5,489 research outputs found
SUSY-breaking Soft Terms in a MSSM Magnetized D7-brane Model
We compute the SUSY-breaking soft terms in a magnetized D7-brane model with
MSSM-like spectrum, under the general assumption of non-vanishing auxiliary
fields of the dilaton and Kahler moduli. As a particular scenario we discuss
SUSY breaking triggered by ISD or IASD 3-form fluxes.Comment: Latex, 27 pages, v2: added reference
Instanton induced charged fermion and neutrino masses in a minimal Standard Model scenario from intersecting D-branes
String instanton Yukawa corrections from Euclidean D-branes are investigated
in an effective Standard Model theory obtained from the minimal U(3)xU(2)xU(1)
D-brane configuration. In the case of the minimal chiral and Higgs spectrum, it
is found that superpotential contributions are induced by string instantons for
the perturbatively forbidden entries of the up and down quark mass matrices.
Analogous non-perturbative effects generate heavy Majorana neutrino masses and
a Dirac neutrino texture with factorizable Yukawa couplings. For this latter
case, a specific example is worked out where it is shown how this texture can
reconcile the neutrino data.Comment: 17 pages, 3 figure
Non-axisymmetric relativistic Bondi-Hoyle accretion onto a Schwarzschild black hole
We present the results of an exhaustive numerical study of fully relativistic
non-axisymmetric Bondi-Hoyle accretion onto a moving Schwarzschild black hole.
We have solved the equations of general relativistic hydrodynamics with a
high-resolution shock-capturing numerical scheme based on a linearized Riemann
solver. The numerical code was previously used to study axisymmetric flow
configurations past a Schwarzschild hole. We have analyzed and discussed the
flow morphology for a sample of asymptotically high Mach number models. The
results of this work reveal that initially asymptotic uniform flows always
accrete onto the hole in a stationary way which closely resembles the previous
axisymmetric patterns. This is in contrast with some Newtonian numerical
studies where violent flip-flop instabilities were found. As discussed in the
text, the reason can be found in the initial conditions used in the
relativistic regime, as they can not exactly duplicate the previous Newtonian
setups where the instability appeared. The dependence of the final solution
with the inner boundary condition as well as with the grid resolution has also
been studied. Finally, we have computed the accretion rates of mass and linear
and angular momentum.Comment: 21 pages, 13 figures, Latex, MNRAS (in press
Transient Behavior near Liquid-Gas Interface at Supercritical Pressure
Numerical heat and mass transfer analysis of a configuration where a cool
liquid hydrocarbon is suddenly introduced to a hotter gas at supercritical
pressure shows that a well-defined phase equilibrium can be established before
substantial growth of typical hydrodynamic instabilities. The equilibrium
values at the interface quickly reach near-steady values. Sufficiently thick
diffusion layers form quickly around the liquid-gas interface (e.g., 3-10
microns for the liquid phase and 10-30 microns for the gas phase in 10-100
microseconds), where density variations become increasingly important with
pressure as mixing of species is enhanced. While the hydrocarbon vaporizes and
the gas condenses for all analyzed pressures, the net mass flux across the
interface reverses as pressure is increased, showing that a clear
vaporization-driven problem at low pressures may present condensation at higher
pressures. This is achieved while heat still conducts from gas to liquid.
Analysis of fundamental thermodynamic laws on a fixed-mass element containing
the diffusion layers proves the thermodynamic viability of the obtained
results.Comment: Submitted for publication in International Journal of Heat and Mass
Transfer. 29 pages, 18 figure
Hyperbolic character of the angular moment equations of radiative transfer and numerical methods
We study the mathematical character of the angular moment equations of
radiative transfer in spherical symmetry and conclude that the system is
hyperbolic for general forms of the closure relation found in the literature.
Hyperbolicity and causality preservation lead to mathematical conditions
allowing to establish a useful characterization of the closure relations. We
apply numerical methods specifically designed to solve hyperbolic systems of
conservation laws (the so-called Godunov-type methods), to calculate numerical
solutions of the radiation transport equations in a static background. The
feasibility of the method in any kind of regime, from diffusion to
free-streaming, is demonstrated by a number of numerical tests and the effect
of the choice of the closure relation on the results is discussed.Comment: 37 pags, 12 figures, accepted for publication in MNRA
Legendre expansion of the neutrino-antineutrino annihilation kernel: Influence of high order terms
We calculate the Legendre expansion of the rate of the process up to 3rd order extending previous results
of other authors which only consider the 0th and 1st order terms. Using
different closure relations for the moment equations of the radiative transfer
equation we discuss the physical implications of taking into account quadratic
and cubic terms on the energy deposition outside the neutrinosphere in a
simplified model. The main conclusion is that 2nd order is necessary in the
semi-transparent region and gives good results if an appropriate closure
relation is used.Comment: 14 pages, 4 figures. To be published in A&A Supplement Serie
Background Symmetries In Orbifolds With Discrete Wilson Lines
Target space symmetries are studied for orbifold compactified string theories
containing Wilson line background fields. The symmetries determined are for
those moduli which contribute to the string loop threshold corrections of the
gauge coupling constants. The groups found are subgroups of the modular group
and depend on the choice of discrete Wilson lines and the shape of
the underlying six-dimensional lattice.Comment: 31 pages, QMW--TH--94/0
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