Download presentation
Presentation is loading. Please wait.
Published byDamian Paul Modified over 9 years ago
1
HYPERNUCLEAR PHYSICS USING CEBAF BEAM PAST AND FUTURE Liguang Tang Hampton University/JLAB 4 th Workshop on Hadron Physics In China and Opportunities with JLAB 12GeV July 16-20, 2012
2
INTRODUCTION – BARYONIC INTERACTIONS Baryonic interaction (B-B) is an important part of nuclear force that builds the “world” - Neutron Stars - Astronomical Scale - Neutron Stars - H H (1p) He ( - 2p, 2n) C C (3 ) Understand B-B interactions is one of the essential tasks in Nuclear Physics
3
, 0 (uds) n (udd) p + (uud) + (uus) - (dds) - (dss) 0 (uss) S Q I S = 0 S = -1 S = -2 I 3 = -1 I 3 = +1/2 I 3 = -1/2 I 3 = +1 I 3 = 0 Nucleon (N) Hyperon (Y) S - Strangeness I - Isospin I - Isospin
4
INTRODUCTION – HYPERNUCLEAR PHYSICS To understand YN and YY interactions Producing Y inside of the nucleus Extract YN and YY interactions by studying the many body system To study short range interactions in baryonic interactions (OPE is absent in N interaction) To better explore nuclear structure using as a probe (not Pauli blocked by nucleons) and to explore new degree of freedom Model the baryonic many body system Study the role and the single particle nature of in various nuclear medium and density N and are the most fundamental interactions. Since decays only weakly ( N or N NN) thus long lifetime, mass spectroscopy - hypernuclei becomes possible analog to the nuclear mass spectroscopy
5
Shell Model with 2-B N Effective Potential (p N s ) ssss V N = V 0 (r) + V (r) s N s + V (r) L N s + V N (r) L N s N + V T (r) S 12 Additional Contribution: - coupling N N Contribute to the repulsive core Introduce an additional term: Observables: Ground state single binding energy Excitation spectroscopy (levels and level spacing) Production and production cross sections Decays V — SS SNSN T 5 Radial Integrals: Coefficients of operators THEORETICAL DESCRIPTION: 2B POTENTIAL
6
BASIC PRODUCTION MECHANISMS AZAZ n AZAZ -- K-K- (K, ) Reaction Low momentum transfer Higher production cross section Substitutional, low spin, & natural parity states Harder to produce deeply bound states AZAZ n A ++ K+K+ ( , K) Reaction High momentum transfer Lower production cross section Deeply bound, high spin, & natural parity states A (Z-1) p AZAZ e e’e’ K+K+ (e, e’K) Reaction High momentum transfer Small production cross section Deeply bound, highest possible spin, & unnatural parity states Neutron rich hypernuclei CERN BNL KEK & DA NE J-PARC (Near Future) Disadvantage: Lack absolute energy calibration and resolution CEBAF at JLAB (MAMI-C Near Future) Advantage: Absolute energy calibration & high resolution
7
4 He 4H4H 3H3H 7 He 7 Li 6 He B (MeV) 5 He 9 Be 9 Li 8 Be 8 Li 8 He 7 Be 13 N 13 C 10 B 12 B 11 B 9B9B Important source of data but lack statistics and resolution Reliability: Questionable Nevertheless, emulsion experiments before 80’s provided the most complete set of measured single binding energy B of s- and p-shell -hypernuclei
8
Missing predicted gamma ray Advantages: High resolution (~ few keV) and precise level spacing Disadvantages: low rate (statistics) and unable to measure the ground state binding energy
9
KEK336 2 MeV(FWHM) KEK E369 1.5 MeV(FWHM) High resolution, high yield, and systematic study is essential and is the key to unlock the “gate” Meson beam lacks absolute mass calibration (no free neutron target) BNL 3 MeV(FWHM)
10
ELECTRO-PRODUCTION USING CEBAF BEAM High quality primary beam allows high precision mass spectroscopy on -hypernuclei Producing and 0 from proton simultaneously allows absolute mass calibration – precise binding energy Mirror and neutron rich hypernuclei comparing those from ( +,K + ) reaction Spectroscopy dominated by high spin-stretched spin-flip states Results are important in determining , S N and V 0 terms from s states and S term from states with at higher orbits
11
