689c
Nuclear Physics A525 (1991) 689c-69% North-Ho~and, Amsterdam
PROTON
RAPIDITY
DISTRIBUTIONS
Lawrence
FROM 60 GEV/N
S.R. Tonse Berkeley Lab., Berkeley CA 94720 and
‘sO+Au
COLLISIONS
USA
The NA35 Collaboration: J.Baechler,’ J. Bartke,3 H. Bialkowska,4 R. Bock,‘R. Brockmanqs P.Buncic,’ S.I. Chase,s I. Derado,’ V. Eckardt,’ J. Eschke,” C. Favuzzi,’ D. Ferenc,’ B. Fleischmann,‘~” M. Fuchqs,‘* M. Gazdzicki,” H.J. Gebauer,’ E. Gladysz, C. Guerra,’ 0.Hansen,i5 J.W. Harris,’ W. Heck,” ~~.Hoffman,’ T. Humaniq5 S.Kabana,” K. Kadija,‘,’ A. Karabarbounis,” R. Keidel,13 J. Kosiec,‘1p’4M. Kowalski,3s A.Kiihmichel,” M.Lahanas,” Y. Lee ” M. LeVine,2 A. Ljubicic,’ S. Margetis,” E. Nappi, G. 0dynieq6 G. Paic,g A. Panagiotou,” A. Petridis,” A. Piper,13 F. Posa,’ H.G. Pugh,‘F. Piihlhofert3 G. Rai,’ W. Rauch,’ R. Renfordt,‘i D. R6hrich,” H. Rothard,” K. Runge,’ A. Sandoval,’ E. Schmidt” N. Schmitz,8 E. Schmoetten,’ I.Schneider,l’ P. Seyboth,’ J. Seyerleiq8 E. Skrzypczak,‘* I’. Spine%,? R. Stock ii H. StrGbete,” L. Teitelbaum, S. Tonse,s G. Vassileiadis,‘* G. Vesztergombi,’ D! Vraniqg and S. Wenig” ‘Fakultit fiir Physik, Universitat Freiburg, D-7800 Freiburg, Germany ‘Brookhaven National Laboratory, Upton, NY 11973, USA 31nstitute of Nuclear Physics, PL-30055 Cracow, Poland 41nstitute of Nuclear Studies, PL-00681 Warszawa, Poland ‘Gesellschaft fiir Schwerionenforschung, D-6100 Darmstadt 11, Germany ‘Lawrence Berkeley Laboratory, University of California, Berkeley CA 94720, USA 7Dipartimento di Fisica, Universita di Bari, and INFN, I-70126 Bari Italy ‘Mu-Planck-Institut fiir Physik und Astrophysik, D-8000 Miinchen, Germany ‘Rudjer Boskovic Institute, 41001 Zagreb, Yugoslavia “Institut fiir Hochenergiephysik, Universit;it Heidelberg, D-6900 Heidelberg, Germany “Fachbereich Physik, Universitit Frankfurt, D-6000 Frankfurt, Germany “Physics Department, University of Athens, GR-157-71 Athens, Greece 13Fachbereich Physik, Universitat Marburg, D-3550 Marburg, Germany 141nstitute of Experimental Physics, University of Warsaw, PL-00681 Warszawa, Poland Abstract; An analysis of the proton rapidity distribution in central 160+Au collisions at 60 GeV/n measured in the NA35 streamer chamber detector at the CERN SPS is presented. The charge excess of positive particles over negative particles was measured. The rapidity distribution of the charge excess which can be associated with the primordial protons in the collision is studied in terms of the nuclear stopping power and is compared to the predictions of various models.
