scholarly journals Dynamical critical phenomena and large-scale structure of the Universe: The power spectrum for density fluctuations

1997 ◽  
Vol 38 (8) ◽  
pp. 637-642 ◽  
Author(s):  
J. F. Barbero G. ◽  
A Dominguez ◽  
T Goldman ◽  
J Pérez-Mercader
Keyword(s):  
Power Spectrum ◽  
Critical Phenomena ◽  
Large Scale ◽  
Large Scale Structure ◽  
Density Fluctuations ◽  
Scale Structure ◽  
Dynamical Critical Phenomena ◽  
The Universe

scholarly journals Large Scale Structure of the Universe

1998 ◽  
Vol 179 ◽  
pp. 317-328 ◽  
Author(s):  
N.A. Bahcall
Keyword(s):  
Large Scale ◽  
Initial Conditions ◽  
Large Scale Structure ◽  
Density Fluctuations ◽  
Scale Structure ◽  
Sloan Digital Sky Survey ◽  
Sky Survey ◽  
Initial Spectrum ◽  
Formation And Evolution ◽  
The Universe

How is the universe organized on large scales? How did this structure evolve from the unknown initial conditions of a rather smooth early universe to the present time? The answers to these questions will shed light on the cosmology we live in, the amount, composition and distribution of matter in the universe, the initial spectrum of density fluctuations that gave rise to this structure, and the formation and evolution of galaxies, lusters of galaxies, and larger scale structures.To address these fundamental questions, large and accurate sky surveys are needed—in various wavelengths and to various depths. In this presentation I review current observational studies of large scale structure, present the constraints these observations place on cosmological models and on the amount of dark matter in the universe, and highlight some of the main unsolved problems in the field of large-scale structure that could be solved over the next decade with the aid of current and future surveys. I briefly discuss some of these surveys, including the Sloan Digital Sky Survey that will provide a complete imaging and spectroscopic survey of the high-latitude northern sky, with redshifts for the brightest ∼ 106 galaxies, 105 quasars, and 103.5 rich clusters of galaxies. The potentialities of the SDSS survey, as well as of cross-wavelength surveys, for resolving some of the unsolved problems in large-scale structure and cosmology are discussed.

The DWT power spectrum analysis of the large scale structure in the universe : Method and simulation tests

2001 ◽  
Vol 44 (5) ◽  
pp. 669-680
Author(s):  
Xiaohu Yang ◽  
Longlong Feng ◽  
Yaoquan Chu
Keyword(s):  
Power Spectrum ◽  
Spectrum Analysis ◽  
Large Scale ◽  
Large Scale Structure ◽  
Power Spectrum Analysis ◽  
Scale Structure ◽  
The Universe

scholarly journals The cosmic web: a selective history and outlook

2014 ◽  
Vol 11 (S308) ◽  
pp. 125-142
Author(s):  
John A. Peacock
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Matter Content ◽  
Density Fluctuations ◽  
Scale Structure ◽  
Central Importance ◽  
The Future ◽  
The Universe

AbstractIn the Century since Slipher's first observations, roughly three million galaxy redshifts have been measured. The resulting maps of large-scale structure have taught us much of central importance in cosmology, ranging from the matter content of the universe to the study of the primordial density fluctuations. This talk aims to review some of the key observational and theoretical milestones on this journey, and to speculate about what the future may bring.

scholarly journals Formation of the large-scale structure of the Universe

2011 ◽  
Vol 54 (10) ◽  
pp. 983-1005 ◽  
Author(s):  
Vladimir N Lukash ◽  
Elena V Mikheeva ◽  
A M Malinovsky
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
The Universe

The Large‐Scale Structure of the Universe

Physics Today ◽  
1981 ◽  
Vol 34 (8) ◽  
pp. 62-63 ◽  
Author(s):  
P. J. E. Peebles ◽  
Simon D. M. White
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
The Universe

scholarly journals Using the Marked Power Spectrum to Detect the Signature of Neutrinos in Large-Scale Structure

2021 ◽  
Vol 126 (1) ◽  
Author(s):  
Elena Massara ◽  
Francisco Villaescusa-Navarro ◽  
Shirley Ho ◽  
Neal Dalal ◽  
David N. Spergel
Keyword(s):  
Power Spectrum ◽  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure

Orientation of the Spins of Flat Galaxies Relative to Filaments of a Large-Scale Structure of the Universe

2021 ◽  
Vol 76 (3) ◽  
pp. 248-254
Author(s):  
A. V. Antipova ◽  
D. I. Makarov ◽  
D. V. Bizyaev
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
The Universe

scholarly journals THE HORIZON RUNN-BODY SIMULATION: BARYON ACOUSTIC OSCILLATIONS AND TOPOLOGY OF LARGE-SCALE STRUCTURE OF THE UNIVERSE

2009 ◽  
Vol 701 (2) ◽  
pp. 1547-1559 ◽  
Author(s):  
Juhan Kim ◽  
Changbom Park ◽  
J. Richard Gott ◽  
John Dubinski
Keyword(s):  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
Acoustic Oscillations ◽  
And Topology ◽  
Baryon Acoustic Oscillations ◽  
The Universe

scholarly journals The Theory of the Large Scale Structure of the Universe

1978 ◽  
Vol 79 ◽  
pp. 409-421 ◽  
Author(s):  
Ya B. Zeldovich
Keyword(s):  
Early Childhood ◽  
Sigmund Freud ◽  
Large Scale ◽  
Large Scale Structure ◽  
Scale Structure ◽  
The Other ◽  
Childhood Experiences ◽  
Other Hand ◽  
The Universe ◽  
Single Statement

The God-father of psychoanalysis Professor Sigmund Freud taught us that the behaviour of adults depends on their early childhood experiences. in the same spirit, the problem of cosmological analysis is to derive the observed present day situation and structure of the Universe from certain plausible assumptions about its early behaviour. Perhaps the most important single statement about the large scale structure is that there is no structure at all on the largest scale − 1000 Mpc and more. On this scale the Universe is rather uniform, structureless and isotropically expanding - just according to the simplified pictures of Einstein-Friedmann……. Humason, Hubble…. Robertson, Walker. On the other hand there is a lot of structure on the scale of 100 or 50 Mpc and less. There are clusters and superclusters of galaxies.

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