

The physics of particle motion in a Kerr geometry has been extensively studied. The case of motion of particles with spin is less well investigated. We have studied the case of the motion of a spinning particle by applying the Papapetrou equation, which includes a spin - curvature coupling term, and an equation that describes the evolution of the spin of the particle. The motion is considered for a Kerr geometry in the weak field limit. We have obtained numerical solutions to this system of equations. Our results suggest that spin orientation is important for particle trajectories in a manner that is similar to the Stern-Gerlach effect. This could be important for the motion of very low mass neutrinos.
[FE.02] Polarimeter for high energy photons
Bogdan Wojtsekhowski (Jefferson Lab, Newport News, VA), Branislav Vlahovic (North Carolina Central University, Durham, NC), David Tedeschi (University of South Carolina, Columbia, SC), Samuel Danagulian (A amp; T State University, Greensboro, NC), Vladimir Litvienko, Igor Pinayev (FEL-Duke University, Durham, NC)
The physics program at TJNAF includes fundamental experiments with polarized photon beam in few GeV energy range. Development of the Polarimeter for use in Hall B experiments is the subject of present abstract. We have proposed to take advantage of the recent progress in silicon micro strip detectors for measurement of the geometry and angle correlation in electron positron pair production from an amorphous converter. A detailed analysis of the setup including MC simulation shows an experimental asymmetry \sigma_\parallel/\sigma_\perp \sim 1.7 in a wide range of the photon energies.
This asymmetry value is confirmed by our experimental results obtained using 100 percent polarized 40 MeV \gamma rays at Duke FEL.
[FE.03] Weak \Lambda Production in Electron Scattering from Protons
Stephan Mintz (Florida International University)
We calculate the differential cross section for the weak,
strangeness changing, electron scattering process,e^- +
p\longrightarrow \Lambda + \nu for incoming electron
energies from 0.5 GeV to 6.0 GeV. We obtain as well the
contributions of the individual form factors to the
differential cross sections. We find that the differential
cross sections peak as the maximal scattering angle for
\Lambda is approached and that the peak height increases
as the electron energy is increased. The behavior of the
differential cross section near the maximal angle is
discussed as is the possibility of observing this reaction
at TJNAF. We also discuss this reaction as a tool for
studying the weak strangeness changing current. .
[FE.04] Inclusive Neutrino Reactions in ^13C and Neutrino Backgrounds at KARMEN and Los Alamos
Stephan Mintz (Florida International University)
Inclusive neutrino reactions cross sections on ^13C for
the reactions, \nu_e + ^13C\longrightarrow e^- + X and
\nu_\mu + ^13C\longrightarrow \mu^- + X are calculated
from threshold to several hundred MeV. Averaged cross
sections over the Michel spectrum and over the Los Alamos
muon neutrino spectrum are obtained. The method of
calculation is a phenomenological tensor model. The
consequences of these results with respect to the
experiments at LAMPF and KARMEN are discussed.
[FE.05] Light-front quark model analysis for exclusive semileptonic B- and D-Decays
Ho-Meoyng Choi (North Carolina State Univerity), Chueng-Ryong Ji Ji (North Carolina State University)
We present the analysis of exclusive semileptonic B- and
D-decays using the constituents quark model based on the
light-front quantization. Our method of analytic
continuation to obtain the weak form factors avoids the
difficulty associated with the contribution from the
nonvalence quark-antiquark pair creation. Our numerical
results are in a good agreement with the available
experimental data.
[FE.06] The Reaction e^- + p\longrightarrow + \Sigma^0 + \nu_e and the Structure of the Weak Strangeness Changing Current
Stephan Mintz (Florida International Umiversity), Michael Barnett (Florida International University)
We calculate the differential cross section for the
reaction, e^- + p\longrightarrow \Sigma^0 + \nu_e for
incident electron energies from 1.0 to 6.0 GeV. We find the
contributions of the various form factors to the
differential cross section and show that only the vector and
axial vector form factors make major contributions. We
discuss this reaction as a possible test of the isospin
structure of the weak strangeness changing current and
discuss its relationship to weak \Lambda production.
Finally we discuss the possibility of observing this
reaction at TJNAF.
[FE.07] Virtual Antiparticle Pairs and Photon Propagation
David Batchelor (NASA/Goddard Space Flight Center)
Virtual pairs of elementary particles and their
antiparticles, which are spontaneously created and
annihilated in the quantum vacuum, are long-accepted
consequences of quantum field theory. In this talk, it is
shown that the polarizability of these virtual antiparticle
pairs makes them a suitable medium for the propagation of
electromagnetic radiation in vacuo. A semi-classical
model of a photon propagating in this medium is constructed,
and the electric polarizability and the density of virtual
pairs are derived for each species of charged elementary
particles (except quarks). The photon model, virtual pair
polarizability, and resulting pair density together lead to
a wave equation with the correct phase velocity for
electromagnetic waves, c. This model is especially
noteworthy because of the absence of adjustable parameters
that might be required to correspond with observed photon
properties.
