Search results for Electroweak Baryogenesis funakubo/research/... •Introduction – Big Bang Cosmology – Saharov’s

Electroweak Baryogenesis K Funakubo Saga Univ June 4 ‘04 @ KEK Baryon Asymmetry of the Universe nB s ≡ nb − nb̄ s � 037 − 088 × 10−10 1 Big Bang Nucleosynthesis…

LHC Signals of MSSM Electroweak Baryogenesis David Morrissey Department of Physics University of Michigan Michigan Center for Theoretical Physics MCTP With: Csaba Balázs…

Microsoft PowerPoint - Baryogenesis.pptOr Making baryons from nothing in the Big Bang where nB = nb − nb is the difference between the number of baryons and antibaryons

Dark matter, baryogenesis and neutrinos Mikhail Shaposhnikov ISAPP 2011: The dark side of the Universe Heidelberg, 13 and 14 July 2011 – p. 1 Outline 1 Introduction: “No…

Nessun titolo diapositiva LHC Physics Luca Lista INFN - Napoli Electroweak results 1 p p W±, Z, γ* l ± l ∓, νl (−) q q(´) − EWK processes at LHC LHC Physics Measurement…

1. Cyber Bang 1o Πρότσπο Πειραματικό Γσμνάσιο Θεσσαλονίκης 2. Cyber Bang Νιώτης Α όστολος Πανοζάτος Νίκος…

4. Conclusions 1. Introduction sin2 θlept eff = 0.23150 ± 0.00016 0.07% ΓZ[ GeV] = 2.4952 ± 0.0023 0.09% MZ[ GeV] = 91.1875 ± 0.0021 0.002%

Nuclear and Particle Physics Franz Muheim 1 Standard Model Standard Model -- ElectroweakElectroweak InteractionsInteractions Weak Neutral Interactions Neutral Currents NC…

Seminar Cosmology 2008-2009 Baryogenesis η = 6.1± 0.3× 10−10 Author: Jan Weenink Supervisor: Dr. Tomislav Prokopec Institute for Theoretical Physics, Utrecht University…

Modul 6 KESETIMBANGAN BENDA (3D) 1. Kondisi Kesetimbangan Pada modul ini, kita memperluas prinsip dan metode yang telah dikembangkan untuk kesetimbangan dua dimensi pada…

Electroweak physics at LHC Marina Cobal, University of Udine ‘IFAE’, Torino Apr 14 - Apr 16, 2004 Outline Introduction W mass measurement Top mass measurement EW single…

Electroweak Physics Lecture 2 Last Lecture Use EW Lagrangian to make predictions for width of Z boson: Relate this to what we can measure: σ(e+e−→ff) Lots of extracted…

Electroweak Physics Lecture 3 Status so far… 6 parameters out of 18 Today 7 more! The Grand Reckoning Correlations of all yesterday’s Z peak observables from all 4 LEP…

Electroweak Precision Measurements: Today The Electroweak Sector of the SM § EW sector described by 3 parameters @ tree-level » g,g’ Coupling constants of

Electroweak results at the Tevatron Susana Cabrera for the CDF and D0 collaborations XXIIth International Workshop on Deep-Inelastic Scattering Electroweak Physics at Run…

PowerPoint Presentation Echoes of the Big Bang Carolin Crawford Gresham Professor of Astronomy NASA, ESA Planck/ESA 1 Stephen Leshin Credit Stephen Leshin 2 Stephen Leshin…

Electroweak results at the Tevatron Susana Cabrera for the CDF and D0 collaborations XXIIth International Workshop on Deep-Inelastic Scattering Electroweak Physics at Run…

1 Lecture VIII: Cosmic Frontier Connections ACFI NLDBD School 10/31-11/3 2017! M.J. Ramsey-Musolf U Mass Amherst http://www.physics.umass.edu/acfi/ 2 Lecture VIII Goals • …

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cosmo.dviFrequency (GHz) Excess Antenna Temperature at 4080 Mc/s” =⇒ Cosmic Microwave Background Radiation a pure Planckian with temperature TCMBR = 2.728±