Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Oak Ridge National LaboratoryUS200 papers
- Los Alamos National LaboratoryUS198 papers
- Duke UniversityUS187 papers
- Triangle Universities Nuclear LaboratoryUS171 papers
- University of Tennessee at KnoxvilleUS134 papers
- University of WashingtonUS134 papers
- University of North Carolina at Chapel HillUS130 papers
- Lawrence Berkeley National LaboratoryUS119 papers
- University of California, BerkeleyUS103 papers
- Centre National de la Recherche ScientifiqueFR98 papers
- Indiana University BloomingtonUS94 papers
- Massachusetts Institute of TechnologyUS93 papers
11 papers · 2 filters
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…
On the Expansion, Age, and Origin of the Puzzling Shell/Pulsar Wind Nebula G310.6-1.6
Stephen P. Reynolds, Kazimierz J. Borkowski
We present a 142-ks Chandra observation of the enigmatic combination supernova remnant G310.6-1.6 consisting of a bright pulsar-wind nebula driven by an energetic pulsar, surrounde…
Co-production of light and heavy -process elements via fission deposition
Nicole Vassh, Matthew R. Mumpower, Gail C. McLaughlin +2
We apply for the first time fission yields determined across the chart of nuclides from the macroscopic-microscopic theory of the Finite Range Liquid Drop Model to simulations of r…
Wolf-Rayet stars in young massive star clusters as potential sources of Galactic cosmic rays
Maria E Kalyashova, Andrei M Bykov, Sergei M Osipov +2
For most elements, the isotopic ratios seen in cosmic rays (CRs) are similar to those in the solar wind. The most important exception to this is Ne/Ne where the CR va…
Coupling Neutrino Oscillations and Simulations of Core-Collapse Supernovae
Charles J. Stapleford, Carla Fröhlich, James P. Kneller
At the present time even the most sophisticated, multi-dimensional simulations of core-collapse supernovae do not (self-consistently) include neutrino flavor transformation. This p…
Impact of Uncertainties in Astrophysical Reaction Rates on Nucleosynthesis in the Process
T. Rauscher, N. Nishimura, G. Cescutti +3
The process appears in proton-rich, hot matter which is expanding in a neutrino wind and may be realised in explosive environments such as core-collapse supernovae or in outfl…
High-energy cosmic rays from compact galactic star clusters: particle fluxes and anisotropy
A. M. Bykov, M. E. Kalyashova, D. C. Ellison +1
It has been shown that supernova blast waves interacting with winds from massive stars in compact star clusters may be capable of producing cosmic-ray (CR) protons to above $10^{17…
Monte Carlo modelling of particle acceleration in collisionless shocks with an effective mean electric field
Sergei M Osipov, Andrei M Bykov, Donald C Ellison
Relativistic particle acceleration in collisionless shocks of supernova remnants is accompanied by magnetic field amplification from cosmic ray (CR) driven plasma instabilities. Be…
Actinide-rich and Actinide-poor -Process Enhanced Metal-Poor Stars do not Require Separate -Process Progenitors
Erika M. Holmbeck, Anna Frebel, G. C. McLaughlin +3
The astrophysical production site of the heaviest elements in the universe remains a mystery. Incorporating heavy element signatures of metal-poor, -process enhanced stars into…
Neutrino Quantum Kinetics in Compact Objects
Sherwood A. Richers, Gail C. McLaughlin, James P. Kneller +1
Neutrinos play a critical role of transporting energy and changing the lepton density within core-collapse supernovae and neutron star mergers. The quantum kinetic equations (QKEs)…
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…