PPT-Use of Cosmic-Ray Neutron Data in Nuclear Threat Detection

and Other Applications Neutron Monitor Community WorkshopHonolulu Hawaii October 2425 2015 Physicist National Urban Security Technology Laboratory Science and Technology Directorate. 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. Connect the Fluke 415 HV supply output to the input of the voltage distribution box. (Make sure HV is off.). Connect the outputs of the HV distribution box to the HV supply for the phototubes in the cosmic ray . . Wei Wang. National Astronomical Observatories, . B. eijing China. The IAU XXVII General Assembly, Beijing August 20-31 2012. IAUS 291 . Neutron stars and pulsars: Challenges and opportunities after 80 Years. 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, . at. . Hartnell. . College. : A Case Study in Successful Undergraduate Research at a Two-Year College. Leo . Osornio. Hartnell. College. Presented at the 2012 AAPT Summer Meeting, Philadelphia. July 30, 2012. at NPL. Paddy Regan. NPL . Radioactivity Group, AIR Division. & . Department of Physics, . University . of Surrey. Nuclear Data?. ‘Nuclear Data’ and its evaluation underpin many areas of both applied and fundamental nuclear science, including. and Other Applications: Hydrology +. Neutron Monitor Community Workshop—Honolulu, Hawaii . October . 24-25, 2015. Physicist. National Urban Security Technology Laboratory . Science and Technology Directorate. . 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. The Discovery of Antimatter!. In 1932 Carl Anderson studied cosmic rays using a “cloud . chamber”. . Charged particles produced in cosmic rays would enter the chamber and leave “tracks”. The tracks would bend in circles because the chamber was placed in a strong magnetic field. Standards. Paddy Regan. Department of Physics, U. Surrey, UK . p.regan@surrey.ac.uk. &. Nuclear Metrology Department, National Physical Lab. UK, . paddy.regan@surrey.ac.uk. . Outline:. Introduction to radioisotope physics. SecOps Solutions Team. Customer Presentation . Agenda. Packages – What | Why. Business Challenges & Solutions. Market Opportunity. Solution Package Summary. Package Description – Value Proposition, Deployment. Boris Pritychenko. 1. 1 National Nuclear Data Center, Brookhaven National. Laboratory, Upton, NY 11973-5000, USA. Heavy Elements Production in a Neutron Star Merger. Can we apply nuclear data libraries to address current astrophysical observations such as a multi-messenger signal from the NGC 4993 galaxy? . Dec. 9, 2020 ONLINE meeting. Machine learning . in radiation metrology:. Kyushu University . (Fukuoka, Japan). Department of . Advanced Energy Engineering Science. Neutron spectrum unfolding and. Stephen Croft (ORNL). Ramkumar Venkataraman (ORNL). Louise G. Worrall (ORNL). Robert D. McElroy Jr. (ORNL). Andrea Favalli (LANL). Acknowledgement. This work was sponsored in part by the U.S. Department of Energy (DOE), National Nuclear Security Administration (NNSA), Office of Defense Nuclear Nonproliferation Research and Development (NA-22) and in part by ORNL and LANL..