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2021 연구성과별 연구자 정보 (1183 / 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 Bianconi, A. Bianconi, A 16 INFN, Sez Pavia, I-27100 Pavia, 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 Bianconi, A. Bianconi, A 16 Univ Brescia, I-25123 Brescia, 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 Biondo, L. Biondo, L 17 INFN, Sez Catania, I-95123 Catania, 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 Biondo, L. Biondo, L 17 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 Biondo, L. Biondo, L 17 Univ Messina, I-98166 Messina, 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 Biselli, A. S. Biselli, AS 18 Fairfield Univ, Fairfield, CT 06824 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 Bondi, M. Bondi, M 19 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 Bossu, F. Bossù, F 20 Univ Paris Saclay, IRFU, CEA, F-91191 Gif Sur Yvette, 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 Boiarinov, S. Boiarinov, S 21 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 Briscoe, W. J. Briscoe, WJ 22 George Washington Univ, Washington, DC 20052 USA 0000-0001-5899-7622 Briscoe, William
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 Brooks, W. K. Brooks, WK 23 Univ Tecn Federico Santa Maria, Casilla 110-V, Valparaiso, Chile C-8636-2013 Brooks, William
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 Bulumulla, D. Bulumulla, D 24 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 Burkert, V Burkert, VD 25 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 Carman, D. S. Carman, DS 26 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 Carvajal, J. S. Carvajal, JS 27 Florida Int Univ, Miami, FL 33199 USA
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