2,355 research outputs found
Dp-branes, NS5-branes and U-duality from nonabelian (2,0) theory with Lie 3-algebra
We derive the super Yang-Mills action of Dp-branes on a torus T^{p-4} from
the nonabelian (2,0) theory with Lie 3-algebra. Our realization is based on Lie
3-algebra with pairs of Lorentzian metric generators. The resultant theory then
has negative norm modes, but it results in a unitary theory by setting VEV's of
these modes. This procedure corresponds to the torus compactification,
therefore by taking a transformation which is equivalent to T-duality, the
Dp-brane action is obtained. We also study type IIA/IIB NS5-brane and
Kaluza-Klein monopole systems by taking other VEV assignments. Such various
compactifications can be realized in the nonabelian (2,0) theory, since both
longitudinal and transverse directions can be compactified, which is different
from the BLG theory. We finally discuss U-duality among these branes, and show
that most of the moduli parameters in U-duality group are recovered. Especially
in D5-brane case, the whole U-duality relation is properly reproduced.Comment: 1+26 page
High-growth-rate magnetohydrodynamic instability in differentially rotating compressible flow
The transport of angular momentum in the outward direction is the fundamental
requirement for accretion to proceed in an accretion disc. This objective can
be achieved if the accretion flow is turbulent. Instabilities are one of the
sources for the turbulence. We study a differentially rotating compressive flow
in the presence of non vanishing radial and azimuthal magnetic field and
demonstrate the occurrence of a high growth rate instability. This instability
operates in a region where magnetic energy density exceeds the rotational
energy density
Nuclear Shell Model by the Quantum Monte Carlo Diagonalization Method
The feasibility of shell-model calculations is radically extended by the
Quantum Monte Carlo Diagonalization method with various essential improvements.
The major improvements are made in the sampling for the generation of
shell-model basis vectors, and in the restoration of symmetries such as angular
momentum and isospin. Consequently the level structure of low-lying states can
be studied with realistic interactions. After testing this method on Mg,
we present first results for energy levels and properties of Ge,
indicating its large and -soft deformation.Comment: 12 pages, RevTex, 2 figures, to be published in Physical Review
Letter
A Trigonometric Parallax of Sgr B2
We have measured the positions of water masers in Sgr B2, a massive star
forming region in the Galactic center, relative to an extragalactic radio
source with the Very Long Baseline Array. The positions measured at 12 epochs
over a time span of one year yield the trigonometric parallax of Sgr B2 and
hence a distance to the Galactic center of Ro=7.9 (+0.8/-0.7) kpc. The proper
motion of Sgr B2 relative to Sgr A* suggests that Sgr B2 is about 0.13 kpc
nearer than the Galactic center, assuming a low-eccentricity Galactic orbit.Comment: Submitted to ApJ; 4 tables; 3 figures. Version 2 corrects Fig. 2
which was missing some dat
Limits on the Position Wander of Sgr A*
We present measurements with the VLBA of the variability in the centroid
position of Sgr A* relative to a background quasar at 7-mm wavelength. We find
an average centroid wander of 71 +/- 45 micro-arcsec for time scales between 50
and 100 min and 113 +/- 50 micro-arcsec for timescales between 100 and 200 min,
with no secular trend. These are sufficient to begin constraining the viability
of the hot-spot model for the radio variability of Sgr A*. It is possible to
rule out hot spots with orbital radii above 15GM_SgrA*/c^2 that contribute more
than 30% of the total 7-mm flux. However, closer or less luminous hot spots
remain unconstrained. Since the fractional variability of Sgr A* during our
observations was ~20% on time scales of hours, the hot-spot model for Sgr A*'s
radio variability remains consistent with these limits. Improved monitoring of
Sgr A*'s centroid position has the potential to place significant constraints
upon the existence and morphology of inhomogeneities in a supermassive black
hole accretion flow.Comment: 14 pages, 3 figures submitted to Ap
Rotation Curves of Galaxies by Fourth Order Gravity
We investigate the radial behavior of galactic rotation curves by a Fourth
Order Gravity adding also the Dark Matter component. The Fourth Order Gravity
is a Lagrangian containing the Ricci scalar, the Ricci and Riemann tensor, but
the rotation curves are depending only on two free parameters. A systematic
analysis of rotation curves, in the Newtonian Limit of theory, induced by all
galactic sub-structures of ordinary matter is shown. This analysis is presented
for Fourth Order Gravity with and without Dark Matter. The outcomes are
compared with respect to classical outcomes of General Relativity. The
gravitational potential of point-like mass is the usual potential corrected by
two Yukawa terms. The rotation curve is higher or also lower than curve of
General Relativity if in the Lagrangian the Ricci scalar square is dominant or
not with respect to the contribution of the Ricci tensor square. The curves are
compared with the experimental data for the Milky Way and the galaxy NGC 3198.
