EXOTIC ATOMSNUCLEI T Yamazaki RIKEN Yukawa mesons 1935

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EXOTIC ATOMS/NUCLEI T. Yamazaki, RIKEN • • Yukawa mesons (1935) Anderson PR 51(1937), Nishina

EXOTIC ATOMS/NUCLEI T. Yamazaki, RIKEN • • Yukawa mesons (1935) Anderson PR 51(1937), Nishina PR 52(1937): muon Tomonaga-Araki, PR 58(1940): mesonic atom formation Fermi-Teller (1947) Strong-interaction shifts of pion: Jenkins et al. (1966) Ericson-Ericson (1966), Tomozawa-Weinberg (1966) Deeply bound pions: Toki-Yamazaki (1988) First observation (1996)

Exotic Resonance States of Antiprotons, Pions and Kaons in Atomic and Nuclear Systems Toshimitsu

Exotic Resonance States of Antiprotons, Pions and Kaons in Atomic and Nuclear Systems Toshimitsu Yamazaki, RIKEN • • Hadronic systems --> strong nuclear absorption --> short-lived, no discrete states Exceptions: long-lived, discrete states in continuum: Energy spacing >Width --> High-precision spectroscopy Feshbach resonances: Bound states of Xembedded in continuum Exotic atoms/nuclei Negative pions Negative kaons Antiprotons

Hadron-Nucleus Bound-State Spectroscopy Toshimitsu Yamazaki (RIKEN) • Explore Chiral Symmetry Restoration in Nuclear Media

Hadron-Nucleus Bound-State Spectroscopy Toshimitsu Yamazaki (RIKEN) • Explore Chiral Symmetry Restoration in Nuclear Media Brown-Rho scaling: • HOW TO MEASURE In-medium hadron masses and interactions in well defined states and densities? ? POPULAR METHODS: Invariant-mass spectroscopy for decay particles in continuum medium • • NEW METHOD: Bound-state spectroscopy: IF hadron bound states exist with narrow widths? How? Suppression mechanisms for nuclear absorption? Pionic Nuclei (1988 -): observed (1996, 1998, 2001), matured Kaonic Nuclei (2000 -): predicted, no observation yet

Deeply Bound Pionic States 1 s pionic states in heavy (N>Z) nuclei • Shallow

Deeply Bound Pionic States 1 s pionic states in heavy (N>Z) nuclei • Shallow pionic atoms: • Last orbital: • Deeply bound states: ~1 -10 ke. V ~ 0. 5 Me. V ~ 5 Me. V Still discrete states!! Coulomb attraction + Strong Interaction Repulsion ----->> Halo like pionic states (absorption suppressed) E. Friedman and G. Soff (1985) H. Toki et al. (1988): --->> pion transfer reactions First success: (d, 3 He) at GSI

New Frontiers of Exotic Atoms/Nuclei From outside to inside * atomic states of X

New Frontiers of Exotic Atoms/Nuclei From outside to inside * atomic states of X radiative transitions from outer orbitals * terminated cascade EXOTIC ATOMS/NUCLEI From inside to outside * nuclear resonance states * still bound states of X

Pion-Nucleus Potential Parameters s-wave p-wave Light 1 s states in symmetric nuclei Seki-Masutani relation

Pion-Nucleus Potential Parameters s-wave p-wave Light 1 s states in symmetric nuclei Seki-Masutani relation Double-scattering effect

Pionic Bound States Probe Nuclear Surface Overlapping density: maximum at The density-dependent potential parameter:

Pionic Bound States Probe Nuclear Surface Overlapping density: maximum at The density-dependent potential parameter: is transposed to

 in 205 Pb

in 205 Pb

Sn(d, 3 He) spectra K. Suzuki et al. , PRL (2003)

Sn(d, 3 He) spectra K. Suzuki et al. , PRL (2003)

PIONIC NUCLEI as a unique indicator of Chiral Symmetry Restoration in the nuclear medium

PIONIC NUCLEI as a unique indicator of Chiral Symmetry Restoration in the nuclear medium Fundamental building blocks: • Nuclei: protons (938 Me. V) + neutrons (940 Me. V) + virtual mesons (pion: 140 Me. V; etc. ) • Hadrons: quarks + gluons: u (~ 5 Me. V), d (~ 8 Me. V), s (~ 150 Me. V) Surprising discrepancies -->> ascribed to quark condensate in QCD vacuum: order parameter of chiral symmetry breaking QCD vacuum is subject to change: partial restoration of chiral symmetry HOW to prove or disprove this scenario? As in superconductors Pion decay constant in medium ---> Isovector pion-N interaction b 1(free) /b 1*(r) -->>

B 1 s and 1 s in Sn Isotopes

B 1 s and 1 s in Sn Isotopes

Pionic Bound States as an Indicator of Chiral Symmetry Restoration Isovector s-wave interaction --->>

Pionic Bound States as an Indicator of Chiral Symmetry Restoration Isovector s-wave interaction --->> pion decay constant in the medium Weise (2000, 2001) Kienle and TY (2001) Best probe: Pionic 1 s in heavy nuclei GSI experiment on pionic 115 Sn, 119 Sn, 123 Sn K. Suzuki et al. (2002)

Evidence for partial restoration of chiral symmetry in nuclear medium probed by 1 s

Evidence for partial restoration of chiral symmetry in nuclear medium probed by 1 s pionic nuclei (2003) Isovector s-wave N scattering length

Hadron Bound States

Hadron Bound States

Nuclear excited states with strangeness S = -1 as Feshbach resonances ���� p����� ,

Nuclear excited states with strangeness S = -1 as Feshbach resonances ���� p����� , n(940) ������ : stable Hypernuclei: Many observed S������� , S � ������ S Hypernuclei: Unstable: S conversion Exception: 4 SHe �� 405� : K-p bound state K-N(1433) K- nuclear bound states?

