activity
20082026
most citedThe 12C(a,g)16O reaction and its implications for stellar helium burning

255 citations · 365 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

AMReX-Astrophysics Microphysics: A set of microphysics routines for astrophysical simulation codes based on the AMReX library

Astro Microphysics Team, Khanak Bhargava, Abigail Bishop +15

The AMReX-Astrophysics Microphysics library provides a common set of microphysics routines (reaction networks and associated physics, equations of state, and various transport coef…

nucl-ex2017★ 255 cited

The 12C(a,g)16O reaction and its implications for stellar helium burning

R. J. deBoer, J. Gorres, M. Wiescher +10

The creation of carbon and oxygen in our universe is one of the forefront questions in nuclear astrophysics. The determination of the abundance of these elements is key to both our…

astro-ph.SR2016★ 5 cited

White Paper on Nuclear Astrophysics

Almudena Arcones, Dan W. Bardayan, Timothy C. Beers +40

This white paper informs the nuclear astrophysics community and funding agencies about the scientific directions and priorities of the field and provides input from this community…

astro-ph.SR2015★ 81 cited

Carbon-rich presolar grains from massive stars. Subsolar 12C/13C and 14N/15N ratios and the mystery of 15N

M. Pignatari, E. Zinner, P. Hoppe +7

Carbon-rich grains with isotopic anomalies compared to the Sun are found in primitive meteorites. They were made by stars, and carry the original stellar nucleosynthesis signature.…

astro-ph.SR2012★ 24 cited

Theoretical Studies of Accretion of Matter onto White Dwarfs and the Single Degenerate Scenario for Supernovae of Type Ia

S. Starrfield, C. Iliadis, F. X. Timmes +4

We present a brief summary of the Single Degenerate Scenario for the progenitors of Type Ia Supernovae in which it is assumed that a low mass carbon-oxygen white dwarf is growing i…

astro-ph2008

Proton-Rich Nuclear Statistical Equilibrium

I. R. Seitenzahl, F. X. Timmes, A. Marin-Laflèche +3

Proton-rich material in a state of nuclear statistical equilibrium (NSE) is one of the least studied regimes of nucleosynthesis. One reason for this is that after hydrogen burning,…