Published March 1970
| Version Published
Journal Article
Open
Stellar Reaction Rates for ^(28)Si
Abstract
Stellar rates for the reactions ^(27)Al(p,-y)^(28)Si and ^(24)Mg(ɑ,-y)^(28)Si have been calculated from new cross- section data for these reactions. The contributions to the interaction rates, (σv)_(py) and (σv)_(ay), and to the corresponding photodisintegration rates, λ_(yp) and λ_(ya), from the excited states of ^(27)Al, ^(24)Mg, and ^(28)Si are discussed. The calculated interaction rates, N_A(σv), are listed for temperatures from 0.1 X 10^9º to 5.0 X 10^9° K; two- and four-parameter fits are given for N_A(σv) as a function of temperature.
Additional Information
© 1970 American Astronomical Society. Supported in part by the National Science Foundation [GP-9114) and the Office of Naval Research [Nonr-220(47)]. The authors wish to acknowledge the assistance of their colleagues in the Kellogg Radiation Laboratory, particularly B.A. Zimmerman. Informative discussions with Dr. J. W. Truran, on methods for estimating the excited-state interaction rates, are gratefully acknowledged.Attached Files
Published - 1970ApJ___159__913L.pdf
Files
1970ApJ___159__913L.pdf
Files
(164.9 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:8943d1c672e015c59853222c61a19c91
|
164.9 kB | Preview Download |
Additional details
Identifiers
- Eprint ID
- 60127
- Resolver ID
- CaltechAUTHORS:20150909-112604913
Related works
- Describes
- http://adsabs.harvard.edu/abs/1970ApJ...159..913L (URL)
Funding
- NSF
- GP-9114
- Office of Naval Research (ONR)
- Nonr-220(47)
Dates
- Created
-
2015-09-11Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field