indra at gsi
DESCRIPTION
INDRA at GSI. November 1997 – April 1999. Z=3 Au + Au 80 AMeV Very peripheral. Systems:. Au + Au 40 to 150 AMeV Xe + Sn 50 to 250 AMeV C + Au 95 to 1800 AMeV. INDRA at GSI. INDRA at GSI. Phys. Rev. C 66, 064606 (2002). Stability. 336 CsI(Tl). Stability. Stability. - PowerPoint PPT PresentationTRANSCRIPT
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INDRA at GSI
November 1997 – April 1999
Z=3Au + Au80 AMeVVery peripheral
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INDRA at GSI
Systems: Au + Au 40 to 150 AMeVXe + Sn 50 to 250 AMeV C + Au 95 to 1800 AMeV
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INDRA at GSI
Phys. Rev. C 66, 064606 (2002)
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Stability
336 CsI(Tl)
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Stability
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Stability
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Identification
Ring 1
Pârlog parameterization
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Calibration check
12C + 1H at 30 AMeV
coincident
gainsconfirmedwithin 4%
A. Trzciński et al., NIM A 501 (2003) 367
ring 7
r6 r10
r12
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Centrality
Tsang et al. PRL 71, 1502 (1993) Reisdorf & Ritter, Ann. Rev. Nucl. Part. Sci.
Motivation
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Invariant cross sections for Au + Au at peripheral impact parameters
Motivation
From the Fermi to the relativistic domain
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Global variables and impact parameter
Au + Au at 60 A MeV Xe + Sn at 50 A MeV
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Part I:
Central Au + Au
Z = 3 at 100 A MeV
y
γβ
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Multiplicities
in central collisions
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Multiplicities
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Multiplicities
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Multiplicities
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Flow and fragmentation
Statistical model descriptionswith decoupled flow
SMM:F. Lavaud, thesis
MMMC:A. Le Fèvre et al.
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Flow and fragmentation
from MMMC model descriptionwith deformed source (0.7:1) and with decoupled flow
transverse
longitudinal
A. Le Fèvre et al.
Au + Au at 60
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Flow and fragmentation
from MMMC model descriptionwith deformed source (0.7:1) and with decoupled flow
transverse
longitudinal
A. Le Fèvre et al.
Au + Au at 60 variation of flow profile
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Questions
1) Why does the SMM or MMMC work so well in a dynamical situation ?
2) Deformation as a dynamical constraint !
3) Radial flow should be another constraint ! Implicitly contained in parameters ?
Alternatively: early fragment formation ?
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Flow and fragmentation
… shape of these distributions ischaracteristic of the presence of Coulomb forces and close to what is observed …
for early fragment formationsee also Danielewicz and Pan, Dorso and Aichelin, Barz et al. and others
X. Campi et al., Phys. Rev. C 67, 044610 (2003)
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Directed flow
Au + Au, Z = 2midcentralscaled variables
projections on x-z plane
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Directed flow
Au + Au, Z = 2midcentralscaled variables
work in progress J. Łukasik et al.
projections on x-z plane
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Directed flow
Au + Au, Z = 2midcentralscaled variables
work in progressJ. Łukasik et al.
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Directed flow
Au + Au, Z = 2midcentralscaled variables
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Directed flow
Au + Au, Z = 2 and Z = 1midcentralscaled variables
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Directed flow
Z = 2 and Z = 1 and Z
= 3
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Part II:
Peripheral Au + Au
Z = 3 at 100 A MeV
y
γβ
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Rapidity distributions
Z = 3 at 80 A MeV
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Transverse velocity spectra
100 A MeV Z = 3
J. Łukasik et al.,Phys. Rev. C 66, 064606 (2002)
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Contributions to transverseenergies
Fermi motion is not enough
N-N scattering is too much
Compensation due to Coulomb
at midrapidity
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ExtendedGoldhaber model
J. Łukasik et al.,Phys. Lett. B,in print (2003)
in 3 steps
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Model results
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Comparison
model
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Comparison
model
data
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Quantitativedescription of data
Transverse energy spectra
2
01
hard scattered nucleons
Li F C
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Quantitativedescription of data
Transverse energy spectra
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Quantitativedescription of data
Transverse energy spectra
Atomic number Z spectra
40
60
80
100
150
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Questions
1) Where is the equilibrated neck ?
2) Where is the equilibrated target/projectile residue ?
3) Clustering criterion on a nucleon distribution seems to be a general principle !
see also Gaitanos et al., Odeh et al., Gadioli et al. and others
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Summary
1) Central: Good description with deformed statistical source and decoupled radial flow; directed and elliptic flow in progress.
2) Peripheral: Good description with extended Goldhaber model (clustering criterion!).
3) New results also for Xe + Sn and C + Au.
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the end