| | nucl-th | PRC | 5 |
| | nucl-th | EPJA | 6 |
| | nucl-th | NPA | 1 |
| | nucl-th | PRC | 18 |
| | nucl-th | PRC | 5 |
| | nucl-th | PRC | 5 |
| | nucl-th | PRC | 16 |
| | ↳ hep-ex | PRC | 5 |
| | nucl-th | PRC | 21 |
| | nucl-th | Phys.Scripta | 0 |
| | nucl-th | Phys.Part.Nucl.Lett. | 85 |
| | nucl-th | Springer Proc.Phys. | 0 |
| | nucl-th | J.Phys.G | 4 |
| | nucl-th | PRC | 16 |
| | nucl-th | PRC | 18 |
| | nucl-th | PRC | 17 |
| | ↳ nucl-ex | PRC | 11 |
| | nucl-th | PRC | 44 |
| | nucl-th | PRC | 32 |
| | nucl-th | Turk.J.Phys. | 1 |
| Formation of hypermatter and hypernuclei within transport models in relativistic ion collisionsA.S. Botvina (1,2)🇩🇪 · J. Steinheimer (1)🇩🇪 · E. Bratkovskaya (1)🇩🇪 · M. Bleicher (1)🇩🇪 · J. Pochodzalla (3,4) ((1) Frankfurt Institute for Advanced Studies, Frankfurt am Main, Germany (2) Institute for Nuclear Research RAS, Moscow, Russia (3) Helmholtz-Institut Mainz, Mainz, Germany (4) Institut fuer Kernphysik and PRISMA Cluster of Excellence, J.Gutenberg-University Mainz, Germany)🇩🇪 | nucl-th | PLB | 80 |
| | nucl-th | PRC | 10 |
| | nucl-th | PRC | 20 |
| | nucl-th | J.Phys.Conf.Ser. | 4 |
| Production of hypernuclei in peripheral relativistic ion collisionsA. S. Botvina (1 and 2)🇷🇺 · K. K. Gudima (3)🇲🇩 · J. Pochodzalla (2 and 4) ((1) Institute for Nuclear Research, RAS, Moscow, Russia, (2) Helmholtz-Institut Mainz, J.Gutenberg-University, Mainz, Germany, (3) Institute of Applied Physics, ASM, Kishinev, Moldova, (4) Institute for Nuclear Physics and PRISMA Cluster of Excellence, J.Gutenberg-University, Mainz, Germany)🇩🇪 | nucl-th | PRC | 36 |
| | nucl-th | PRC | 32 |
| | nucl-th | — | 1 |
| | nucl-th | ApJ | 33 |
| | nucl-th | NPA | 66 |
| | nucl-th | PLB | 192 |
| | nucl-th | PRC | 52 |
| | nucl-th | IJMPE | 8 |
| | ↳ nucl-ex | PRC | 106 |
| | ↳ nucl-ex | — | 1 |
| Statistical approach for supernova matterA.S. Botvina (1,2)🇷🇺 · I.N. Mishustin (2,3) ((1) INR, Moscow, Russia, (2) FIAS, Frankfurt, Germany, (3) KI, Moscow, Russia.)🇩🇪 | nucl-th | NPA | 89 |
| | nucl-th | — | 1 |
| | nucl-th | — | 1 |
| | nucl-th | PLB | 16 |
| The role of bulk energy in nuclear multifragmentationN. Buyukcizmeci (1)🇷🇺 · A.S.Botvina (2,3)🇹🇷 · I.N. Mishustin (3,4)🇩🇪 · R. Ogul (1) ((1)Department of Physics, University of Selcuk, Konya, Turkey, (2)Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia, (3)Frankfurt Institute for Advanced Studies, J.W. Goethe University, Frankfurt am Main, Germany, (4)Kurchatov Institute, Russian Research Center, Moscow, Russia)🇹🇷 | nucl-th | PRC | 15 |
| Properties of stellar matter in supernova explosions and nuclear multifragmentationA.S. Botvina (1,2,3)🇷🇺 · I.N. Mishustin (3,4)🇩🇪 · W. Trautmann (2) ((1) INR, Moscow, Russia, (2) GSI, Darmstadt, Germany, (3) FIAS, Frankfurt, Germany, (4) KI, Moscow, Russia.)🇩🇪 | nucl-th | — | 1 |
| Modification of surface energy in nuclear multifragmentationA.S. Botvina (1,2)🇩🇪 · N. Buyukcizmeci (3)🇹🇷 · M. Erdogan (3)🇹🇷 · J. Lukasik (1,4)🇩🇪 · I.N. Mishustin (5,6)🇩🇪 · R. Ogul (1,3)🇩🇪 · W. Trautmann (1) ((1) GSI, Darmstadt, Germany, (2) INR, Moscow, Russia, (3) Selcuk University, Konya, Turkey, (4) INP, Krakow, Poland, (5) FIAS, Frankfurt, Germany, (6) KI, Moscow, Russia.)🇩🇪 | nucl-th | PRC | 45 |
| | nucl-th | EPJA | 25 |
| | nucl-th | PRC | 33 |
| | nucl-th | EPJA | 66 |
| | nucl-th | — | 0 |
| 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 | PRC | 43 |
| On pressure versus density dependence in statistical multifragmentation modelsA.S. Botvina (GSI, Darmstadt, Germany and INR, Moscow, Russia)🇩🇪 · I.N. Mishustin (ITP, Frankfurt, Germany; NBI, Copenhagen, Denmark and KI, Moscow, Russia)🇩🇪 | nucl-th | — | 2 |
| | nucl-th | — | 0 |
| | nucl-th | — | 0 |