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Why the Cosmological Constant Is Small and Positive in Science 312 No. 5777 pp. 1180 - 1183, May 26, 2006

Why the Cosmological Constant Is Small and Positive in Science 312 No. 5777 pp. 1180 - 1183, May 26, 2006

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Why the Cosmological Constant Is Small and Positive in Science 312 No. 5777 pp. 1180 - 1183, May 26, 2006

de Steinhardt, Paul J.; Turok, Neil Geoffrey

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Sobre este artículo

New York: AAAS, 2006. 1st Edition. FIRST EDITION IN ORIGINAL WRAPS OF STEINHARDT & TUROK'S EXPLANATION OF HOW THEIR 2002 CYCLIC THEORY OF THE UNIVERSE CAN RESOLVE THE COSMOLOGICAL CONSTANT PROBLEM. Steinhardt and Turok's 2002 cyclic universe theory is a model of cosmic evolution according to which the universe undergoes endless cycles of expansion and cooling, each beginning with a "big bang" and ending in a "big crunch" (Steinhardt, Cyclic Universe Theory, 2009). In the paper offered here, the 2006 paper, the two show "how the cyclic model could naturally incorporate a mechanism for relaxing the cosmological constant to very small values, consistent with current observations" (WP). We separately offer a second copy of both the 2002 paper and the 2002 paper together with the 2006.

The model has also been known as the ekpyrotic cyclic universe theory. Paul Joseph Steinhart is an American theoretical physicist and cosmologist, currently the Albert Einstein Professor in Science at Princeton University. Beginning in 2001 and working with the South African physicist Neil Geoffrey Turok, Steinhardt and Turok put forth the ekpyrotic theory which, in essence, envisions a big bounce rather than a big bang. "According to this model, the current expanding universe emerges from a bounce that occurred 13.7 billion years ago and that is a result of the preceding (contracting) universe. The smoothing and flattening of the universe and the generation of density variations occur during the phase of slow contraction before the bounce and remain after the bounce" (Wikipedia). In their own words: "The Cyclic Model attempts to resolve the homogeneity, isotropy, and flatness problems and generate a nearly scale-invariant spectrum of fluctuations during a period of slow contraction that precedes a bounce to an expanding phase. Here we describe at a conceptual level the recent developments that have greatly simplified our understanding of the contraction phase and the Cyclic Model overall (Steinhardt & Turok, 24 May 2002). CONDITION & DETAILS: New York: AAAS. Complete 1st edition in original wraps, complete. 8vo. Bright and clean inside and out. Near fine condition.

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Detalles

Librería
Atticus Rare Books US (US)
Inventario del vendedor #
1473
Título
Why the Cosmological Constant Is Small and Positive in Science 312 No. 5777 pp. 1180 - 1183, May 26, 2006
Autor
Steinhardt, Paul J.; Turok, Neil Geoffrey
Estado del libro
Usado
Cantidad disponible
1
Edición
1st Edition
Encuadernación
Tapa blanda
Editorial
AAAS
Lugar de publicación
New York
Fecha de publicación
2006

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Atticus Rare Books

Puntuación del vendedor:
Este vendedor ha conseguido 5 de las cinco estrellas otorgadas por los compradores de Biblio.
Miembro de Biblio desde 2010
West Branch, Iowa

Sobre 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.

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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...
Fine
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