Isotopic S-32/S-33 ratio as a diagnostic of presolar grains from novae

TitleIsotopic S-32/S-33 ratio as a diagnostic of presolar grains from novae
Publication TypeJournal Article
Year of Publication2014
AuthorsParikh, A., K. Wimmer, T. Faestermann, R. Hertenberger, J. Jose, H. F. Wirth, C. Hinke, R. Krucken, D. Seiler, K. Steiger, and K. Straub
JournalPhysics Letters B
Volume737
Pagination314-319
Date PublishedOct
ISBN Number0370-2693
Accession NumberWOS:000342757700055
AbstractMeasurements of sulphur isotopes in presolar grains can help to identify the astrophysical sites in which these grains were formed. A more precise thermonuclear rate of the S-33(p, gamma)Cl-34 reaction is required, however, to assess the diagnostic ability of sulphur isotopic ratios. We have studied the S-33(He-3,d)Cl-34 proton-transfer reaction at 25 MeV using a high-resolution quadrupole-dipole-dipole-dipole magnetic spectrograph. Deuteron spectra were measured at ten scattering angles between 10 degrees and 55 degrees. Twenty-four levels in Cl-34 over E-x = 4.6-5.9 MeV were observed, including three levels for the first time. Proton spectroscopic factors were extracted for the first time for levels above the S-33 + p threshold, spanning the energy range required for calculations of the thermonuclear S-33(p, gamma)Cl-34 rate in classical nova explosions. We have determined a new S-33(p, gamma)Cl-34 rate using a Monte Carlo method and have performed new hydrodynamic nova simulations to determine the impact on nova nucleosynthesis of remaining nuclear physics uncertainties in the reaction rate. We find that these uncertainties lead to a factor of <= 5 variation in the S-33(p, gamma)Cl-34 rate over typical nova peak temperatures, and variation in the ejected nova yields of S-Ca isotopes by <= 20%. In particular, the predicted S-32/S-33 ratio is 110-130 for the nova model considered, compared to 110-440 with previous rate uncertainties. As recent type II supernova models predict ratios of 130-200, the S-32/S-33 ratio may be used to distinguish between grains of nova and supernova origin. (C) 2014 The Authors. Published by Elsevier B.V.
URL<Go to ISI>://WOS:000342757700055
DOI10.1016/j.physletb.2014.08.071
Short TitleIsotopic S-32/S-33 ratio as a diagnostic of presolar grains from novae
Website development by Checkmark Media. Designed by Armada.

a place of mind, The University of British Columbia

Faculty of Science
Department of Physics and Astronomy
6224 Agricultural Road
Vancouver, BC V6T 1Z1
Tel 604.822.3853
Fax 604.822.5324

Emergency Procedures | Accessibility | Contact UBC | © Copyright The University of British Columbia