Title: Summary%20Talk%20Few%20Body%2018%20Ivo%20
1Summary Talk Few Body 18Ivo ŠlausR. Boškovic
Institute and TUNL, Duke U niversity
- I. 50 years ago
- II. Paradigm change in the NN studies
- III. Paradigm change in 3B theories
- IV. Technology we develop changes us
- V. Few-body research - results, questions
- VI. Is there an end for few-body research?
- VII. Few-body research community
- VIII. Challenges
- IX. On being a physicist (Acknowledgement)
2- Nuclear Forces Experiments Few-body theory
- Gartenhouse 55 LASL 53-69
- Signell- Zagreb 61-70 Faddeev
60 - Marshak58 ann -21.71 fm
- OBE 3H-183, 7Li(n,ta)n - fusion
- Bryan- Rice, BNL 65-74 Mitra 62
- Scott 69 Sequential (FSI), QFS
Amado63 - 3NF Caltech, UC Berkeley
separable - Primakoff- 4He levels, 3He? Alt -
- Holstein 39 UCLA 64-72
Grassberger - - n!/ m!(n-m)! nn QFS, NN? Sandhas 67
- Fujita- IKO - Ad, Zagreb 71
AGS - Miyazawa 57 BOL-system, 4p emuls. (NN on
off, 3NF)
3II. Paradigm change in the NN studies
- Hybrid OBE Phenomenological 3NF
- Kukulin CDBonn AV14 TM
- Doleschall
- Shirokov TM99(?S)
- AV18 UIX
- IL 1-5
- ?EFT ?PT (Q/?)n
- next-to-next-to-next-to-leading order N3LO
- R. Machleidt et al, J.J. De Swart et al, V.J.
Pandaripandhe et al, U. G. Meissner et al
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5TABLE 1 ?2 for various NN potentials compared to
NN data
YEAR No of data Nijmegen PSA CD-Bonn AV18 N3LO N2LO NLO
1992 pp (1787) 1.00 1.00 1.10
1999 pp (2932) 1.09 1.01 1.35
1999 NN (5990) 1.04 1.02 1.21
0-290 MeV NN data
1999 np 1.04 1.10 10.1 36.2
1999 pp 1.38 1.50 35.4 80.1
No of parametrs 35 38 24 9
6TABLE 2 Deuteron and some very light nuclei
Observ-able Experi-ment CD-Bonn AV18 JISP Kukulin Doleschall N3LO
Ed 2.224575 2.224575 2.224575 2.224575 2.224575 2.224575
?d .8574 0.8521 0.8548
Qd 2.859 2.70 2.70 2.915 2.754
AD/AS .0256 .0256 .0250 .0252
Pd 4.85 5.76 4.14 5.22 3.6 4.51
Et 8.488 8.013 7.628 8.46 8.48 7.855
E(3He) 7.72 7.288 6.917
E(4He 28.296 24.07 28.6
7TABLE 3. BE (MeV) of 3 ? A ? 16 with 3NF
3H 3He 4He 6He 6Li 7Li 8He 8Be 16O
Experiment 8.488 7.72 28.296 29.27 31.99 39.2 31.598 56.50 127.619
FCDBTM AV18UIX 8.478 8.478 7.735 7.733 29.15 28.34
G AV18UIX AV18IL2 8.487 8.43 7.739 7.67 28.33 28.37 28.1 29.4 31.1 32.3 27.2 31.3 54.4 56.6
N AV8TM JISP16 8.496 7.797 28.374 28.189 28.32 31.0 53.3 133.8
NN2LO NN Full 34.6 36.7-38
8CONCLUSIONS
- High precision NN potentials ? ?2 1.0 to NN
data below 350 MeV - ?sT / ?sL data ? ?2 1.08
- 2) N3LO needed
- 3) Correct ordering of energy levels of light
nuclei, e.g. 9Be, 10B with IL 2 (strong LS) - AV18 contains EM
- AV18 fit to 17 states ? ave deviation 7.32 MeV
- AV18UIX 2.02 MeV
- AV18 IL 3 0.04 MeV
- AV18IL2 fit to 39 states below 12C lt 0.7 MeV
9III. Paradigm change in 3B theories
- Rigorous 3B Glöckle, Witala, Sauer, Deltuva,
Fonseca ? EM - GFMC
- NCSM
- - sensitivities
- - excellent fit
- - evidence for 3NF energy levels of light
nuclei and elastic and inelastic scattering - (NB strong LS in Ay and in ordering levels)
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14IV. Technology we develop changes our research
and us
- ACCELERATORS 17,500
- 120 (E gt 1 GeV) 1000 low E research 100
synchrotrons - more than 7,500 radiotherapy and 7,000 ion
implantation - IUCF, TUNL, HI?S, KVI, MAMI, CELSIUS, LEGS,
RIKEN..Jlab... - RIB ISOLDE, SPIRAL, ISAC, Lln, RIBF,
RIBBL...2011? - 14Be(4ms), 8He(119ms)....10C(19s), 18Ne(17s)
- COSY, Nuclotron, DAFNE
- PANDAFAIRHESR 1011 p to study c in hadron
media - DETECTORS 76Ge, KamLAND, IceCube (South P)....
