| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9851303 | Nuclear Physics A | 2005 | 4 Pages |
Abstract
This paper reports on the detailed rp-process reaction flow on an accreting neutron star and the resulting ashes of a type I X-ray burst. It is obtained by coupling a 298 isotope reaction network to a self-consistent one-dimensional model calculation with a constant accretion rate of MË=1017Â g/s.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
J.L. Fisker, E.F. Brown, M. Liebendörfer, F.-K. Thielemann, M. Wiescher,