|
Student
Abstracts: Nuclear Science at LBNL
Vertex Tracking for the Pixel Detector Group at STAR.
KENNETH GARMON (University of North Carolina, Chapel Hill, NC 27514) HOWARD
MATIS (Ernest Orlando Lawrence Berkley National Laboratory, Berkley, CA 94720)
.
The goal of the Solenoidal Tracker at RHIC (STAR) experiment is to search for a
phase transition in nuclear matter from confinement in hadronic particles to a
quark gluon plasma (QGP). The STAR experiment makes use of the new Relativistic
Heavy Ion Collider (RHIC) that has been built at Brookhaven National Laboratory
(BNL). One important signature that a quark gluon plasma has been created is
the enhanced production of D0 mesons. However, the present equipment lacks the
sensitivity necessary for detecting D0 mesons. A few members of the STAR group
at LBNL are now working on building a new detector component, designed
specifically to detect D0 mesons. The main component of this detector will be a
chip, which makes use of the new Active Pixel Sensor technology. My work in the
Pixel Detector Group has mainly focused on helping to determine the best
resolution for the chip. My mentor, Howard Matis, has created Monte Carlo
simulations of D0 meson decays and what data will be taken as a result in the
detector. My goal has been to write software (using C) that will re-create
particle trajectories and find the vertex (where the D0 meson originally
decayed). Once we have determined the most accurate algorithm for re-creating
D0 meson decays, we can then determine the most accurate resolution for the
chip. In addition, my algorithms can also be used in the final software that
will be used to actually analyze data from the detector. By actually running my
code using a Monte Carlo simulation, I have found that my program produces the
correct answers in all except for a few cases (in which the vertex lies very
close to the origin).
Gamma-ray Spectroscopy Using A Novel Sorting Routine:
"Blue". SEPEHR HOJJATI (Contra Costa College, San Pablo, CA
94806) STEVE ASZTALOS (Ernest Orlando Lawrence Berkley National Laboratory,
Berkley, CA 94720) .
Studying the coincident g-rays is one of the most powerful means to learn about
nuclear structure. The GANDS collaboration uses GAMMASPHERE in conjunction with
252Cf (with ~3% spontaneous fission branching ratio) to study the structure of
neutron-rich nuclei. For the purposes of studying the coincident relationship
between g-rays, one needs to construct a database of coincident g-ray events.
Blue, a computer software developed by Mario Cromaz (LBNL), provides a library
of subroutines that can be utilized both to construct such a database and to
access the database in the desired way by executing queries which would
construct one-dimensional histograms from multi-fold database. By writing
interfaces in C code, one can call the subroutines provided in Blue to produce
spectra which can then be displayed using standard nuclear physics data
analysis software. To date, we have read about 60 tapes into Blue and have
created several multi-fold (3 through 6-fold) databases which can be used to
resolve overlapping photo-peaks which are not otherwise resolvable using
traditional nuclear physics databases due to the typical data compression
invoked in creating such databases. Moreover, Blue reduces the size of a
traditional histogram by ~1000 folds.
The Recyclotron Project. MAISHA MURRY (Tuskegee
University, Tuskegee, AL 36088) MARGARET MCMAHAN (Ernest Orlando Lawrence
Berkley National Laboratory, Berkley, CA 94720) .
The objectives of the Recyclotron project are to produce medium-lifetime radioactive
beams, to test the limits and feasibility of working with them, and to run
future reactions with these beams. To produce radioactive beams, radioactive
isotopes are prepared in the 88-Inch Cyclotron. The radioactive isotopes are
collected and introduced into the Advanced Electron Cyclotron Resonance source
(AECR), where a charged particle beam is created and recycled back through the
cyclotron to produce a beam of the radioactive isotope. However precautions
must be taken to only medium-lifetime radioactive isotopes to prevent
contamination of the ion source. The preliminary radioactive beam attempted was
Krypton-76, which has a 14.8-hour half-life. In efforts to produce Krypton-76
there was the possibility of creating Selenium-75 with a 119.78-day half-life
and Arsenic-73 with a 80.3-day half-life, which are both long-lived radioactive
isotopes. It was determined during a test run on June 7, 2001 that very little
of the two contaminates were produced and therefore not a problem. Future
radioactive beams are anticipated such as bromine-77, -78 and Niobium-92 to
study the p-process nuclei, nuclear structure and magnetic moments.
Neutral Kaon-Kaon Correlations at STAR. CHARLES
STEINHARDT (Princeton University, Princeton, NJ 08544) NU XU (Ernest Orlando
Lawrence Berkley National Laboratory, Berkley, CA 94720) .
Bose-Einstein statistics predict identical bosons will tend towards the same
quantum state. We consider the relativistic momentum difference between a pair
of kaons, and pairs of kaons from the same event, which might interact, should
have a smaller difference than pairs of kaons from different events, which
cannot possibly interact. Theory predicts that the ratio of the two
distributions, when properly normalized, should be 1 for large values of
momentum difference but should be augmented by a Gaussian of some radius and
amplitude 1 for small values. The radius is the uncertainty in momentum, so the
uncertainty principle lets us determine a radius of the interaction. We used
data taken from Au-Au collisions at RHIC (Relativistic Heavy Ion Collider) and
observed by STAR (Solenoidal Tracker at RHIC) and examined the Bose-Einstein
correlation of kaons, unstable spinless bosons. The energy at RHIC is initially
high enough that the kaons are in equilibrium, and we measure them after they
decouple, or "freeze out". One of the reasons this is interesting is
that our energies are nearly high enough to create the Quark-Gluon Plasma, a
postulated state that existed just after the big bang, and a large freeze out
radius would be evidence of quark deconfinement that accompanies this state.
However, our preliminary results are that we do not find any correlation. This
would appear to conflict with published results from other experiments and
other particles, though we developed some theoretical models that remove that
conflict.
|