106 citations · 359 across the 12 of their papers we have counts for
12 papers
Comparison of Electron Capture Rates in the N=50 Region using 1D Simulations of Core-collapse Supernovae
Zac Johnston, Sheldon Wasik, Rachel Titus +4
Recent studies have highlighted the sensitivity of core-collapse supernovae (CCSNe) models to electron-capture (EC) rates on neutron-rich nuclei near the N=50 closed-shell region.…
Neutrino flavor mixing with moments
McKenzie Myers, Theo Cooper, MacKenzie Warren +5
The successful transition from core-collapse supernova simulations using classical neutrino transport to simulations using quantum neutrino transport will require the development o…
Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
Brandon L. Barker, Chelsea E. Harris, MacKenzie L. Warren +2
Observations of core-collapse supernovae (CCSNe) reveal a wealth of information about the dynamics of the supernova ejecta and its composition but very little direct information ab…
Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
Michael A. Pajkos, MacKenzie L. Warren, Sean M. Couch +2
The gravitational wave (GW) signal resulting from stellar core collapse encodes a wealth of information about the physical parameters of the progenitor star and the resulting core-…
Reaction Rate Sensitivity of the Production of -ray Emitting Isotopes in Core-Collapse Supernova
Kirby Hermansen, Sean M. Couch, Luke F. Roberts +2
Radioactive isotopes produced in core-collapse supernovae (CCSNe) provide useful insights into the underlying processes driving the collapse mechanism and the origins of elemental…
Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
MacKenzie L. Warren, Sean M. Couch, Evan P. O'Connor +1
With the advent of modern neutrino and gravitational wave detectors, the promise of multi-messenger detections of the next galactic core-collapse supernova has become very real. Su…