Spectrum and decays of hadronic atoms

We describe the spectra and decays of pi pi and pi K atoms within a non-relativistic effective field theory. The evaluations of the energy shifts and widths are performed at next-to-leading order in isospin symmetry breaking. The prediction for the lifetime of the pi K atom in its ground-state yields tau = (3.7 \pm 0.4) * 10^{-15} sec.Comment: To appear in the proceedings of MESON 2004: 8th International Workshop on Meson Production, Properties and Interaction, Cracow, Poland, 4-8 June 2004. 7 page

An Experimental Study of Warranty Coverage and Dispute Resolution in Competitive Markets

In service and product markets where warranties are offered, disputes over warranty performance frequently occur between buyer and seller. Resolving such disputes in a fair and effective way has become an increasingly important and controversial question in recent years. Some observers have gone so far as to argue that the pervasiveness of such disputes and the inability to resolve them effectively is having a corrosive effect on society.1 This is probably somewhat extreme, but even a less excited perspective suggests that the design of procedures to handle consumer disputes is a matter for serious concern

Spectrum and Variability of Mrk501 as observed by the CAT Imaging Telescope

The CAT Imaging Telescope has observed the BL Lac object Markarian 501 between March and August 1997. We report here on the variability over this time including several large flares. We present also preliminary spectra for all these data, for the low emission state, and for the largest flare.Comment: 4 pages, 4 figures, Late

Observation of the Crab Nebula Gamma-Ray Emission Above 220 Gev by the Cat Cherenkov Imaging Telescope

The CAT imaging telescope, recently built on the site of the former solar plant Themis (French Pyrenees), observed gamma-rays from the Crab nebula from October 1996 to March 1997. This steady source, often considered as the standard candle of very-high-energy gamma-ray astronomy, is used as a test-beam to probe the performances of the new telescope, particularly its energy threshold (220 GeV at 20 degrees zenith angle) and the stability of its response. Due to the fine-grain camera, an accurate analysis of the longitudinal profiles of shower images is performed, yielding the source position in two dimensions for each individual shower.Comment: 5 pages, 3 figures, Tex, contribution to 25th ICRC Durba