Strangeness Nuclear Physics • Nuclei: many body systems of nucleons – Can be extended by adding other flavors: strangeness, charm, ... Unexplored “space” S=0 “surface” Physics interests • New interaction – Extended nuclear force to flavor SU(3) world – Unified understanding of Baryon-Baryon force – What is its origin? – Is traditional meson exchange model enough? Need quark/gluon picture? • Property of hyperons in nuclei? – Hyperons can mix easily (e.g., LN-SN, LL-XN) → Dynamical systems can be made – Effective mass, magnetic moment, ...? • What happens to nuclei? Impurity effect? – Collective motion? High density matter? Relation with neutron star • Naively, hyperons are expected to appear in NS – E.g., Fermi gas model w/o interaction Fermi energy of n: πΈπΉ = ππΉ 2 /2m~58(π/π0 )2/3 MeV ο πΈπΉ > πΛ − ππ at π~5π0 – L, S-, X- may be important • Of course, details depend on nuclear interaction – Most of present calculations expect hyperons at 2~3π0 – Can be studied by SNP at J-PARC – Especially, X potential in nuclei is a key • Mass, size, ...? Nuclear & Hadron Physics in J-PARC Experiments at aPhysics glanceat(not all) Nuclear & Hadron J-PARC d High Density Nuclear Matter, Nucelar Force u Strange ness Hypernuclei 6 LLHe K0 → p0 nn L s d u Pentaquark ο+ Origin of Mass Confinement LL, X Hypernuclei Z -1 0 Quark L, S Hypernuclei -2 N L,X SKS Free quarks K1.8 Bound quarks Why are bound quarks heavierοΌ Mass without Mass Puzzle K1.8BR KL K1.1 K-meson Implantation of High Density Kaon and the nuclear shrinkage Nuclear Matter, Nucelar Force COMET Beam line οΌ«− T-Viola tion οΌΈray Kaonic atom Kaonic nucleus nucleus m-e conversion ο μ− e- Part I. (selected) Results from recent experiments E27, E15, & E13 Deeply bound Kaonic nuclei L(1405) = K-p bound state ο deeply bound nuclei? Kaon condensation in neutron stars? DISTO (PRL 94, 212303) FINUDA PRL104, 132502 Akaishi & Yamazaki, PRC 65 (2002) 044005 ο³ No observation in HADES, LEPS, … BK > 100 MeV?? E27 • Search for K-pp by d(p,K+) reaction – missing mass spectroscopy Decay counter to detect ppp from Kpp ο Lp ο ppp d(π+, K+) at 1.69 GeV/c (Inclusive spectrum) Y* peak; data = 2400.6 ± 0.5(stat.) ± 0.6(syst.) MeV/c2 +2.8 sim = 2433.0 -1.6 (syst.) MeV/c2 +2.9 ``shift” = οΌ32.4 ± 0.5(stat.) -1.7 (syst.) MeV/c2 Mass shift of L*(1405) and/or S*(1385)? due to final state interaction? Gaussian fit PTEP 101D03 (2014) 10 Range counter array(RCA) for the coincidence measurement • RCA is installed to measure the proton from the K-pp. – K-pp→Λp→pπ-p; K-pp→Σ0p→pπ-γp; K-pp→Ypπ→pπp+(etc.) • Proton is also the produced from the QF processes. We suppress QF background by tagging a proton. +Λπ0, Λ→pπ–β π+``n’’→K Seg2 and 5 are free from QF background. More strongly suppress by tagging two protons. • However, these proton’s kinematics is different. K+ p p π+ 11 ``K-pp’’-like structure(coincidence) • Broad enhancement ~2.28 GeV/c2 has been observed in the Σ0p spectrum. PTEP 021D01 (2015) • Mass: • Width: • dσ/dΩ``Kβpp’’→Σ p = (BE: ) 0 T. Sekihara, D. Jido and Y. Kanada-En’yo, PRC 79, 062201(R) (2009). • [Theoretical value: ~1.2] <2proton coincidence analysis> π+d→K+X, X→Σ0p <1 proton coincidence