'Mass dependence' diaporamas de présentation

Recent results from lattice QCD

Recent results from lattice QCD. Tetsuya Onogi (YITP, Kyoto Univ.) for JLQCD collaboration. JLQCD Collaboration. KEK S. Hashimoto, T. Kaneko, H. Matsufuru, J. Noaki, M. Okamoto E. Shintani, N. Yamada RIKEN/Niels Bohr H. Fukaya

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Issues for Jet Algorithms: A Quick Review, (But No Quick Answers)

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The QCD equation of state and transition at zero chemical potential

The QCD equation of state and transition at zero chemical potential . Michael Cheng Lawrence Livermore National Laboratory. Strong Interaction in the 21 st Century February 11, 2010 Tata Institute of Fundamental Research, Mumbai. 10 -5 sec of QGP. Heavy Ion Colliders. LHC. RHIC.

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Probing the Top Quark Mass with Leptons: The Framework University of Athens

Probing the Top Quark Mass with Leptons: The Framework University of Athens. Costas Vellidis. Why measure the Top Mass. The Higgs mass is tied to m top and m W. QCD Production (~6pb) dominates at Tevatron: 85%: 15%:. proton. e-e(1/81). mu-mu (1/81). tau-tau (1/81).

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Neutron EDM with external electric field

Neutron EDM with external electric field. Eigo Shintani (Univ. of Tsukuba) In collaboration with S. Aoki, Y. Kuramashi and CP-PACS collaboration. Introduction. parameter Both CKM matrix phase and QCD vacuum effects contribute to CP violation (T and P violation) parameter.

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Semileptonic Hyperon Decays in Full QCD

Semileptonic Hyperon Decays in Full QCD. Huey-Wen Lin. in collaboration with Kostas Orginos. Outline. Motivation/Background Quick Review of Lattice Calculations Lattice Techniques/Parameters Numerical Results Summary and Outlook. Semileptonic Decays and CKM Matrix.

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Raimond Snellings For the STAR Collaboration

A critical assessment of evidence obtained in the first three years of RHIC running for QGP formation. Raimond Snellings For the STAR Collaboration. Introduction. The main goal of RHIC is to search for QGP formation in the laboratory and study the properties of this state of matter

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Update on Combinatorial Background for Partially Reconstructed Modes

Update on Combinatorial Background for Partially Reconstructed Modes. Amanda Deisher B Mixing and Lifetimes May 30, 2006. Outline. Mass Distributions Mass shape of WS in partially reconstructed mass regions Possible physics backgrounds in WS Lifetime Distributions

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Multiplicity in the Chamaeleon I SFR

Multiplicity in the Chamaeleon I SFR. Mirza Ahmic University of Toronto Ray Jayawardhana, Alexis Brandeker, Aleks Scholz, Ivana Damjanov, Marten van Kerkwijk. Multiplicity properties important to constrain formation mechanisms of stars and brown dwarfs Ejection In situ

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( SPH) Simulations of Binary N eutron Star Coalescence

Examining the Mass Ratio Dependence of. Post-Newtonian Smoothed Particle Hydrodynamics. ( SPH) Simulations of Binary N eutron Star Coalescence. Jonathon Meyers, Yi Mei, Rick Hallett , Margie Michna. Purdue University North Central. Advisor: Dr. Aaron Warren. 2012. Introduction.

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Stellar Structure

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