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2021 연구성과별 연구자 정보 (1189 / 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 Marchand, D. Marchand, D 88 Univ Paris Saclay, CNRS, IN2P3, IJCLab, F-91405 Orsay, France
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 Markov, N. Markov, N 89 Univ Connecticut, Storrs, CT 06269 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 Markov, N. Markov, N 89 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 Marsicano, L. Marsicano, L 90 INFN, Sez Genova, I-16146 Genoa, Italy KPB-4594-2024 Marsicano, Luca 0000-0002-8931-7498 Marsicano, Luca
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 Mascagna, V Mascagna, 91 INFN, Sez Pavia, I-27100 Pavia, Italy HLQ-1103-2023 Mascagna, Valerio
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 Mascagna, V Mascagna, 91 Univ Insubria, I-22100 Como, Italy HLQ-1103-2023 Mascagna, Valerio
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 McCracken, M. E. McCracken, ME 92 Carnegie Mellon Univ, Pittsburgh, PA 15213 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 McKinnon, B. McKinnon, B 93 Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland J-2928-2018 McKinnon, Bryan
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 McLauchlin, C. McLauchlin, C 94 Univ South Carolina, Columbia, SC 29208 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 Meziani, Z. E. Meziani, ZE 95 Argonne Natl Lab, Argonne, IL 60439 USA 0000-0001-9450-2914 Meziani, Zein-Eddine
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 Migliorati, S. Migliorati, S 96 INFN, Sez Pavia, I-27100 Pavia, Italy 0000-0002-1562-5201 Migliorati, Stefano
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 Migliorati, S. Migliorati, S 96 Univ Brescia, I-25123 Brescia, Italy 0000-0002-1562-5201 Migliorati, Stefano
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 Mineeva, T. Mineeva, T 97 Univ Connecticut, Storrs, CT 06269 USA MDT-1592-2025 Mineeva, Taisiya
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 Mineeva, T. Mineeva, T 97 Univ Tecn Federico Santa Maria, Casilla 110-V, Valparaiso, Chile MDT-1592-2025 Mineeva, Taisiya
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 Mirazita, M. Mirazita, M 98 INFN, Lab Nazl Frascati, I-00044 Frascati, Italy
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