4,170 research outputs found
QCD Green functions in a gluon field
We formulate a dressed perturbative expansion of QCD, where the standard
diagrams are evaluated in the presence of a constant external gluon field whose
magnitude is gaussian distributed. The approach is Poincar{\'e} and gauge
invariant, and modifies the usual results for hard processes only by power
suppressed contributions. Long distance propagation of quarks and gluons turns
out to be inhibited due to a branch point singularity instead of a pole at
in the quark and gluon propagators. The dressing keeps the (massless)
quarks in q qbar fluctuations of the photon at a finite distance from each
other.Comment: 21 pages, 7 figures. Minor modifications in text. Version to be
published in JHE
Interpretation of High Energy String Scattering in terms of String Configurations
High energy string scattering at fixed momentum transfer, known to be
dominated by Regge trajectory exchange, is interpreted by identifying families
of string states which induce each type of trajectory exchange. These include
the usual leading trajectory and its daughters as
well as the ``sister'' trajectories and their
daughters. The contribution of the sister to high energy scattering
is dominated by string excitations in the mode. Thus, at large ,
string scattering is dominated by wee partons, consistently with a picture of
string as an infinitely composite system of ``constituents'' which carry zero
energy and momentum.Comment: 14 pages, phyzzx, psfig required, Florida Preprint UFIFT-94-
Stellar laboratories. V. The Xe VI ultraviolet spectrum and the xenon abundance in the hot DO-type white dwarf RE0503-289
For the spectral analysis of spectra of hot stars with a high resolution and
high signal-to-noise ratio (S/N), advanced non-local thermodynamic equilibrium
(NLTE) model atmospheres are mandatory. These are strongly dependent on the
reliability of the atomic data that are used for their calculation.
Reliable Xe VI oscillator strengths are used to identify Xe lines in the
ultraviolet spectrum of the DO-type white dwarf RE0503-289 and to determine its
photospheric Xe abundance.
We publish newly calculated oscillator strengths that are based on a recently
measured Xe VI laboratory line spectrum. These strengths were used to consider
their radiative and collisional bound-bound transitions in detail in our NLTE
stellar-atmosphere models to analyze Xe VI lines exhibited in high-resolution
and high S/N UV observations of RE0503-289.
We identify three hitherto unknown Xe VI lines in the ultraviolet spectrum of
RE0503-289 and confirm the previously measured photospheric Xe abundance of
this white dwarf (log Xe = -4.2 +/- 0.6).
Reliable measurements and calculations of atomic data are prerequisite for
stellar-atmosphere modeling. Observed Xe VI line profiles in the ultraviolet
spectrum of the white dwarf RE0503-289 were well reproduced with the newly
calculated Xe VI oscillator strengths.Comment: 3 pages, 4 figure
The hbar Expansion in Quantum Field Theory
We show how expansions in powers of Planck's constant hbar = h/2\pi can give
new insights into perturbative and nonperturbative properties of quantum field
theories. Since hbar is a fundamental parameter, exact Lorentz invariance and
gauge invariance are maintained at each order of the expansion. The physics of
the hbar expansion depends on the scheme; i.e., different expansions are
obtained depending on which quantities (momenta, couplings and masses) are
assumed to be independent of hbar. We show that if the coupling and mass
parameters appearing in the Lagrangian density are taken to be independent of
hbar, then each loop in perturbation theory brings a factor of hbar. In the
case of quantum electrodynamics, this scheme implies that the classical charge
e, as well as the fine structure constant are linear in hbar. The connection
between the number of loops and factors of hbar is more subtle for bound states
since the binding energies and bound-state momenta themselves scale with hbar.
The hbar expansion allows one to identify equal-time relativistic bound states
in QED and QCD which are of lowest order in hbar and transform dynamically
under Lorentz boosts. The possibility to use retarded propagators at the Born
level gives valence-like wave-functions which implicitly describe the sea
constituents of the bound states normally present in its Fock state
representation.Comment: 8 pages, 1 figure. Version to be published in Phys. Rev.
Regulation of CYP3A5 in Pancreatic Ductal Adenocarcinoma
CYP3A5 is a drug metabolism enzyme that is polymorphically expressed in normal tissues and expressed in high amounts in some cancers, including pancreatic ductal adenocarcinoma (PDAC). There have been several published studies regarding CYP3A5 regulators, but there is still much to be discovered concerning CYP3A5 regulation in cancer. To further understand the regulation of CYP3A5, a high-throughput screen was performed in the AsPC-1 PDAC cell line. This screen employed small interfering RNA (siRNA) targeting transcription factors and chromatin-associated proteins. We identified siRNA that decreased CYP3A5 mRNA and protein levels in AsPC-1 cells and probed into the potential mechanisms. Taken together, this study brought to light a previously undescribed regulator of CYP3A5 expression
Complete spectral energy distribution of the hot, helium-rich white dwarf RX J0503.9-2854
In the line-of-sight toward the DO-type white dwarf RX J0503.9-2854, the
density of the interstellar medium (ISM) is very low, and thus the
contamination of the stellar spectrum almost negligible. This allows us to
identify many metal lines in a wide wavelength range from the extreme
ultraviolet to the near infrared. In previous spectral analyses, many metal
lines in the ultraviolet spectrum of RX J0503.9-2854 have been identified. A
complete line list of observed and identified lines is presented here. We
compared synthetic spectra that had been calculated from model atmospheres in
non-local thermodynamical equilibrium, with observations. In total, we
identified 1272 lines (279 of them were newly assigned) in the wavelength range
from the extreme ultraviolet to the near infrared. 287 lines remain
unidentified. A close inspection of the EUV shows that still no good fit to the
observed shape of the stellar continuum flux can be achieved although He, C, N,
O, Al, Si, P, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Cr, Ni Zn, Ga, Ge, As, Kr, Zr, Mo,
Sn, Xe, and Ba are included in the stellar atmosphere models. There are two
possible reasons for the deviation between observed and synthetic flux in the
EUV. Opacities from hitherto unconsidered elements in the model-atmosphere
calculation may be missing and/or the effective temperature is slightly lower
than previously determined.Comment: 92 pages, 45 figure
Nutrient Limitation of Periphyton in a Spring-Fed, Coastal Stream in Florida, USA.
There is strong evidence to suggest that ground-water
nitrate concentrations have increased in recent years and
further increases are expected along portions of the central
Gulf coast of Florida. Much of the nitrate enriched groundwater
is discharged into surface waters through numerous
freshwater springs that are characteristic of the area and the
potential for eutrophication of their receiving waters is a
legitimate concern. To test the potential effects of elevated
nutrient concentrations on the periphyton community an
in
situ
nutrient addition experiment was conducted in the
spring-fed Chassahowitzka River, FL, USA, during the summer
of 1999. Plastic tubes housing arrays of glass microscope
slides were suspended in the stream. Periphyton colonizing
the microscope slides was subjected to artificial increases in
nitrogen, phosphorus or a combination of both. Slides from
each tube were collected at 3- to 4- day intervals and the
periphyton communities were measured for chlorophyll concentration.
The addition of approximately 10 μg/L of phosphate
above ambient concentrations significantly increased
the amount of periphyton on artificial substrates relative to
controls; the addition of approximately 100 μg/L of nitrate
above ambient concentrations did not. The findings from
this experiment implicated phosphorus, rather than
nitrogen, as the nutrient that potentially limits periphyton
growth in this system.(PDF contains 4 pages.
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