- SALAD, SCANDAL, WASA, ANKE, Crystal ball.......
- COMPUTERS valves/cards ? PC (25),
supercomputers, DNA (Shapiro),
quantum computer
15V. Few-body research - results, questions
- V 1. Evidence for 3NF
- Energy levels A 16, 10B (3) Ili full N3LO
- PSA of Nd 4PJ vs NN 3PJ
- st (E150 - 200 MeV)
- smin(?100o-160o) at E 95 MeV and other E
- Kkij Ep 22.7 MeV
- Ay, iT11 Cyy Ep 197 MeV
- 72 kinematic configurations KVI Ed 130 MeV
16Comparison between 3B and 130 MeV data
Force ?2 (NN) ?2 (NN3N)
AV18TM 4.48 3.80
AV18UIX 4.48 3.67
CD BonnTM 4.04 3.80
? 3.83 3.63
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18V 2. Symmetries
- CKM
- ?1 (Vud2 Vus2 Vub2)0.00430.0019, 2
s! - Vud0.973770.00024 Vus0.22720.001
Vub3.96x10-3 - ?fr 0.00040.011, ?sr 0.0320.181,
- ?fc 0.0010.005 compatible with unitarity
- CP violation
- Elect. dipole nlt6x10-26ecm
e (0.070.07)10-26ecm - A non-zero value requires both P and T violation.
- Neutrino vs antineutrino ? lepton sector
- (neutrino have mass, Si mi 1eV from WMAP)
19- 3) CPT invariance - equality of masses and t of
particles and antiparticles (mKo mKo)/mKolt
5x10-18 - 4) Conservation of lepton numbers
- Neutrinoless double ß decay ?L 2
- (Z,A) ? (Z2,A)e-e- 76Ge t gt 1.9x1025 y (CL
90) - 5) Time variation of fundamental constants
- ?a/a 10-3 , (6.41.3) 10-16/y from quasar line
absorption - BBN 2H and Li primordial abundances
- np?d? 30 - 130 keV (HI?S EFT)
20- 6) Supersymmetric particle searches
- neutralino m(?oi) gt 46 GeV CL 95
- chargino m(?i) gt 94 GeV CL 95
- selectron m(se) gt 73 GeV CL 95
- squark m(sq) gt 259 GeV CL 95
- gluino m(g) gt 195 GeV CL 95
217) CD from ppo and CSB from md?mu, ed?eu
- 1) Exptl and ? quark model values for scattering
lengths - anp app ann (fm)
- Exp -23.748?0.009 -17.3?0.3
-18.9?0.4 - ? QM -23.749 -17.807
-18.539 - Experimental result is 7.813?0.004
- 2) 3H 3He BE difference (keV)
- Experimental 764 Coulomb 676
- Mn?Mp 14
- CSB NN 65 ? 22
- CSB 3N 5
- Total 760 ? 22
22- 3) Nolen Schiffer anomaly
- 4) Superratio pp- on 3H/3He
- 5) D(d,a)po 228 232 MeV IUCF
- 12.72.2 15.13.1 pb vs EFT 23 30.8
pb - 6) Asymmetry in s(?) of H(n,d)po TRIUMF
- (17.2 8st 5.5sy)10-4 vs EFT 69x10-4
- 7) CS pN small CSB
- 8) ? separation energies in 3?H vs 3?He after
removing Coulomb 390 keV - 9) ?A An - Ap
23?A An Ap (in 10-4)
Energy (MeV) 477 347 183
Experiment 47 ? 22st ? 8sy 59 ? 7st ? 9sy 34.8 ? 6.2st ? 4.1sy
1 ? exchange 5 3 8
1 ? exchange 43 42 7
2 ? exchange -0.4 0.1 -0.5
? exchange 8 6 1
?-? mixing -18 -9 15
Total 38 42 31
24TABLE 5 Charge Symmetry Breaking (energies in
