Results 41 to 50 of about 49,997 (277)

Cosmic Microwave Background from Effective Field Theory

open access: yesUniverse, 2019
In this work, we study the key role of generic Effective Field Theory (EFT) framework to quantify the correlation functions in a quasi de Sitter background for an arbitrary initial choice of the quantum vacuum state. We perform the computation in unitary
Sayantan Choudhury
doaj   +1 more source

Photonic Integrated Circuits for Microwave Astronomy

open access: yesInventions, 2023
One of the main objectives of cosmology is the measurement of the Cosmic Microwave Background (CMB) polarization and, in particular, the so-called B-modes, which could demonstrate the existence of the primordial gravitational waves generated at the early
Guillermo Pascual-Cisneros   +2 more
doaj   +1 more source

Heating of the intergalactic medium by the cosmic microwave background during cosmic dawn [PDF]

open access: yesPhysical Review D, 2018
The intergalactic medium is expected to be at its coldest point before the formation of the first stars in the universe. Motivated by recent results from the EDGES experiment, we revisit the standard calculation of the kinetic temperature of the neutral ...
T. Venumadhav   +3 more
semanticscholar   +1 more source

Optimization of a Microwave Polarimeter for Astronomy with Optical Correlation and Detection

open access: yesSensors, 2023
Cosmic Microwave Background (CMB) B-modes detection is the main focus of future CMB experiments because of the valuable information it contains, particularly to probe the physics of the very early universe. For this reason, we have developed an optimized
Guillermo Pascual-Cisneros   +2 more
doaj   +1 more source

Probing decoupling in dark sectors with the cosmic microwave background [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2018
The acoustic peaks in the angular power spectrum of cosmic microwave background (CMB) temperature and polarization anisotropies play an important role as a probe of the nature of new relativistic particles contributing to the radiation density in the ...
Gongjun Choi   +2 more
semanticscholar   +1 more source

Self-Similar Symmetry Model and Cosmic Microwave Background

open access: yesFrontiers in Applied Mathematics and Statistics, 2016
In this paper, we present the self-similar symmetry (SSS) model that describes the hierarchical structure of the universe. The model is based on the concept of self-similarity, which explains the symmetry of the cosmic microwave background (CMB).
Tomohide eSonoda
doaj   +1 more source

General constraints on dark matter decay from the cosmic microwave background [PDF]

open access: yes, 2016
Precise measurements of the temperature and polarization anisotropies of the cosmic microwave background can be used to constrain the annihilation and decay of dark matter. In this work, we demonstrate via principal component analysis that the imprint of
T. Slatyer, Chih-Liang Wu
semanticscholar   +1 more source

Polarization in the cosmic microwave background [PDF]

open access: yesBrazilian Journal of Physics, 2006
Cosmic microwave background (CMB) studies underpin our understanding of the universe and its history. Until recently, we have relied principally on CMB temperature observations to build our standard cosmological model, but today the field forges ahead into its next frontier - CMB polarization anistropy.
openaire   +5 more sources

Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter [PDF]

open access: yes, 2017
The cosmic microwave background (CMB) places strong constraints on models of dark matter (DM) that deviate from standard cold DM (CDM), and on initial conditions beyond the scalar adiabatic mode.
R. Hložek, D. Marsh, D. Grin
semanticscholar   +1 more source

Microwave background temperature at a redshift of 6.34 from H2O absorption [PDF]

open access: yesNature, 2022
Distortions of the observed cosmic microwave background provide a direct measurement of the microwave background temperature at redshifts from 0 to 1 (refs. 1,2).
D. Riechers   +6 more
semanticscholar   +1 more source

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