Analyzing the Cosmic Variance Limit of Remote Dipole Measurements of the Cosmic Microwave Background Using the Large-Scale Kinetic Sunyaev Zel’Dovich Effect
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Probing the Dark Flow Signal in WMAP 9Yr and PLANCK CMB Maps
Probing the Dark Flow signal in WMAP 9yr and PLANCK CMB Maps. Fernando Atrio-Barandela. Departamento de F´ısica Fundamental. Universidad de Salamanca. eml: [email protected] In collaboration with: H. Ebeling, D. Fixsen, A. Kashlinsky, D. Kocevski. Ibericos 2015 Aranjuez, March 30th - April 1st, 2015. 1 Summary. Introduction: The CMB dipole. Measuring Peculiar Velocities. Results with WMAP. Results with PLANCK (Planck Collaboration). Results with PLANCK (Our Analysis). Cosmological Implications and Conclusions. Ibericos 2015 Aranjuez, March 30th - April 1st, 2015. 2 Introduction: The CMB dipole. Ibericos 2015 Aranjuez, March 30th - April 1st, 2015. 3 The Cosmic Microwave Background. Monopole T=2.73K Dipole T=3mK Octupole O=33 K Planck Nominal Map at 353GHz Ibericos 2015 Aranjuez, March 30th - April 1st, 2015. 4 The CMB dipole. If density perturbations are adiabatic, generated during inflation, then the low order • multipoles verify: ℓ(ℓ + 1)C = const 2C = 12C = 12 1000(µK)2 D 70µ 1mK ℓ ⇒ 1 3 ∗ ⇒ ∼ ≪ Then, the dipole CAN NOT BE PRIMORDIAL. It is a Doppler effect due to the local motion of the Local Group with velocity 600km/s in the direction of l = 2700, b = 300. ∼ Ibericos 2015 Aranjuez, March 30th - April 1st, 2015. 5 The convergence of the CMB dipole. COMA VIRGO CENTAURUS HYDRA PERSEUS (Left) CMB dipole measured by COBE. (Right) Large Scale Structure and gas distribution in the Local Universe. What are the scales that contribute to the 600km/s peculiar velocity of the LG? ∼ Ibericos 2015 Aranjuez, March 30th - April 1st, 2015. 6 Bulk Flows. The zero order moment of the velocity field is the mean peculiar velocity of a sphere of radius R or bulk flow 1 V 2(R) = P (k)W 2(kR)dk P (k) = δ(k) 2. -
The Silk Damping Tail of the CMB
The Silk Damping Tail of the CMB 100 K) µ ( T ∆ 10 10 100 1000 l Wayne Hu Oxford, December 2002 Outline • Damping tail of temperature power spectrum and its use as a standard ruler • Generation of polarization through damping • Unveiling of gravitational lensing from features in the damping tail Outline • Damping tail of temperature power spectrum and its use as a standard ruler • Generation of polarization through damping • Unveiling of gravitational lensing from features in the damping tail • Collaborators: Matt Hedman Takemi Okamoto Joe Silk Martin White Matias Zaldarriaga Outline • Damping tail of temperature power spectrum and its use as a standard ruler • Generation of polarization through damping • Unveiling of gravitational lensing from features in the damping tail • Collaborators: Matt Hedman Takemi Okamoto Joe Silk Microsoft Martin White Matias Zaldarriaga http://background.uchicago.edu ("Presentations" in PDF) Damping Tail Photon-Baryon Plasma • Before z~1000 when the CMB had T>3000K, hydrogen ionized • Free electrons act as "glue" between photons and baryons by Compton scattering and Coulomb interactions • Nearly perfect fluid Anisotropy Power Spectrum Damping • Perfect fluid: no anisotropic stresses due to scattering isotropization; baryons and photons move as single fluid Damping • Perfect fluid: no anisotropic stresses due to scattering isotropization; baryons and photons move as single fluid • Fluid imperfections are related to the mean free path of the photons in the baryons −1 λC = τ˙ where τ˙ = neσT a istheconformalopacitytoThomsonscattering -
The Triple-Quasar Is an Optical Image of Milkyway, Andromeda and Triangulum Galaxies – Implies Expansion in the Direction of Dark Flow
