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Dileptons from Resonance Matter and the DLS Puzzle :

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<strong>Dileptons</strong> <strong>from</strong> <strong>Resonance</strong> <strong>Matter</strong><br />

<strong>and</strong> <strong>the</strong> <strong>DLS</strong> <strong>Puzzle</strong> :<br />

Recent results <strong>from</strong> HADES<br />

Béatrice Ramstein<br />

Institut de Physique Nucléaire d’Orsay, France


Outline<br />

On related topics, topics,<br />

this morning … B. Kämpfer<br />

V. Metag’s<br />

Introduction: motivations <strong>and</strong> role of Δ resonance<br />

The DiLepton Spectometer puzzle:<br />

comparison of HADES <strong>and</strong> <strong>DLS</strong> C+C 1 AGeV dilepton<br />

spectra<br />

Discussion of HADES C+C, pp <strong>and</strong> pn data<br />

briefly…some<br />

briefly some o<strong>the</strong>r results<br />

Conclusion <strong>and</strong> outlook<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 2


The Collaboration<br />

SIS<br />

� Catania (INFN - LNS), Italy<br />

� Cracow (Univ.), Pol<strong>and</strong><br />

� Darmstadt (GSI), Germany<br />

� Dresden (FZD), Germany<br />

� Dubna (JINR), Russia<br />

� Frankfurt (Univ.), Germany<br />

� Giessen (Univ.), Germany<br />

� Milano (INFN, Univ.), Italy<br />

� München (TUM), Germany<br />

� Moscow (ITEP,MEPhI,RAS), Russia<br />

� Nicosia (Univ.), Cyprus<br />

� Orsay (IPN), GSI<br />

France<br />

� Rez (CAS, NPI), Czech Rep.<br />

� Sant. de Compostela (Univ.), Spain<br />

� Valencia (Univ.), Spain<br />

� Coimbra (Univ.), LIP, Portugal<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 3


Motivations of HADES experiment<br />

RHIC<br />

SPS<br />

AGS<br />

hadrons<br />

QGP<br />

SIS‐100<br />

SIS‐300<br />

SIS‐18<br />

KEK,JLAB,TAPS<br />

From B.J. Schäfer, J. Wambach priv. communication<br />

Instrumental challenge!<br />

– Low dilepton pair yields <strong>from</strong> vector<br />

meson<br />

~ 1 reaction per 10 5 -10 6 !<br />

– Conversion:<br />

main source π 0 � γγ (BR 99%)<br />

– Combinatorial background<br />

Di leptons : penetrating probes<br />

� medium modifications of vector meson<br />

properties (ρ,ω)<br />

� electromagnetic structure of hot <strong>and</strong> dense<br />

baryonic matter<br />

� ρ/ρ o ~ 1-3, T < 100 MeV<br />

� N π /A part ≈ 10%<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 4


Specificity of 1-2 1 2 A GeV energy range<br />

� long life time of <strong>the</strong> dense system<br />

(up to 15 fm/c) τ ρ ~ 1.3 fm/c, τ ω ~ 23 fm/c<br />

� dominance of Δ resonance<br />

UrQMD calculations Au+Au 1 AGeV<br />

� resonance matter (Δ33 ) ρ/ρ0<br />

1-2 GeV<br />

↔<br />

Δ<br />

tot<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 5<br />

π<br />

N -1<br />

ρ/ρ 0<br />

ρ/ρ 0<br />

n,p<br />

Δ<br />

15 fm/c<br />

Δ Δ<br />

π<br />

N -1


!<br />

inconsistent formula can<br />

be found in litterature<br />

Δ Dalitz decay: decay:<br />

what is known? known?<br />

exact QED calculation :<br />

3 amplitudes: e.g. Magnetic, Electric <strong>and</strong> Coulomb<br />

( ) ( ) ( ) ( ) ⎟ ⎟<br />

2<br />

⎛<br />

⎞<br />

2 ⎜ 2<br />

2 q<br />

2<br />

2<br />

2 2<br />

m , ⎜ q + 3 q + q<br />

2<br />

Δ q G M G E<br />

C<br />

+ -<br />

dΓ(Δ<br />

→ Ne e )<br />

= f 2 dq<br />

G<br />

⎜<br />

2<br />

⎝<br />

m Δ<br />

Form factors G M (q 2 ), G E (q 2 ), G C (q 2 )<br />

q 2 ≥0 : « Time like « electromagnetic structure of N - Δ transition<br />

known only at q 2 =0 ( γN → Δ → πN)<br />

G M (0)=3, G E (0)=0.04, G C (0)=0.2<br />

radiative decay: Δ→Nγ BR=0.56%±0.06%<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 6<br />

