150 research outputs found
The CMB Derivatives of Planck's Beam Asymmetry
We investigate the anisotropy in cosmic microwave background Planck maps due
to the coupling between its beam asymmetry and uneven scanning strategy.
Introducing a pixel space estimator based on the temperature gradients, we find
a highly significant (~20 \sigma) preference for these to point along ecliptic
latitudes. We examine the scale dependence, morphology and foreground
sensitivity of this anisotropy, as well as the capability of detailed Planck
simulations to reproduce the effect, which is crucial for its removal, as we
demonstrate in a search for the weak lensing signature of cosmic defects.Comment: 5 pages, 9 figures Published in MNRA
Studying the Peculiar Velocity Bulk Flow in a Sparse Survey of Type-Ia SNe
Studies of the peculiar velocity bulk flow based on different tools and
datasets have been consistent so far in their estimation of the direction of
the flow, which also happens to lie in close proximity to several features
identified in the cosmic microwave background, providing motivation to use new
compilations of type-Ia supernovae measurements to pinpoint it with better
accuracy and up to higher redshift. Unfortunately, the peculiar velocity field
estimated from the most recent Union2.1 compilation suffers from large
individual errors, poor sky coverage and low redshift-volume density. We show
that as a result, any naive attempt to calculate the best-fit bulk flow and its
significance will be severely biased. Instead, we introduce an iterative method
which calculates the amplitude and the scatter of the direction of the best-fit
bulk flow as deviants are successively removed and take into account the
sparsity of the data when estimating the significance of the result. Using 200
supernovae up to a redshift of z=0.2, we find that while the amplitude of the
bulk flow is marginally consistent with the value expected in a LCDM universe
given the large bias, the scatter of the direction is significantly low (at >=
99.5 C.L.) when compared to random simulations, supporting the quest for a
cosmological origin.Comment: 7 pages, 6 figures; typos fixed; clarifications made; important
references adde
Henri Temianka Correspondence; (rathaus)
https://digitalcommons.chapman.edu/temianka_correspondence/2684/thumbnail.jp
Disputa teologica in un mondo alla rovescia: il dramma su Abramo di Moshè Zacuto
Theological controversy in a reversed world; Moshe Zacuto's drama on Abraham.The foundation of the world (Yessod 'Olam) is believed to be the first Biblical drama written in Hebrew. It was composed in the first half of the 17th century by the mystical and rabbinical author Moshe Zacuto, who immigrated to Italy from Amsterdam. In fact the work is mostly based on rabbinic legends about Abraham and his struggle against idolatry, and includes many theological debates between the patriarch and King Nimrod, the pagan tyrant who condemns him to be burnt for his ideas. This paper deals with the ideological background of the drama and the peculiar and paradoxical atmosphere created by the theological debates. As asserted by several scholars (Berliner, Schirmann. Levy), Zacuto, who was born in a refugees family of Marrano origin, alluded in his play to the persecutions of the Jews by the Inquisition in Spain and Portugal. On the other hand, it seems that the play also alludes to 17th Century materialistic philosophy and hedonism, symbolized by the words of Nimrod and his sages. At any rate, the struggle between Abraham and Nimrod takes place in a highly absurd ideological frame, in which right and wrong are meaningless concepts and true faith is considered as a sort of moral perversion: a reversed world. The paper underlines this hidden and ironic aspect of the play and discusses it, on the basis of some classic works on Carnival reversion, like Cocchiara's Il mondo alla rovescia and Bakhtin' s Rabelais and his world
How Sensitive is the CMB to a Single Lens?
We study the imprints of a single lens, that breaks statistical isotropy, on
the CMB and calculate the signal to noise ratio (S/N) for its detection. We
emphasize the role of non-Gaussianities induced by LCDM weak lensing in this
calculation and show that typically the S/N is much smaller than expected. In
particular we find that the hypothesis that a void (texture) is responsible for
the WMAP cold spot can barely (cannot) be tested via weak lensing of the CMB.Comment: Accepted for publication in JCAP, 24 pages, 5 figure
CMB Imprints of a Pre-Inflationary Climbing Phase
We discuss the implications for cosmic microwave background (CMB)
observables, of a class of pre-inflationary dynamics suggested by string models
where SUSY is broken due to the presence of D-branes and orientifolds
preserving incompatible portions of it. In these models the would-be inflaton
is forced to emerge from the initial singularity climbing up a mild exponential
potential, until it bounces against a steep exponential potential of "brane
SUSY breaking" scenarios, and as a result the ensuing descent gives rise to an
inflationary epoch that begins when the system is still well off its eventual
attractor. If a pre-inflationary climbing phase of this type had occurred
within 6-7 e-folds of the horizon exit for the largest observable wavelengths,
displacement off the attractor and initial-state effects would conspire to
suppress power in the primordial scalar spectrum, enhancing it in the tensor
spectrum and typically superposing oscillations on both. We investigate these
imprints on CMB observables over a range of parameters, examine their
statistical significance, and provide a semi-analytic rationale for our
results. It is tempting to ascribe at least part of the large-angle anomalies
in the CMB to pre-inflationary dynamics of this type.Comment: 38 pages, LaTeX, 11 eps figures, references added, matches version to
appear in JCA
Gas Accretion and Galactic Chemical Evolution: Theory and Observations
This chapter reviews how galactic inflows influence galaxy metallicity. The
goal is to discuss predictions from theoretical models, but particular emphasis
is placed on the insights that result from using models to interpret
observations. Even as the classical G-dwarf problem endures in the latest round
of observational confirmation, a rich and tantalizing new phenomenology of
relationships between , , SFR, and gas fraction is emerging both in
observations and in theoretical models. A consensus interpretation is emerging
in which star-forming galaxies do most of their growing in a quiescent way that
balances gas inflows and gas processing, and metal dilution with enrichment.
Models that explicitly invoke this idea via equilibrium conditions can be used
to infer inflow rates from observations, while models that do not assume
equilibrium growth tend to recover it self-consistently. Mergers are an overall
subdominant mechanism for delivering fresh gas to galaxies, but they trigger
radial flows of previously-accreted gas that flatten radial gas-phase
metallicity gradients and temporarily suppress central metallicities. Radial
gradients are generically expected to be steep at early times and then
flattened by mergers and enriched inflows of recycled gas at late times.
However, further theoretical work is required in order to understand how to
interpret observations. Likewise, more observational work is needed in order to
understand how metallicity gradients evolve to high redshifts.Comment: Invited review to appear in Gas Accretion onto Galaxies, Astrophysics
and Space Science Library, eds. A. J. Fox & R. Dav\'e, to be published by
Springer. 29 pages, 2 figure
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