1,551 research outputs found
Visualization of Active Faulting using 3-D GPR Data Recorded Across the Alpine Fault, New Zealand
Three-dimensional (3-D) GPR data were acquired
across braided river sediments cut by the Alpine Fault at Calf
Paddock, New Zealand. We used 100 MHz antennas to obtain
images of the subsurface to a depth of 15 m. Cross-sections and
depth-converted time slices selected from the migrated data volume
show both the structural contrast generated by recent offsets
of the fault and the variable orientation of the dipping structures
within the braided river deposits. A trace-correlation technique is
used to generate dip and dip-direction attribute maps that allow us
to visualize the 3-D orientation of the dipping structures. The
attribute maps reveal at least 3 different reflection patterns and the
presence of minor faulting away from the main fault. A correlation-
based migration technique applied to a 2-D GPR profile resulted
in the successful identification of the main fault and subsidiary
faults at distances up to 50 m from the main fault
One-Loop Renormalization and Asymptotic Behaviour of a Higher-Derivative Scalar Theory in Curved Spacetime
A higher-derivative, interacting, scalar field theory in curved spacetime
with the most general action of sigma-model type is studied. The one-loop
counterterms of the general theory are found. The renormalization group
equations corresponding to two different, multiplicatively renormalizable
variants of the same are derived. The analysis of their asymptotic solutions
shows that, depending on the sign of one of the coupling constants, we can
construct an asymptotically free theory which is also asymptotically conformal
invariant at strong (or small) curvature. The connection that can be
established between one of the multiplicatively renormalizable variants of the
theory and the effective theory of the conformal factor, aiming at the
description of quantum gravity at large distances, is investigated.Comment: 11 pages, LaTeX file (some mistakes have been corrected and a
reference has been added), UB-ECM-PF 94/
Seabed characterization: developing fit for purpose methodologies
We briefly describe three methods of seabed characterization which are âfit for purposeâ, in
that each approach is well suited to distinct objectives e.g. characterizing glacial
geomorphology and shallow glacial geology vs. rapid prediction of seabed sediment
distribution via geostatistics. The methods vary from manual âexpertâ interpretation to
increasingly automated and mathematically based models, each with their own attributes
and limitations. We would note however that increasing automation and mathematical
sophistication does not necessarily equate to improve map outputs, or reduce the time
required to produce them. Judgements must be made to select methodologies which are
most appropriate to the variables mapped, and according to the extent and presentation
scale of final maps
Potential-density pairs for axisymmetric galaxies: the influence of scalar fields
We present a formulation for potential-density pairs to describe axisymmetric
galaxies in the Newtonian limit of scalar-tensor theories of gravity. The
scalar field is described by a modified Helmholtz equation with a source that
is coupled to the standard Poisson equation of Newtonian gravity. The net
gravitational force is given by two contributions: the standard Newtonian
potential plus a term stemming from massive scalar fields. General solutions
have been found for axisymmetric systems and the multipole expansion of the
Yukawa potential is given. In particular, we have computed potential-density
pairs of galactic disks for an exponential profile and their rotation curves.Comment: 8 pages, no figures, corrected version to the one that will appear in
Gen. Relativ. Gravit., where a small typo in eq. (13) is presen
Fermion Masses and Gauge Mediated Supersymmetry Breaking from a Single U(1)
We present a supersymmetric model of flavor. A single U(1) gauge group is
responsible for both generating the flavor spectrum and communicating
supersymmetry breaking to the visible sector. The problem of Flavor Changing
Neutral Currents is overcome, in part using an `Effective Supersymmetry'
spectrum among the squarks, with the first two generations very heavy. All
masses are generated dynamically and the theory is completely renormalizable.
