PPT-Neutron

beams for nuclear data measurements Arnd Junghans HelmholtzZentrum Dresden Rossendorf Germany Table of Content Introduction of the speaker Neutron sources . the Supernova Engine. Bounce Masses. Mass at Explosion. Fallback . Neutron Star Masses. Observations of neutron star binaries provide a growing list of neutron star mass estimates.. Current observations predict a range of NS masses from 1.0 to >2 solar masses.. Miguel A. Gonzalez. Institut. Laue-. Langevin. (Grenoble, France). gonzalezm@ill.eu. Outline. General remarks and reminders. The main equations and their physical meaning. QENS models for translational diffusion and localized motions. Richard Kouzes. Ken Conlin, James Ely, Luke Erikson, Azaree Lintereur, Emily Mace, Edward Siciliano, Daniel Stephens, David Stromswold, Renee Van Ginhoven, Mitch Woodring. Pacific Northwest National Laboratory. A.. S. . Chepurnov. . a. ,. . V.Y. . Ionidi. . a. , . O.O. . Ivashchuk. . b. , . A.S. . Kubankin. . b. ,. c. , . . A.N. . Oleinik. . b. ,. . A.V. Shchagin . b. ,. d. a . Skobeltsyn. Institute of Nuclear Physics, . Phil Rosenfield, . Fridolin. Weber, Horst . Lenske. Outline. Neutron stars: a short synopsis. The structure of neutron stars. Modeling neutron stars. The equation of state. . Rotating or non-rotating. and Other Applications: Hydrology +. Neutron Monitor Community Workshop—Honolulu, Hawaii . October . 24-25, 2015. Physicist. National Urban Security Technology Laboratory . Science and Technology Directorate. Contents. Breakup reactions. of . 14. Be on a proton target. Inelastic scattering (. 14. Be). One-neutron removal reaction (. 13. Be). Y. Kondo. RIKEN . Nishina. Center. 2. Collaborators. Y. Kondo. . Ana Becerril-Reyes, Sanjib S. Gupta and Hendrik Schatz. . Comparison between the two compilations of electron capture rates:. We start by comparing the EC rates at the lowest values of temperature and density (T9=0.01 and Log. By. . Kraml E.. 09.01.2017. A Neutron-Star. (not . actually. ). The Sun. Source: NASA. A Neutron-Star. Comparison. Diameter:. Mass. :. Density. :. Diameter:. Mass. :. Density. :. 1.4 x 10^6 km. 2 x 10^30 kg. for high power deuterium beams. Corso di Dottorato in Fisica e Astronomia: ciclo XXX. Seminario di fine primo anno. Andrea . Muraro. Outline. What is ITER . Neutral Beam Injector for ITER (PRIMA). CNESM Principle. Position-Sensitive . MCP . detector. Personnel. : . Mr. Blake Wiggins . (graduate student), Davinder . Siwal. , . RdS. (PI), Indiana University. Whether detecting photons, neutrons, or ions ultimately one is inevitably dealing with electrons.. Rauno . Julin. Accelerator Laboratory. Department . of Physics . . University of . Jyväskylä. . JYFL. Finland. Nuclear spectrocopy . is required to understand behaviour of nuclei far from stability.  . On behalf of Sichuan University CDEX Group. Haoyang. Xing. . School of Physical Science and Technology, Sichuan University. Symposium of Sino-German GDT. 2013/4/11. 1. CDEX Collaboration. Outline. Prompt . Neutron . Emission . During. Acceleration in Fission. T.. . Ohsawa. . Kinki University. Japanese Nuclear Data Committee. IAEA/CRP on PFNS, Vienna, Dec. 13-16, 2011. q. ε. Overall agreement between.