101 research outputs found
B-mode Detection with an Extended Planck Mission
The Planck satellite has a nominal mission lifetime of 14 months allowing two
complete surveys of the sky. Here we investigate the potential of an extended
Planck mission of four sky surveys to constrain primordial B-mode anisotropies
in the presence of dominant Galactic polarized foreground emission. An extended
Planck mission is capable of powerful constraints on primordial B-modes at low
multipoles, which cannot be probed by ground based or sub-orbital experiments.
A tensor-scalar ratio of r=0.05 can be detected at a high significance level by
an extended Planck mission and it should be possible to set a 95% upper limit
on r of 0.03 if the tensor-scalar ratio is vanishingly small. Furthermore,
extending the Planck mission to four sky surveys offers better control of
polarized Galactic dust emission, since the 217 GHz frequency band can be used
as an effective dust template in addition to the 353 GHz channel.Comment: 10 pages, 3 figure
Measuring CMB Polarization with BOOMERANG
BOOMERANG is a balloon-borne telescope designed for long duration (LDB)
flights around Antarctica. The second LDB Flight of BOOMERANG took place in
January 2003. The primary goal of this flight was to measure the polarization
of the CMB. The receiver uses polarization sensitive bolometers at 145 GHz.
Polarizing grids provide polarization sensitivity at 245 and 345 GHz. We
describe the BOOMERANG telescope noting changes made for 2003 LDB flight, and
discuss some of the issues involved in the measurement of polarization with
bolometers. Lastly, we report on the 2003 flight and provide an estimate of the
expected results.Comment: 12 pages, 8 figures, To be published in the proceedings of "The
Cosmic Microwave Background and its Polarization", New Astronomy Reviews,
(eds. S. Hanany and K.A. Olive). Fixed typos, and reformatted citation
A Constraint on Planck-scale Modifications to Electrodynamics with CMB polarization data
We show that the Cosmic Microwave Background (CMB) polarization data gathered
by the BOOMERanG 2003 flight and WMAP provide an opportunity to investigate
{\it in-vacuo} birefringence, of a type expected in some quantum pictures of
space-time, with a sensitivity that extends even beyond the desired
Planck-scale energy. In order to render this constraint more transparent we
rely on a well studied phenomenological model of quantum-gravity-induced
birefringence, in which one easily establishes that effects introduced at the
Planck scale would amount to values of a dimensionless parameter, denoted by
, with respect to the Planck energy which are roughly of order 1. By
combining BOOMERanG and WMAP data we estimate at
the 68% c.l. Moreover, we forecast on the sensitivity to achievable by
future CMB polarization experiments (PLANCK, Spider, EPIC), which, in the
absence of systematics, will be at the 1- confidence of (PLANCK), (Spider), and
(EPIC) respectively. The cosmic variance-limited sensitivity from CMB is
.Comment: 16 page
SPIDER: Probing the Early Universe with a Suborbital Polarimeter
We evaluate the ability of SPIDER, a balloon-borne polarimeter, to detect a
divergence-free polarization pattern ("B-modes") in the Cosmic Microwave
Background (CMB). In the inflationary scenario, the amplitude of this signal is
proportional to that of the primordial scalar perturbations through the
tensor-to-scalar ratio r. We show that the expected level of systematic error
in the SPIDER instrument is significantly below the amplitude of an interesting
cosmological signal with r=0.03. We present a scanning strategy that enables us
to minimize uncertainty in the reconstruction of the Stokes parameters used to
characterize the CMB, while accessing a relatively wide range of angular
scales. Evaluating the amplitude of the polarized Galactic emission in the
SPIDER field, we conclude that the polarized emission from interstellar dust is
as bright or brighter than the cosmological signal at all SPIDER frequencies
(90 GHz, 150 GHz, and 280 GHz), a situation similar to that found in the
"Southern Hole." We show that two ~20-day flights of the SPIDER instrument can
constrain the amplitude of the B-mode signal to r<0.03 (99% CL) even when
foreground contamination is taken into account. In the absence of foregrounds,
the same limit can be reached after one 20-day flight.Comment: 29 pages, 8 figures, 4 tables; v2: matches published version, flight
schedule updated, two typos fixed in Table 2, references and minor
clarifications added, results unchange
Inflation Physics from the Cosmic Microwave Background and Large Scale Structure
Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the nature of the earliest moments of time. The next generation of CMB and large-scale structure (LSS) experiments are poised to test the leading paradigm for these earliest moments---the theory of cosmic inflation---and to detect the imprints of the inflationary epoch, thereby dramatically increasing our understanding of fundamental physics and the early universe. A future CMB experiment with sufficient angular resolution and frequency coverage that surveys at least 1 of the sky to a depth of 1 uK-arcmin can deliver a constraint on the tensor-to-scalar ratio that will either result in a 5-sigma measurement of the energy scale of inflation or rule out all large-field inflation models, even in the presence of foregrounds and the gravitational lensing B-mode signal. LSS experiments, particularly spectroscopic surveys such as the Dark Energy Spectroscopic Instrument, will complement the CMB effort by improving current constraints on running of the spectral index by up to a factor of four, improving constraints on curvature by a factor of ten, and providing non-Gaussianity constraints that are competitive with the current CMB bounds
Planck intermediate results. VIII. Filaments between interacting clusters
About half of the baryons of the Universe are expected to be in the form of
filaments of hot and low density intergalactic medium. Most of these baryons
remain undetected even by the most advanced X-ray observatories which are
limited in sensitivity to the diffuse low density medium. The Planck satellite
has provided hundreds of detections of the hot gas in clusters of galaxies via
the thermal Sunyaev-Zel'dovich (tSZ) effect and is an ideal instrument for
studying extended low density media through the tSZ effect. In this paper we
use the Planck data to search for signatures of a fraction of these missing
baryons between pairs of galaxy clusters. Cluster pairs are good candidates for
searching for the hotter and denser phase of the intergalactic medium (which is
more easily observed through the SZ effect). Using an X-ray catalogue of
clusters and the Planck data, we select physical pairs of clusters as
candidates. Using the Planck data we construct a local map of the tSZ effect
centered on each pair of galaxy clusters. ROSAT data is used to construct X-ray
maps of these pairs. After having modelled and subtracted the tSZ effect and
X-ray emission for each cluster in the pair we study the residuals on both the
SZ and X-ray maps. For the merging cluster pair A399-A401 we observe a
significant tSZ effect signal in the intercluster region beyond the virial
radii of the clusters. A joint X-ray SZ analysis allows us to constrain the
temperature and density of this intercluster medium. We obtain a temperature of
kT = 7.1 +- 0.9, keV (consistent with previous estimates) and a baryon density
of (3.7 +- 0.2)x10^-4, cm^-3. The Planck satellite mission has provided the
first SZ detection of the hot and diffuse intercluster gas.Comment: Accepted by A&
Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest all-sky catalogue of galaxy clusters. It contains 1653 detections, of which 1203 are confirmed clusters with identified counterparts in external data-sets, and is the first SZ-selected cluster survey containing > confirmed clusters. We present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, we find that the Y5R500 estimates are robust to pressure-profile variation and beam systematics, but accurate conversion to Y500 requires. the use of prior information on the cluster extent. We describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infra-red, optical and X-ray data-sets, and which places emphasis on the robustness of the counterpart match. We discuss the physical properties of the new sample and identify a population of low-redshift X-ray under- luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but are almost absent from ROSAT X-ray selected samples
The BOOMERanG experiment and the curvature of the Universe
We describe the BOOMERanG experiment and its main result, i.e. the
measurement of the large scale curvature of the Universe. BOOMERanG is a
balloon-borne microwave telescope with sensitive cryogenic detectors. BOOMERanG
has measured the angular distribution of the Cosmic Microwave Background on
of the sky, with a resolution of arcmin and a sensitivity
of per pixel. The resulting image is dominated by hot and cold
spots with rms fluctuations and typical size of . The
detailed angular power spectrum of the image features three peaks and two dips
at and , respectively. Such very characteristic
spectrum can be explained assuming that the detected structures are the result
of acoustic oscillations in the primeval plasma. In this framework, the
measured pattern constrains the density parameter to be (95% confidence interval). Other cosmological parameters, like the
spectral index of initial density fluctuations, the density parameter for
baryons, dark matter and dark energy, are detected or constrained by the
BOOMERanG measurements and by other recent CMB anisotropy experiments. When
combined with other cosmological observations, these results depict a new,
consistent, cosmological scenario.Comment: Proc. of the Erice School on "Neutrinos in Astro, Particle and
Nuclear Physics", 18.-26. September 2001, Amand Faessler, Jan Kuckei eds,
"Progress in Particle and Nuclear Physics", vol. 4
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