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20032019
most citedGalactic Evolution of Sr, Y, Zr: A Multiplicity of Nucleosynthetic Processes

642 citations · 746 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2019★ 1 cited

Impact of Uncertainties in Nuclear Reaction Cross Sections on p-Nucleosynthesis in Thermonuclear Supernovae

T. Rauscher, N. Nishimura, G. Cescutti +3

The propagation of uncertainties in reaction cross sections and rates of neutron-, proton-, and alpha-induced reactions into the final isotopic abundances obtained in nucleosynthes…

astro-ph.HE2014

Production of 92Nb, 92Mo, and 146Sm in the gamma-process in SNIa

T. Rauscher, C. Travaglio, R. Gallino +2

The knowledge of the production of extinct radioactivities like 92Nb and 146Sm by photodisintegration processes in ccSN and SNIa models is essential for interpreting abundances in…

astro-ph.SR2014★ 54 cited

Testing the role of SNe Ia for Galactic chemical evolution of p-nuclei with 2D models and with s-process seeds at different metallicities

C. Travaglio, R. Gallino, T. Rauscher +2

The bulk of p isotopes is created in the 'gamma processes' mainly by sequences of photodisintegrations and beta decays in explosive conditions in Type Ia supernovae (SNIa) or in co…

astro-ph.SR2014★ 49 cited

Radiogenic p-isotopes from SNIa, nuclear physics uncertainties and Galactic chemical evolution compared with values in primitive meteorites

C. Travaglio, R. Gallino, T. Rauscher +3

The nucleosynthesis of proton-rich isotopes is calculated for multi-dimensional Chandrasekhar-mass models of Type Ia supernovae with different metallicities. The predicted abundanc…

astro-ph.SR2012

Impact of Nuclear Reaction Uncertainties on AGB Nucleosynthesis Models

S. Bisterzo, R. Gallino, F. Kaeppeler +2

Asymptotic giant branch (AGB) stars with low initial mass (1 - 3 Msun) are responsible for the production of neutron-capture elements through the main s-process (main slow neutron…

astro-ph2003★ 642 cited

Galactic Evolution of Sr, Y, Zr: A Multiplicity of Nucleosynthetic Processes

Claudia Travaglio, Roberto Gallino, Enrico Arnone +3

We follow the Galactic enrichment of three easily observed light n-capture elements Sr,Y,and Zr.Input stellar yields have been first separated into their respective main and weak s…