Astrophysical relevance of gamma transition energies

dc.contributor.author	Rauscher, T.
dc.date.accessioned	2013-04-30T08:30:00Z
dc.date.available	2013-04-30T08:30:00Z
dc.date.issued	2008-09
dc.identifier.citation	Rauscher , T 2008 , ' Astrophysical relevance of gamma transition energies ' , Physical Review C (nuclear physics) , vol. 78 , no. 3 , 032801 . https://doi.org/10.1103/PhysRevC.78.032801
dc.identifier.issn	2469-9985
dc.identifier.uri	http://hdl.handle.net/2299/10607
dc.description.abstract	The relevant gamma energy range is explicitly identified where additional gamma strength must be located to have an impact on astrophysically relevant reactions. It is shown that folding the energy dependences of the transmission coefficients and the level density leads to maximal contributions for gamma energies of 2	en
dc.format.extent	5
dc.format.extent	157434
dc.language.iso	eng
dc.relation.ispartof	Physical Review C (nuclear physics)
dc.subject	PHOTON SCATTERING
dc.subject	R-PROCESS
dc.subject	PROCESS NUCLEOSYNTHESIS
dc.subject	DENSITY
dc.subject	RATES
dc.subject	MODES
dc.subject	DIPOLE STRENGTH
dc.subject	NUCLEI
dc.subject	NEUTRON
dc.subject	CROSS-SECTION
dc.title	Astrophysical relevance of gamma transition energies	en
dc.contributor.institution	Centre for Astrophysics Research
dc.description.status	Peer reviewed
rioxxterms.versionofrecord	10.1103/PhysRevC.78.032801
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true