연구성과로 돌아가기

2021 연구성과별 연구자 정보 (1192 / 2991)

※ 현재 Web of Science 저자 정보만 집계되어 있습니다.
※ 컨트롤 + 클릭으로 열별 다중 정렬 가능합니다.
Excel 다운로드
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 Sharabian, Y. G. Sharabian, YG 124 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 Shrestha, U. Shrestha, U 125 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 Sokhan, D. Sokhan, D 126 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 Soto, O. Soto, O 127 INFN, Lab Nazl Frascati, I-00044 Frascati, Italy 0000-0002-8613-0310 Soto, Orlando
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 Sparveris, N. Sparveris, N 128 Temple Univ, Philadelphia, PA 19122 USA C-4751-2008 Sparveris, Nikolaos
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 Strakovsky, I. I. Strakovsky, II 129 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 Strauch, S. Strauch, S 130 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 Tyson, R. Tyson, R 131 Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland LRC-4125-2024 Tyson, Richard 0000-0002-0635-4198 Tyson, Richard
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 Ungaro, M. Ungaro, M 132 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 Ungaro, M. Ungaro, M 132 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 Venturelli, L. Venturelli, L 133 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 Venturelli, L. Venturelli, L 133 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 Voskanyan, H. Voskanyan, H 134 Yerevan Phys Inst, Yerevan 375036, Armenia
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 Vossen, A. Vossen, A 135 Duke Univ, Durham, NC 27708 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 Vossen, A. Vossen, A 135 Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA
페이지 이동: