Hot bottom burning in massive AGB stars (> 4 solar masses) (T 9 ~ 0.08) Nova explosions on accreting white…

Breakout from the Hot-CNO cycle in X-Ray Bursters via the 18Ne(α,p) reaction International Workshop on Physics of Nuclei at Extremes 26 January 2010 Adam Tuff, Postgraduate…

Breakout from the Hot-CNO cycle in X-Ray Bursters via the 18Ne(α,p) reaction International Workshop on Physics of Nuclei at Extremes 26 January 2010 Adam Tuff, Postgraduate…

Diapositiva 1 Trojan Horse method and radioactive ion beams: study of 18F(p,a)15O reaction at astrophysical energies Nucleus-Nucleus 2012 San Antonio (TX) Marisa Gulino INFN,LNS,…

Caroline Nesaraja, Michael Smith, Daniel Bardayan, Jeffery Blackmon, Eric Lingerfelt, Jason Scott, W. Raphael Hix Physics Division, Oak Ridge National Laboratory Kyungyuk…

Abstract The 13N(p,γ)14O reaction is very important for our understanding of explosive astrophysical sites, such as novae and supernovae. This reaction determines the conditions…