Central 160+-Au collisions at 60 GeV/n were studied using the NA35 streamer chamber detector. The emphasis of this study was to determine the degree of nuclear stopping at an incident energy intermediate between 14.6 GeV/n and 200 GeV/n since these two energies have been studied extensively [I, 2,3] and may be representative of different stopping regimes. Most 0375.9474/91/$03.50 0 1991 - Elsevier Science Publishers B.V. (North-Holland)
690~
S.R. Tonse et al. / Proton mpidiy distributions
fixed-target
experiments
at relativistic
due to high track densities. is used to measure the total E$’
emission
is expected
with
all initial
energy
a transverse
state
whereas
at 60 GeV/n
GeV/n,
experiments
A more results
model
than obtained
60 GeV/n
transverse
energy calorimeter
to 1% of the total nucleus
taken
inelastic
interacts
trajectories
collisions
measurement
along the beam
trigger
component
average
2-dimensionsal
of the projected
is labelled
the difference
between
true rapidity
units in the kinematic
increases
of matching
from different
(10,500
(fi
statistics
model
positive
collisions
nucleons
component
for pi,
for the since the
in magnitude
studies
the
by 2/r.
the distribution
of
was found to have a width of a=O.OS
in one view only, compared
than a factor
views is eliminated.
Therefore
of momentum
To compensate
vector is diminished
Measuring
by greater
the 160 Particle
and charge sign
three was used.
From simulation
that
(25~ + 30n).
(7r/2)pY is substituted
and
A high
corresponding
it is estimated
pv of the momentum.
calculation,
tracks
= 10.7 GeV/n).
the longitudinal
and quasi-rapidity
region of interest.
3-view processing,
In this approach
offline to yield the momentum
quasi-rapidity.
of This
since more energy is allowed
O-Au events
of 55 target
of a 3-dimensional
quantity
emission.
to be 1.0, 0.93 and 0.84 at incident
view of a possible
component
At 200 [2].
distribution
energy available.
of 60 GeV/n
quantities:
of pr in the rapidity
stopping[l],
reactions
for isotropic
method
In a geometrical
one camera
resulting
tracks
momentum
on film and measured
projection
particle
respectively.
of 89 central
with a cylinder
complete
for the rapidity
was used to select the most central
and one transverse
missing The
at a beam
In this analysis
consists
width
is estimated
and 200 GeV/n
cross-section.
were recorded
of each particle.
compares
and 0.9 in 160+W[2].
than that obtained
from the previous
consist
on the average
to determine
method
in isotropic
and 0.7 in 160+W
and hence there is less transverse
The data used in this analysis tracks)
in ‘60+Au[4]
[5] a 11ows a broader
of 14.5 GeV/n,
results
at 14.6 GeV/ n reveals
in i60+Au[3],
experimentally,
in 160+Au
7400 negative
which
This
= r/4(& - m;), where m; is the total mass of of stopping in an event is then given by Ey/EF”“.
0.5 stopping
of stopping
I&*).
sum ET,
collisions
ET,=
of mid-rapidity
energy distributions
uses calorimetry
= CEsin
projectile,
0.6 stopping
report
method
(EF’
the data exhibit
longitudinally
the amount
stopped
measure
as observed
in a smaller
to propagate
The simplest
a study of “Si+Au
sophisticated
particles,
energies
The
forward
derived from transverse
per event
a fully
energy
particles.
Using this approach
produced
of particles from
lack good acceptance
information
the degree of stopping.
transverse
to what
energies
Therefore
to conventional
of three since the J-view
The overall efficiency
practice
for the data sample
is 299%. The proton bution
quasi-rapidity
of negative
distribution
is obtained
by subtracting
the quasi-rapidity
distri-
ones, both calculated using the proton mass. This assumes a cancellation of produced X+ with ?r-, K+ with K- and protons with antiprotons, In isospin-symmetric systems equal number8 of leaving the original non-produced protons. produced assumed The
particles
7r+ and T-
from positive
are expected.
to be equal for rapidities data
system). 8 protons calculations
is displayed
The
integrated
initially
for the region contents
forward
those predicted
of the proton
forward
projectile
hydrodynamical
of mid-rapidity
an estimate in a 16-on-55
is displayed
distribution in Fig.1.
(Yc~=1.8
of 10.88f0.68
but smaller
quasi-rapidity
by various models
tion of the Landau
furnish
a+ and n-
production
are
of the center-of-mass.
of mid-rapidity,
for a fully stopped
A comparison
Since 160 is isospin-symmetric forward
than
protons,
the 16.5 protons
in the
16-on-55
larger
than
the
expected
from
collisions
with
collision. measured
in i60+Au
The dashed line represents
model [S] with complete
stopping
for the system
the predic16-on-55.
