1,455 research outputs found
Features in the Primordial Spectrum from WMAP: A Wavelet Analysis
Precise measurements of the anisotropies in the cosmic microwave background
enable us to do an accurate study on the form of the primordial power spectrum
for a given set of cosmological parameters. In a previous paper (Shafieloo and
Souradeep 2004), we implemented an improved (error sensitive) Richardson-Lucy
deconvolution algorithm on the measured angular power spectrum from the first
year of WMAP data to determine the primordial power spectrum assuming a
concordance cosmological model. This recovered spectrum has a likelihood far
better than a scale invariant, or, `best fit' scale free spectra (\Delta ln L =
25 w.r.t. Harrison Zeldovich, and, \Delta ln L = 11 w.r.t. power law with
n_s=0.95). In this paper we use Discrete Wavelet Transform (DWT) to decompose
the local features of the recovered spectrum individually to study their effect
and significance on the recovered angular power spectrum and hence the
likelihood. We show that besides the infra-red cut off at the horizon scale,
the associated features of the primordial power spectrum around the horizon
have a significant effect on improving the likelihood. The strong features are
localised at the horizon scale.Comment: 8 pages, 4 figures, uses Revtex4, matches version accepted to Phys.
Rev. D, main results and conclusions unchanged, references adde
The Small Scale Velocity Dispersion of Galaxies: A Comparison of Cosmological Simulations
The velocity dispersion of galaxies on small scales ( Mpc),
, can be estimated from the anisotropy of the galaxy-galaxy
correlation function in redshift space. We apply this technique to
``mock-catalogs'' extracted from N-body simulations of several different
variants of Cold Dark Matter dominated cosmological models to obtain results
which may be consistently compared to similar results from observations. We
find a large variation in the value of in different
regions of the same simulation. We conclude that this statistic should not be
considered to conclusively rule out any of the cosmological models we have
studied. We attempt to make the statistic more robust by removing clusters from
the simulations using an automated cluster-removing routine, but this appears
to reduce the discriminatory power of the statistic. However, studying
as clusters with different internal velocity dispersions are
removed leads to interesting information about the amount of power on cluster
and subcluster scales. We also compute the pairwise velocity dispersion
directly and compare this to the values obtained using the Davis-Peebles
method, and find that the agreement is fairly good. We evaluate the models used
for the mean streaming velocity and the pairwise peculiar velocity distribution
in the original Davis-Peebles method by comparing the models with the results
from the simulations.Comment: 20 pages, uuencoded (Latex file + 8 Postscript figures), uses AAS
macro
Meeting the Goals of Service Learning in Pharmacy Education through Community Campus Partnerships
Healthy People 2010, published by the US Department of Health and Human Services, is a statement of health objectives for the nation to be achieved by the end of this decade. The goals are to increase quality and years of healthy life and to eliminate health disparities. In 2006, the West Virginia University School of Pharmacy began a revision to its Doctor of Pharmacy curriculum to include pharmacy practice experiences that would provide students with experience in developing disease prevention and health promotion programming in the community. Thus, the School of Pharmacy began a three-semester longitudinal service learning program which focused on advancing the objectives of Healthy People 2010 through service learning. The experiences of the School of Pharmacy service learning program from 2006 to the present are detailed
Large Scale Fluctuations in the X-Ray Background
We present an attempt to measure the large angular scale fluctuations in the
X-Ray Background (XRB) from the HEAO1-A2 data, expressed in terms of spherical
harmonics. We model the harmonic coefficients assuming a power spectrum and an
epoch-dependent bias parameter, and using a phenomenological scenario
describing the evolution of the X-ray sources. From the few low-order
multipoles detected above shot noise, we estimate the power-spectrum
normalization on scales intermediate between those explored by local galaxy
redshift surveys (~ 100 Mpc) and by the COBE Microwave Background measurements
(~ 1000 Mpc). We find that the HEAO1 harmonics are consistent with present
epoch rms fluctuations of the X-ray sources bx(0)sigma8 ~ 1-2 in 8 Mpc spheres.
Therefore the observed fluctuations in the XRB are roughly as expected from
interpolating between the local galaxy surveys and the COBE CMB experiment. We
predict that an X-ray all-sky surface brightness survey resolving sources a
factor of 10 fainter than HEAO1, may reveal fluctuations to significantly
larger angular scales and therefore more strongly constrain the large scale
structure of the Universe on scales of hundreds of Mpcs.Comment: 14 pages, 3 Postscript figures, uses aaspp4.sty and psfig. Revised
following referee's report. Accepted for publication in Ap
Percolation Analysis of a Wiener Reconstruction of the IRAS 1.2 Jy Redshift Catalog
We present percolation analyses of Wiener Reconstructions of the IRAS 1.2 Jy
Redshift Survey. There are ten reconstructions of galaxy density fields in real
space spanning the range to , where
, is the present dimensionless density and
is the bias factor. Our method uses the growth of the largest cluster
statistic to characterize the topology of a density field, where Gaussian
randomized versions of the reconstructions are used as standards for analysis.
For the reconstruction volume of radius, Mpc,
percolation analysis reveals a slight `meatball' topology for the real space,
galaxy distribution of the IRAS survey.
cosmology-galaxies:clustering-methods:numericalComment: Revised version accepted for publication in The Astrophysical
Journal, January 10, 1997 issue, Vol.47
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