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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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