Published December 27, 2004 | Version v1
Journal article

Element synthesis calculations for stellar explosions: robust uncertainties, sensitivities, and radioactive ion beam measurements

  • 1. Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN (United States)
  • 2. Dept. of Physics and Astronomy, Univ. of Tennessee, Knoxville, TN (United States)
  • 3. Department of Physics and Astronomy, Arizona State Univ., Tempe, AZ (United States)
  • 4. Nuclear Engineering Division, Argonne National Laboratory, Argonne, IL (United States)

Description

We utilize multiple-zone, post-processing element synthesis calculations to determine the impact of recent ORNL radioactive ion beam measurements on predictions of novae and X-ray burst simulations. We also assess the correlations between all relevant reaction rates and all synthesized isotopes, and translate nuclear reaction rate uncertainties into abundance prediction uncertainties, via a unique Monte Carlo technique

Additional details

Identifiers

DOI
10.1016/j.nuclphysa.2004.09.091;
PII
S0375-9474(04)01056-5;

Publishing Information

Journal Title
Nuclear Physics. A
Journal Volume
746
Journal Issue
3-4
Journal Page Range
p. 565-568
ISSN
0375-9474
CODEN
NUPABL

Conference

Title
6. international conference on radioactive nuclear beams
Acronym
RNB6
Dates
22-26 Sep 2003
Place
Argonne, IL (United States)

Optional Information

Copyright
Copyright (c) 2004 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.