probability> 12 Discussion on the ``K pp’’-like structure • Obtained mass (BE ~ 100 MeV) and broad width are not inconsistent with the FINUDA and DISTO values. – Theoretical calculation for the K-pp is difficult to reproduce such a deep binding energy about 100 MeV. – Other possibilities? • A dibaryon as πΛN – πΣN bound states? H. Garcilazo and A. Gal, NPA 897, 167 (2013). (It should not decay to the Λp mode because of I = 3/2.) T. Uchino et al., NPA 868, 53 (2011). • Λ*N bound state? A. Dote, T. Inoue and T. Myo, PTEP 2015 4, 043D02 (2015). • A lower πΣN pole of the K-pp? (The K-pp might have the double pole structure like Λ(1405).) β • Partial restoration of chiral symmetry on the KN interaction? S. Maeda, Y. Akaishi and T. Yamazaki, Proc. Jpn. B 89, 418 (2013). 13 E15 E15 result PTEP 2015, 061D01 • No peak below Kpp threshold ο³E27 result • Not a kaonic bound state, but NSp resonance?? E13 g-ray spectroscopy of hypernuclei • 4 He: L Charge symmetry breaking in LN interaction? compare the mirror nuclei: 4 He and 4 H L L • 19LF: First g-ray measurement on sd-shell hypernuclei – How effective interaction changes compared to p-shell hypernuclei? • Hyperball-J – 28 germanium detectors + PWO Compton suppressor dedicated for hypernuclei arXiv:1508.00376 E13 result (1) – 4LH 1+ 1/2+ 3He 0+ 4 LHe • Eg=1406±2±2 keV • Corresponding energy in 4 H: 1090±20 keV L ο Indication of large charge symmetry breaking • LN-SN coupling effect with S mass difference? E13 result (2) – 19LF Doppler shift not corrected ππ selected unbound π ππ π²π π+ π− annhilation Selected ππ π²π ππ π²π ππ π²π g.s. Unbound ππ π Analysis in progress Part II. Coming experiments E03 & E07 E03 experiment • World first measurement of X rays from X-atom – Gives direct information on the XA optical potential • Produce X- by the Fe(K-,K+) reaction, make it stop in the target, and measure X rays. • Aiming at establishing the experimental method X- Fe target (dss) K- K+ X- Fe X ray X ray Energy (arbitrary scale) X atom level scheme ... l=n-3 l=n-1 (circular state) l=n-2 ... Z nuclear absorption ... ... X Z l (orbital angular momentum) X ray energy shift – real part Width, yield – imaginary part Successfully used for p-, K-,`p, and S- X paration of KURAMA spectrometer system Detectors are ready for installation 6 / 13 st all detectors are cated and being tested. TOF L oster : 303 H. Ekawa Hyperball-J CH CH (Charge Hodoscope) SSD K+ X- K- am Hodoscope) K+ Tagging ‘p’(K-,K+ )X - KURAMA (1.66 GeV/c) TOF DC3 DC3 BAC K- PVAC (Proton Veto AC) X- DC2 BAC FBH BH2 KURAMA PVAC FAC DC1 DC2 E07 LL Hypernuclei Hybrid emulsion method Goal: • 10000 stopped X- on emulsion • 100 or more double-L HN events • 10 nuclides Chart of double-L hypernuclei Production of LL-nuclei by fragmentation Xp ο LL stay in the nucleus οΌ~10οΌ οΌ Systematics of LL binding energy • LL binding energy may be different for each nucleus – For example by hyperon mixing effect 5 LLHe 6 LLHe p n L p n L p n X p n X Suppressed Enhanced E03/07 run plan in 2015-2017 • Test beam for 3 days in October 2015 – Confirm detector performance – Measurement of beam profile • Installation of KURAMA spectrometer