S.R Tome et al. / Proton rapiditya%tributions
691~
'"OtAu 60 GeV (NA35) ~-'-'--w'l ‘\
‘\
\
.
Fritiof Landau Marco a
l
protcms
IL 2
Figure
1: Proton
3
Rapidity
(Quasi-rapidity
rapidity
distributions
--*: T)
4
for protons)
for the data and several models
It has a maximum at mid-rapidity which is far above the data points. This excess of protons forward of mid-rapidity compared to the data is a result of isotropic emission in the model. Comparisons were also made varying the number of target participants in the Landau model but a reasonable fit could not be made to the data. The rapidity distribution of protons from 60 GeV/n 160+Au collisions in a multiple nucleonnucleon collision model, MARCO[‘I], is displayed in Fig.1. Using a linearly increasing x distribution (LY=~), where x is the fraction of energy plus longitudinal momentum retained per nucleon-nucleon collision the MARCO calculations reproduce the data. However, MARCO requires a flat x distribution (a=l) to fit transverse energy spectra from the same data set [7]. The rapidity spectrum from FRITIOF is also displayed in Fig.1. It has a broad peak centered at Y,,,=3.3 whereas the data continue to rise toward mid-rapidity. It thus appears that there is more stopping of protons in the data, despite the fact that FRITIOF was generated with zero impact parameter, i.e. maximum centrality. Our substitution of the charge-excess distributon for the proton distribution neglects any inequality between the K+ and K- production rates. This can be caused when the contribution of K+‘s from associated production is not cancelled by negative particles in the same rapidity bin. The expected excess of K+ production cannot be precisely estimated as sufficient kaon data have not been measured at 60 GeV/c. In the present analysis it is neglected, since the effect is estimated to be approximately 10% compared to the differences observed between the data and the models in Fig.1. This estimate is derived from the FRITIOF model which predicts only 0.5 K+ forward of center of mass, spread over about 2 units of rapidity. A comparison of the proton and 7r- rapidity distributions for the same data set is displayed in Fig.2. The data plotted forward of mid-rapidit,y show similar shapes for the two. The protons are lower by a factor of 0.35. A similarity of shape can be interpreted as emission from ii common source.
S.R Tonse et al. / Proton rapid9 distributions
692~
lGO I Au 60 GeV (NA35) .__I~ '~_~~'.-.'--,-.~ ""-7 I
.
protolIs TT-
.
I . f
oLILL--L
f
**
Quasi-rapidity
distributions
I
., I
,
,_I1
4
3
2
Figure 2:Rapidity
.
I
I for protons,
of protons
rapidity
5
for 6
and rr- from 160+Au
collisions
at 60 GeV/n
hydrodynamical model[6] indicates In summary, a comparison of our data with the Landau that the 160projectile does not stop completely in the Au target for central collisions at 60 GeV/n. energy
The MARCO distribution
measurements
multiple collision and the proton
of stopping
and that rapidity
derived
distributions
This work was supported
model does not simultaneously
rapidity
distribution.
from transverse
of primordial
These
energy spectra
baryons
in part by the United
[2] J. Schukraft
(1989).
et al, Nuc1.Phys.A
[3] J. W. Harris et al, Nuc1.Phys.A [4] W. Heck et al, Z.Phys.C
498,79c 498,133c
States Dept.
of Energy
(1989).
38,19 (1988).
[5] J. Stachel and P. Braun-Munzinger, [6] Von Gersdorff et al, Phys.Rev.C (71 C.Y. Wong et al, Phys.Rev.D
Nuc1.Phys.A
39,1385 (1989). 39,2606
(1989).
indicate
that
must be considered.
References (1990).
the transverse
alone may not be reliable
DE-AC03-76SF00098.
[l] J. Barrete et al, Phys.Rev.Lett.64,1219
describe
discrepancies
495,577c
(1989).
under contract