⎠<br />

Δ + →pe + e -<br />

Δ +<br />

q 2 = M 2 inv (e+ e - ) = M γ* 2 > 0<br />

Not measured<br />

p<br />

γ*<br />

e -<br />

Dalitz decay<br />

Δ + → γp<br />

Δ +<br />

q 2 = 0<br />

p<br />

γ<br />

e +<br />

Radiative decay


Δ Dalitz decay : form factors<br />

Form factors G M (q 2 ), G E (q 2 ), G C (q 2 )<br />

« photon point » G M(0)=3, G E (0)=0.04, G C (0)=0.2<br />

in transport models :<br />

constant G M : HSD, IQMD, UrQMD<br />

extended-VDM extended VDM model: model:<br />

RQMD<br />

G M (q 2 )<br />

0.6m 2 ρ<br />

two component Iachello<br />

model = « VMD like »<br />

Wan & Iachello, Iachello,<br />

int. int.<br />

J. Mod. Mod.<br />

Phys. A<br />

20(2005) 1846 1846<br />

dΓ/dM<br />

MΔ =1232 MeV/c2 GM =3.0<br />

GM (q2 ) Iachello<br />

M Δ =1480 MeV/c 2<br />

(E th =1.25 GeV)<br />

M Δ =1830 MeV/c 2<br />

(E th =2.2 GeV)<br />

Δ Dalitz decay<br />

branching ratio<br />

BR ~ 4.2 10 -5<br />

M ee (GeV/c 2 )<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 7


The DiLepton Spectrometer puzzle<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 8


A prominent result in <strong>the</strong> 1-2 1 2 AGeV energy range:<br />

Dilepton Spectrometer at <strong>the</strong> Bevalac<br />

The puzzle !<br />

Calculation: E.L.Bratkovskaya et al.<br />

Phys. Lett. B445 (1999) 265<br />

Observed excess remained<br />

unexplained over years<br />

Porter et al., Phys. Rev. Lett 79 (1997)<br />

Calculation: Ernst et al.<br />

Phys. Rev. C58 (1998) 447<br />

Calculation: C. Fuchs et al.<br />

Phys. Rev. C68 (2003) 014904<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 9<br />

1 AGeV


Acceptance: Full azimuth, polar angles 18 o -85 o<br />

Pair acceptance ≈ 0.35<br />

Particle identification:<br />

RICH, Time Of Flight, Pre-Shower (pad<br />

chambers & lead converter) ( also MDC (K ± ))<br />

Trigger:<br />

1st Level: charged particle multiplicity (~10 kHz)<br />

2' Level: single electron trigger (~2.5 kHz)<br />

Momentum measurement<br />

Magnet: ∫Bdl = 0.1-0.34 Tm<br />

MDC: 24 Mini Drift Chambers<br />

Leptons: Δx~ 140 μ per cell, Δp/p ~ 1-2 %<br />

ΔM/M ~ 2% at ρ mass<br />

HADES<br />

2 nd generation dilepton<br />

spectrometer<br />

START<br />

Side View<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 10<br />

FW


Dielectron DATA analysis: analysis<br />

normalization to π0 (Nπo (N = ½ (N π- + N π+)) ))<br />

Comb. Background (CB) subtraction<br />

Mee ee < 150 MeV/c 2 Like-sign Like sign pairs<br />

Mee ee > 150 MeV/c 2 event mixing<br />

Signal: ~ 18400 counts<br />

Me+e- ≥ 150 MeV/c2 : ~ 646 counts<br />

Efficiency correction<br />

Measured rates span over 5<br />

orders of magnitude<br />

Systematic errors:<br />

20% efficiency correction<br />

10% combinatorial background<br />

15% π 0 normalization<br />

22% - 27% Total<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 11


HADES <strong>and</strong> <strong>DLS</strong> Phase Space Coverage<br />

mid-rapidity<br />

HADES<br />

<strong>DLS</strong><br />

mid-rapidity<br />

Method for HADES/<strong>DLS</strong> comparison:<br />

� HADES yield extrapolated to full phase space.<br />

� <strong>DLS</strong> acceptance filter applied<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 12


C+C 1 A GEV : result of HADES / <strong>DLS</strong> comparison<br />

HADES/<strong>DLS</strong> M e+e- spectra HADES/<strong>DLS</strong> pt spectra<br />

HADES: G. Agakishiev et al., PLB 663<br />

(2008) 43<br />

<strong>DLS</strong>: J. Carroll – presentation<br />

International Workshop on Soft Dilepton Production<br />

August 20-22,1997, LBNL<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 13<br />

<strong>DLS</strong> data confirmed → dilepton enhancement has to be explained !!