keV, ERP in fm)
Experi-ment ?-? Mn?Mp AV18 CDB ? quark cluster
?ann 1.6 ? 0.6 1.508 1.508 1.654 1.508 1.46 (1.37-1.67)
?rnn 0.10 ? 0.12 0.29 0.26 0.31 0.26
3H-3He 65 ? 22
1S0 60.9 57.6 62.1 57.6
All T1 65.8 60.0 65.1 60.0
Nuclear matter
1S0 168 154 180
All T1 367 311 301
160 3542 3367 3361 3401 3350 3326(d5/2)
? CSB 93 87 92 72 49
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26V 3. Experimental data not compatible with
current theories
- Discrepancies between pNN cc from ?observables
- 3He(?,p)d and 3He(?,pp)n at 10.2 and 16 MeV at
TERAS - Cross sections for the reactions 3He(?,p)d and
3He(?,pp)n - E(MeV) AV18 AV18UIX Exptl
- ?(?,p)d (mb) 10.2 1.01
0.96 0.77?0.05 - ?(?,p)d (mb) 16.0 0.71
0.72 0.65?0.05 - ?(?,pp)n (mb) 10.2 0.55
0.49 0.15?0.05 - ?(?,pp)n (mb) 16.0 1.07
1.04 0.91?0.06 - Prel. 12.8 MeV linearly polarized ? from HI?S at
forward angles n energy spectra peak at lower En
? CDBCoulomb.
27- 3) pd capture XS, Axx and Ayy at 140 200 MeV
RCNP ? calc with 3NF - 4) s(?) 108 190 MeV
- 5) Ay puzzle E 25 MeV at E 150 190 MeV
- 6) s(?), Ay. Kyy and Kxx at 250 MeV
- 7) ann
- 8) s(?) and Ayy at 19 MeV H(d,pp)n in SCRE
- 9) Space star pd 10.3 - 130 MeV nd 10.3 -
25 MeV - 10) pp and nn QFS (25 MeV nn this conf)
- 11) Axx, Ayy, Axz in H(d,pp)n at 135 MeV/nucleon
- 12) Lithium problem 7Li BBN 2x observational
values
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31Einc (MeV) Type of measurements Analysis ann (fm)
13 ?n1?n2 20.5o, 28o, 35o, 43o ?F 0o, TOF1, TOF2, Ep Absolute cross section Shape of FSI peak anp measured simultaneously with ?n3 55.5o, 69o and 83.5o corresponding to 43o- 28o, ?F 180o Nijmegen CDBonn, BonnB -18.720.13st0.65sy -18.840.47 -23.50.8
13 ?n1?n2 25o ?F 0o, TOF1, TOF2, Ep Absolute cross section Shape BonnB -14.40.3 -17.90.5
16.6 ?n155.5o, ?p 41.2o , ?F 180o TOF1, Ep Abs. cross section normalized to np- QFS CD-Bonn -16.20.3
17.4 kinematically incomplete ?p0o Extended geometry and moderate resolution, absolute cross section CD-Bonn -16.50.69st0.52sy
19 ?n1?n2 35.5o ,?F 0o, TOF1, TOF2, Ep Absolute cross section ?n135.5o, ?n2 73.5o ,?F 180o, TOF1, TOF2, Ep Absolute cross section ?n151.7o, ?p 45o , ?F 180o TOF1, Ep CD-Bonn -17.6 0.2st0.9sy anp -22.7 1.0st1.3sy
25.3 ?n155.5o, ?p 41.2o , ?F 180o TOF1, Ep Abs. cross section Normalized to np QFS CD-Bonn -16.30.4 -16.10.4
25.2 ?n1?p 32o , ?F 0o TOF1, Ep Abs. cross section CD-Bonn -24.3 1.1
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35VI. Is there an end for few-body
research?DarkEnergy 73, DarkMatter 22.6,
BM 4.4 T 13.7 0.2 Gy