Zero degree e’ tagging High e’ single rate Low beam luminosity High accidental rate Low yield rate A first important milestone for hypernuclear physics with electro- production Beam Dump Target Electron Beam Focal Plane ( SSD + Hodoscope ) K + K + Q D _ D 0 1m Q D _ D Side View Top View Target (1.645 GeV) Phase I E89-009 K+K+ e’ Phase II E01-011 Common Splitter Magnet New HKS spectrometer large Tilted Enge spectrometer Reduce e’ single rate by a factor of 10 -5 High beam luminosity Accidental rate improves 4 times High yield rate First possible study beyond p shell
12
New HES spectrometer larger Same Tilt Method High beam luminosity Further improves accidental rate Further improves resolution and accuracy High yield rate First possible study for A > 50 Beam 2.34 GeV e’ K+K+ e Phase III E05-115 Common Splitter Magnet
13
6GEV PROGRAM HIGHLIGHTS 6GEV PROGRAM HIGHLIGHTS 00 Allowing precise calibration of mass scale p(e, e’K+) and 0 (CH2 target)
14
-B (MeV) -6.68 0.02 0.2 MeV from nn 7 He E94-107 in Hall A (2003 & 04) s (2 - /1 - ) p (3 + /2 + ’s) Core Ex. States ~635 keV FWHM 12 B 6GEV PROGRAM HIGHLIGHTS– CONT. K+K+ _ D K+K+ 1.2GeV/c Local Beam Dump E89-009 12 Λ B spectrum ~800 keV FWHM HNSS in 2000 ss pp Phase I in Hall C (E89-009) Phase II in Hall C (E01-011) B (MeV) 28 Si(e, e’K + ) 28 Al (Hall C E01-011) HKS JLAB Counts (150 keV/bin) 28 Al ss pp dd Accidentals Phase II in Hall C (E01-011) ~500 keV FWHM HKS in 2005 12 B 16 N (Hall A) F. Cusanno et al, PRL 103 (2009) 16 N F. Cusanno et al, PRL 103 (2009) ss pp Phase III in Hall C (E05-115) ss pp
15
6GEV PROGRAM TECHNIQUE SUMMARY Hall A experiment (Pair of Septums + two HRS) Advantage: Almost no accidental background and be able to study elementary process at low Q 2 at forward angle Disadvantage: Low yield rate and cannot study heavier hypernuclei Hall C experiment (Common Splitter + HKS + HES/Enge) Advantage: High yield rate and high precision in binding energy measurement Disadvantage: High accidental background and solid targets only Future program: Combination
16
EXPERIMENTAL LAYOUT IF IN HALL C HKS - Kaons Enge - Pions HES - Electrons Hodoscope Lucite Č Drift Chamber 64mg/cm 2 22mg/cm 2 K+K+ -- Trigger I: HKS(K) & Enge( ) for Decay Pion Spectroscopy Experiment Trigger II: HKS(K) & HES(e’) for Mass Spectroscopy Experiment
17
High quality with low background High precision on binding energy and high resolution High yield rate which leads to wide range of physics: Elementary production at forward angle Detailed and precise level structure of light and medium heavy hypernuclei (shell models) Precise shell structure of heavy hypernuclei (single particle nature and field theory) High efficiency and productivity: one exp. Four 6GeV experiments New physics: Decay pion spectroscopy (Light Hypernuclei) Precise ground state B Determination of ground state J p Search for neutron rich limit (high Isospin states ) Technical Features of Future Program
18
DECAY PION SPECTROSCOPY TO STUDY -HYPERNUCLEI 12 C - Weak mesonic two body decay 1-1- 0.0 2-2- ~150 keV Ground state doublet of 12 B B and Direct Production p e’ e 12 C K +K + Example: Hypernuclear States: s (or p ) coupled to low lying core nucleus 12 B g.s. E.M. ** 12 B
19
DECAY PION SPECTROSCOPY FOR LIGHT AND EXOTIC -HYPERNUCLEI Fragmentation Process p e’ e 12 C Example: K +K + ** s 12 B * Highly Excited Hypernuclear States: s coupled to High-Lying core nucleus, i.e. particle hole at s orbit 4H4H Fragmentation (<10 - 16 s) 4 H g.s. 4 He - Weak mesonic two body decay (~10 - 10 s) Access to variety of light and exotic hypernuclei, some of which cannot be produced or measured precisely by other means
20
110 ~ 160 MeV/c110.05 ~ 160.05 MeV/c110.1 ~ 160.1 MeV/c 110.15 ~ 160.15 MeV/c 110.2 ~ 160.2 MeV/c Possible observation 4 H ground state Central Mom. : 133.5 MeV/c → B Λ ( 4 Λ H) : ~ - 1.60 MeV Width : 97 keV/c FWHM Target straggling loss was not corrected Spec-C momentum calibration was not yet done MAMI-C Short Test Run on Decay Pion Spectroscopy
21
SUMMARY Hypernuclear Physics is an important part of nuclear physics Program with CEBAF beam is the only one that provides precise B and features as Precision mass spectroscopy program Future program will be highly productive
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.