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          July 26–30, 2014
        
        
          
            Tuesday afternoon
          
        
        
          APS Plenary: Sponsored by the Division
        
        
          of Particles and Fields
        
        
          Location:  Northrop Auditorium
        
        
          Date:         Tuesday, July 29
        
        
          Time:        3:30–5 p.m.
        
        
          Presider:  Ken Heller
        
        
          
            1. Physics at the CERN Large Hadron Collider, the Past, the Present
          
        
        
          
            and the Future
          
        
        
          Roger Rusack, School of Physics and Astronomy, University of Minnesota
        
        
          Physicists working at the Energy Frontier using the Large Hadron Collider (LHC) at CERN announced
        
        
          last year the observation of the Higgs boson at 125.6 GeV. I will tell a small part of the story of what we
        
        
          did to be able to make that announcement and discuss what is happening now at the LHC as we get ready
        
        
          to start data taking at double the collision energy. I will also speak about the plans for the future and pos-
        
        
          sibilities that lie ahead.
        
        
          
            2. Explorations in the Cosmic Frontier: Shedding Light on the Dark?
          
        
        
          Lucy Fortson, School of Physics and Astronomy, University of Minnesota
        
        
          The last decade has seen an amazing investment in instruments in particle astrophysics. These experi-
        
        
          ments are exploring the “cosmic frontier” in an effort to find the answers to some of the biggest ques-
        
        
          tions in physics: What is Dark Energy? What is the nature of Dark Matter and what is it going to take to
        
        
          discover it? What is the physics of the high-energy Universe and where do the highest-energy cosmic rays
        
        
          come from?  In this round-up of the cosmic frontier, I will review what we are learning about these “big
        
        
          questions” with a focus on some of the progress made in the effort to detect Dark Matter, both with direct
        
        
          detection experiments such as CDMS and indirect detection through the use of very high-energy photons
        
        
          observed by VERITAS. Along the way, I will touch on topics such as the characteristics of Nature’s particle
        
        
          accelerators – astrophysical jets emanating from supermassive black holes at the centers of active galaxies
        
        
          and how we can use their emissions as probes of the existence of a specific Dark-Matter candidate-Axion-
        
        
          like particles.
        
        
          
            3. The Turn of the Screw: A Chilling Ghost Story of Nature’s Most
          
        
        
          
            Unusual Fermion
          
        
        
          Dan Cronin-Hennessy, School of Physics and Astronomy, University of Minnesota
        
        
          The Standard Model of particle physics is arguably the most successful theory ever and yet we still do
        
        
          not have a proper theory of flavor. Working at the Intensity Frontier, the flavor oscillations of neutrinos
        
        
          provide crucial information concerning mass, mixing, and the matter/anti-matter asymmetry of our
        
        
          Universe. I will review several of the most active areas of particle physics that exploit the neutrinos’ unique
        
        
          properties in order to advance our knowledge of fundamental laws.
        
        
          
            Rioger Rusack
          
        
        
          
            Lucy Fortson
          
        
        
          
            Dan Cronin-
          
        
        
          
            Hennessy
          
        
        
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