Nuclear reaction rates and the nova outburst

Sumner Starrfield, Christian Iliadis, James W. Truran, Michael Wiescher, Warren M. Sparks

Research output: Contribution to journalArticle

8 Scopus citations

Abstract

In this paper we examined the consequences of improving the nuclear reaction library on our simulations of TNRs on 1.25M WD and 1.35M WDs. We have found that the changes in the rates have affected the nucleosynthesis predictions of our calculations but not, to any great extent, the gross features. In addition, we have used a lower mass accretion rate than in our previous studies in order to accrete (and eject) more material. This has, as expected, caused the peak values of some important parameters to increase over our previous studies at the same WD mass. However, because some important reaction rates have declined in the new compilation this has not increased the abundances for nuclei above aluminum and, in fact, they have declined while the abundances of both 26Al and 27Al have increased at both WD masses. In contrast, the abundance of 22Na has declined at both WD masses over the values predicted in our earlier work. This has important implications with respect to predictions of the observability of novae with INTEGRAL.

Original languageEnglish (US)
Pages (from-to)110-117
Number of pages8
JournalNuclear Physics A
Volume688
Issue number1-2
DOIs
StatePublished - May 21 2001

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Fingerprint Dive into the research topics of 'Nuclear reaction rates and the nova outburst'. Together they form a unique fingerprint.

  • Cite this

    Starrfield, S., Iliadis, C., Truran, J. W., Wiescher, M., & Sparks, W. M. (2001). Nuclear reaction rates and the nova outburst. Nuclear Physics A, 688(1-2), 110-117. https://doi.org/10.1016/S0375-9474(01)00679-0