The Triple-quasar is an optical image of Milkyway, Andromeda and Triangulum galaxies – implies expansion in the direction of Dark Flow Jose P Koshy [email protected] Abstract: Based on the concept that light follows a circular path of radius 2.5 billion light-years, here I show that the triple-quasar LBQS 1429-008 is the 10.5 billion years old image of 'Milkyway, Andromeda and Triangulum' galaxies. From this, the position of our galaxy at two different times can be ascertained, and the direction of expansion of the universe can be estimated. The 'surprise finding' is that the direction thus obtained is in agreement with the direction of so- called 'Dark flow', implying the possibility that the expansion is due to actual motion of bodies, and hence LCDM model is wrong. 1. Introduction: The standard cosmological model (LCDM) visualizes metric expansion of the universe. In such a model, the motion of galaxy clusters with respect to the cosmic microwave background should be randomly distributed in all directions. However, using WMAP data, Alexander Kashlinsky1 et al have found evidence for a possible non-random component in the motion of galaxy clusters; this is referred to as 'dark flow'. This implies the possibility that expansion is due to actual 'physical motion' of bodies. An alternate model, explained in my previous papers, visualizes expansion as a consequence of 'actual motion' of galaxy-clusters. Also, the model visualizes that light follows a 'circular path', and so the returning rays can create past images of bodies that have moved out. So, based on that model, it becomes possible to ascertain 'the direction' in which the universe in our region expands. -
Astrophysics Notre Dame’S Partnership in the Large Binocular Telescope
NOTRE DAME ASTROPHYSICS NOTRE DAME’S PARTNERSHIP IN THE LARGE BINOCULAR TELESCOPE The Large Binocular Telescope (LBT) stands on carbon and oxygen are created, and the LBT will Mt. Graham in Arizona, at 10,700 feet above sea support our quest for understanding. level, and next to the 1.8-m Vatican Advanced Technology Telescope. The unique facility is Telescopes not only look at distant objects, actually two 8.4-m telescopes that act in tandem but also act as time machines. Because light to produce images unlike any seen before. The may travel for billions of years before being LBT has the equivalent collecting power of a captured by the LBT’s mirrors, the images 12-m and the resolution of a 22-m telescope, far reveal the Universe as it was long ago. One of better than any other telescope today. It is the the big mysteries uncovered by the Hubble forerunner of the next generation of ultra-large Space Telescope program is the existence of telescopes. fully formed galaxies in the early universe, much earlier than physicists predicted. Their formation The LBT has extraordinary capabilities. will be a key research program for the LBT and Its design allows it to directly observe distant Origins Institute faculty Dinshaw Balsara and stars systems and to actually see planets in the Christopher Howk, who aim to understand the systems. Its ability to measure very precise atomic dynamics that govern the formation of galaxies spectra even enables researchers to determine the and with them the beginnings of life. chemical makeup of the planets’ atmospheres. -
The Reionization of Cosmic Hydrogen by the First Galaxies Abstract 1
David Goodstein’s Cosmology Book The Reionization of Cosmic Hydrogen by the First Galaxies Abraham Loeb Department of Astronomy, Harvard University, 60 Garden St., Cambridge MA, 02138 Abstract Cosmology is by now a mature experimental science. We are privileged to live at a time when the story of genesis (how the Universe started and developed) can be critically explored by direct observations. Looking deep into the Universe through powerful telescopes, we can see images of the Universe when it was younger because of the finite time it takes light to travel to us from distant sources. Existing data sets include an image of the Universe when it was 0.4 million years old (in the form of the cosmic microwave background), as well as images of individual galaxies when the Universe was older than a billion years. But there is a serious challenge: