S. Subedi

most citedSensitivity of

^{44}

Ti and

^{56}

Ni production in CCSN shock-driven nucleosynthesis to reaction rates

18 citations · 23 across the 2 of their papers we have counts for

collaborators

3 papers

nucl-ex2022★ 5 cited

$^{57}$ Zn $β$ -delayed proton emission establishes the $^{56}$ Ni $r p$ -process waiting point bypass

M. Saxena, W. -J Ong, Z. Meisel +32

We measured the $^{57}$ Zn $β$ -delayed proton ( $β$ p) and $γ$ emission at the National Superconducting Cyclotron Laboratory. We find a $^{57}$ Zn half-life of 43.6 $\pm$ 0.2 ms, $β$ p…

astro-ph.HE2020★ 18 cited

Sensitivity of $^{44}$ Ti and $^{56}$ Ni production in CCSN shock-driven nucleosynthesis to reaction rates

Shiv K. Subedi, Zach Meisel, Grant Merz

Recent observational advances have enabled high resolution mapping of $^{44}$ Ti in core-collapse supernova (CCSN) remnants. Comparisons between observations and models provide st…

nucl-ex2020

Constraining the destruction rate of $^{40}$ K in stellar nucleosynthesis through the study of the $^{40}$ Ar(p,n) $^{40}$ K reaction

P. Gastis, G. Perdikakis, J. Dissanayake +13

40K plays a significant role in the radiogenic heating of earth-like exoplanets, which can affect the development of a habitable environment on their surfaces. The initial amount o…

57Zn β-delayed proton emission establishes the 56Ni rp-process waiting point bypass

Sensitivity of 44Ti and 56Ni production in CCSN shock-driven nucleosynthesis to reaction rates

Constraining the destruction rate of 40K in stellar nucleosynthesis through the study of the 40Ar(p,n)40K reaction

$^{57}$ Zn $β$ -delayed proton emission establishes the $^{56}$ Ni $r p$ -process waiting point bypass

Sensitivity of $^{44}$ Ti and $^{56}$ Ni production in CCSN shock-driven nucleosynthesis to reaction rates

Constraining the destruction rate of $^{40}$ K in stellar nucleosynthesis through the study of the $^{40}$ Ar(p,n) $^{40}$ K reaction