'2 mev' presentation slideshows

Recent Results from KamLAND

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Feng-Shou Zhang College of Nuclear Science and Technology

The 9th Japan- China Joint Nuclear Physics Symposium, Nov. 7-13, 2015, Osaka. Production cross sections for superheavy and neutron-rich nuclei. Feng-Shou Zhang College of Nuclear Science and Technology Beijing Normal University, Beijing, China Collaborators:

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Synthesis of Element 113 in the Reaction 209 Bi( 70 Zn, n) 278 113

Synthesis of Element 113 in the Reaction 209 Bi( 70 Zn, n) 278 113 Morita Kosuke, Morimoto Kouji, Kaji Daiya*, Yoshida Atsushi, Suda Toshimi, Yoneda Akira, Haba Hiromitsu*, Ohnishi Tetsuya, Kanungo Rituparna, Katori Kenji, Akiyama Takahiro, Ideguchi Eiji,

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Evidence for Exotic Mesons

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Galaxies and Cosmology

Galaxies and Cosmology. 5 points, vt-2007 Teacher: Göran Östlin Lectures 10-11. FRW-models, summary. Properties of the Universe set by 3 parameters:  m,  ,  k of Which only 2 are Independent:  m +   +  k = 1.

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ZEUS New Results

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Nuclear Reactions at Low Energies

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NDM09, Madison, Wisconsin Sept. 2, 2009

Neutrino-Induced Reactions on Fe and Ni Isotopes and Nucleosynthesis in Stars Toshio Suzuki Nihon University. NDM09, Madison, Wisconsin Sept. 2, 2009. New evaluation of reaction rates in fp-shell and light (p-shell) nuclei ? New shell model Hamiltonians

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Conceptual design and performance of high throughput cold spectrometer : MACS

Conceptual design and performance of high throughput cold spectrometer : MACS. Collin Broholm Johns Hopkins University and NIST Center for Neutron Research. Why MACS Layout and key elements Performance Data collection Scientific program Budget and schedule Conclusion.

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CBETA RF Systems

CBETA RF Systems. Peter Quigley. CBETA RF Systems: Overview. RF Hardware Cryogenic Systems Warmup/ Cooldown Tuning RF Control Future Plans. CBETA RF Systems: RF Hardware Injector Cryomodule (ICM). Twin Input Power Coupler. HGRP with three sections.

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Sketch of a competitive experiment on dense nuclear matter

Sketch of a competitive experiment on dense nuclear matter in the (future) Nuclotron energy range (2-5 AGeV). Helmholtz Summer School 2006, Dubna, Student Seminar Peter Senger, GSI. 1. The physics case: ? Nuclear equation of state at high baryon densities

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Discussion of Proposed mini-TimeCube

Discussion of Proposed mini-TimeCube. UH Team: Michelle Alderman, Steve Dye, John Learned, Shige Matsuno, Marc Rosen, Michinari Sakai, Stefanie Smith, Gary Varner.

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Nilsson Model 50 years

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Study of the Halo Nucleus 6 He using the 6 Li( g,p + ) 6 He Reaction

Study of the Halo Nucleus 6 He using the 6 Li( g,p + ) 6 He Reaction. Derek Branford - Edinburgh University for the A2-Collaboration MAMI-B Mainz.

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The EMMA Project

The EMMA Project. Rob Edgecock STFC Rutherford Appleton Laboratory & Huddersfield University. *BNL, CERN, CI, FNAL, JAI, LPSC Grenoble, STFC, TRIUMF. Outline. Why we needed to build EMMA How we got to where we are Design of the machine Construction Commissioning Conclusions.

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Fission and Fusion

Fission and Fusion. 3224 Nuclear and Particle Physics Ruben Saakyan UCL. Induced fission. Recall that for a nucleus with A ?240, the Coulomb barrier is 5-6 MeV

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Electromagnetic Radiation Hardness for the ILC BeamCal Sensors

Electromagnetic Radiation Hardness for the ILC BeamCal Sensors. Argonne SiD Workshop Friday, June 4 2010 Bruce Schumm Santa Cruz Institute for Particle Physics. The SCIPP/UCSC ILC R&D GROUP. Faculty/Senior Vitaliy Fadeyev Bruce Schumm. Collaborators Takashi Maruyama Tom Markiewicz

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APD

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MOON ... M olybdenum O bservatory O f N eutrinos

MOON ... M olybdenum O bservatory O f N eutrinos. H. Ejiri et al. PRL 85 (2000) 2917. Physics Goals:. Low Energy Solar Neutrino Spectroscopy Search for 0 ??? in 100 Mo Supernova Neutrino. Peter Doe, University of Washington NeSS 2002, Washington DC, 19 - 21 September, 2002. 100 Mo.

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