Comparison of HADES Data with Simulated Dilepton Cocktails<br />

PLUTO event generator I. Froehlich et al., al. arXiv:0708.2382<br />

Excess in <strong>the</strong> intermediate mass region<br />

�Cocktail A: π 0 + η + ω<br />

= “long-lived” components only<br />

� π 0 → e + e - γ (Dalitz) , η → e + e - γ (Dalitz)<br />

� ω→ e + e - (direct) , ω →e + e - π 0 (Dalitz)<br />

� π 0 /η constrained by TAPS data<br />

Cocktail B: Cocktail A + Δ + ρ<br />

= “short-lived”<br />

“short lived” sources added<br />

� Δ → e + e - p (Dalitz decay)<br />

N(Δ) =3/2 N( π 0 )<br />

� ρ → e + e - (direct)<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 14


Cocktail A: π0 Excess yield scales like π<br />

+ η + ω<br />

= “long-lived” components only<br />

0<br />

(related to Δ in cocktail)<br />

π<br />

Δ regeneration<br />

Δ N →<br />

←<br />

NN<br />

Comparison of HADES Data with Pluto Cocktails<br />

N -1<br />

Δ<br />

π<br />

Δ<br />

Excess in <strong>the</strong> intermediate<br />

Need for transport<br />

mass region<br />

models<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 15<br />

N -1


New <strong>the</strong>oretical calculations !!<br />

1997: transport models failed to explain <strong>DLS</strong> data<br />

2007: <strong>DLS</strong> <strong>and</strong> HADES agree <strong>and</strong> are compatible with new transport model<br />

calculations<br />

Calculation: E.L.Bratkovskaya et al.<br />

HSD Giessen<br />

Nucl. Phys. A634 (1998) 168<br />

E. Bratkovskaya <strong>and</strong> W.Cassing, nucl-th/0712.0635<br />

1/N 0 dN/dM [1/GeV /c<br />

π 2<br />

]<br />

10 -2<br />

10 -3<br />

10 -4<br />

10 -5<br />

10 -6<br />

10 -7<br />

10 -8<br />

C+C, 1.0 A GeV<br />

no medium effects<br />

HADES<br />

HADES <strong>DLS</strong><br />

0.0 0.2 0.4 0.6 0.8<br />

M [GeV/c²]<br />

HSD:<br />

π 0<br />

Dalitz<br />

η Dalitz<br />

Δ Dalitz<br />

ω Dalitz<br />

ω<br />

ρ<br />

Brems. NN<br />

Brems. πN<br />

All<br />

dσ/dM [μb/(GeV c 2<br />

)]<br />

0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9<br />

M [GeV/c²]<br />

new treatments of Bremsstrahlung: R. Shyam & U.Mosel, PRC67 (2003) 065202<br />

L.P. Kaptari, B. Kämpfer, NPA 764 (2006) 338<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 16<br />

10 2<br />

10 1<br />

10 0<br />

10 -1<br />

10 -2<br />

10 -3<br />

C+C, 1.04 A GeV<br />

no medium effects<br />

<strong>DLS</strong><br />

<strong>DLS</strong><br />

π 0 Dalitz<br />

η Dalitz<br />

Δ Dalitz<br />

ω Dalitz<br />

ω<br />

ρ<br />

Brems. NN<br />

Brems. πN<br />

All


Soft photon approximation<br />

γ*<br />

γ*<br />

Full OBE: meson exchange currents<br />

R. Shyam & U.Mosel, PRC67 (2003) 065202<br />

+<br />

N,Δ<br />

Kaptari&Kämpfer, NPA 764 (2006) 338<br />

Gauge invariance → contact terms<br />

NN Bremsstrahlung:<br />

Amplitude calculated for real photon<br />

+ phase space correction<br />

pn Bremsstrahlung by Kaptari & Kämpfer<br />

factor 4 larger than SPA<br />

Same result for pp Bremsstrahlung, Bremsstrahlung,<br />

but still<br />

much smaller than pn<br />

Δ graphs also present<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 17


BUU Barz et al.<br />

More transport models results ....<br />

RQMD: E.Santini et al<br />

UrQMD Bleicher et al. IQMD Thomere et al.<br />

Δ Dalitz<br />

pn<br />

C+C 2 AGeV<br />

pn Bremsstrahlung <strong>and</strong> Delta Dalitz decay<br />

Important issues for underst<strong>and</strong>ing<br />

intermediate mass dilepton yield<br />

Need for elementary pp, pn reactions<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 18