from January – Commissioning beam time in Spring. • E07 beam time in 2016 with full statistics • E03 beam time is expected after E07. – Likely in early 2017. – We will have more than 1x1011 K- on target (10% of proposal) – Observation of X-atomic X ray should be possible, though finite shift/width may not be observable. Even further... Extended Hadron Hall Details under discussion Summary • Search for deeply bound Kaonic nuclei (E27, E15) – Mass shift of L*(1405) and/or S*(1385)? – Hint of deeply bound “Kpp”-like structure observed in d(p+,K+) reaction, but not observed in (K-,n) reaction – Kaonic nuclei?, SpN?, OR, something else? • E13: g-ray spectroscopy of hypernuclei – g-ray from 4LHe observed ο large charge symmetry breaking – Several g rays are seen from 19LF (analysis in progress) • Coming experiments – on doubly strange systems – E03: X-ray spectroscopy of X atom – E07: Systematic study of double-L hypernuclei in emulsion – Expect to run in 2016 & 2017 BACK UPS Calibration: p(π+, K+)Σ+ at 1.69 GeV/c Σ+ Σ(1385)+ Data: M = 1381.1 ± 3.6 MeV/c2 Γ = 42 ± 13 MeV PDG: M = 1382.8 ± 0.35 MeV/c2, Γ = 36.1 ± 0.7 MeV 32 θπK dependence (οΌdata, βsim) Y* peak positions are shifted to the low mass side for all scattering angles. < Peak position > οΌ data οΌ simulation 33 HADES experiment for Λ(1405) The peak position of Λ(1405) is shifted to low-mass side. M = 1385 MeV/c2, Γ = 50 MeV S-wave Breit Wigner function 34 E19 Experiment Search for pentaquark, ο+ • There are two kinds of usual hadrons (= feel strong force) – Baryon (Fermion): Meson (Boson): – Color neutrality required from QCD But they are not the only cases ο Exotic hadrons – Pentaquark = 5 quarks Pentaquark ο+ • First reported in 2003 by LEPS collaboration • Both positive and negative results – Still controversial • Mysteries – Why so narrow? G < 1 MeV – Spin-parity? – What’s that eventually? T. Nakano et al.,PRC79 (2009) 025210 High resolution search by p(p-,K-)ο • A good resolution: ~2 MeV (FWHM) – thanks to SKS • Why high resolution? – Good S/N ratio – Width measurement Almost certainly G < 1 MeV • Typical resolution in the past ~ 10 MeV – No high resolution search – There is a good chance Moritsu et al., PRC90 (2014) 035205 • Spectra well represented by known backgrounds at both energies Upper limit on decay width • Based on an effective Lagrangian approach: Hyodo et al., PTP128 (2012) 523 • Upper limit: 0.36 MeV for ½+ 1.9 MeV for ½For most conservative cases, taking theoretical uncertainties into account • Comparable to DIANA result E10 Neutron rich hypernuclei via (p-,K+) reaction L-hypernuclei N~Z (I=0 or 1/2) Non Charge-Exchange (NCX) ( K - , p - ) (p + , K + ) hyperfragments by emulsions exp. ordinary nuclei N>>Z (I=3/2 or 2) ( K - , p + ) (p - , K + ) Double Charge-Exchange (DCX) J-PARC E10 41 ΛN-ΣN Mixing in Λ Hypernuclei • Smaller mass difference ~300 MeV in DN vs ~80 MeV • Suppressed in I=0 core – Stronger mixing expected for neutron rich hypernuclei if core isospin=0 A(I=0) L A(I=0) S if core isospinοΉ0 A(IοΉ0) A(IοΉ0) OK! L S Result PLB 729 (2014) 39 • No peak observed • ds/dW < 1.2 nb/sr – 10 times smaller than 10 Li L – Does it really bind?