scholarly journals THE LINEARITY OF THE COSMIC EXPANSION FIELD FROM 300 TO 30, 000 km s–1AND THE BULK MOTION OF THE LOCAL SUPERCLUSTER WITH RESPECT TO THE COSMIC MICROWAVE BACKGROUND

2010 ◽  
Vol 714 (2) ◽  
pp. 1441-1459 ◽  
Author(s):  
A. Sandage ◽  
B. Reindl ◽  
G. A. Tammann
Keyword(s):  
Cosmic Microwave Background ◽  
Microwave Background ◽  
Cosmic Expansion ◽  
Bulk Motion ◽  
Local Supercluster

THE IMPRINT OF DARK ENERGY

2004 ◽  
Vol 19 (13n16) ◽  
pp. 1063-1070 ◽  
Author(s):  
ROBERT CALDWELL
Keyword(s):  
Dark Energy ◽  
Energy Density ◽  
Cosmic Microwave Background ◽  
Cosmological Constant ◽  
Negative Pressure ◽  
Inhomogeneous Field ◽  
Time Varying ◽  
Microwave Background ◽  
Cosmic Expansion ◽  
Cosmological Observations

Diverse cosmological observations indicate the existence of dark energy, comprising ~ 70% of the total cosmic energy density and driving the accelerated cosmic expansion. Possible explanations for the dark energy include a cosmological constant and quintessence — a time-varying, inhomogeneous field with negative pressure. In this article we summarize how the dark energy imprints features on the cosmic microwave background. Observation of these features could be useful in discriminating amongst various theories, and could reveal clues as to the nature of the dark energy.

Small‐Scale Cosmic Microwave Background Observations at 8.4 GHz

1997 ◽  
Vol 483 (1) ◽  
pp. 38-50 ◽  
Author(s):  
R. Bruce Partridge ◽  
Eric A. Richards ◽  
Edward B. Fomalont ◽  
K. I. Kellerman ◽  
Rogier A. Windhorst
Keyword(s):  
Cosmic Microwave Background ◽  
Small Scale ◽  
Microwave Background

scholarly journals The evolution of the cosmic microwave background temperature

2011 ◽  
Vol 526 ◽  
pp. L7 ◽  
Author(s):  
P. Noterdaeme ◽  
P. Petitjean ◽  
R. Srianand ◽  
C. Ledoux ◽  
S. López
Keyword(s):  
Cosmic Microwave Background ◽  
Microwave Background ◽  
Cosmic Microwave Background Temperature ◽  
Background Temperature

scholarly journals Revisiting cosmic microwave background radiation using blackbody radiation inversion

2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Koustav Konar ◽  
Kingshuk Bose ◽  
R. K. Paul
Keyword(s):  
Temperature Distribution ◽  
Cosmic Microwave Background ◽  
Background Radiation ◽  
Big Bang ◽  
Blackbody Radiation ◽  
Microwave Background ◽  
Background Spectrum ◽  
Microwave Background Radiation ◽  
Mathematical Process

AbstractBlackbody radiation inversion is a mathematical process for the determination of probability distribution of temperature from measured radiated power spectrum. In this paper a simple and stable blackbody radiation inversion is achieved by using an analytical function with three determinable parameters for temperature distribution. This inversion technique is used to invert the blackbody radiation field of the cosmic microwave background, the remnant radiation of the hot big bang, to infer the temperature distribution of the generating medium. The salient features of this distribution are investigated and analysis of this distribution predicts the presence of distortion in the cosmic microwave background spectrum.

scholarly journals Model-Independent Test for Scale-Dependent Non-Gaussianities in the Cosmic Microwave Background

2009 ◽  
Vol 102 (13) ◽  
Author(s):  
C. Räth ◽  
G. E. Morfill ◽  
G. Rossmanith ◽  
A. J. Banday ◽  
K. M. Górski
Keyword(s):  
Cosmic Microwave Background ◽  
Microwave Background ◽  
Independent Test ◽  
Model Independent

scholarly journals Anisotropies of the cosmic microwave background

2002 ◽  
Vol 25 (9) ◽  
pp. 1-82
Author(s):  
M. Bersanelli ◽  
D. Maino ◽  
A. Mennella
Keyword(s):  
Cosmic Microwave Background ◽  
Microwave Background
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