* e.g. J Andruszkow et al., Phys. Rev. Lett., 85, 3825, (2000).**e.g. G. R. Neil et al., Phys. Rev. Lett. 84, 662, (2000).*** e.g. H Wabnitz et al., Nature, 420, 467, (2002), T Laarmann et al., Phys. Rev. Lett., 95, 063402 (2005)
| Paper | Title | Page |
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| FRZKI01 | Physics from Tevatron to LHC and ILC | 3830 |
| The physics reach of LHC and the need of ILC beams in the investigation of the physics of weak and strong electroweak symmetry breaking, supersymmetric models, new gauge theories, models with extra dimensions, and electroweak and QCD precision physics. | ||
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| FRZKI02 | Neutrino Physics | 3835 |
| Twenty years have passed after the supernova SN1987A. Before SN1987A, it was often said that neutrino physics was largely an art of learning a great deal by observing nothing. But after SN1987A, the neutrino became a little less mysterious. The solar neutrino deficit which was observed in the Homestake solar neutrino experiment, was confirmed by Kamiokande, Gallex and SAGE. An atmospheric neutrino anomaly was observed in Kamiokande. IMB, MACRO and SUDEN reconfirmed this anpmaly. In 1998 Super-Kamiokande obtained the evidence of atmospheric neutrino oscillations. This was the first discovery of a finite neutrino mass. The atmospheric neutrino oscillations were reconfirmed by K2K. In 2002 SNO detected the evidence of flavor-transformation of solar neutrinos, and KamLAND detected the evidence of reactor antineutrino oscillations. In my talk what we learned from the above neutrino experiments is briefly reviewed, and what we will learn by on-going and proposed neutrino experiments is discussed. | ||
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| FRZKI03 | Next Generation Advanced Light Source Science | 3840 |
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Recent advances in accelerator science make feasible the provision of XUV and harder X-ray FELs that will generate short (fs regime) pulses of light that is broadly tuneable and >106 times more intense than spontaneous undulator radiation*. Energy recovery technology** offers the promise of short pulse, high peak flux spontaneous radiation, with particular advantages in the IR and THz parts of the spectrum. The new science enabled by these 4th generation sources is reviewed. A key feature is dynamic measurements. Pump-probe experiments will allow real-time measurements of reaction pathways and short-lived intermediates. The high intensity of FEL radiation will allow very high resolution in imaging applications. The very high field intensity of the XUV radiation will lead to the creation of new states of matter, while at the highest X-ray energies, the goal is to achieve single molecule diffraction. The talk will be illustrated by experiments proposed in the Science Cases for the major world 4th generation projects. Some of the science already undertaken using IR and UV FELs, and results obtained from new XUV sources (such as FLASH at DESY***) will be discussed.
* e.g. J Andruszkow et al., Phys. Rev. Lett., 85, 3825, (2000).**e.g. G. R. Neil et al., Phys. Rev. Lett. 84, 662, (2000).*** e.g. H Wabnitz et al., Nature, 420, 467, (2002), T Laarmann et al., Phys. Rev. Lett., 95, 063402 (2005) |
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| FRZKI04 | Plasma Accelerators - Progress and the Future | 3845 |
| In recent months plasma accelerators have set new records: The first laser wakefield accelerator to demonstarte near GeV beam with large charge and good beam quality in a table-top device at LBNL, and the energy-doubling of the SLAC beam in a short plasma channel by the plasma wakefield acceleration technique. These two events, happening at two different laboratories signifies a coming of age of advanced accelerator R&D. | ||
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