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2021 연구성과별 연구자 정보 (1191 / 2991)
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| Document Title | Author Full Name | Author Short Name | Index | Corresponding | Address | ResearcherID | ResearcherID Author Name | ORCID | ORCID Author Name | Related Email |
|---|---|---|---|---|---|---|---|---|---|---|
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Pappalardo, L. L. | Pappalardo, LL | 111 | INFN, Sez Genova, I-44100 Ferrara, Italy | R-3305-2016 | Pappagallo, Marco | ||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Pasyuk, E. | Pasyuk, E | 112 | Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Pogprelko, O. | Pogprelko, O | 113 | Kurchatov Inst ITEP, Nat Res Ctr, Moscow 117259, Russia | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Prok, Y. | Prok, Y | 114 | Old Dominion Univ, Norfolk, VA 23529 USA | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Prok, Y. | Prok, Y | 114 | Univ Virginia, Charlottesville, VA 22901 USA | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Reed, T. | Reed, T | 115 | Florida Int Univ, Miami, FL 33199 USA | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Ripani, M. | Ripani, M | 116 | INFN, Sez Genova, I-16146 Genoa, Italy | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Ritman, J. | Ritman, J | 117 | Inst Kernphys Juelich, D-52425 Julich, Germany | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Rizzo, A. | Rizzo, A | 118 | INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Rizzo, A. | Rizzo, A | 118 | Univ Roma Tor Vergata, I-00133 Rome, Italy | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Rosner, G. | Rosner, G | 119 | Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Sabatie, F. | Sabatie, F | 120 | Univ Paris Saclay, IRFU, CEA, F-91191 Gif Sur Yvette, France | K-9066-2015 | Sabatie, Franck | ||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Salgado, C. | Salgado, C | 121 | Norfolk State Univ, Norfolk, VA 23504 USA | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Schmidt, A. | Schmidt, A | 122 | George Washington Univ, Washington, DC 20052 USA | ||||||
| Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State | Schumacher, R. A. | Schumacher, RA | 123 | Carnegie Mellon Univ, Pittsburgh, PA 15213 USA | K-6455-2013 | Schumacher, Reinhard |
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