| Vacuum creation of quarks at the time scale of QGP thermalization and strangeness enhancement in heavy-ion collisionsA.V. Prozorkevich (1)🇷🇺 · S.A. Smolyansky (1)🇷🇺 · V.V. Skokov (2)🇷🇺 · E.E. Zabrodin (3,4) (1 - Physics Department, Saratov State University, Russia; 2 - BLTP, JINR, Dubna, Russia; 3 - Centre of Mathematics for Applications, University of Oslo, Norway; 4 - SINP MSU, Moscow, Russia)🇳🇴 | nucl-th | PLB | 17 |
| | nucl-th | PLB | 33 |
| | ↳ hep-ph | PLB | 14 |
| | nucl-th | PLB | 35 |
| | nucl-th | PLB | 27 |
| | ↳ hep-ph | PLB | 34 |
| | nucl-th | PLB | 2 |
| | nucl-th | PLB | 27 |
| | ↳ hep-ph | PLB | 77 |
| | nucl-th | PLB | 18 |
| | ↳ hep-ph | PLB | 88 |
| Formation of hot heavy nuclei in supernova explosionsA.S. Botvina (Cyclotron Institute TAMU, College Station TX, USA and INR, Moscow, Russia)🇺🇸 · I.N. Mishustin (ITP, Frankfurt, Germany; NBI, Copenhagen, Denmark and KI, Moscow, Russia)🇩🇪 | nucl-th | PLB | 70 |
| | nucl-th | PLB | 70 |
| | ↳ hep-ph | PLB | 36 |
| | ↳ hep-ph | PLB | 29 |
| | nucl-th | PLB | 392 |
| | nucl-th | PLB | 69 |
| | nucl-th | PLB | 7 |
| | ↳ hep-ph | PLB | 55 |
| | nucl-th | PLB | 176 |
| | ↳ hep-ph | PLB | 26 |
| | ↳ hep-ph | PLB | 19 |
| | ↳ hep-ph | PLB | 120 |
| | nucl-th | PLB | 9 |
| | nucl-th | PLB | 25 |
| | ↳ hep-lat | PLB | 259 |
| | nucl-th | PLB | 13 |
| | nucl-th | PLB | 31 |
| | ↳ hep-ph | PLB | 48 |
| | ↳ hep-ph | PLB | 59 |
| | ↳ hep-ph | PLB | 38 |
| | nucl-th | PLB | 294 |
| | ↳ hep-ph | PLB | 2 |
| | nucl-th | PLB | 89 |
| | ↳ nucl-ex | PLB | 45 |
| | ↳ hep-ph | PLB | 43 |
| | nucl-th | PLB | 1 |
| | nucl-th | PLB | 73 |
| | nucl-th | PLB | 56 |
| | ↳ hep-ph | PLB | 10 |
| | ↳ hep-ph | PLB | 16 |
| | nucl-th | PLB | 8 |
| | nucl-th | PLB | 26 |
| | nucl-th | PLB | 10 |
| | nucl-th | PLB | 28 |
| | ↳ hep-ph | PLB | 159 |
| | nucl-th | PLB | 23 |
| | nucl-th | PLB | 14 |
| | ↳ hep-ph | PLB | 3 |
| | nucl-th | PLB | 8 |