Although the Fourth Order Gravity gives more rotational contributions, in the
limit of large distances the Keplerian behavior is present, and it is missing
if we add a Dark Matter component. By modifying the theory of Gravitation
consequently also the spatial description of Dark Matter could undergo a
modification. At last we compare the gravitational potential by Fourth Order
Gravity with respect to more used potential induced by power law of Ricci
scalar.Comment: 14 pages, 10 figure
Description of superdeformed nuclei in the interacting boson model
The interacting boson model is extended to describe the spectroscopy of
superdeformed bands. Microscopic structure of the model in the second minimum
is discussed and superdeformed bosons are introduced as the new building
blocks. Solutions of a quadrupole Hamiltonian are implemented through the
expansion method. Effects of the quadrupole parameters on dynamic moment of
inertia and electric quadrupole transition rates are discussed and the results
are used in a description of superdeformed bands in the Hg-Pb and Gd-Dy
regions.Comment: 18 pages revtex, 9 figures available upon reques
A New Approach to Large-Scale Nuclear Structure Calculations
A new approach to large-scale nuclear structure calculations, based on the
Density Matrix Renormalization Group (DMRG), is described. The method is tested
in the context of a problem involving many identical nucleons constrained to
move in a single large-j shell and interacting via a pairing plus quadrupole
interaction. In cases in which exact diagonalization of the hamiltonian is
possible, the method is able to reproduce the exact results for the ground
state energy and the energies of low-lying excited states with extreme
precision. Results are also presented for a model problem in which exact
solution is not feasible.Comment: 6 pages + 1 eps figur
Improved VLBI astrometry of OH maser stars
Aims: Accurate distances to evolved stars with high mass loss rates are
needed for studies of many of their fundamental properties. However, as these
stars are heavily obscured and variable, optical and infrared astrometry is
unable to provide enough accuracy.
Methods: Astrometry using masers in the circumstellar envelopes can be used
to overcome this problem. We have observed the OH masers of a number of
Asymptotic Giant Branch (AGB) stars for approximately 1 year with the Very Long
Baseline Array (VLBA). We have used the technique of phase referencing with
in-beam calibrators to test the improvements this technique can provide to Very
Long Baseline Interferometry (VLBI) OH maser astrometric observations.
Results: We have significantly improved the parallax and proper motion
measurements of the Mira variable stars U Her, S CrB and RR Aql.
Conclusions: It is shown that both in-beam phase-referencing and a decrease
in solar activity during the observations significantly improves the accuracy
of the astrometric observations. The improved distances to S CrB (418 +21 -18
pc) and RR Aql (633 +214 -128 pc) are fully consistent with published P-L
relations, but the distance to U Her (266 +32 -28 pc) is significantly smaller.
We conclude that for sources that are bright and have a nearby in-beam
calibrator, VLBI OH maser astrometry can be used to determine distances to OH
masing stars of up to ~2 kpc.Comment: 15 pages, 10 figures; accepted for publication in A&A; for a version
with high-resolution figures see
http://www.astro.uni-bonn.de/~wouter/papers/astrom/astrom.shtm
Intrinsic electronic superconducting phases at 60 K and 90 K in double-layer YBaCuO
We study superconducting transition temperature () of oxygen-doped
double-layer high-temperature superconductors YBaCuO (0
1) as a function of the oxygen dopant concentration
() and planar hole-doping concentration (). We find that ,
while clearly influenced by the development of the chain ordering as seen in
the plot, lies on a universal curve originating at the
critical hole concentration () = 1/16 in the plot.
Our analysis suggests that the universal behavior of () can be
understood in terms of the competition and collaboration of chemical-phases and
electronic-phases that exist in the system. We conclude that the global
superconductivity behavior of YBaCuO as a function of
doping is electronically driven and dictated by pristine electronic phases at
magic doping numbers that follow the hierarchical order based on , such as
2 , 3 and 4 . We find that there are
at least two intrinsic electronic superconducting phases of = 60 K at 2
= 1/8 and = 90 K at 3 = 3/16.Comment: 4 pages, 2 figure
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