H. Jayatissa

most citedFirst direct measurement of the

^{13}

α

p

)

^{16}

O reaction relevant for core-collapse supernovae nucleosynthesis

10 citations · 24 across the 4 of their papers we have counts for

collaborators

4 papers

physics.data-an2022

Classification of events from $α$ -induced reactions in the MUSIC detector via statistical and ML methods

Krishnan Raghavan, Melina L. Avila, Prasanna Balaprakash +2

The Multi-Sampling Ionization Chamber (MUSIC) detector is typically used to measure nuclear reaction cross sections relevant for nuclear astrophysics, fusion studies, and other app…

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…

physics.ins-det2022★ 9 cited

In-flight production of an isomeric beam of $^{16}$ N

C. R. Hoffman, T. L. Tang, M. Avila +10

An in-flight beam of $^{16}$ N was produced via the single-neutron adding ( $d$ , $p$ ) reaction in inverse kinematics at the recently upgraded Argonne Tandem Linear Accelerator System…

nucl-ex2022★ 10 cited

First direct measurement of the $^{13}$ N( $α$ , $p$ ) $^{16}$ O reaction relevant for core-collapse supernovae nucleosynthesis

H. Jayatissa, M. L. Avila, K. E. Rehm +10

Understanding the explosion mechanism of a core-collapse supernova (CCSN) is important to accurately model CCSN scenarios for different progenitor stars using model-observation com…

Classification of events from α-induced reactions in the MUSIC detector via statistical and ML methods

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

In-flight production of an isomeric beam of 16N

First direct measurement of the 13N(α,p)16O reaction relevant for core-collapse supernovae nucleosynthesis

Classification of events from $α$ -induced reactions in the MUSIC detector via statistical and ML methods

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

In-flight production of an isomeric beam of $^{16}$ N

First direct measurement of the $^{13}$ N( $α$ , $p$ ) $^{16}$ O reaction relevant for core-collapse supernovae nucleosynthesis