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The kaonic 3He and 4He X-rays emitted in the 3d-2p transitions were measured in the SIDDHARTA experiment. The widths of the kaonic 3He and 4He 2p states were determined to be Gamma_2p(3He) = 6 pm 6 (stat.) pm 7 (syst.) eV, and Gamma_2p(4He) = 14 pm 8 (stat.) pm 5 (syst.) eV, respectively. Both results are consistent with the theoretical predictions. The width of kaonic 4He is much smaller than the value of 55 pm 34 eV determined by the experiments performed in the 70s and 80s, while the width of kaonic 3He was determined for the first time.
180 - M. Bazzi , G. Beer , L. Bombelli 2012
Kaonic hydrogen atoms provide a unique laboratory to probe the kaon-nucleon strong interaction at the energy threshold, allowing an investigation of the interplay between spontaneous and explicit chiral symmetry breaking in low-energy QCD. The SIDDHA RTA Collaboration has measured the $K$-series X rays of kaonic hydrogen atoms at the DA$Phi$NE electron-positron collider of Laboratori Nazionali di Frascati, and has determined the most precise values of the strong-interaction induced shift and width of the $1s$ atomic energy level. This result provides vital constraints on the theoretical description of the low-energy $bar{K}N$ interaction.
90 - M. Bazzi , G. Beer , L. Bombelli 2011
The $bar{K}N$ system at threshold is a sensitive testing ground for low energy QCD, especially for the explicit chiral symmetry breaking. Therefore, we have measured the $K$-series x rays of kaonic hydrogen atoms at the DA$Phi$NE electron-positron co llider of Laboratori Nazionali di Frascati, and have determined the most precise values of the strong-interaction energy-level shift and width of the $1s$ atomic state. As x-ray detectors, we used large-area silicon drift detectors having excellent energy and timing resolution, which were developed especially for the SIDDHARTA experiment. The shift and width were determined to be $epsilon_{1s} = -283 pm 36 pm 6 {(syst)}$ eV and $Gamma_{1s} = 541 pm 89 {(stat)} pm 22 {(syst)}$ eV, respectively. The new values will provide vital constraints on the theoretical description of the low-energy $bar{K}N$ interaction.
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