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1st Joint ILIAS-CAST-CERN Axion Training

Europe/Zurich
500/1-001 - Main Auditorium (CERN)

500/1-001 - Main Auditorium

CERN

400
Show room on map
Markus Kuster
Description

An accompanying presentation in the CERN seminar will be given by Karl van Bibber on Tuesday 29. November 2005

Conference web-page Axion-Training 2005


    • Lectures I 500/1-001 - Main Auditorium

      500/1-001 - Main Auditorium

      CERN

      400
      Show room on map
      • 1
        Introduction
        Speaker: Konstantin Zioutas (University of Patras)
        transparencies
        Video in CDS
      • 2
        The Strong CP Problem and Axions

        Outline of the lecture:

        In this lecture I will explain the origin of the Strong CP Problem, which is connected to the non- trivial structure of the vacuum state of the Standard Model. The most natural solution to this problem involves introducing an additional global chiral U(1) symmetry in the theory. Because this symmetry is both spontaneously broken and anomalous, this solution necessitates the presence of a very light, very weakly coupled boson, known as the axion. Physical properties of axions, including their mixing with pions and etas and their coupling to two-photons are described. Using these results, it is possible to rule out weak-scale axions. However, invisible axions models are still viable. Some of the properties of these latter models will be also discussed.
        Speaker: Roberto Peccei (University of California)
        transparencies
      • 10:40
        Break
      • 3
        Axion Searches, Old and New

        Outline of the lecture:

        Constraints from laboratory searches and astrophysics, axion cosmology, the cavity detector of dark matter axions, solar axion searches, laser experiments, a telescope search, macroscopic forces mediated by axions.
        Speaker: Pierre Sikivie (Institute for Advanced Study and University of Florida)
        transparencies
        Video in CDS
    • Presentations I 500/1-001 - Main Auditorium

      500/1-001 - Main Auditorium

      CERN

      400
      Show room on map

      Please note that the time indicated for each presentation includes 5 minutes for discussions.

      • 4
        Coherence
        Speaker: Yannis Semertzidis (Brookhaven National Laboratory)
        transparencies
      • 5
        Introduction to X-ray Optics
        Speaker: Peter Friedrich (Max-Planck Institut fuer extraterrestrische Physik)
        transparencies
      • 6
        The BMV Project : Axions Search with a Pulsed Magnet
        Speaker: Remy Battesti (Universite Paul Sabatier)
        transparencies
      • 7
        Large Extra Dimensions and CAST
        Speaker: Biljana Lakic (Rudjer Boskovic Institute)
        transparencies
      • 8
        Astrophysical Signatures for Axion(-like) Particles
        Speaker: Konstantin Zioutas (University of Patras)
        transparencies
      • 16:10
        Break
    • Presentations II 500/1-001 - Main Auditorium

      500/1-001 - Main Auditorium

      CERN

      400
      Show room on map

      Please note that the time indicated for each presentation includes 5 minutes for discussions.

      • 9
        Photon-Axion Conversion as a Mechanism for Supernova Dimming: Limits from CMB Spectral Distortion
        Speaker: Alessandro Mirizzi (University of Bari)
        transparencies
      • 10
        Detecting Solar Axions Using Earth's Magnetic Field
        Speaker: Hooman Davoudiasl (University of Wisconsin)
        transparencies
      • 11
        Search for KK axions with a low pressure gas TPC
        Speaker: Neil Spooner (University of Sheffield)
        transparencies
      • 12
        PVLAS-Recent Results
        Speaker: Giovanni Cantatore (Universita di Trieste - I.N.F.N.)
        transparencies
      • 13
        Round Table Discussion
        Speaker: All
    • Lectures II 500/1-001 - Main Auditorium

      500/1-001 - Main Auditorium

      CERN

      400
      Show room on map
      • 14
        Axions and Astrophysics

        Outline of the lecture:

