'Heavy nuclei' diaporamas de présentation

Protons for Breakfast Do we need Nuclear Power Week 6

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Chapter 14

Chapter 14. Cosmology. Cosmology . Cosmology , the study of the universe as a whole, can tell you where your matter came from and where it is going.

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Discovery of a Quasi Dynamical Symmetry and Study of a possible Giant Pairing Vibration

Discovery of a Quasi Dynamical Symmetry and Study of a possible Giant Pairing Vibration. R.F. Casten WNSL, Yale May 11,2011. Evidence for a Quasi Dynamical Symmetry along the arc of regularity with an intro to the relevant Group Theory of dynamical symmetries

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Galactic Cosmic Rays

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Regularities of many-body systems in the presence of random two-body interactions

Regularities of many-body systems in the presence of random two-body interactions. Yu-Min ZHAO. 1 Department of Physics, Shanghai Jiao Tong University, China; 2 Center of Theoretical Nuclear physics, IMP, CAS, Lanzhou, China; 3 Cyclotron Center, RIKEN, Japan; 4 CCAST, CAS, Beijing, China.

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Effect of tensor interaction on shell structure of heavy and superheavy nuclei

Effect of tensor interaction on shell structure of heavy and superheavy nuclei. Xian-Rong Zhou Department of physics, Xiamen University, Xiamen, China. Collaborator: H. Sagawa, University of Aizu, Japan. Magic numbers. Z. N.

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397 views • 28 slides

Mini Quiz- Half Sheet H = 1.01 g/ mol , O = 16.00 g/ mol S = 32.07 g/ mol , N = 14.01 g/ mol , I = 126.90 g/ mol

Mini Quiz- Half Sheet H = 1.01 g/ mol , O = 16.00 g/ mol S = 32.07 g/ mol , N = 14.01 g/ mol , I = 126.90 g/ mol. How many grams in 3.4 x 10 23 molecules of H 2 SO 4 ? 2. How many molecules are there in 0.40 g of N 2 I 6 ?. Nuclear Chemistry. Unstable Nuclei.

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The case for High energy neutrino astronomy

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Nuclear and Hadron Physics group at Yonsei University and our physics interests

Nuclear and Hadron Physics group at Yonsei University and our physics interests. Su Houng Lee Hungchong Kim, Taesoo Song, Yongjae Park, Yongshin Kwon (Osaka), Youngsoo Son, Kyungchul Han, Kyungil Kim. Research Interests. Potential. Time. Space-Time Wilson Loop. Separation. Space.

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p +

MODERN PHYSICS. By 1932, the basic building blocks of matter were known:. p +. e-. n. The Bohr model of the atom was the basis for our understanding of what the solar system atom looked like:. e-. p +. n. n. p +. e-.

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CH.VIII: RESONANCE REACTION RATES

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Alpha Decay

Alpha Decay. Readings Nuclear and Radiochemistry: Chapter 3 Modern Nuclear Chemistry: Chapter 7 Energetics of Alpha Decay Theory of Alpha Decay Hindrance Factors Heavy Particle Radioactivity Proton Radioactivity Identified at positively charged particle by Rutherford

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Charged Particles

Charged Particles. Charged particles can come from nuclear decay. Nuclear physics figures into particle detection. Use terminology from nuclear physics. Isotopes share Z Isotones share N. Nucleus consists of protons and neutrons. Protons: Z ( atomic number ) Neutrons: N

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Nuclear Chemistry

Nuclear Chemistry. L. Scheffler. The Nucleus. The nucleus is comprised of the two nucleons : protons and neutrons. The number of protons is the atomic number. The number of protons and neutrons together is effectively the mass of the atom. Isotopes.

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with S . Mavrodiev (INRNE, BAS, Sofia, Bulgaria D . Vlasenko (NPU, Odessa, Ukraine)

Kramers Diffusive Mechanism of Alpha Decay, Proton/Cluster Radioactivity and Spontaneous Fission, Induced by Vacuum Zero-point Radiation Vitaliy Rusov Department of Theoretical and Experimental Nuclear Physics, Odessa National Polytechnic University, Ukraine. with

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Welcome to Jefferson Lab

Welcome to Jefferson Lab. R. D. McKeown Jefferson Lab. Hypernuclear Workshop May 27 , 2014. 12 GeV Upgrade Project. New Hall. Add 5 cryomodules. 20 cryomodules. Add arc. 20 cryomodules. Add 5 cryomodules. Enhanced capabilities in existing Halls.

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star.le.ac.uk /~ mbu / lectures.html

Lecture course slides can be seen at:. http:// www.star.le.ac.uk /~ mbu / lectures.html. Ch. 40. Nuclear size and Shape. Nuclei exist bcse strong nuclear force overcomes electrostatic repulsion force over close distances inside nucleus

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Newly Born Pulsars as Sources of High and Ultrahigh Energy Cosmic Rays

Newly Born Pulsars as Sources of High and Ultrahigh Energy Cosmic Rays. Ke Fang University of Chicago ISCRA - Jul 9, 2012. KF, Kotera , Olinto 2012, ApJ , 750, 118 KF, Kotera , Olinto 2012, in prep. UHECR Observational Facts. GRB AGN Clusters Pulsars. ?? ??. ????.

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A L arge I on C ollider E xperiment

A L arge I on C ollider E xperiment. A L arge I on C ollider E xperiment. is the dedicated experiment to study collisions of heavy nuclei. A Large Ion Collider Experiment. ALICE will study collisions of heavy nuclei, like Pb. WHY?.

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