in between these two epochs was a period when the Universe was dark, stars had not yet formed, and the cosmic microwave background no longer traced the distribution of matter. And this is precisely the most interesting period, when the primordial soup evolved into the rich zoo of objects we now see. The observers are moving ahead along several fronts. The first involves the construction of large infrared telescopes on the ground and in space, that will provide us with new photos of the first galaxies. Current plans include ground-based telescopes which are 24-42 meter in diameter, and NASA’s successor to the Hubble Space Telescope, called the James Webb Space Telescope. In addition, several observational groups around the globe are constructing radio arrays that will be capable of mapping the three-dimensional distribution of cosmic hydrogen in the infant Universe. -
Constraining Stochastic Gravitational Wave Background from Weak Lensing of CMB B-Modes
Prepared for submission to JCAP Constraining stochastic gravitational wave background from weak lensing of CMB B-modes Shabbir Shaikh,y Suvodip Mukherjee,y Aditya Rotti,z and Tarun Souradeepy yInter University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune- 411007, India zDepartment of Physics, Florida State University, Tallahassee, FL 32304, USA E-mail: [email protected], [email protected], [email protected], [email protected] Abstract. A stochastic gravitational wave background (SGWB) will affect the CMB anisotropies via weak lensing. Unlike weak lensing due to large scale structure which only deflects pho- ton trajectories, a SGWB has an additional effect of rotating the polarization vector along the trajectory. We study the relative importance of these two effects, deflection & rotation, specifically in the context of E-mode to B-mode power transfer caused by weak lensing due to SGWB. Using weak lensing distortion of the CMB as a probe, we derive constraints on the spectral energy density (ΩGW ) of the SGWB, sourced at different redshifts, without assuming any particular model for its origin. We present these bounds on ΩGW for different power-law models characterizing the SGWB, indicating the threshold above which observable imprints of SGWB must be present in CMB. arXiv:1606.08862v2 [astro-ph.CO] 20 Sep 2016 Contents 1 Introduction1 2 Weak lensing of CMB by gravitational waves2 3 Method 6 4 Results 8 5 Conclusion9 6 Acknowledgements 10 1 Introduction The Cosmic Microwave Background (CMB) is an exquisite tool to study the universe. It is being used to probe the early universe scenarios as well as the physics of processes happening in between the surface of last scattering and the observer. -
Cosmic Microwave Background
1 29. Cosmic Microwave Background 29. Cosmic Microwave Background Revised August 2019 by D. Scott (U. of British Columbia) and G.F. Smoot (HKUST; Paris U.; UC Berkeley; LBNL). 29.1 Introduction The energy content in electromagnetic radiation from beyond our Galaxy is dominated by the cosmic microwave background (CMB), discovered in 1965 [1]. The spectrum of the CMB is well described by a blackbody function with T = 2.7255 K. This spectral form is a main supporting pillar of the hot Big Bang model for the Universe. The lack of any observed deviations from a 7 blackbody spectrum constrains physical processes over cosmic history at redshifts z ∼< 10 (see earlier versions of this review). Currently the key CMB observable is the angular variation in temperature (or intensity) corre- lations, and to a growing extent polarization [2–4]. Since the first detection of these anisotropies by the Cosmic Background Explorer (COBE) satellite [5], there has been intense activity to map the sky at increasing levels of sensitivity and angular resolution by ground-based and balloon-borne measurements. These were joined in 2003 by the first results from NASA’s Wilkinson Microwave Anisotropy Probe (WMAP)[6], which were improved upon by analyses of data added every 2 years, culminating in the 9-year results [7]. In 2013 we had the first results [8] from the third generation CMB satellite, ESA’s Planck mission [9,10], which were enhanced by results from the 2015 Planck data release [11, 12], and then the final 2018 Planck data release [13, 14]. Additionally, CMB an- isotropies have been extended to smaller angular scales by ground-based experiments, particularly the Atacama Cosmology Telescope (ACT) [15] and the South Pole Telescope (SPT) [16]. -
