| | ↳ astro-ph | PRL | 116 |
| | nucl-th | PRL | 90 |
| | ↳ cond-mat | PRL | 71 |
| | ↳ hep-ph | PRL | 315 |
| | nucl-th | PRL | 92 |
| | nucl-th | PRL | 105 |
| | nucl-th | PRL | 8 |
| | ↳ hep-lat | PRL | 20 |
| | nucl-th | PRL | 18 |
| | ↳ hep-ph | PRL | 107 |
| | ↳ hep-ph | PRL | 81 |
| | ↳ astro-ph | PRL | 179 |
| | ↳ hep-ph | PRL | 701 |
| Simulation of the Spherically Symmetric Stellar Core Collapse, Bounce, and Postbounce Evolution of a 13 Solar Mass Star with Boltzmann Neutrino Transport, and Its Implications for the Supernova MechanismAnthony Mezzacappa (1,2)🇺🇸 · Matthias Liebendoerfer (1,2,3)🇺🇸 · O. E. Bronson Messer (1,2,4)🇺🇸 · W. Raphael Hix (1,2,4)🇺🇸 · Friederich-Karl Thielemann (1,3)🇺🇸 · Stephen W. Bruenn (5) ((1) Oak Ridge National Laboratory, (2) University of Tennessee, (3) University of Basel, (4) Joint Institute for Heavy Ion Research, (5) Florida Atlantic University)🇺🇸 | ↳ astro-ph | PRL | 185 |
| | nucl-th | PRL | 18 |
| | nucl-th | PRL | 253 |
| | nucl-th | PRL | 655 |
| | ↳ hep-ph | PRL | 144 |
| | nucl-th | PRL | 60 |
| | nucl-th | PRL | 13 |
| | ↳ hep-ph | PRL | 94 |
| | ↳ hep-ph | PRL | 558 |
| | ↳ astro-ph | PRL | 107 |
| | ↳ hep-ph | PRL | 37 |
| | nucl-th | PRL | 495 |
| | ↳ cond-mat | PRL | 131 |
| | nucl-th | PRL | 111 |
| | nucl-th | PRL | 42 |
| | nucl-th | PRL | 206 |
| | nucl-th | PRL | 62 |
| | ↳ astro-ph | PRL | 26 |
| | ↳ hep-ph | PRL | 522 |
| | ↳ cond-mat.mes-hall | PRL | 38 |
| | nucl-th | PRL | 9 |
| | ↳ cond-mat | PRL | 92 |
| | ↳ hep-ph | PRL | 59 |
| | nucl-th | PRL | 35 |
| | nucl-th | PRL | 77 |
| | ↳ hep-ph | PRL | 132 |
| | ↳ hep-ph | PRL | 61 |
| | nucl-th | PRL | 166 |
| | ↳ astro-ph | PRL | 35 |
| | ↳ astro-ph | PRL | 181 |
| | ↳ hep-ph | PRL | 14 |
| | nucl-th | PRL | 72 |
| | ↳ hep-ph | PRL | 44 |
| | ↳ hep-ex | PRL | 31 |
| | ↳ hep-ph | PRL | 12 |
| | nucl-th | PRL | 81 |
| | nucl-th | PRL | 6 |