First measurement of the 34S(p,gamma)35Cl reaction rate through indirect methods for presolar nova grains

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dc.contributor	Universitat Politècnica de Catalunya. Departament de Física
dc.contributor	Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.contributor.author	Gillespie, S
dc.contributor.author	Parikh, A.
dc.contributor.author	Barton, C
dc.contributor.author	Faestermann, Thomas
dc.contributor.author	José Pont, Jordi
dc.contributor.author	Hertenberger, R.
dc.contributor.author	Wirth, Hans Friedrich
dc.contributor.author	de Séréville, N
dc.contributor.author	Riley, J
dc.contributor.author	Williams, M
dc.date	2017-08-02
dc.identifier.citation	Gillespie, S., Parikh, A., Barton, C., Faestermann, T., Jose, J., Hertenberger, R., Wirth, H., de Séréville, N., Riley, J., Williams, M. First measurement of the 34S(p,gamma)35Cl reaction rate through indirect methods for presolar nova grains. "Physical Review C", 2 Agost 2017, vol. 96, núm. 2, p. 1-8.
dc.identifier.citation	2469-9985
dc.identifier.citation	10.1103/PhysRevC.96.025801
dc.identifier.uri	http://hdl.handle.net/2117/109218
dc.language.iso	eng
dc.publisher	AMER PHYSICAL SOC
dc.relation	https://journals.aps.org/prc/abstract/10.1103/PhysRevC.96.025801
dc.rights	Attribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights	info:eu-repo/semantics/openAccess
dc.rights	http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Astrophysics
dc.subject	Astrofísica
dc.title	First measurement of the 34S(p,gamma)35Cl reaction rate through indirect methods for presolar nova grains
dc.type	info:eu-repo/semantics/submittedVersion
dc.type	info:eu-repo/semantics/article
dc.description.abstract	Sulphur isotopic ratio measurements may help to establish the astrophysical sites in which certain presolar grains were formed. Nova model predictions of the 34S/32S ratio are, however, unreliable due to the lack of an experimental 34S(p,¿)35Cl reaction rate. To this end, we have measured the 34S(3He,d)35Cl reaction at 20 MeV using a high resolution quadrupole-dipole-dipole-dipole magnetic spectrograph. Twenty-two levels over 6.2 MeV

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