PPT-Neutron transfer reactions at large

internuclear distances studied with the PRISMA spectrometer and the AGATA demonstrator Nuclei at large distance t unneling effects Relative role of one and multinucleon transfer channels Overlap between transfer and fusion reactions. Varun Bhalerao. California Institute of Technology. Collaborators: F. Harrison, S. . Kulkarni. , Marten van . Kerkwijk. , and others. Weighing in on Neutron Stars. Varun Bhalerao. Why?. How?. What?. Classes of objects. 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.. 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. 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. Irradiation Measurement . for. Superconducting Magnet Materials . at. Low Temperature. Tatsushi NAKAMOTO. KEK. Collaborators/Supporters. [KEK] M. Yoshida, M. Sugano, M. . Iio. , S. . Mihara. , . H. . 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.. flipper. Collimator with guide field. S-bender supermirror polarizer. HB-3A. High neutron polarization ratio (>95%) has been achieved at the HFIR HB-3A single crystal neutron diffractometer. This is the first use of this capability on an experiment approved through the General User program. We succeeded in detecting a weak itinerant ferromagnetic moment of 0.11(1). V. . Variale*. , B. Skarbo. 2. 1Istituto Nazionale Fisica Nucleare,INFN Sezione di Bari, Italy. 2 . Budcker. Institute of Nuclear Physics, Novosibirsk, Russia. * Vincenzo Variale. Tel.: +39 080 5442344; fax: +39 080 5443190.. 1. G.Croci. 2,1,3. , . A. Muraro. 1. , . E. . Perelli Cippo. 2,3. , M.Tardocchi. 1,3. , G.Grosso. 1. ,. . M.Rebai. 2,3. ,F. Murtas. 4. , R. Hall-Wilton. 5,6. , C. Höglund. 5. , L. Robinson. 5. , K. Kanaki. 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.