The Hadron Experimental Facility (HEF) of the Japan Proton Accelerator Research Complex (J-PARC) provides the world highest intensity hadron beams, such as kaons, pions, and so on, for various experimental researches in particle and nuclear physics. Currently, HEF operates two charged and one neutral secondary beam lines, K1.8, K1.1, and KL, sharing secondary beams produced at a primary target, T1. In addition, a high-momentum beam line is being constructed, which is branched from the primary beam line to deliver a fraction of the primary proton beam. We have a plan to extend HEF and construct a several new beam lines, which would enhance physics opportunities at HEF. A floor plan of extended HEF and physics scopes are presented.
KEYWORDS:Diquark, Exotic hadron, Hadron Spectroscopy, Chiral Symmetry, Hypernuclear Spectroscopy, Neutron Star, Baryon-baryon Interaction, Kaon Rare Decay, Hadron Beam
OverviewIn the Hadron Experimental Facility (HEF) of the Japan Proton Accelerator Research Complex (J-PARC), we aim to investigate how matter in the universe has been developed from elementary particles.It is still difficult to describe hadrons directly from current quarks. This is due to non-perturbative nature of Quantum Chromo-Dynamics (QCD) below the energy scale of Λ QCD~2 00 MeV, where the quarks change themselves drastically. Therefore, effective degrees of freedom, such as constituent quarks, seem to work rather well to describe hadrons as building blocks. We could learn how QCD works in hadrons through spectroscopic studies of hadrons and/or changes of hadron properties in nuclear medium.It is a longstanding issue how nuclei are formed from hadrons. We have been constructing a precise baryon-baryon (BB) interaction model, which must be basic to describe nuclei. Furthermore, it is demonstrated by an ab-initio calculation that 3-body nuclear forces are necessary to reproduce nuclear binding energies. Multi-body inter-baryon interactions have yet to be established. They would play an essential role to describe the nuclear matter at higher density, such as in neutron star (NS) cores. It is naturally thought that hyperons are emerged in NS cores because chemical potential of neutrons becomes large beyond the mass difference between neutron and hyperon.