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Large-Scale Structure of the Universe
US $13.49
ApproximatelyRM 56.95
Condition:
Good
A book that has been read but is in good condition. Very minimal damage to the cover including scuff marks, but no holes or tears. The dust jacket for hard covers may not be included. Binding has minimal wear. The majority of pages are undamaged with minimal creasing or tearing, minimal pencil underlining of text, no highlighting of text, no writing in margins. No missing pages.
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Located in: Sault Sainte Marie, Michigan, United States
Delivery:
Estimated between Fri, 22 Aug and Tue, 26 Aug to 94104
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14 days return. Buyer pays for return shipping. If you use an eBay shipping label, it will be deducted from your refund amount.
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eBay item number:335572141616
Item specifics
- Condition
- ISBN
- 9780691082400
About this product
Product Identifiers
Publisher
Princeton University Press
ISBN-10
0691082405
ISBN-13
9780691082400
eBay Product ID (ePID)
616384
Product Key Features
Number of Pages
440 Pages
Language
English
Publication Name
Large-Scale Structure of the Universe
Publication Year
1980
Subject
Physics / Astrophysics, Cosmology
Type
Textbook
Subject Area
Science
Series
Princeton Series in Physics Ser.
Format
Trade Paperback
Dimensions
Item Height
1 in
Item Weight
22 Oz
Item Length
9.1 in
Item Width
7.6 in
Additional Product Features
Intended Audience
College Audience
LCCN
79-084008
TitleLeading
The
Series Volume Number
96
Illustrated
Yes
Dewey Decimal
523.1/12
Synopsis
Opinions on the large-scale structure of the early universe range widely from primeval chaos to a well-ordered mass distribution. P.J.E. Peebles argues that the evolution proceeded from a nearly uniform initial state to a progressively more irregular and clumpy universe. The discussion centers on the largest known structures--the clusters of galaxies, the empirical evidence of the nature of the clustering, and the theories of how the clustering evolves in an expanding universe., From the Nobel Prize-winning physicist Opinions on the large-scale structure of the early universe range widely from primeval chaos to a well-ordered mass distribution. P. J. E. Peebles argues that the evolution proceeded from a nearly uniform initial state to a progressively more irregular and clumpy universe. The discussion centers on the largest known structures, the clusters of galaxies, the empirical evidence of the nature of the clustering, and the theories of how the clustering evolves in an expanding universe. In Chapter One the author provides an historical introduction to the subject. Chapter Two contains a survey of methods used to deal with the Newtonian approximation to the theory of the evolution of the mass distribution. Recent progress in the use of statistical measures of the clustering is described in Chapter Three. Chapters Four and Five return to techniques for dealing with cosmic evolution, in the statistical measures of clustering and under general relativity theory. Lastly, in Chapter Six Professor Peebles assesses the progress in attempts to link theory and observation to arrive at a well established physical picture of the nature and evolution of the universe., Opinions on the large-scale structure of the early universe range from primeval chaos to a well-ordered mass distribution. This work argues that the evolution proceeded from a nearly uniform initial state to a progressively irregular and clumpy universe. It also describes progress in the use of statistical measures of the clustering., From the Nobel Prize-winning physicist Opinions on the large-scale structure of the early universe range widely from primeval chaos to a well-ordered mass distribution. Phillip James Edwin Peebles argues that the evolution proceeded from a nearly uniform initial state to a progressively more irregular and clumpy universe. The discussion centers on the largest known structures, the clusters of galaxies, the empirical evidence of the nature of the clustering, and the theories of how the clustering evolves in an expanding universe. In Chapter One the author provides an historical introduction to the subject. Chapter Two contains a survey of methods used to deal with the Newtonian approximation to the theory of the evolution of the mass distribution. Recent progress in the use of statistical measures of the clustering is described in Chapter Three. Chapters Four and Five return to techniques for dealing with cosmic evolution, in the statistical measures of clustering and under general relativity theory. Lastly, in Chapter Six Professor Peebles assesses the progress in attempts to link theory and observation to arrive at a well established physical picture of the nature and evolution of the universe.
LC Classification Number
QB857 .P43
Item description from the seller
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- t***s (485)- Feedback left by buyer.Past monthVerified purchaseThis item is authentic and fits perfect, and I’m very excited to wear it this Oktoberfest season!
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