activity
20152022
most citedNew ANC measurement of the 1/2 state in O at 6.356 MeV, that dominates the C(,n)O reaction rate at temperatures relevant for the s-process

36 citations · 53 across the 5 of their papers we have counts for

collaborators

6 papers

physics.data-an2022

Classification of events from -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…

physics.ins-det20229 cited

In-flight production of an isomeric beam of N

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

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

nucl-ex20203 cited

Observation of T=3/2 Isobaric Analog States in 9Be using p+8Li resonance scattering

C. Hunt, G. V. Rogachev, S. Almaraz-Calderon +10

Background: Resonance scattering has been extensively used to study the structure of exotic, neutron-deficient nuclei. Extension of the resonance scattering technique to neutron-ri…

astro-ph.HE20195 cited

Catching Element Formation In The Act

Chris L. Fryer, Frank Timmes, Aimee L. Hungerford +216

Gamma-ray astronomy explores the most energetic photons in nature to address some of the most pressing puzzles in contemporary astrophysics. It encompasses a wide range of objects…

nucl-ex2018

Stellar ArAr reactions and their effect on light neutron-rich nuclide synthesis

M. Tessler, M. Paul, S. Halfon +22

The ArAr ( = 35 d) and ArAr (269 y) reactions were studied for the first time with a quasi-Maxwellian ( keV) neutron flux…

nucl-ex201536 cited

New ANC measurement of the 1/2 state in O at 6.356 MeV, that dominates the C(,n)O reaction rate at temperatures relevant for the s-process

M. L. Avila, G. V. Rogachev, E. Koshchiy +5

Background: Accurate knowledge of the C(,)O reaction cross section is important for the understanding of the s-process in AGB stars, since it is considered to b…