Axion

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Georg Raffelt, Max-Planck-Institut für Physik, München, Germany Limits on Axion-Photon Photon-Coupling PONT d‘Avignon, 21-25 April 2008, Avignon, France Axion-photon photon-coupling g aγ [GeV -1 ] 10 -4 10 -6 10 -8 10 -10 10 -12 10 -14 10 -16 Laser PVLAS expected Tokyo Helioscope CAST Sensitivity DM Search Future DFSZ model KSVZ model PVLAS Signature Helio seis mology +Gas Telescope Axion Line HB Stars 10 -7 10 -6 10 -5 10 -4 10 -3 10 -2 10 -1 1 10 100 Axion mass m a [eV]
Georg Raffelt, Max-Planck-Institut für Physik, München, Germany PONT d‘Avignon, 21-25 April 2008, Avignon, France Alps Axion-like particles (ALPs) (Pseudo)-scalar scalar particles with a two-photon vertex
Page 1 and 2: Georg G. Raffelt, Max-Planck Planck
Page 3 and 4: Georg Raffelt, Max-Planck-Institut
Page 5 and 6: Peccei-Quinn Mechanism Proposed in
Page 17 and 18: Supernova 1987A Energy-Loss Argumen
Page 19 and 20: Series of Papers on Axion Cosmology
Page 21 and 22: Series of Papers on Axion Cosmology
Page 23 and 24: Production of Cold Axion Population
Page 27 and 28: Axion Hot Dark Matter from Thermali
Page 29 and 30: Axion Hot Dark Matter Limits from P
Page 31 and 32: Experimental Tests of the Invisible
Page 43 and 44: Results and Plans of Tokyo Axion He
Page 45 and 46: LHC Magnet Mounted as a Telescope t
Page 49: Georg Raffelt, Max-Planck-Institut
Page 53 and 54: Dimming of Supernovae without Cosmi
Page 59: Technological Applications of PVLAS

Axion

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