PPT-Higgs Mechanism at Finite Chemical Potential

with TypeII Nambu Goldstone Boson Based on arXiv11024145v2 hep ph Yusuke Hama 　 Univ Tokyo Tetsuo Hatsuda Univ Tokyo Shun Uchino Kyoto Univ 420 2011 　 Dense Strange Nuclei and Compressed Baryonic Matter. (s). Why do we need them?. What do they look like?. Have we found them?. γ. Quantum Electrodynamics. predicts one . massless. . spin-1. . gauge boson. PHOTON. g. Quantum . Chromodynamics. . predicts . Tim Wiser. Splash P2506. 3 Nov 2012. Plan . Standard Model of Particle Physics. Particles, interactions, and the Higgs field. Drawing Feynman diagrams. These simple pictures are actually . calculational. : data . vs. theory. Joey Huston. Bruce . Mellado. 1. Higgs(->. gg. )+jets. Most of the excess observed for Higgs production is in >=1 jet final states. Maybe CMS does not see as large of an excess. (s). Why do we need them?. What do they look like?. Have we found them?. γ. Quantum Electrodynamics. predicts one . massless. . spin-1. gauge boson. PHOTON. g. Quantum . Chromodynamics. . predicts . December 12th-16th, 2011. Table of Contents. CERN Higgs boson Flash Report. . Executive Summary & Findings 3-4. Background 5. Pre-announcement overview 6. Announcement overview 7. Chapter 2. Finite Element Analysis (F.E.A.) of 1-D Problems. Historical Background . Hrenikoff, 1941 – “frame work method” . Courant, 1943 – “piecewise polynomial interpolation” . Turner, 1956 – derived stiffness matrices for truss, beam, etc. S. Dawson. CMS HH Workshop. January 18, 2016. 1. S. Dawson. Outline. Why measure the Higgs-self couplings?. What do we expect?. Standard Model. Issues with the top mass dependence. Beyond the Standard Model. (probably). Not just another fundamental particle…. July 27, 2012. Purdue QuarkNet Summer Workshop. 1. Matthew Jones. Purdue University. 27-July-2012. The Standard Model. Charge. 1. st. family. 2. Christian Grefe, . Tomáš Laštovička. , Blai Pie Valls, Jan Strube and Frederic Teubert . WG6 Meeting . 16/02/2011. Channels Summary. H→. μμ. Very rare decay (≈5.10. -4. ). Difficult to observe at the LHC (3. Kei . Yagyu. . (National Central U). M. Aoki, S. . Kanemura. , KY, PRD85 (2012), . S. . Kanemura. , KY, PRD85 (2012), . M. Aoki, S. . Kanemura. , M. Kikuchi, KY, PLB714 (2012), . M. Aoki, S. . Kanemura. after the Higgs Discovery. M.V. . Chizhov. Sofia University, Bulgaria and JINR, Russia. 09/06/2014. 2. Why do we need the Higgs boson?. S = ½. S = 1. S = 0. 09/06/2014. Harmonic Oscillator. (Analytical . W. Verkerke. (NIKHEF). Introduction. Enormous effort to search for Higgs signature in many decay channels. Results .  many plots with signal, . background expectations, each with . (systematic) uncertainties, and data. M. Veltman. NIKHEF. Amsterdam. Cern, 4 dec. 2009. Higgs search. Higgs hunting. In 1974 I asked myself: if the Higgs is all around us in the vacuum. we should really be able to see it. Since the Higgs field in the vacuum. in support of US air quality management: application to the GEOS-Chem model. Daniel Jacob. with Kelvin Bates, Xuan Wang. 1. , Viral Shah, Lu Shen, Makoto Kelp, Bob Yantosca . An EPA STAR Chemical Mechanisms for Air Quality Modeling Project.