- 1) Strange matter, strangelets, 3?H to 209?Bi,
6??He, 10??Be and 13??B. - ? ? interaction weaker than thought before,
- N, ?, S and ? interactions Nijmegen group
- 2) Exotic states 4He(Kstop,p)3baryon, M
3117, - Glt21 MeV (?), states around 2 GeV QM predicted
not found - 3) ?-physics, ?-mesic nuclei, ?N scattering
length - ?? po?? Gex0.450.09st 0.08sy eV
- test for ?PT G0.420.2eV
36- 4) Hybrids (qqg) and Glueballs (gg)
- Smoking guns JPC 0--, 1-, 2-....
- Evidence in pp-?p-pp-p at 18 GeV/c 1-,
- 5) Hadron in media could ? from free ?
- 6) Neutron and proton drip-lines, e.g. X(31F,x)
pb - Efimov effect, Thomas effect
- QFR and 2 spectators QFS
- Borromean, samba and tango nuclei
- 7) NN?off-shell NN amplitude is as a matter of
principle an unmeasurable quantity in NN?
(1964?75?2000) - (Brayshaw, Noyes, Polyzou and Glöckle off shell
3NF) - SURPRISES ARE MORE THAN LIKELY
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38VII. Few-body research community
- astrophysics
-
- particle, nuclear - FB - atomic, condensed
matter -
- chemistry, biomed
- FB conferences every 2-3 years since 1967
- European FB since 1975, Asian-Pacific since 1999
- (typically 200-400 participants from 20 40
countries) - FewBody Systems 1986 (W. Plessas)
- APS FB 330 vs APS NP 2476
39VIII CHALLENGES
- Nuclear interaction at N3LO (with 3NF) even N4LO
implying CD and CSB - More EFT ?PT studies required
- Rigorous 3B, 4B, GFMC, NCSM using NnLO with n 3
and CD CSB - Relativity
- Short range dibaryon Moscow/Tübingen p-e EFT
potentials should give the same result for all
observables - Can all EFT parameters be uniquel determined?
- Latitude in fine tuning PS and parameters?
40- 8) p-N scattering data should get pNN cc
- 9) Several potentials - temporary
- 10) N hyperon and H H interaction
- 11) Mesons, baryons, resonances hybrids,
glueballs, etc topics of conferences NSTAR,
MENU, ETAMESON, e.g. - np?d? relativistic descriptions
- and PWA workshops, eg Abilene, Zagreb,
Tuzla - 12) Symmetries
4113) FB systems ideal for new physics search
- weak charge of p (Jlab) - KN
scatt. length to test ?SB in systems with
strangenness using DEAR and SIDDHARTA 14)
New facilities Bernal Polanyi polemics 15)
Discrepancies solved using proper 3NF
or ? However, there are other discrepancies 16)
Therefore, several approaches desirable 17)
Rennaisance of nuclear physics 3B actually
more complex !
42IX. On being a physicist
- Knowledge-based society
- Paul Crutzen, Martin Rees
- John Carey The Faber Book of Science
- A.Toffler
- Aristotle Rurtherford
- G. Galilei