Study of few-body problems at WASA Wasa-at-Cosy
Content General overview General overview – decays – dd 0 – -mesic helium The ABC effect The ABC effect – d –
See talk A. Winnemoeller Friday 18:40
The ABC effect
ABC effect Experimentally Experimentally – low-mass enhancement in M – low-mass enhancement in M – observed in many fusion reactions – accompanied with ΔΔ excitations Theoretically Theoretically –originates from t-channel ΔΔ excitation –expected double-hump structure in M –expected double-hump structure in M (not supported by experimental observations)
pn d 0 0
2D x-section
Total x-section pn d + - pn d 0 0 ( + 0 )= (I=1) ( + - )=0.5 (I=1)+2 (I=0) ( 0 0 )= (I=0)=0.2 (I=1) pp d + 0 t - channel
Total x-section d threshold mass
Total x-section d threshold mass
Qualitative description n p n Δ Δ d π π + Δ Δ d π π p
Total xsection slices: qualitative description
Dalitz plot (peak region)
pn d 0 0 and pp d + 0 (p-spectator)(n-spectator)
+ 0 invariant mass T p 1GeV pp 2 He pp d
ABC in 3 He
M.Bashkanov et. al, Phys. Lett. B637 (2006) (I=0,1) (I=0) pd 3 Heππ, T p =0.89 GeV
dd 4 He Invariant Mass GeV 0.9 GeV 1.05 GeV See talk A. Pricking Tuesday 17:30
Conclusion Conclusion ABC effect due to narrow s -channel resonance with ABC effect due to narrow s -channel resonance with – – – More data next year More data next year – -decays –dd 0 –dd ( ) 3He+N+
* *
Outlook Finish data analysis Finish data analysis Perform Partial Wave Analysis (J PC ) Perform Partial Wave Analysis (J PC ) –Do we need polarization? Analysis of Analysis of Measure Measure Measure pn elastic scattering Measure pn elastic scattering
Multiplet 10 10=35 28 27 10 * * Y( )=2 I( )=0 Kim Maltman, Nucl. Phys. A501 (1989) 843
Data analyzed so far Tp = 1.0 GeV : 70 kEvents(80%) Tp = 1.0 GeV : 70 kEvents(80%) Tp = 1.1 GeV : Tp = 1.1 GeV : Tp = 1.2 GeV : 26 kEvents(15%) Tp = 1.2 GeV : 26 kEvents(15%) Tp = 1.3 GeV : Tp = 1.3 GeV : Tp = 1.4 GeV : 47 kEvents(25%) Tp = 1.4 GeV : 47 kEvents(25%)
Angular distribution (in the peak)
Dalitz plot
Additional corrections and cross-checks
Angular distribution (in the peak)
Total x-section Tp = 1.0 GeV Tp = 1.2 GeV Tp = 1.4 GeV
Corrections for Fermi-motion
Cross-checks at pn d 0 0 0 d CW: pn d 000000000000 WaC: pn d 0 0 0
Check of resolution 3 0 PS
Resolution In pn d 0 0 0 the width 30MeV In pn d 0 0 0 the width 30MeV From MC, X-section resolution in pn d 0 0 30MeV From MC, X-section resolution in pn d 0 0 30MeV
pn d 0 0 and pp d + 0 (p-spectator)(n-spectator)
pp d + 0 analysis
+ 0 invariant mass
Total xsection slices: qualitative description
Parameters of a new state M R = GeV = 53 MeV
Total x-section Tp = 1.0 GeV Tp = 1.2 GeV Tp = 1.4 GeV
ΔΔ versus Δ pd 3 Heππ, T p =895 MeV
ΔΔ ΔΔ π N Δ π N Δ π N Δ π N Δ Large π π invariant mass Small π π invariant mass
pn dππ, T p =1.03 GeV
M.Bashkanov et. al, Phys. Lett. B637 (2006) (I=0,1) (I=0) pd 3 Heππ, T p =0.89 GeV
ΔΔ Resonance p n p n Δ Δ d π π Δ Δ d π π +
ΔΔ resonance in differential distributions Δ Δ π π Δ π π Δ Δ π π Δ + Parameter of F(q) is fitted here pd 3 Heππ q ΔΔ q
ΔΔ resonance parameters
Consistent description for d and 3 He case With ΔΔ resonance Without ΔΔ resonance pd 3 He pn d T p =0.895 GeV T p =1.03 GeV T p =1.35 GeV
Angular distributions ΔΔ bound ΔΔ peak full pd 3 He T p =0.895 GeV
Angular distributions ΔΔ bound ΔΔ pn d T p =1.03 GeV
Quantum numbers of the resonance From Fermi-statistics: J=1 +,3 + if L ΔΔ =0 3 S 1 ( d ) : S wave only 3 D 1 ( d ) : S + D waves 3 D 3 ( d ) : no S wave pn R d 0 pn d 0 0 pn d 0 0 I=0,1I=0I=0,2 I=0
pp d + 0 no ABC * (k 1 x k 2 ) T p =1.1 GeV Control channel (NO ABC expected)
Data collected for pn d 0 0 T p =1.0, 1.1, 1.2, 1.3, 1.4 GeV T p =1.0, 1.1, 1.2, 1.3, 1.4 GeV To cover full resonance region To cover full resonance region To have overlaps between different energies, due to Fermi To have overlaps between different energies, due to Fermi To reduce systematical errors. To reduce systematical errors.
Results from dd +X beamtime Collected energies: T d = 0.8, 0.9, 1.01, 1.05, 1.117, 1.2, 1.25, 1.32, 1.4 GeV
Phase shifts pn pn Elastic scattering
Outlook Wasa-at-Cosy Wasa-at-Cosy Nov07-Dec07 dd runs Nov07-Dec07 dd runs Feb08 pd runs Feb08 pd runs
ΔΔ - FSI
Energy dependence of the low-mass enhancement unbound (ΔΔ) bound ΔΔ 27 MeVbound (ΔΔ) 27 MeV
FSI p n p n p n n n p n p n p n p p n d p n d p n d p n … +++…
3 S 1 phase shifts
3 D 3 phase shifts
ΔΔ resonance parameters
Effect of collision damping Without collision damping With collision damping
Δ resonance π N Δ π N Δ π N Δ L=1
Total x-section for ΔΔ resonance ABC channels (I=0) No ABC (I=1)
First step into the ABC Alexander Abashian, Norman E. Booth and Kenneth M. Crowe, Phys. Rev. Lett. 5, 258 (1960) Alexander Abashian, Norman E. Booth and Kenneth M. Crowe, Phys. Rev. Lett. 5, 258 (1960) π 2 π Phase Space
All of ABC No ABC effect! ABC effect
Δ resonance π N Δ π N Δ π N Δ L=1
F. Plouin et. al. Nucl. Phys. A302 (1978), ABC and ΔΔ models π π π π π π F. Plouin, P. Fleury, C. Wilkin PRL 65 (1990) 692
ΔΔ versus Reality
Total x-section for ABC channels (I=0) No ABC (I=1) pp d + 0
NΔ state in pp + d pp
Total x-section for ABC channels (I=0) No ABC (I=1) pp d + 0