A.-A. Chen

activity

20032022

e^{+} e^{-} \to ϕ f_{0} (980)

Observed via Initial-State Radiation

148 citations · 424 across the 17 of their papers we have counts for

collaborators

Showing 2013Show all

2 papers · 1 filter

nucl-ex2013★ 48 cited

Classical-Nova Contribution to the Milky Way's $^{26}$ Al Abundance: Exit Channel of the Key $^{25}$ Al( $p, γ$ ) $^{26}$ Si Resonance

M. B. Bennett, C. Wrede, K. A. Chipps +21

Classical novae are expected to contribute to the 1809-keV Galactic $γ$ -ray emission by producing its precursor $^{26}$ Al, but the yield depends on the thermonuclear rate of the un…

astro-ph.SR2013★ 16 cited

Constraining nova observables: direct measurements of resonance strengths in 33S(p,γ)34Cl

J. Fallis, A. Parikh, P. F. Bertone +32

The 33S(p,γ)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abu…

Classical-Nova Contribution to the Milky Way's 26Al Abundance: Exit Channel of the Key 25Al(p,γ)26Si Resonance

Constraining nova observables: direct measurements of resonance strengths in 33S(p,γ)34Cl

Classical-Nova Contribution to the Milky Way's $^{26}$ Al Abundance: Exit Channel of the Key $^{25}$ Al( $p, γ$ ) $^{26}$ Si Resonance