1,071 research outputs found
Analisis Hukum Peranan Lembaga Penjamin Simpanan Dalam Melindungi Nasabah Bank
Lembaga Penjamin Simpanan adalah lembaga yang dibentuk dengan maksud untuk meningkatkan kepercayaan nasabah terhadap industri perbankan. Lembaga Penjamin Simpanan merupakan mekanisme untuk mempermudah bank bermasalah dilikuidasi. Fungsi dari Lembaga Penjamin Simpanan ini adalah untuk mengatur kesehatan bank secara umum. Lembaga Penjamin Simpanan dibentuk berdasarkan Undang – Undang Nomor 24 Tahun 2004 tentang Lembaga Penjamin Simpanan dan telah diubah dengan Undang – Undang Nomor 7 Tahun 2009. Pembentukan Lembaga Penjamin Simpanan diharapkan dapat menjamin dana simpanan masyarakat di bank – bank. Dengan adanya Lembaga Penjamin Simpanan, maka apabila terdapat bank yang mengalami kesulitan USAha, kemudian dicabut izin USAhanya, kedudukan nasabah tetap terjamin. Adapun yang menjadi permasalahan dalam penulisan skripsi ini adalah bagaimana peran Lembaga Penjamin Simpanan ditinjau dari Undang – Undang Lembaga Penjamin Simpanan dan bagaimana upaya Lembaga Penjamin Simpanan dalam membantu menyelesaikan bank gagal. Untuk menganalisis hal tersebut dilakukan penelitian normatif yang bersifat deskriptif dengan menggunakan data sekunder berupa bahan hukum primer, sekunder dan tersier. Bersifat deskriptif maksudnya menggambarkan bagaimana keadaan – keadaan atau fakta yang terjadi di masyarakat sehingga di dapatkan data yang seakurat mungkin
Noncommutative Einstein-Maxwell pp-waves
The field equations coupling a Seiberg-Witten electromagnetic field to
noncommutative gravity, as described by a formal power series in the
noncommutativity parameters , is investigated. A large
family of solutions, up to order one in , describing
Einstein-Maxwell null pp-waves is obtained. The order-one contributions can be
viewed as providing noncommutative corrections to pp-waves. In our solutions,
noncommutativity enters the spacetime metric through a conformal factor and is
responsible for dilating/contracting the separation between points in the same
null surface. The noncommutative corrections to the electromagnetic waves,
while preserving the wave null character, include constant polarization, higher
harmonic generation and inhomogeneous susceptibility. As compared to pure
noncommutative gravity, the novelty is that nonzero corrections to the metric
already occur at order one in .Comment: 19 revtex pages. One refrence suppressed, two references added. Minor
wording changes in the abstract, introduction and conclusio
Standing gravitational waves from domain walls
We construct a plane symmetric, standing gravitational wave for a domain wall
plus a massless scalar field. The scalar field can be associated with a fluid
which has the properties of `stiff' matter, i.e. matter in which the speed of
sound equals the speed of light. Although domain walls are observationally
ruled out in the present era the solution has interesting features which might
shed light on the character of exact non-linear wave solutions to Einstein's
equations. Additionally this solution may act as a template for higher
dimensional 'brane-world' model standing waves.Comment: 4 pages two-column format, no figures, added discussion of physical
meaning of solution, added refernces, to be published PR
Comparison of CFD and DSMC Using Calibrated Transport Parameters
Hypersonic re-entry flows span a wide range of length scales where regions of both rarefied and continuum flow exist. Traditional computational fluid dynamics (CFD) techniques do not provide an accurate solution for the rarefied regions of such mixed flow fields. Although direct simulation Monte Carlo (DSMC) can be used to accurately capture both the continuum and rarefied features of mixed flow fields, they are computationally expensive when employed to simulate the low Knudsen number continuum regimes. Thus, a hybrid framework for seamlessly combining the two methodologies, CFD and DSMC, continues to be a topic of significant research effort. Ensuring consistency in the reaction kinetics and transport models employed within CFD and DSMC is a crucial requirement for obtaining a reliable solution from a hybrid framework for combined continuum/rarefied high speed flows. This paper represents one of the first studies to utilize the calibrated transport parameters developed to ensure consistency between CFD and DSMC solvers. The new variable soft sphere (VSS) parameters are compared to both previous standard variable hard sphere (VHS) parameters and also to solutions from the CFD transport properties that the new parameters were developed to reproduce
Born-Infeld-Einstein theory with matter
The field equations associated with the Born-Infeld-Einstein action including
matter are derived using a Palatini variational principle. Scalar,
electromagnetic, and Dirac fields are considered. It is shown that an action
can be chosen for the scalar field that produces field equations identical to
the usual Einstein field equations minimally coupled to a scalar field. In the
electromagnetic and Dirac cases the field equations reproduce the standard
equations only to lowest order. The spherically symmetric electrovac equations
are studied in detail. It is shown that the resulting Einstein equations
correspond to gravity coupled to a modified Born-Infeld theory. It is also
shown that point charges are not allowed. All particles must have a finite
size. Mass terms for the fields are also considered.Comment: 12 pages, LaTe
Isotropy, shear, symmetry and exact solutions for relativistic fluid spheres
The symmetry method is used to derive solutions of Einstein's equations for
fluid spheres using an isotropic metric and a velocity four vector that is
non-comoving. Initially the Lie, classical approach is used to review and
provide a connecting framework for many comoving and so shear free solutions.