The model contains a simple Froggatt-Nielsen sector and communicates
supersymmetry breaking via gauge mediation without requiring a separate
messenger sector. By forcing the theory to be consistent with SU(5) Grand
Unification, the model predicts a large tan beta and a massless up quark. While
respecting the experimental bounds on CP violation in the K-system, the model
leads to a large enhancement of CP violation in B-(B bar) mixing as well as in
B decay amplitudes.Comment: LaTeX, 25 pages, 8 figure
Viability of primordial black holes as short period gamma-ray bursts
It has been proposed that the short period gamma-ray bursts, which occur at a
rate of , may be evaporating primordial black holes
(PBHs). Calculations of the present PBH evaporation rate have traditionally
assumed that the PBH mass function varies as . This mass
function only arises if the density perturbations from which the PBHs form have
a scale invariant power spectrum. It is now known that for a scale invariant
power spectrum, normalised to COBE on large scales, the PBH density is
completely negligible, so that this mass function is cosmologically irrelevant.
For non-scale-invariant power spectra, if all PBHs which form at given epoch
have a fixed mass then the PBH mass function is sharply peaked around that
mass, whilst if the PBH mass depends on the size of the density perturbation
from which it forms, as is expected when critical phenomena are taken into
account, then the PBH mass function will be far broader than . In this paper we calculate the present day PBH evaporation rate,
using constraints from the diffuse gamma-ray background, for both of these mass
functions. If the PBH mass function has significant finite width, as recent
numerical simulations suggest, then it is not possible to produce a present day
PBH evaporation rate comparable with the observed short period gamma-ray burst
rate. This could also have implications for other attempts to detect
evaporating PBHs.Comment: 5 pages, 2 figures, version to appear in Phys. Rev. D with additional
reference
Where do graduates Develop their Enterprise Skills? The Value of the Contribution of Higher Education Institutionsâ Context
This study investigates the value of the contribution of HEIsâ context in developing graduates enterprise skills. HEIs are under pressure to develop more enterprising graduates, particularly with the increasing numbers of graduates seeking employment and the growing dissatisfaction of employers. This study explores where graduates develop enterprise skills through investigating the impact of HE and employment contexts on their development. The paper draws on a qualitative study in the social constructionist paradigm within the pharmacy context, where interviews were conducted with pharmacy academics and employers. Results show that ability to demonstrate skills in one context does not necessarily mean ability to demonstrate them in another since the development and demonstration of enterprise skills is impacted by the contexts in which they are developed and demonstrated. The study adds value by highlighting the significant role of both HE and employment contexts in developing enterprise skills, while emphasising that these skills become more transferable through exposure to more contexts
A pulsating white dwarf in an eclipsing binary
White dwarfs are the burnt-out cores of Sun-like stars and are the fate of 97 per cent of the stars in our Galaxy. The internal structure and composition of white dwarfs are hidden by their high gravities, which causes all elements apart from the lightest ones to settle out of their atmospheres. The most direct method of probing the inner structure of stars and white dwarfs in detail is via asteroseismology. Here we present a pulsating white dwarf in an eclipsing binary system, enabling us to place extremely precise constraints on the mass and radius of the white dwarf from the lightcurve, independent of the pulsations. This 0.325-solar-mass white dwarfâone member of the SDSS J115219.99+024814.4 systemâwill serve as a powerful benchmark with which to constrain empirically the core composition of low-mass stellar remnants and to investigate the effects of close binary evolution on the internal structure of white dwarfs
Constraints from CMB in the intermediate Brans-Dicke inflation
We study an intermediate inflationary stage in a Jordan-Brans-Dicke theory.
In this scenario we analyze the quantum fluctuations corresponding to adiabatic
and isocurvature modes. Our model is compared to that described by using the
intermediate model in Einstein general relativity theory. We assess the status
of this model in light of the seven-year WMAP data.Comment: 17 pages, 6 figure
Two-fermion bound state in a Bose-Einstein condensate
A nonlinear Schr\"odinger equation is derived for the dynamics of a beam of
ultracold fermionic atoms traversing a Bose-Einstein condensate. The condensate
phonon modes are shown to provide a nonlinear medium for the fermionic atoms. A
two-fermion bound state is predicted to arise, and the signature of the bound
state in a nonlinear atom optics experiment is discussed.Comment: 4 pages, 1 figure
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