CaltechTHESIS
  A Caltech Library Service

The ^(26)Al(p,γ)^(27)Si reaction : stellar origins of galactic ^(26)Al

Citation

Vogelaar, Robert Bruce (1989) The ^(26)Al(p,γ)^(27)Si reaction : stellar origins of galactic ^(26)Al. Dissertation (Ph.D.), California Institute of Technology. http://resolver.caltech.edu/CaltechTHESIS:08262013-145328209

Abstract

To explain the ^(26)Mg isotopic anomaly seen in meteorites (^(26)Al daughter) as well as the observation of 1809-keV γ rays in the interstellar medium (live decay of 26Al) one must know, among other things, the destruction rate of ^(26)Al. Properties of states in ^(27)Si just above the ^(26)Al + p mass were investigated to determine the destruction rate of ^(26)Al via the ^(26)Al(p,γ)^(27)Si reaction at astrophysical temperatures.

Twenty micrograms of ^(26)Al were used to produce two types of Al_2O_3 targets by evaporation of the oxide. One was onto a thick platinum backing suitable for (p,γ) work, and the other onto a thin carbon foil for the (^3He,d) reaction.

The ^(26)Al(p,γ)^(27)Si excitation function, obtained using a germanium detector and voltage-ramped target, confirmed known resonances and revealed new ones at 770, 847, 876, 917, and 928 keV. Possible resonances below the lowest observed one at E_p = 286 keV were investigated using the ^(26)Al(^3He,d)^(27)Si proton-transfer reaction. States in 27Si corresponding to 196- and 286-keV proton resonances were observed. A possible resonance at 130 keV (postulated in prior work) was shown to have a strength of wγ less than 0.02 µeV.

By arranging four large Nal detector as a 47π calorimeter, the 196-keV proton resonance, and one at 247 keV, were observed directly, having wγ = 55± 9 and 10 ± 5 µeV, respectively.

Large uncertainties in the reaction rate have been reduced. At novae temperatures, the rate is about 100 times faster than that used in recent model calculations, casting some doubt on novae production of galactic ^(26)Al.

Item Type:Thesis (Dissertation (Ph.D.))
Subject Keywords:Physics
Degree Grantor:California Institute of Technology
Division:Physics, Mathematics and Astronomy
Major Option:Physics
Thesis Availability:Restricted to Caltech community only
Research Advisor(s):
  • Kavanagh, Ralph William
Thesis Committee:
  • Unknown, Unknown
Defense Date:4 April 1989
Record Number:CaltechTHESIS:08262013-145328209
Persistent URL:http://resolver.caltech.edu/CaltechTHESIS:08262013-145328209
Default Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:7945
Collection:CaltechTHESIS
Deposited By: Benjamin Perez
Deposited On:26 Aug 2013 23:40
Last Modified:26 Aug 2013 23:40

Thesis Files

[img] PDF - Final Version
Restricted to Caltech community only
See Usage Policy.

24Mb

Repository Staff Only: item control page