The purpose of the PHENIX Muon Arms is to facilitate the study of
vector mesons decaying into dimuons, to allow the study of the
Drell-Yan process, and to provide the muon detection in as part of both the relativistic heavy ion and
spin physics programs of PHENIX. Each muon arm must both track and
identify muons, as well as provide good rejection of pions and kaons;
therefore, both a Muon Tracker and a Muon Identifier are needed. Each
arm of the Muon Tracker comprises three stations of tracking chambers,
with three planes of cathode strip chambers each, mounted inside the
end-cap muon magnet. Two different construction techniques are being
used for the chambers. The first and third stations are constructed
as honeycomb panels with cathode strips on the inside surfaces. The
second (central) stations are constructed as stacks of wires and
etched foils attached to aluminum frames. The position resolution will
be 100
m per plane which provides a mass resolution sufficient to
separate the
from the
and the
from the
.
Full-scale prototypes are currently being constructed and tested for the muon tracker station 1 honeycomb lattice CSC and the station 2 etched foil CSC. A prototype of the charge-sensitive preamplifier for CSC readout will be made and tested this summer.
The north and south muon identifiers, placed behind the 30 cm magnet endplate, each consist of 6 gaps instrumented with plastic proportional tubes interleaved with 5 layers of steel. Four large plus four small panels are used to tile a gap with tubes. The largest size panel is approximately 4 m x 6 m x 10 cm. The individual tubes are Iarocci limited streamer tubes operated at reduced voltage in order to maximize their longevity. The tubes have a resistive graphite coating on the inner surface that serves as the cathode. The eight wires in each tube are ganged together into one read-out channel to allow for low resolution tracking and to provide signals for the first and second level muon triggers.
A full-scale prototype of a large muon identifier panel is under construction and will be tested this summer. Mass fabrication of certain parts of the muon subsystems will begin in 1997.
The primary goal of the Relativistic Heavy Ion Physics program of
PHENIX is to detect the quark-gluon plasma (QGP) and measure its
properties with as many different experimental probes as the detector
will allow. The Muon Arms are a major contributor to the total
physics program. This subsystem will be used to measure the
production of vector mesons decaying into dimuons in heavy ion
collisions for masses ranging from that of the to the
. Measurement of the differential suppression of
and
production will provide information concerning
``deconfinement,'' i.e. Debye screening of the QCD potential.
The two muon
arms provide large acceptance for high mass pairs at central rapidity.
The Muon Arms allow study of the continuum dilepton spectra in a much
broader region of rapidity and mass than is accessible with the central arms
alone. Additionally, the coincidence using electrons detected
by the central arm will probe charm production and aid in the
understanding of the shape of the continuum dielectron spectrum. This
is because unlike-sign
pairs are primarily from
,
while like-sign pairs are mainly due to the combinatorial
background.
The following table provides the number of detected dimuons per RHIC
year (2000 hours at a luminosity of
cm
s
) for minimum-bias Au+Au collisions, with
GeV/c.
TOP: Contributions to the unlike-sign dimuon yield per central event as a function of the invariant mass. The dashed line shows the combinatoric background, the dotted line shows the signal and the solid line their sum. BOTTOM: Results from a like-sign subtraction. The solid line is the assumed signal again; the dashed line is constructed by subtracting the like-sign combinatoric background from the total unlike sign distribution.
This figure is an example of how well the simulated signal can be
restored by subtracting the like-sign invariant mass spectrum from the
total spectrum. Note the clear separation of the from
the
in the figure at the bottom.
Polarized pp collisions at from 50 to 500 GeV are
to be analyzed to measure the helicity distributions of quarks and
anti-quarks and gluon polarization in the nucleon. This information
is probed by studying the polarized Drell-Yan process, vector boson
production, polarized gluon fusion, and polarized gluon Compton
scattering. Antiquark structure function measurements rely on
analyzing Drell-Yan and vector boson production data. Gluon
polarization measurements rely on analyzing heavy quark,
,
and prompt photon data. Efforts to understand the contributions
of the spin of sea quarks and the polarization of gluons to
the total nucleon spin should help explain deviation of experimental
data from the Ellis-Jaffe sum rule.
A muon spectrometer with two arms has a greatly enhanced detection
capability for large muon pairs. It is at large
values of
where polarization effects are likely
to be maximal. Mass resolution at the
is approximately
5.3 GeV/c
which is quite acceptable for spin physics in this region.
As an example of part of the spin physics program, consider the Drell-Yan process
for which the longitudinal spin asymmetry is given by:
where . The superscripts
refer to parton spin projections parallel (+) or antiparallel (-) to
the parent hadron's spin projection.
Two theoretical predictions for using a
model by Bourrely and Soffer. Error bars shown on the lower curve
indicate PHENIX's sensitivity based on an integrated luminosity of
cm
at
GeV, yielding 10.8k muon
pairs; beam polarizations are taken to be 0.7.
The figure demonstrates how the expected experimental accuracy could
be used to distinguish between theoretical predictions.
Shown below are the number of Drell-Yan dimuons that would be detected
by the PHENIX muon spectrometer for an integrated luminosity of
cm
at
GeV.