Low energy interaction studies of negative kaons in light nuclear targets by AMADEUS
CENTRO FERMI - Museo Storico della Fisica e Centro Studi e Ricerche ‘Enrico Fermi’, Rome, Italy
2 INFN Laboratori Nazionali di Frascati, Frascati, Rome, Italy
3 Politecnico di Milano, Dip. di Elettronica, Informazione e Bioingegneria, Milano, Italy
4 Horia Hulubei National Institute of Physics and Nuclear Engineering, Magurele, Romania
5 University of Zagreb, Zagreb, Croatia
6 INFN Sezione di Milano, Milano, Italy
7 Stefan-Meyer-Institut für Subatomare Physik, Wien, Austria
8 Università degli Studi di Roma Tor Vergata, Rome, Italy
9 Excellence Cluster ‘Origin and Structure of the Universe’, Garching, Germany
10 Physik Department E12, Technische Universität München, Garching, Germany
11 INFN Sezione di Roma I, Rome, Italy
12 Istituto Superiore di Sanità, Rome, Italy
13 The University of Tokyo, Tokyo, Japan
14 RIKEN, The Institute of Physics and Chemical Research, Saitama, Japan
15 Institute of Physics, Jagiellonian University, Kracow, Poland
16 National Centre for Nuclear Research, Warsaw, Poland
* e-mail: firstname.lastname@example.org
Published online: 25 June 2018
The AMADEUS collaboration is performing experimental investigations in the sector of the low energy strangeness hadron physics by taking advantage of the DAΦNE collider, which provides a unique source of monochromatic low-momentum kaons and exploiting the KLOE detector as an active target. The K− single and multi-nuclear absorption on H, 4He, 9Be and 12C, both at-rest and in-flight, are studied with the aim to determine the nature of the controversial Λ(1405), the non-resonant hyperon pion formation amplitude below the K̅N threshold, the yield and cross sections of K− multi-nucleon absorptions intimately connected to the antikaon multi-nucleon clusters properties and the K− scattering cross sections on light nuclear targets.
These studies have a strong impact on the non-perturbative strangeness QCD with implications ranging from nuclear physics to the equation of state of neutron stars.
© The Authors, published by EDP Sciences, 2018
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