'5 mev' diaporamas de présentation

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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General view of CYCLONE C18/18

Yerevan Physics Institute R.Avakian, G.Bazoyan, M.Hakobyan, I.Kerobyan The Possibility of Obtaining Intense Neutron Source on the base of proton Cyclotron C18 . New Accelerator Complex for Science and Application. General view of CYCLONE C18/18. The technical features of CYCLONE C18/18 :.

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The MAX-lab facility

The MAX-lab facility. The MAX-lab facility. MAX I storage ring (550 MeV)/stretcher 1986 MAX II storage ring (1.5 GeV) 1995 MAX III storage ring (.7 GeV) 2007 FEL (test facility) 2007 MAX IV proposal 2007 ( VR ? governement). MAX I. MAX III. MAX II. Injector. FEL. Nuclear Physics area.

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CHARMONIUM

CHARMONIUM. New era (~after 2001). This lecture is about the. where I hope to convince you that charmonium still has the potential to surprise us. B-factories. Superconducting Coil (1.5T). Silicon Vertex Tracker (SVT)[5 layers]. e + (3 GeV). e - (9 GeV). Aerogel Cherenkov cnt.

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Over 1 million reconstructed!!

Over 1 million reconstructed!!. Successor to E687. Designed to study charm particles produced by ~200 GeV photons using a fixed target spectrometer with upgraded Vertexing , Cerenkov , E+M Calorimetry , and Muon id capabilities. Includes groups from USA, Italy, Brazil, Mexico, Korea

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Fisica del b in CMS

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Theoretical analysis of the deuteron-induced activation at low and medium energies

Theoretical analysis of the deuteron-induced activation at low and medium energies. FENDL-3 3rd RCM NDS/IAEA, Vienna, 6-9 December 2011. Marilena Avrigeanu and Vlad Avrigeanu. “Horia Hulubei” National Institute for Physics and Nuclear Engineering, P.O.Box MG-6, Bucharest, Romania.

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Proton Drivers & Muon Sources at Fermilab

Proton Drivers & Muon Sources at Fermilab. David Neuffer Fermilab. Introduction–Fermilab Future Plans (~Oddone). (Tevatron shuts down ~2009) First Priority – ILC Global Study ~1 year –present to DOE (end of 2006) IF favorable, push for near-term construction at Fermilab

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Resonances and thresholds in charmonium spectra

Resonances and thresholds in charmonium spectra. Yu.S.Kalashnikova, ITEP. Charmonium. Theory: Godfrey-Isgur. M, MeV. ?. 4250. 4000. ?. 3750. DD. 3500. 3250. 3000. 0 -+. 1 --. 0 ++. 1 ++. 2 ++. 1 +-. 2 --. 3 --. 2 -+. 1++(3872). 1--(4260). JPC?(4430). I=1 !?.

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Coulomb excitation at intermediate energies

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D 0 K + mass spectra for:

D 0 K + mass spectra for:. B + ? D 0 D 0 K + B 0 ? D - D 0 K + B 0 ? D* - D 0 K +. for ? 25 0fb -1 (exp7-3 7 ). Outline : B + ? D 0 D 0 K + B 0 ? D - D 0 K + B 0 ? D* - D 0 K + for ? 250fb -1 Dalitz plots and projections B ackground subtracted M(D 0 K + ) distributions

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? 0 -threshold measurements ( unpol. photons )

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Neutron Gamma Discrimination in Agata

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Results from the Borexino experiment

Milano. Perugia. Results from the Borexino experiment. Cracow Epiphany Conference 5-8 January, 2010 Krakow, Poland. M. Misiaszek ( Institute of Physics, Jagellonian U., Krakow ) on behalf of the Borexino C ollaboration. Princeton University. Genova. APC Paris. Virginia Tech.University.

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High Current Energy Recovery Linac at BNL

High Current Energy Recovery Linac at BNL.

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279 views • 16 slides

What is the charmed analog of L (1405)?

What is the charmed analog of L (1405)?. Kiyoshi Tanida (Seoul National University) Aug. 23, 2011 APFB2011, Seoul. ? ? 1405 ?. How is it in charmed sector?. Large mass difference of ?? and DN ? mixing should be small Both of ?? resonance and ND bound state can be seen as separate peaks?.

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Fusion of Heavy Ions

Fusion of Heavy Ions. Students: Paduraru Catalin (Univ. of Bucharest, RO) Sporea Ciprian (West Univ. of Timisoara, RO) Pasca Horia (“Babes-Bolyai” Univ., RO) Supervisors: Dr. Alexander Karpov Dr. Andrey Denikin. Objectives.

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Gravitational Potential Energy

Potential Energy and Principle of Conservation of Energy. Gravitational Potential Energy. is the energy that an object of mass m at a distance y from the earth has due to the gravitational attraction between the object and the earth. Conservation of total mechanical energy

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Second C LIC T est F acility (CTF-II) !! Two beam acceleration !!

Second C LIC T est F acility (CTF-II) !! Two beam acceleration !!. q train 375 nC q bunch 7.8 nC 30 GHz power out of PETS 1/2 27/22 MW 30 GHz power into CAS 1/2 21/17 MW RF pulse length 16 ns Gradient in CAS 1/2 57/51 MV/m 30 GHz acceleration 30.5 MeV.

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