This provides the basis for the derivation of the classical point symmetries
for the more general and mathematicaly less tractable description of Einstein's
equations in the non-comoving frame. Although the range of symmetries is
restrictive, existing and new symmetry solutions with non-zero shear are
derived. The range is then extended using the non-classical direct symmetry
approach of Clarkson and Kruskal and so additional new solutions with non-zero
shear are also presented. The kinematics and pressure, energy density, mass
function of these solutions are determined.Comment: To appear in Classical and Quantum Gravit
Frame dragging and super-energy
We show that the vorticity appearing in stationary vacuum spacetimes is
always related to the existence of a flow of super-energy on the plane
orthogonal to the vorticity vector. This result, toghether with the previously
established link between vorticity and super--energy in radiative (Bondi-Sachs)
spacetimes strength further the case for this latter quantity as the cause of
frame dragging.Comment: 12 pages Latex. To appear in Phys.Rev. D. Typos correcte
Gravitational wave recoil in Robinson-Trautman spacetimes
We consider the gravitational recoil due to non-reflection-symmetric
gravitational wave emission in the context of axisymmetric Robinson-Trautman
spacetimes. We show that regular initial data evolve generically into a final
configuration corresponding to a Schwarzschild black-hole moving with constant
speed. For the case of (reflection-)symmetric initial configurations, the mass
of the remnant black-hole and the total energy radiated away are completely
determined by the initial data, allowing us to obtain analytical expressions
for some recent numerical results that have been appeared in the literature.
Moreover, by using the Galerkin spectral method to analyze the non-linear
regime of the Robinson-Trautman equations, we show that the recoil velocity can
be estimated with good accuracy from some asymmetry measures (namely the first
odd moments) of the initial data. The extension for the non-axisymmetric case
and the implications of our results for realistic situations involving head-on
collision of two black holes are also discussed.Comment: 9 pages, 6 figures, final version to appear in PR
Degeneracy measures for the algebraic classification of numerical spacetimes
We study the issue of algebraic classification of the Weyl curvature tensor,
with a particular focus on numerical relativity simulations. The spacetimes of
interest in this context, binary black hole mergers, and the ringdowns that
follow them, present subtleties in that they are generically, strictly
speaking, Type I, but in many regions approximately, in some sense, Type D. To
provide meaning to any claims of "approximate" Petrov class, one must define a
measure of degeneracy on the space of null rays at a point. We will investigate
such a measure, used recently to argue that certain binary black hole merger
simulations ring down to the Kerr geometry, after hanging up for some time in
Petrov Type II. In particular, we argue that this hangup in Petrov Type II is
an artefact of the particular measure being used, and that a geometrically
better-motivated measure shows a black hole merger produced by our group
settling directly to Petrov Type D.Comment: 14 pages, 7 figures. Version 2 adds two references
Declining Unions and the Coverage Wage Gap: Can German Unions Still Cut It?
That German trade unionism is in profound decline seems to be beyond dispute. More controversial is the implied change in union impact on worker wages. A linked employer-employee dataset is deployed over an interval of continuing decline in unionism to address this issue. Over the sample period 2000–2010 it is found that joining a sectoral agreement always produces higher wages, while exiting one no longer leads to wage losses if the transition is to a firm agreement. Leaving a firm agreement to non-coverage also leads to wage reductions, while joining one from non-coverage appears decreasingly favorable. The one constant is the persistence of a small positive union wage gap
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