Skip to content

Corrections and Additional Remarks to Our Paper (Einstein & Strauss) WITH On a New Theory of Weizsäcker on the Origin of the Solar System in Reviews of Modern Physics, 18, January 1946, pp. 148-149; pp. 94-103

Corrections and Additional Remarks to Our Paper (Einstein & Strauss) WITH On a New Theory of Weizsäcker on the Origin of the Solar System in Reviews of Modern Physics, 18, January 1946, pp. 148-149; pp. 94-103

Click for full-size.

Corrections and Additional Remarks to Our Paper (Einstein & Strauss) WITH On a New Theory of Weizsäcker on the Origin of the Solar System in Reviews of Modern Physics, 18, January 1946, pp. 148-149; pp. 94-103

by Einstein, Albert; Ernst G. Straus AND Chandrasekhar S

  • Used
  • Paperback
  • first
Condition
See description
Seller
Seller rating:
This seller has earned a 5 of 5 Stars rating from Biblio customers.
West Branch, Iowa, United States
Item Price
£145.19
Or just £130.67 with a
Bibliophiles Club Membership
£4.03 Shipping to USA
Standard delivery: 7 to 14 days

More Shipping Options

Payment Methods Accepted

  • Visa
  • Mastercard
  • American Express
  • Discover
  • PayPal

About This Item

Lancaster: American Physical Society, 1946. 1st Edition. FIRST EDITION IN ORIGINAL WRAPS OF SIGNIFICANT CORRECTIONS & ADDITIONS BY EINSTEIN & STRAUS TO AN IMPORTANT PAPER; AS WELL, A PAPER BY CHANDRASEKHAR ON THE ORIGIN OF THE SOLAR SYSTEM.

In 1945 Albert Einstein and Ernst G. Straus introduced their Swiss cheese model of the universe in a paper entitled "The Influence of the Expansion of Space on the Gravitation Fields Surrounding the Individual Stars". (Weil 216). The following year they published "Corrections and Additional Remarks to Our Paper" (the 1945 paper), the paper offered here.

In early 1945, Einstein returned to long held cosmological questions as he sought to try to understand whether the expansion of the universe caused the solar system to expand as well — or more specifically, the influence of the expansion of space on the gravitational field in the neighborhood of a star. Working with Straus, the two began studying the effect of inhomogeneities in an expanding model.

"By the spring of 1945, Einstein and Straus had found a new type of possible universe using Einstein's equations. It described a universe which looked largely like one of the simple expanding universes of Friedmann and Lemaître containing material (like galaxies) which exerted no pressure. But it has spherical regions removed from it, like bubbles in a Swiss cheese. Each empty hole then had a mass placed at its centre. The mass was equal in magnitude to what had been excavated to create the hole. This was a step towards a more realistic universe in which the matter was not smoothly spread with the same density everywhere but gathered up into lumps, like galaxies, which were spread about in empty space. (Barrow, The Book of Universes, 106-107).

ALSO INCLUDED: S. Chandrasekhar's "On a New Theory of Weizsäcker on the Origin of the Solar System". In 1945, C. F. v. Weizsäcker proposed a new theory of the origin of the solar system which appeared to merit consideration. Weizsäcker argued "that there [would be] turbulence in the solar nebula which would give rise to the formation of eddies having angular motion opposite to that of the rotation of the nebula" (Abhyankar, The Origin, BASI, 26, 339). Weizsäcker's "principal idea [was] to regard the formation of a planetary system around a star as a possible last stage in the formation of the star itself" (Chandrasekhar, 1946, 94). He believed that "the protoplanets were supposed to have formed at the sites of the ball bearing eddies and the merger of the protoplanets in the same orbit produced the known planets" (Abhyankar, 343). In the paper offered here, the Indian American astrophysicist S. Chandrasekhar challenged Weizsäcker's theory and showed "that there will be a wide spectrum of turbulence with smaller eddies within the larger ones and there would be no regular pattern as suggested by Weizsäcker. Further the life time of the eddies will be too short for the formation of the planets" (ibid). In other words, Chandrasekhar's work "indicated that the regular pattern of vortices originally postulated by Weizsäcker could not occur, but instead must be replaced by a range of eddy sizes" (Brush, A History of Modern Planetary Physics, 14). Chandrasekhar's work led to the abandonment of Weizsäcker's theories.

INCLUDED: Nobel Prize winner Percy Williams Bridgman's "Recent Work in the Field of High Pressures," pp. 1-94 (an important review of work done in the field of high pressure physics between Bridgman's seminal 1930 work and 1946, the year he won the prize) and R. Samuel's "The Dissociation Spectra of Covalent Polyatomic Molecules", pp. 103-148. CONDITION & DETAILS: Lancaster: American Physical Society. Complete issue in original wraps. 4to. (10.5 x 8 inches; 263 x 200mm). Very slight wear at the edges of the wraps and head and foot of the spine; small closed tear (see images). Bright and clean throughout. Very good condition.

Reviews

(Log in or Create an Account first!)

You’re rating the book as a work, not the seller or the specific copy you purchased!

Details

Bookseller
Atticus Rare Books US (US)
Bookseller's Inventory #
858
Title
Corrections and Additional Remarks to Our Paper (Einstein & Strauss) WITH On a New Theory of Weizsäcker on the Origin of the Solar System in Reviews of Modern Physics, 18, January 1946, pp. 148-149; pp. 94-103
Author
Einstein, Albert; Ernst G. Straus AND Chandrasekhar S
Book Condition
Used
Quantity Available
1
Edition
1st Edition
Binding
Paperback
Publisher
American Physical Society
Place of Publication
Lancaster
Date Published
1946

Terms of Sale

Atticus Rare Books

30 day return guarantee, with full refund including shipping costs for up to 30 days after delivery if an item arrives misdescribed or damaged.

About the Seller

Atticus Rare Books

Seller rating:
This seller has earned a 5 of 5 Stars rating from Biblio customers.
Biblio member since 2010
West Branch, Iowa

About Atticus Rare Books

We specialize in rare and unusual antiquarian books in the sciences and the history of science. Additionally, we specialize in 20th century physics, mathematics, and astronomy.

Glossary

Some terminology that may be used in this description includes:

Edges
The collective of the top, fore and bottom edges of the text block of the book, being that part of the edges of the pages of a...
New
A new book is a book previously not circulated to a buyer. Although a new book is typically free of any faults or defects, "new"...
G
Good describes the average used and worn book that has all pages or leaves present. Any defects must be noted. (as defined by AB...
First Edition
In book collecting, the first edition is the earliest published form of a book. A book may have more than one first edition in...

Frequently asked questions

tracking-