Secondary Cosmic Microwave Background Anisotropies in A
THE ASTROPHYSICAL JOURNAL, 508:435È439, 1998 December 1 ( 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A. SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES IN A UNIVERSE REIONIZED IN PATCHES ANDREIGRUZINOV AND WAYNE HU1 Institute for Advanced Study, School of Natural Sciences, Princeton, NJ 08540 Received 1998 March 17; accepted 1998 July 2 ABSTRACT In a universe reionized in patches, the Doppler e†ect from Thomson scattering o† free electrons gener- ates secondary cosmic microwave background (CMB) anisotropies. For a simple model with small patches and late reionization, we analytically calculate the anisotropy power spectrum. Patchy reioniza- tion can, in principle, be the main source of anisotropies on arcminute scales. On larger angular scales, its contribution to the CMB power spectrum is a small fraction of the primary signal and is only barely detectable in the power spectrum with even an ideal, i.e., cosmic variance limited, experiment and an extreme model of reionization. Consequently, patchy reionization is unlikely to a†ect cosmological parameter estimation from the acoustic peaks in the CMB. Its detection on small angles would help determine the ionization history of the universe, in particular, the typical size of the ionized region and the duration of the reionization process. Subject headings: cosmic microwave background È cosmology: theory È intergalactic medium È large-scale structure of universe 1. INTRODUCTION tion below the degree scale. Such e†ects rely on modulating the Doppler e†ect with spatial variations in the optical It is widely believed that the cosmic microwave back- depth. Incarnations of this general mechanism include the ground (CMB) will become the premier laboratory for the Vishniac e†ect from linear density variations (Vishniac study of the early universe and classical cosmology. -
Proof for a Rotational Double Torus Universe
Proof For A Rotational Double Torus Universe. Author: Dan Visser, Almere, the Netherlands. Date: January 19 2014 (version-1); April 28 2014 (version-2) Abstract. The Universe rotates. We live in a Double Torus Universe. A dark matter torus rotates in a larger time torus of refined time smaller than the Planck-time. The Planck-satellite showed a more detailed picture of the CMB related to Big Bang cosmology. However, I have put that in perspective of a new set of equations that belong to the framework of the Double Torus Theory. That shows my proof for a rotational dark matter Flow by warm and cold areas in the CMB. I also explain why the accelerated space-expansion in the Big Bang cosmology is an illusion. Introduction. I refer to an article that was published in Physics World. In that article Professor Peter Coles of the University of Sussex, UK, explained the Planck perspectives [1]. I wrote him an email explaining I found proof for a rotational Double Torus Universe, instead of a Big Bang. I also found the argument why an accelerated space-time is observed and why this is an illusion from the perspective of the Double Torus Theory. I have printed a copy of that email, as follows: Dear Peter Coles, I read your article in Physics World about ‘Planck Perspectives’. Very well. But that is what I needed to make a statement the Big Bang cannot be maintained as the current cosmological model. I have gathered proof for that. I published my articles in the Vixra- archive (www.vixra.org/author/dan_visser). -
Does Dark Energy Really Exist?
