S. Subedi

activity

20202026

^{44}

Ti and

^{56}

Ni production in CCSN shock-driven nucleosynthesis to reaction rates

18 citations · 51 across the 9 of their papers we have counts for

collaborators

Showing 2026Show all

3 papers · 1 filter

nucl-ex2026

Thick-target Yield of $^{65}$ Cu( $α, n)^{68}$ Ga Near Threshold and Implications for Nuclear Medicine, Deep Underground Detector Backgrounds, and Nucleosynthesis

Zach Meisel, Gula Hamad, Kristyn Brandenburg +8

We report thick target yields of $^{65} Cu (α, n)^{68} Ga$ from $α$ energies $E_{α}$ $=$ 6.5--8~MeV measured via neutron-counting at the Edwards Accelerator Laboratory at Ohio…

nucl-ex2026

$β$ -decay Measurements Near the $N = 40$ Island of Inversion to Quantify Cooling of Accreted Neutron Star Crusts

K. Hermansen, W. -J. Ong, H. Schatz +18

Understanding the thermal structure of the outer crust of accreting neutron stars is important to interpret astronomical X-ray observations. Ground-state to ground-state $β$ -decay…

nucl-ex2026

Differential cross sections for $^{12} C (n, α_{0})$ , $^{16} O (n, α_{0})$ and $^{16} O (n, α_{1, 2, 3})$ between $E_{n}$ = 7.2 and 10 MeV with an active-target Time Projection Chamber

J. Bishop, C. E. Parker, R. Smith +24

Data for the $^{12} C (n, α_{0})$ , $^{16} O (n, α_{0})$ and $^{16} O (n, α_{1, 2, 3})$ differential cross sections are important for several different a…

Thick-target Yield of 65Cu(α,n)68Ga Near Threshold and Implications for Nuclear Medicine, Deep Underground Detector Backgrounds, and Nucleosynthesis

β-decay Measurements Near the N=40 Island of Inversion to Quantify Cooling of Accreted Neutron Star Crusts

Differential cross sections for 12C(n,α0​), 16O(n,α0​) and 16O(n,α1,2,3​) between En​ = 7.2 and 10 MeV with an active-target Time Projection Chamber

Thick-target Yield of $^{65}$ Cu( $α, n)^{68}$ Ga Near Threshold and Implications for Nuclear Medicine, Deep Underground Detector Backgrounds, and Nucleosynthesis

$β$ -decay Measurements Near the $N = 40$ Island of Inversion to Quantify Cooling of Accreted Neutron Star Crusts

Differential cross sections for $^{12} C (n, α_{0})$ , $^{16} O (n, α_{0})$ and $^{16} O (n, α_{1, 2, 3})$ between $E_{n}$ = 7.2 and 10 MeV with an active-target Time Projection Chamber