[FE.08] Many Body Coulomb Gauge Hamiltonian Approach to the Hadrons
Felipe J. Llanes-Estrada, Stephen R. Cotanch (North Carolina State University)
We report progress in approximately diagonalizing an
effective QCD Hamiltonian by utilizing many body techniques.
A confining potential determined by lattice gauge
calculations and similar to the Cornell potential
supplements our perturbative Hamiltonian.The effective
Hamiltonian is then divided into the quark and the glue
sectors The Bardeen-Cooper-Schrieffer (BCS) approximation is
used for the ground state (vacuum) in both sectors to
generate spontaneus chiral symmetry breaking and an improved
quasi-particle basis, followed by the Tamm-Dancoff and
Random Phase Approximations to reasonably reproduce the
excited states (the particle spectrum). Here we focus on the
quark sector and study the angular momentum splittings due
to the relativistic Hamiltonian and the central role of
chiral symmetry to generate the hyperfine splitting for the
light flavor mesons. Finally, we discuss applications to
many quark and gluon systems.
[FE.09] Compton Photon Polarimeter for the SLAC Linear Collider.
Steven Berridge, William Bugg, Hans Cohn, Yuri Efremenko, Yuri Kamyshkov, Dmitry Onoprienko, Achim Weidemann (University of Tennessee, Knoxville), Michael Woods (Stanford Linear Accelerator Center)
The longitudinal and transverse polarization of a high
energy electron beam can be measured by the detection of
photons produced in Compton scattering of the electrons from
an intense polarized laser beam. We have built a
calorimetric device based on the quartz fiber technology to
perform polarization measurement at the SLAC Linear
Collider. This detector was used to provide a cross check of
the polarization measurement by the SLD Compton Polarimeter
and allowed for improvement in the overall accuracy of many
physics results produced by the SLD. Possible use of this
technology in the polarimetry at future linear colliders is
discussed.
[FE.10] Polarized Parity Violating Electron Scattering on ^3H and Its Relation to the ^3He Case
Stephan Mintz, George Gerstner, Michael Barnett, Mohsen Pourkaviani (Florida International University)
We calculate the asymmetry parameters,A, and figures of
merit for polarized parity violating electron scattering
from ^3H via the reaction,e^- + ^3H \longrightarrow ^3H +
e^- for incident electron energies from 1.0 to 4.0 GeV. We
find sharp variations in A due to cancellations similar to
those reported for the reaction e^- + ^3He\longrightarrow
e^- + ^3He but at different angles due to differences in
the form factors for the two cases. We find that at small
angles the asymmetry may be obtained to reasonably high
accuracy for all energies considered here. We show that it
might be possible to observe strange quark current
contributions in this region. We also discuss the
relationship between the ^3H and ^3He cases.
[FE.11] Using Micro Ion Beam Induced Current to Characterize and Improve Diamond Microstrip Detector
Branislav Vlahovic, Angeraulerio Soldi (North Carolina Central University Durham, NC), Milko Jaksic (Institute Rudjer Boskovic, Zagreb, Croatia), Zlatko Sitar (North Carolina State Universiti, Raleigh, NC)
Diamond microstrip detectors are promising for use in intermediate and high energy experiments with large luminosity that requires high resolution tracking.
For this purppose, a thin 250 micron, (100) highhly oriented polycrystalline diamond film, has been developed by chemical vapor deposition (CVD) method. Characterization of this film is performed by measuring its transmitance in the spectrum region from IR to UV; by Raman measurement; and by electrical measurents. Thus far, the results have shown a high quality of diamond film.
A 6 MeV proton microbeam of few micrometers spot size is used to measure charge collection efficiency profile along the thickness of the detector. The measurements were carried out at several bias voltages and shaping times. Relative large collection distance were obtained, and assuming that the mobilities and trapping times are uniform, the electric field profile is obtained too.
[FE.12] Analytic Approximation for the Vacuum Polarization of Fermions in Static, Spherically Symmetric Spacetimes
Peter Groves, Paul Anderson (Wake Forest University)
A method for the computation of the vacuum polarization of fermions in static, spherically symmetric spacetimes is presented. It is found that one contribution to the vacuum polarization can be calculated analytically, and can serve as an analytical approximation for massless fermions. It is likely that a generalization of this method could be used to calculate the stress-energy tensor for fermions in static, spherically symmetric spacetimes.