COSMOLOGY Does DARK ENERGY Maybe not. Really Exist? The observations that led astronomers to deduce its existence could have another explanation: that our galaxy lies at the center of a giant cosmic void By Timothy Clifton and Pedro G. Ferreira n science, the grandest revolutions are often of a universe populated by billions of galaxies triggered by the smallest discrepancies. In the that stretch out to our cosmic horizon, we are led I16th century, based on what struck many of to believe that there is nothing special or unique his contemporaries as the esoteric minutiae of ce- about our location. But what is the evidence for KEY CONCEPTS lestial motions, Copernicus suggested that Earth this cosmic humility? And how would we be able ■ The universe appears to be was not, in fact, at the center of the universe. In to tell if we were in a special place? Astronomers expanding at an accelerat- our own era, another revolution began to unfold typically gloss over these questions, assuming ing rate, implying the exis- 11 years ago with the discovery of the accelerat- our own typicality sufficiently obvious to war- tence of a strange new ing universe. A tiny deviation in the brightness of rant no further discussion. To entertain the no- form of energy—dark ener- exploding stars led astronomers to conclude that tion that we may, in fact, have a special location gy. The problem: no one is they had no idea what 70 percent of the cosmos in the universe is, for many, unthinkable. Never- sure what dark energy is. -
Mysterious Cosmic 'Dark Flow' Tracked Deeper Into Universe (W/ Video) 10 March 2010
Mysterious Cosmic 'Dark Flow' Tracked Deeper into Universe (w/ Video) 10 March 2010 but right now our data cannot state as strongly as we'd like whether the clusters are coming or going," Kashlinsky said. The dark flow is controversial because the distribution of matter in the observed universe cannot account for it. Its existence suggests that some structure beyond the visible universe -- outside our "horizon" -- is pulling on matter in our vicinity. Cosmologists regard the microwave background -- The colored dots are clusters within one of four distance a flash of light emitted 380,000 years after the ranges, with redder colors indicating greater distance. universe formed -- as the ultimate cosmic reference Colored ellipses show the direction of bulk motion for the frame. Relative to it, all large-scale motion should clusters of the corresponding color. Images of representative galaxy clusters in each distance slice are show no preferred direction. also shown. Credit: NASA/Goddard/A. Kashlinsky, et al. The hot X-ray-emitting gas within a galaxy cluster scatters photons from the cosmic microwave background (CMB). Because galaxy clusters don't (PhysOrg.com) -- Distant galaxy clusters precisely follow the expansion of space, the mysteriously stream at a million miles per hour wavelengths of scattered photons change in a way along a path roughly centered on the southern that reflects each cluster's individual motion. constellations Centaurus and Hydra. A new study led by Alexander Kashlinsky at NASA's Goddard This results in a minute shift of the microwave Space Flight Center in Greenbelt, Md., tracks this background's temperature in the cluster's direction. -
Observational Prospects I Have Cut This Lecture Back to Be Mostly About BAO Because I Still Have Holdover Topics from Previous Lectures to Cover
Precision Cosmology with Large Scale Structure David Weinberg Precision Cosmology With Large Scale Structure David Weinberg, Ohio State University ICTP Cosmology Summer School 2015 Lecture 3: Observational Prospects I have cut this lecture back to be mostly about BAO because I still have holdover topics from previous lectures to cover. Where are we now? CMB Planck: All sky (40,000 deg2), near cosmic-variance limited for temperature anisotropy, noise lim- ited for polarization. ACT and SPT: Higher resolution experiments over smaller areas (hundreds or thousands of deg2), frequency coverage for Sunyaev-Zeldovich as well as primary anisotropy, polarization. Smaller area high-sensitivity experiments for B-mode polarization (e.g., BICEP). Type Ia Supernovae Data sets are compilations of surveys of different redshift ranges, local to z 1.2. ≈ “Compilation” requires enormous effort to bring different data sets to common calibration and analysis. Union 2.1, broad compilation. JLA – local samples, SDSS-II from z = 0.1 0.4, SNLS (Canada-France-Hawaii Telescope) from z = 0.4 1, HST at z > 1. − − Approaching 1000 SNe (740 for JLA). Optical imaging/weak lensing SDSS – 104 deg2, 5 bands (ugriz), depth r 22, weak lensing source density approximately − 1 arcmin 2; SDSS “Stripe 82” went 2 magnitudes≈ deeper over 200 deg2 Pan-STARRS – 3 104 deg2, depth comparable to SDSS × CFHTLens – 150 deg2, Dark Energy Survey (DES) is ongoing, discussed at the end. Redshift surveys SDSS-I/II: 106 galaxies, broadly selected, median z = 0.1 ; 105 luminous red galaxies (LRGs) sparsely sampling structure to z = 0.45 SDSS-III BOSS: 1.5 106 luminous galaxies, z = 0.2 0.7, 7 effective volume of SDSS-I/II LRGs; spectra of 160,000 quasars× at z = 2 4 for Lyα forest− analysis× − Clusters Variety of cluster catalogs selected by different methods.