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Systematic study of two-pion production in NN collisions – from single-baryon to di-baryon excitations T. Skorodko, Physikalisches Institut, Univ.Tubingen
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Content * NN→NN * NN→d + -, 0 0 production at T p < 1.0 GeV: Roper resonance * Summary Theoretical and experimental situation 0 0, + + production at T p > 1.0 GeV: , (1600) isospin decomposition d + 0 production at T p = 1.1 GeV: , no ABC effect d 0 0 production at T p > 1.0 GeV: , ABC effect Motivation
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WASA 4 detector
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NN→NN : Valencia model L.Alvarez-Ruso et al., Nucl.Phys. A 633(1998) 519
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Theory ↔ Experiment N * →N( ) I=0 N * → pp→pp + - pp→pp 0 0 N * →N( ) I=0 N * →
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Theory ↔ Experiment pp→nn + + pp→pn + 0
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0 0 production at T p < 1 GeV Valencia model A(tot) A(N * →N )+A(N * → ) T p =0.775 GeV T p =0.895 GeV At Roper mass M=1440 MeV
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+ - production at T p = 0.8 GeV S. Abd El-Bary at el.,Eur.Phys.J. A 37(2008) 267 (COSY-TOF)
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Decay branchings of Roper -decay R= (N * → →N )/ (N*→N →N ) N * mass [MeV]1371 1440 CELSIUS-WASA ** PDG Bonn-Gatchina * 0.28(3) 1.0(1) 4(2) 0.9(1) * Partial Wave Analysis γp→p 0 0 N→ N γp→p 0 - p→ n 0 0 A. Sarantsev et al., Phys. Lett. B 659(2008) 94 ** T.Skorodko et al., Eur. Phys. J. A 35(2008) 317
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Isospin decomposition T. Skorodko et al., Phys. Lett. B 679(2009), 30
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M 121 M 101 M 101 (N * ) Total cross section N* (Valencia) (Valencia) cosφ=1 T. Skorodko et al., Phys. Lett. B 679(2009), 30
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pp→pp 0 0 T p = 1 GeVT p = 1.1 GeV Valencia calculations with readjusted N * → branch Valencia calculations with total Roper contribution reduced according to isospin decomposition
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Cross section pp → nn CELSIUS/WASA excitation experiment
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+ + I=2 (1232) (1600) very small amplitude according to Valencia model M =1500─1700 MeV threshold energy threshold energy =200─400 MeV can contribute at low energy Additional resonance with I=3/2
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Conclusions I The main isoscalar production mechanism is the Roper excitation and its decay The branching ratio of the Roper decays N * →N /N * → at a pole mass of 1371 MeV is 4:1 This result is in favor of a monopole mode interpretation of the Roper excitation According to the isospin decomposition the energy dependence of the Roper total cross section behaves like a s-channel excitation Description of the + + production data both in total and differential cross sections requires additional contribution from a resonance with isospin 3/2. A good candidate is (1600)
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From unbound to bound system: ABC effect
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First step into the ABC Alexander Abashian, Norman E. Booth and Kenneth M. Crowe, Phys. Rev. Lett. 5, 258 (1960) π 2 π Phase Space C
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ABC and ΔΔ models T.Risser, M.D. Shuster, Phys.Lett. B 43, 68(1973) F.Plouin et all, Nucl.Phys. A 302(1978) 413
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pn→d 0 0 T p =1.03 GeV T p =1.36 GeV conventional calculation M.Bashkanov et al., Phys.Rev.Lett. 102(2009), 052301
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Total cross section M.Bashkanov et al., Proc. PANIC09, 239
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pn→d 0 0 T p =1.03 GeV T p =1.36 GeV calculation with a s-channel resonance calculation without a s-channel resonance M.Bashkanov et al., Phys.Rev.Lett. 102(2009), 052301
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Crucial test of t-channel : pp→d + 0
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pp→d + 0 at T p =1.1 GeV ( S=2.36 GeV) calculations for iso- scalar channel calculations for iso- vector channel F.Kren et al., Int.J.Mod.Phys. A 24(2009), 561
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Total cross section (t-channel) F.Kren et al., nucl-ex/0910.0995 J.Bystricry et al. F.Shimizy et al. CELSIUS-WASA
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Conclusion II pn→d 0 0 - ABC effect: isoscalar s-channel resonance with M ABC 2M - 90 MeV ABC 50 MeV << 2 pp→d + 0 - no ABC effect: t-channel excitation
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Thank you
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conventional t-channel model ANKE ‘ABC’ data
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Total xsection 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
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Qualitative description n p n Δ Δ d π π + Δ Δ d π π p
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Theory ↔ Experiment pp→nn + + pp→pn + 0
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Theory ↔ Experiment N * →N( ) I=0 N * → pp→pp + - pp→pp 0 0 N * →N( ) I=0 N * →
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production at T p > 1.2 GeV pp→pp + - @ T p =1.36 GeV pp→pp 0 0 @ T p =1.3 GeV Valencia calculations
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0 0 production at T p > 1 GeV original Valencia calculations
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pp → nn p MeV Valencia predictions + (1600)
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Spin of ABC effect L=0
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production → Roper ansatz T p =0.75 GeV Phys.Rev.Lett. 88, 192301(2002) N * → Nσ N * → Δ N*N* ΔΔ NσNσ N All theoretical curves are normalized in area to the data
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Event selection pp→pp → pp4 T p =0.775 GeV T p =1.1 GeV p 1 angle lab p 2 angle lab angle lab Central Detector
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Particle identification (Central Detector) Momentum vs deposited energy in Plastic Barrel Energy deposited in CsI vs deposited energy in Plastic Barrel Momentum vs deposited energy in CsI
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Particle identification → 2 s) reconstruction from detection proton identification: dE/E method 2 identification M p
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Experimental evidence for a „narrow“ Roper p → X @ 4.2 GeV (Saturne) J J/ → N N* and N N* (BES) M Roper = 1358 MeV Roper = 179 MeV M Roper = 1390 MeV Roper = 190 MeV
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pp (WASA) pp → pn @ 1.3 GeV (WASA) Experimental evidence for a „narrow“ Roper M N* =1380 MeV, Γ=180 MeV
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T p =0.895 GeV Interference between Roper and ΔΔ
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M 121 in 4 times bigger cross section in pp 0 0 no contribution from
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M 121 in 4 times bigger cross section in pp 0 0 no contribution from
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cosφ +1
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pp → pn 0 + prediction
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