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The Cosmic Microwave Background (CMB) radiation offers a unique window into the early Universe, facilitating precise examinations of fundamental cosmological theories. However, the quest for detecting B-modes in the CMB, predicted by…

Cosmic reionization holds the key to understand structure formation in the Universe, and can inform us about the properties of the first sources, as their star formation efficiency and escape fraction of ionizing photons. By combining the…

宇宙学与河外天体物理 · 物理学 2015-10-07 Sourav Mitra , T. Roy Choudhury , Andrea Ferrara

Patchy reionization leaves a number of imprints on the small-scale cosmic microwave background (CMB) temperature fluctuations, the largest of which is the kinematic Sunyaev-Zel'dovich (kSZ), the Doppler shift of CMB photons scattering off…

宇宙学与河外天体物理 · 物理学 2018-12-26 Simone Ferraro , Kendrick M. Smith

With the imminent promise of constraints on the epoch of reionization from observations of microwave background anisotropies, the question of whether or not the standard Cold Dark Matter (CDM) model permits early reionization has been…

天体物理学 · 物理学 2015-06-24 Andrew R Liddle , David H Lyth

The large-scale CMB B-mode polarization is the direct probe to the low frequency primordial gravitational wave signal. However, unambiguous measurement of this signal requires a precise understanding of the possible contamination. One such…

宇宙学与河外天体物理 · 物理学 2019-05-06 Suvodip Mukherjee , Sourabh Paul , Tirthankar Roy Choudhury

The paper is devoted to the methods of determination of the cosmological parameters from recent CMB observations. We show that the more complex models of kinetics of recombination with a few "missing" parameters describing the recombination…

天体物理学 · 物理学 2009-11-07 A. G. Doroshkevich , I. P. Naselsky , P. D. Naselsky , I. D. Novikov

The next generation of instruments designed to measure the polarization of the cosmic microwave background (CMB) will provide a historic opportunity to open the gravitational wave window to the primordial Universe. Through high sensitivity…

Cosmic microwave background (CMB) anisotropy is our richest source of cosmological information; the standard cosmological model was largely established thanks to study of the temperature anisotropies. By the end of the decade, the Planck…

天体物理学 · 物理学 2009-11-11 James G. Bartlett

DASI has ended a 34-year quest to detect the CMB polarization, sounding the starting gun for a new race to peer further back in time, with more precision than ever before. Many more CMB polarization experiments are in progress or planned.…

天体物理学 · 物理学 2007-05-23 Eric Hivon , Marc Kamionkowski

We study the relationship between signatures of high redshift ionization in large-angle CMB polarization power spectra and features in the Planck 2015 data. Using a principal component (PC) ionization basis that is complete to the cosmic…

宇宙学与河外天体物理 · 物理学 2018-09-19 Chen Heinrich , Wayne Hu

In this report we discuss the impact of polarized foregrounds on a future CMBPol satellite mission. We review our current knowledge of Galactic polarized emission at microwave frequencies, including synchrotron and thermal dust emission. We…

We study the signal from patchy reionization in view of the future high accuracy polarization measurements of the Cosmic Microwave Background (CMB). We implement an extraction procedure of the patchy reionization signal analogous to CMB…

宇宙学与河外天体物理 · 物理学 2018-05-18 Anirban Roy , Andrea Lapi , David Spergel , Carlo Baccigalupi

The epoch of reionization probes the state of our universe when the very first stars formed and ionized the hydrogen atoms in the surrounding medium. Since the epoch has not yet been probed observationally, it is often called the "final…

宇宙学与河外天体物理 · 物理学 2022-09-20 Tirthankar Roy Choudhury

The search for primordial gravitational waves through the $B$-mode polarization pattern in the CMB is one of the major goals of current and future CMB experiments. Besides foregrounds, a potential hurdle in this search is the anisotropic…

宇宙学与河外天体物理 · 物理学 2021-01-06 Anirban Roy , Girish Kulkarni , P. Daniel Meerburg , Anthony Challinor , Carlo Baccigalupi , Andrea Lapi , Martin G. Haehnelt

The effects of reionization, occurring after standard recombination in cold dark matter-dominated models, on CMB anisotropies are investigated. Late-time reionization reduces the CMB anisotropies, in particular, on degree scales. It is…

天体物理学 · 物理学 2009-10-22 Naoshi Sugiyama , Joseph Silk , Nicola Vittorio

Current data of high-redshift absorption-line systems imply that hydrogen reionization occurred before redshifts of about 5. Previous works on reionization by the first stars or quasars have shown that such scenarios are described by a…

天体物理学 · 物理学 2009-10-31 Aparna Venkatesan

Observations of the polarization of the cosmic microwave backround (CMB) have the potential to place much tighter constraints on cosmological parameters than observations of the fluctuations in temperature alone. We discuss using CMB…

天体物理学 · 物理学 2009-10-30 William H. Kinney

The study of cosmic reionization has acquired increasing significance over the last few years because of various reasons. On the observational front, we now have good quality data of different types at high redshifts (quasar absorption…

天体物理学 · 物理学 2007-05-23 T. Roy Choudhury , A. Ferrara

One of the main goals of modern cosmic microwave background (CMB) missions is to measure the tensor-to-scalar ratio $r$ accurately to constrain inflation models. Due to ignorance about the reionization history $X_{e}(z)$, this analysis is…

宇宙学与河外天体物理 · 物理学 2014-06-03 King Lau , Jiayu Tang , M. -C. Chu

The Universe is the grandest conceivable scale on which the human mind can strive to understand nature. The amazing aspect of cosmology, the branch of science that attempts to understand the origin and evolution of the Universe, is that it…

宇宙学与河外天体物理 · 物理学 2011-04-19 Tarun Souradeep