Lifetimes of states in 19Ne above the 15 O + alpha breakup threshold

Simple item page
dc.creatorMythili, S.
dc.creatorDavids, B.
dc.creatorAlexander, T. K.
dc.creatorBall, G. C.
dc.creatorChicoine, M.
dc.creatorChakrawarthy, R. S.
dc.creatorChurchman, R.
dc.creatorForster, J. S.
dc.creatorGujrathi, S.
dc.creatorHackman, G.
dc.creatorHowell, D.
dc.creatorKanungo, R.
dc.creatorLeslie, J. R.
dc.creatorPadilla, E.
dc.creatorPearson, C. J.
dc.creatorRuiz, C.
dc.creatorRuprecht, G.
dc.creatorSchumaker, M. A.
dc.creatorTanihata, I.
dc.creatorVockenhuber, C.
dc.creatorWalden, P.
dc.creatorYen, S.
dc.date2007-11-06
dc.date.accessioned2026-07-07T11:12:56Z
dc.date.available2026-07-07T11:12:56Z
dc.descriptionThe 15O(alpha,gamma)19Ne reaction plays a role in the ignition of Type I x-ray bursts on accreting neutron stars. The lifetimes of states in 19Ne above the 15O + alpha threshold of 3.53 MeV are important inputs to calculations of the astrophysical reaction rate. These levels in 19Ne were populated in the 3He(20Ne,alpha)19Ne reaction at a 20Ne beam energy of 34 MeV. The lifetimes of six states above the threshold were measured with the Doppler shift attenuation method (DSAM). The present measurements agree with previous determinations of the lifetimes of these states and in some cases are considerably more precise.
dc.identifierhttps://arxiv.org/abs/0711.0777
dc.identifierhttp://arxiv.org/abs/0711.0777
dc.identifierPhys.Rev.C77:035803,2008
dc.identifierdoi:10.1103/PhysRevC.77.035803
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191547
dc.subjectNuclear Experiment
dc.titleLifetimes of states in 19Ne above the 15 O + alpha breakup threshold
dc.typetext

Files

Collections

arXiv