pp reaction at 1.25 GeV: GeV:<br />

Δ Dalitz decay<br />

LH2 target, normalisation to elastic scattering<br />

(syst.error ~ 30 %)<br />

preliminary<br />

E=1.25 GeV < η threshold<br />

pp Bremsstrahlung is small<br />

Pluto simulations<br />

1) pp→pΔ pp +<br />

σ(pp pp→pΔ + ) = 6 mb<br />

~ 3/2 σ(pp pp→pπ° )<br />

Δ Dalitz decay <strong>from</strong> QED vertex<br />

a) G M=3 =3<br />

b) Iachello GM (q 2 )<br />

2) dσ/dM d dM <strong>from</strong> OBE model (Kaptari ( Kaptari & Kämpfer) K mpfer)<br />

with assumption on γ* * angular distribution<br />

a) Delta graphs only<br />

b) all graphs ( bremstrahlung +FSI)<br />

Dalitz decay <strong>from</strong> simple model + Iachello G M (q 2 ) OK<br />

BR ~ 4.2 10 -5 sensitivity to N-Δ electromagnetic structure !<br />

G M (q 2 )<br />

Even better<br />

in exclusive<br />

e + e - p events<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 19<br />

p<br />

p<br />

Δ +<br />

p<br />

p<br />

γ*<br />

e --<br />

e +


Dilepton spectra in OBE :<br />

a « hot » <strong>and</strong> controversial subject<br />

------ Kaptari <strong>and</strong> Kämpfer<br />

___ Shyam <strong>and</strong> Mosel<br />

Δ <strong>from</strong> our model:<br />

pp→pΔ pp→p + ~ 6 mb<br />

np →nΔ →n + ~ 12 mb<br />

Δ Dalitz decay : GM =3<br />

p<br />

p<br />

G M (q 2 )<br />

Δ +<br />

p<br />

p<br />

γ*<br />

e --<br />

e +<br />

……..… news <strong>from</strong> last week ……………….<br />

arXiv:nucl-th 08110739 Shyam <strong>and</strong> Mosel<br />

« Dilepton production in nucleon-nucleon revisited »<br />

including Δ contribution<br />

Dilepton spectra in 4π acceptance<br />

M(GeV/c 2 )<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 20


dp at 1.25 GeV: GeV:<br />

pn Bremstrahlung sensitivity<br />

selection of np reactions: spectator<br />

proton in Forward Wall ( 0.5°–7°)<br />

Test of pn bremsstrahlung contribution<br />

Fermi momentum → η contribution<br />

normalisation to elastic scattering<br />

(syst.error ~ 30 %)<br />

PRELIMINARY<br />

PRELIMINARY<br />

HADES np data: a new puzzle ??<br />

PLUTO simulations<br />

1) σ (np np→nΔ+) = 12 mb ~ 3/2 σ(np np→np npπ°)<br />

η production (COSY/CELSIUS) added<br />

2) Kaptari <strong>and</strong> Kämpfer full OBE<br />

CC scales as ½(pp+pn) !!<br />

no enhancement ?<br />

PRELIMINARY<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 21


2001/2<br />

2004<br />

2004<br />

2005<br />

2006<br />

2007<br />

2007<br />

2008<br />

HADES experimental program<br />

C + C 2 AGeV<br />

C + C 1 AGeV<br />

p + p 2.2 GeV<br />

pp elastic,<br />

exclusive ppe+e- ppe+e (π°,η)<br />

Ar + KCl 1.75 AGeV<br />

p + p 1.25 GeV<br />

exclusive ppe+e- ppe+e (π°,Δ)<br />

p + p 3.5 GeV<br />

d + p 1.25 AGeV<br />

p+Nb 3.5 GeV<br />

1 PRL (e+e-) + 1 submitted (hadron)<br />

1 PLB (e+e-) + 1 submitted (hadron)<br />

Analysis finished (draft)<br />

Validation of detector performance,<br />

measures of π° <strong>and</strong> η Dalitz decays (helicity<br />

distribution), “free” cocktail<br />

Analysis ongoing dielectron spectra, medium<br />

effects<br />

inclusive analysis finished (draft)<br />

Δ Dalitz decay first measurement<br />

ω line shape <strong>and</strong> cocktail (π, Δ, η, ω, ρ, φ...)!<br />

Contribution of pn Bremstrahlung / Δ Dalitz decay<br />

Reference for medium effects<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 22