Akaishi KN Potential Y. Akaishi and TY, PRC (2002)

Akaishi KN Potential Y. Akaishi and TY, PRC (2002)

Diagram Kaon Bound System

Diagram Kaon Bound System

pp. K- bound system - kaonic hydrogen nuclear molecule

pp. K- bound system - kaonic hydrogen nuclear molecule

K- potentials and bound states • • Y. Akaishi and TY, PRC (2002) TY

K- potentials and bound states • • Y. Akaishi and TY, PRC (2002) TY and Y. Akaishi, PLB (2002)

Shrinkage effect: Competition between K-p attraction and nuclear incompressibility

Shrinkage effect: Competition between K-p attraction and nuclear incompressibility

3 He Antisymmetric Molecular Dynamics Method Isovector Deformation Dote et al. ---> 3 He.

3 He Antisymmetric Molecular Dynamics Method Isovector Deformation Dote et al. ---> 3 He. K- shrinkage !!

Very exotic systems kaonic tri-protons kaonic tetra-protons

Very exotic systems kaonic tri-protons kaonic tetra-protons

Kaonic Be-8: Contracted Alpha Cluster Dote et al. (2002)

Kaonic Be-8: Contracted Alpha Cluster Dote et al. (2002)

(K, ) and ( , K) reactions for various K- bound systems * Large

(K, ) and ( , K) reactions for various K- bound systems * Large q: good for large internal momentum * Varieties (K-, -) ( -, K 0) ( +, K+) DQ -1 0 target p L L* S +, S +* [n] L L* d pn. Kpp. K 3 He ppn. Kppp. K 4 He ppnn. Kpppn. K- ( �, K 0) +1 S +, S +* pppp. K-

Experimental Search M. Iwasaki et al. , at KEK 4 He (stopped K-, n)K-

Experimental Search M. Iwasaki et al. , at KEK 4 He (stopped K-, n)K- 3 He

L -doorway and L -compound mechanisms T. Yamazaki and Y. Akaishi, PLB 535 (2002)

L -doorway and L -compound mechanisms T. Yamazaki and Y. Akaishi, PLB 535 (2002) 70 Hepp et al. , N. P. B 115 (1976) 82

K Compound Nuclei • 1520 + p + n +…. ---> K- + p

K Compound Nuclei • 1520 + p + n +…. ---> K- + p + n +… • ---> K- bound state +

Predicted (K-, -) Spectra Y. Akaishi

Predicted (K-, -) Spectra Y. Akaishi

How about pp. K K , ppn. K K ? ?

How about pp. K K , ppn. K K ? ?

Double kaonic nucleus // ppn. K-K- // 4 fm Density [fm-3] 0. 00 0.

Double kaonic nucleus // ppn. K-K- // 4 fm Density [fm-3] 0. 00 0. 07 4 fm 0. 14 Density [fm-3] 0. 00 0. 75 4 fm 1. 50 Density [fm-3] 0. 0 1. 5 3. 0 ppn. K-K- total B. E. = 6. 0 Me. V central density = 0. 14 fm-3 rms. R= 1. 59 fm total B. E. = 118 Me. V central density = 1. 50 fm-3 rms. R= 0. 72 fm total B. E. = 221 Me. V central density = 3. 01 fm-3 rms. R= 0. 69 fm

Kaonic Nuclei - Future Scope Very strong K--p attraction • • • Very deep

Kaonic Nuclei - Future Scope Very strong K--p attraction • • • Very deep discrete states: predicted BK ~ 100 Me. V Highly excited resonance states In-medium KN interactions modified? Dense nuclear systems formed Possibly, Quark-Gluon phase at T = 0 Kaon condensation; strange matter Nuclear dynamics under extreme conditions

Strangeness at high nuclear densities The nuclear incompressibility is overcome by the Strong K-

Strangeness at high nuclear densities The nuclear incompressibility is overcome by the Strong K- p attraction At high density K- matter [K- p] + …+ n +… may be more stable

Spectroscopy ** Entrance channel spectroscopy Direct reactions: A+a --> X + b Missing-mass spectroscopy

Spectroscopy ** Entrance channel spectroscopy Direct reactions: A+a --> X + b Missing-mass spectroscopy ** Decay channel spectroscopy Compound reactions --> X + anything X --> x 1 + x 2 + … Invariant-mass spectroscopy: Minv 2 = (E 1 + E 2 +. . )2 - (P 1 + P 2 +. . )2

Search for K- cluster fragments in HI reactions high-density environment provided by HI fireball

Search for K- cluster fragments in HI reactions high-density environment provided by HI fireball Invariant mass spectroscopy for their decays K-pp --> L + p, K-ppn --> L + d

Kbar cluster decay in the freeze-out phase t. K (=10 fm/c) > tfreeze-out

Kbar cluster decay in the freeze-out phase t. K (=10 fm/c) > tfreeze-out

FOPI from Kusche (Ph. D) 1999

FOPI from Kusche (Ph. D) 1999

FOPI from Kusche (Ph. D) 1999

FOPI from Kusche (Ph. D) 1999

Search for K- clusters as residues in heavy-ion reactions • • High density medium

Search for K- clusters as residues in heavy-ion reactions • • High density medium accommodated in fire balls Deep self-trapping centers in fire balls Freeze-out phase Invariant mass spectroscopy for fragments pp. K- ---> + p ppn. K- ---> + d