activity
20162026
most citedBeta decay of deformed r-process nuclei near A = 80 and A= 160, including odd-A and odd-odd nuclei, with the Skyrme finite-amplitude method

53 citations · 64 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

The Interplay of Magnetic Fields, Turbulence and Vorticity in Core-Collapse Supernovae

David Calvert, Michael Redle, Bibek Gautam +4

The convective turbulent motion of the fluid below the shock in a core-collapse supernova stretches and amplifies the magnetic field of the progenitor star. The energy contained in…

astro-ph.HE2026

Propagating Uncertainties from Nuclear Physics to Gamma-rays in Core Collapse Supernovae

Chris L Fryer, Hendrik Schatz, Samuel Jones +18

Nuclear yields are powerful probes of supernova explosions, their engines and their progenitors. In addition, as we improve our understanding of these explosions, we can use nuclea…

astro-ph.HE2019★ 6 cited

Synthetic Spectra of Pair-Instability Supernovae in 3D

E. Chatzopoulos, M. S. Gilmer, R. T. Wollaeger +2

Pair-Instability Supernovae (PISNe) may signal the deaths of extremely massive stars in the local Universe or massive primordial stars after the end of the Cosmic Dark Ages. Hydrod…

nucl-th2016★ 53 cited

Beta decay of deformed r-process nuclei near A = 80 and A= 160, including odd-A and odd-odd nuclei, with the Skyrme finite-amplitude method

T. Shafer, J. Engel, C. Fröhlich +3

After identifying the nuclei in the regions near A =80 and A = 160 for which beta-decay rates have the greatest effect on weak and main r-process abundance patterns, we apply the f…

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…