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2021 연구성과별 연구자 정보 (1190 / 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 Mokeev, V Mokeev, 99 Lomonosov Moscow State Univ, Inst Nucl Phys, Moscow 119234, 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 Mokeev, V Mokeev, 99 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 Munevar, E. Munevar, E 100 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 Camacho, C. Munoz Camacho, CM 101 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 Nadel-Turonski, P. Nadel-Turonski, P 102 Catholic Univ Amer, Washington, DC 20064 USA 0009-0001-6067-2277 Nadel-Turonski, Pawel
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 Nadel-Turonski, P. Nadel-Turonski, P 102 Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA 0009-0001-6067-2277 Nadel-Turonski, Pawel
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 Neupane, K. Neupane, K 103 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 Niccolai, S. Niccolai, S 104 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 Niculescu, G. Niculescu, G 105 James Madison Univ, Harrisonburg, VA 22807 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 O'Connell, T. R. O'Connell, TR 106 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 Osipenko, M. Osipenko, M 107 INFN, Sez Genova, I-16146 Genoa, Italy N-8292-2015 Osipenko, Mikhail
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 Ostrovidov, A., I Ostrovidov, A 108 Florida State Univ, Tallahassee, FL 32306 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 Pandey, P. Pandey, P 109 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 Paolone, M. Paolone, M 110 New Mexico State Univ, POB 30001, Las Cruces, NM 88003 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 Pappalardo, L. L. Pappalardo, LL 111 Univ Ferrara, I-44121 Ferrara, Italy R-3305-2016 Pappagallo, Marco
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