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Duration of Nucleosynthesis

Wasserburg, G. J. and Fowler, William A. and Hoyle, F. (1960) Duration of Nucleosynthesis. Physical Review Letters, 4 (3). pp. 112-114. ISSN 0031-9007. http://resolver.caltech.edu/CaltechAUTHORS:WASprl60

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Abstract

In a recent Letter on a determination of the age of the elements, Reynolds[1] reported the important discovery of isotopically anomalous xenon in the stony meteorite Richarton. The isotopes which appear to occur in significant excess over atmospheric xenon are Xe128, Xe129, Xe130, and Xe131, with the Xe129 dominant by an order of magnitude. At present it does not appear possible to explain all of these data by any single mechanism. Because of the existence of these four anomalies, it is difficult to conclude that the Xe129 excess is simply the product of I129 decay.


Item Type:Article
Additional Information:©1960 The American Physical Society Received 11 January 1960 Supported in part by the Alfrd P. Sloan Foundation and the joint program of the Office of Naval Research and the U.S. Atomic Energy Commission.
Record Number:CaltechAUTHORS:WASprl60
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:WASprl60
Alternative URL:http://dx.doi.org/10.1103/PhysRevLett.4.112
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:5262
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:06 Oct 2006
Last Modified:18 Sep 2014 18:11

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