First peaks at 3.5 GeV<br />

ω→e + e - decay observed for a first time at SIS/Bevalac energy<br />

Cocktail normalized to π° (no abs. norm.)<br />

pp at 3.5 GeV<br />

Δ<br />

η<br />

Mass resolution in <strong>the</strong><br />

ω region < 2,7 %<br />

Apr 2007<br />

ρ<br />

π0 ω<br />

PRELIMINARY<br />

φ<br />

pNb at 3.5 GeV<br />

Oct 2008<br />

On-line pNb spectrum<br />

PRELIMINARY<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 23


Hadronic channels: channels:<br />

high quality by-products<br />

by products !!<br />

M nπ+<br />

pp→pnπ + E=1.25 GeV<br />

Δ production mechanism<br />

Submitted to EPJA<br />

C+C<br />

1 <strong>and</strong> 2 AGeV<br />

π ± mt spectra<br />

Δ ++ M pπ+<br />

pn FSI<br />

pp elastic scattering<br />

Data normalisation <strong>and</strong> consistency checks<br />

First φ mt spectrum at SIS<br />

Ar+KCl<br />

1.75 AGeV<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 24<br />

SQM08


Exclusive reconstruction of <strong>the</strong> π,η → γe + e- Δ1232<br />

π<br />

N1440 N1535 Δ1600<br />

Yields <strong>and</strong> invariant mass<br />

agree with resonance model<br />

Teis et al, ZPA356 (97) 421<br />

Refinements:<br />

Δ Decay ang. Distr. (Wicklund<br />

et al.)<br />

N(1440) production angle<br />

( Aichelin et al.)<br />

ppe + e - detected<br />

η<br />

π,η → γ γ* γ → γe + e- Helicity distributions γ* * → e + e- dσ/d /dΩe~ ~ 1+cos 2θ (QED prediction, first measurement !<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 25


Conclusions <strong>and</strong> outlook<br />

HADES is in a very productive period<br />

C+C data have confirmed <strong>DLS</strong> data <strong>and</strong> triggered new <strong>the</strong>oretical<br />

calculations which are much closer to data<br />

E=1.25 GeV :<br />

pp data as expected <strong>from</strong> π ° <strong>and</strong> Δ contributions<br />

pn data unexplained<br />

critical test for <strong>the</strong>oretical inputs<br />

check contribution of pn Bremsstrahlung <strong>and</strong> ΔΔ Dalitz decay<br />

A lot of o<strong>the</strong>r promising data (exclusive channels, strangeness, …)<br />

Focus on « high precision hadronic physics tests »<br />

�� electromagnetic structure of hadrons<br />

�� Inclusive production of mesons (off-shell (off shell effects) effects<br />

Necessary (<strong>and</strong> interesting !) step before studying medium<br />

effects….. effects…..<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 26


2001/2<br />

2004<br />

2008/9<br />

2004<br />

2009-2011 2009 2011<br />

2011<br />

2005<br />

> 2013<br />

2006<br />

2007<br />

2007<br />

2008<br />

A program for <strong>the</strong> future<br />

C + C 2 AGeV<br />

C + C 1 AGeV<br />

p + p 2.2 GeV<br />

Ni + Ni, Au+Au<br />

pp elastic,<br />

π +<br />

elastic,<br />

+ N, π + A<br />

exclusive ppe+e- ppe+e (π°,η)<br />

Ar + KCl 1.75 AGeV<br />

p + p 1.25 GeV<br />

exclusive ppe+e- ppe+e (π°,Δ)<br />

p + p 3.5 GeV<br />

d + p 1.25 AGeV<br />

p+Nb 3.5 GeV<br />

1 PRL (e+e-) + 1 submitted (hadron)<br />

1 PLB (e+e-) + 1 submitted (hadron)<br />

Upgrade RPC, DAQ, MDC1<br />

Analysis finished (draft)<br />

Validation of detector performance,<br />

measures of π° <strong>and</strong> Planned η Dalitz decays (helicity<br />

distribution), “free” cocktail<br />

Analysis ongoing dielectron spectra, medium<br />

Hades goes<br />

effects<br />

goes FAIR ( 8 AGeV) AGeV<br />

effects<br />

inclusive analysis finished (draft)<br />

Δ Dalitz decay first measurement<br />

2010 Planned<br />

ω line shape <strong>and</strong> cocktail (π, Δ, η, ω, ρ, φ...)!<br />

Contribution of pn Bremstrahlung / Δ Dalitz decay<br />

Reference for medium effects<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 27


Vielen Dank<br />

ISHIP 2008, GSI Beatrice Ramstein, IPN Orsay, France 28

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