7,362 research outputs found
Inhomogeneous reionization and the polarization of the cosmic microwave background
In a universe with inhomogeneous reionization, the ionized patches create a
second order signal in the cosmic microwave background polarization anisotropy.
This signal originates in the coupling of the free electron fluctuation to the
quadruple moment of the temperature anisotropy. We examine the contribution
from a simple inhomogeneous reionization model and find that the signal from
such a process is below the detectable limits of the Planck Surveyor mission.
However t he signal is above the fundamental uncertainty limit from cosmic
variance, so th at a future detection with a high accuracy experiment on
sub-arcminute scales is possible.Comment: 10 pages, 2 eps figures, final version accepted for publication in
ApJ Letter
EUV and X-ray spectroheliograph study
The results of a program directed toward the definition of an EUV and X-ray spectroheliograph which has significant performance and operational improvements over the OSO-7 instrument are documented. The program investigated methods of implementing selected changes and incorporated the results of the study into a set of drawings which defines the new instrument. The EUV detector performance degradation observed during the OSO-7 mission was investigated and the most probable cause of the degradation identified
Long range Kelvin wave propagation of transport variations in Pacific Ocean equatorial currents
Two 100 km scale arrays of moored upper ocean current meters, one near 0, 152W, the other near 0, 110W, were used to study the zonal transport of the strong equatorial currents in and above the thermocline. At long periods (several days), fluctuations· in the vertically integrated zonal velocity (transport per unit meridional distance) at a single equatorial mooring were highly correlated with fluctuations in the total transport across the section 0-250 m and 1N-1S, which includes most of the Equatorial Undercurrent...
Variational discrete variable representation for excitons on a lattice
We construct numerical basis function sets on a lattice, whose spatial
extension is scalable from single lattice sites to the continuum limit. They
allow us to compute small and large bound states with comparable, moderate
effort. Adopting concepts of discrete variable representations, a diagonal form
of the potential term is achieved through a unitary transformation to Gaussian
quadrature points. Thereby the computational effort in three dimensions scales
as the fourth instead of the sixth power of the number of basis functions along
each axis, such that it is reduced by two orders of magnitude in realistic
examples. As an improvement over standard discrete variable representations,
our construction preserves the variational principle. It allows for the
calculation of binding energies, wave functions, and excitation spectra. We use
this technique to study central-cell corrections for excitons beyond the
continuum approximation. A discussion of the mass and spectrum of the yellow
exciton series in the cuprous oxide, which does not follow the hydrogenic
Rydberg series of Mott-Wannier excitons, is given on the basis of a simple
lattice model.Comment: 12 pages, 7 figures. Final version as publishe
Cosmic Microwave Background Anisotropy Window Functions Revisited
The primary results of most observations of cosmic microwave background (CMB)
anisotropy are estimates of the angular power spectrum averaged through some
broad band, called band-powers. These estimates are in turn what are used to
produce constraints on cosmological parameters due to all CMB observations.
Essential to this estimation of cosmological parameters is the calculation of
the expected band-power for a given experiment, given a theoretical power
spectrum. Here we derive the "band power" window function which should be used
for this calculation, and point out that it is not equivalent to the window
function used to calculate the variance. This important distinction has been
absent from much of the literature: the variance window function is often used
as the band-power window function. We discuss the validity of this assumed
equivalence, the role of window functions for experiments that constrain the
power in {\it multiple} bands, and summarize a prescription for reporting
experimental results. The analysis methods detailed here are applied in a
companion paper to three years of data from the Medium Scale Anisotropy
Measurement.Comment: 5 pages, 1 included .eps figure, PRD in press---final published
versio
Additions and intramolecular migrations of nucleophiles in cationic diruthenium µ-allenyl complexes
Hydride and halide anions readily replace the acetonitrile ligand in the diruthenium μ-allenyl complex 3b. The hydride can successively migrate to the Cα carbon of the allenyl moiety, and then to Cβ, affording 9 as the most stable product. The μ-vinyl-chlorocarbene adduct 10 is believed to be formed from 4b by chloride migration to Cα and hydrogen migration from Cα to Cβ
Probing the equation of state of the early universe with a space laser interferometer
We propose a method to probe the equation of state of the early universe and
its evolution, using the stochastic gravitational wave background from
inflation. A small deviation from purely radiation dominated universe () would be clearly imprinted on the gravitational wave spectrum
due to the nearly scale invariant nature of inflationary
generated waves.Comment: 10 pages, 1 figur
Spectro-microscopy of single and multi-layer graphene supported by a weakly interacting substrate
We report measurements of the electronic structure and surface morphology of
exfoliated graphene on an insulating substrate using angle-resolved
photoemission and low energy electron diffraction. Our results show that
although exfoliated graphene is microscopically corrugated, the valence band
retains a massless fermionic dispersion, with a Fermi velocity of ~10^6 m/s. We
observe a close relationship between the morphology and electronic structure,
which suggests that controlling the interaction between graphene and the
supporting substrate is essential for graphene device applications.Comment: 10 pages of text, 4 JPEG figure
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