        Axion emission from stars, astrophysical limits on axion parameters: from globular clusters, SN 1987A, ...
        Axions as hot dark matter, limits from cosmological structure formation.
        Speaker: Georg Raffelt (Max-Planck Institut fuer Physik)
        transparencies
        Video in CDS
      • 10:30
        Break
      • 15
        Electric and Magnetic Dipole Moments

        Outline of the lecture:

        The stringent limit on the electric dipole moment of the neutron forced the issue on the strong CP-problem. The most elegant solution of which is the axion field proposed by Peccei and Quinn. The current limit on the QCD parameter theta coming from the limit on the neutron EDM is of order 10-10. I am going to describe the present status on the neutron EDM searches and further prospects on getting down to theta_qcd sensitivity of 10-13 with the new deuteron EDM in storage rings proposal. For completeness the current status and prospects of the muon g-2 experiment will also be given.
        Speaker: Yannis Semertzidis (Brookhaven National Laboratory)
        transparencies
        Video in CDS
    • Workshop on Future Axion Searches 500/1-001 - Main Auditorium

      500/1-001 - Main Auditorium

      CERN

      400
      Show room on map

      Please note that the time indicated for each presentation includes 5 minutes for discussions.

      • 16
        Introduction
        Speaker: Konstantin Zioutas (University of Patras)
      • 17
        Laboratory Experiments for Axion Search Using Decommissioned LHC Superconducting Dipoles
        Speaker: Pierre Pugnat (CERN)
        transparencies
        Video in CDS
      • 18
        Search for (solar) Axions in the Visible
        Speaker: Konstantin Zioutas (University of Patras)
        transparencies
      • 19
        Towards a Large-Scale Axion Laser Experiment
        Speaker: Andreas Ringwald (DESY)
        transparencies
      • 20
        Some Remarks About Light Pseudoscalar Particles
        Speaker: Raul Rabadan (Institute for Advanced Study, Princeton)
        transparencies
      • 21
        Round Table Discussion
        Speaker: All
    • CAST Visit 0--CAST Experiment

      0--CAST Experiment

      CERN

      A shuttle bus from CERN to the experimental area of CAST will be available.

    • Lectures III 500/1-001 - Main Auditorium

      500/1-001 - Main Auditorium

      CERN

      400
      Show room on map
      • 22
        Cavity Microwave Searches for Cosmological Axions

        Outline of the lecture:

        The lecture will cover the searches for dark matter axions based on the microwave cavity experiment of Sikivie. The topics will begin with a brief overview of halo dark matter, and the axion as a candidate. The principle of resonant conversion of axions in an external magnetic field will be described, and practical considerations in optimizing the experiment as a signal-to-noise problem. A major focus of the lecture will be the two complementary strategies for ultra-low noise detection of the microwave photons - the "photon-as-wave" approach (i.e. conventional heterojunction amplifiers and soon quantum-limited SQUID devices), and "photon-as-particle" (i.e. Rydberg-atom single-quantum detection). Experimental results will be presented; these experiments have already reached well into the range of sensitivity to exclude plausible axion models, for limited ranges of mass. The lecture will conclude with a discussion of future plans and challenges for the microwave cavity experiment.
        Speaker: Karl van Bibber (LLNL)
        transparencies
        Video in CDS
      • 10:30
        Break
      • 23
        Axions and Their Relatives

        Outline of the lecture:

        A summary of the status of axions and axion-like particles will be given. Special attention is devoted to the recent results of the PVLAS collaboration, which are in conflict with CAST data and with astrophysical constraints. Solutions to this puzzle and the implications for new physics are dicussed. The subject of axion-like particles as dark matter will be included in the lecture. Finally some new results on new forces mediated by light scalars are debated.
        Speaker: Eduard Masso (University of Barcelona)
        transparencies
        Video in CDS
      • 24
        Summary and Closing Remarks
        Speaker: Konstantin Zioutas (University of Patras)
        transparencies