Novel technique for constraining r-process (n,$γ$) reaction rates
A. Spyrou, S. N. Liddick, A. C. Larsen, M. Guttormsen, K. Cooper, A. C. Dombos, D. J. Morrissey, F. Naqvi, G. Perdikakis, S. J. Quinn, T. Renstrøm, J. A. Rodrig… 展开作者
A. Spyrou, S. N. Liddick, A. C. Larsen, M. Guttormsen, K. Cooper, A. C. Dombos, D. J. Morrissey, F. Naqvi, G. Perdikakis, S. J. Quinn, T. Renstrøm, J. A. Rodriguez, A. Simon, C. S. Sumithrarachchi, R. G. T. Zegers
A novel technique has been developed, which will open exciting new opportunities for studying the very neutron-rich nuclei involved in the r-process. As a proof-of-principle, the $γ$-spectra from the $β$-decay of $^{76}$Ga have been measured with the SuN detector at the National Superconducting Cyclotron Laboratory. The nuclear level density and $γ$-ray strength function are extracted and used as input to Hauser-Feshbach calculations. The present technique is shown to strongly constrain the $^{75}$Ge($n,γ$)$^{76}$Ge cross section and reaction rate.
Constraining the 6.05 MeV 0$^+$ and 6.13 MeV 3$^-$ cascade transitions in the $^{12}$C($α$,$γ$)$^{16}$O reaction using the Asymptotic Normalization Coefficients
First direct measurement constraining the $^{34}$Ar($α$,p)$^{37}$K reaction cross section for mixed hydrogen and helium burning in accreting neutron stars
Constraining the equation of state of nuclear matter from competition of fusion and quasi-fission in the reactions leading to production of the superheavy elements
Constraining Neutron Capture Cross Sections for $^{88}\mathrm{Y}$ with Gamma-ray Strength Function in $(p,p^\primeγ)$ Surrogate Reaction
University of South China（南华大学）；Key Laboratory of Advanced Nuclear Energy Design and Safety, Ministry of Education（教育部先进核能安全与设计重点实验室）；Beihang University（北京航空航天大学）；China Institute of Atomic Energy（中国原子能科学研究院）
Constraining the Synthesis of the Lightest p Nucleus 74Se
Michigan State University（密歇根州立大学）；Central Michigan University（中密歇根大学）；Hope College（霍普学院）；University of Notre Dame（圣母大学）；University of Victoria（维多利亚大学）；Mississippi State University（密西西比州立大学）；Pacific Northwest National Laboratory（太平洋西北国家实验室）；University of Tennessee, Knoxville（田纳西大学诺克斯维尔分校）；Duke University（杜克大学）；Ohio University（俄亥俄大学）；Istituto Nazionale di Fisica Nucleare-Laboratori Nazionali del Sud（意大利国家核物理研究所南方实验室）；Konkoly Observatory, Research Centre for Astronomy and Earth Sciences（孔科利天文台，天文学与地球科学研究中心）；CSFK HUN-REN, MTA Centre of Excellence（匈牙利科学与研究网络（HUN-REN）孔科利天文学研究所卓越中心）
Constraining r-process nucleosynthesis via enhanced accuracy neutron-capture experiments
Instituto de Física Corpuscular, CSIC - Universitat de València（粒子物理研究所，西班牙科学理事会-瓦伦西亚大学）；School of Physics and Astronomy, University of Edinburgh（爱丁堡大学物理与天文学学院）；Agenzia nazionale per le nuove tecnologie, l’energia e lo sviluppo economico sostenibile (ENEA)（国家新技术、能源和可持续经济发展局）；Istituto Nazionale di Fisica Nucleare, Sezione di Bologna（意大利国家核物理研究所博洛尼分所）；European Organization for Nuclear Research (CERN)（欧洲核子研究组织）
The Regulated GeAs Cycles with the New $^{63}$Ga(p,$γ$)$^{64}$Ge and $^{64}$Ge(p,$γ$)$^{65}$As Reaction Rates and Their Impact on the GS 1826$-$24 Clocked Bursts and SAX J1808.4$-$3658 Photospheric Radius Expansion Bursts
Zhejiang Sci-Tech University（浙江理工大学）；RIKEN（理化学研究所）；Lanzhou University（兰州大学）；Monash University（蒙纳士大学）；University of Bonn（波恩大学）；Michigan State University（密歇根州立大学）；the University of Tokyo（东京大学）；National Astronomical Observatory of Japan（日本国立天文台）
A Gaussian Process framework for constraining the nuclear equation of state from microscopic calculations with correlated uncertainties
Ohio University（俄亥俄大学）；Argonne National Laboratory（阿贡国家实验室）；University of Washington（华盛顿大学）；University of California, Berkeley（加州大学伯克利分校）；Michigan State University（密歇根州立大学）
