activity
20042026
most citedActivation measurement of the 3He(alpha,gamma)7Be cross section at low energy

153 citations · 2.1k across the 63 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2024★ 22 cited

Solar fusion III: New data and theory for hydrogen-burning stars

B. Acharya, M. Aliotta, A. B. Balantekin +47

In stars that lie on the main sequence in the Hertzsprung-Russel diagram, like our sun, hydrogen is fused to helium in a number of nuclear reaction chains and series, such as the p…

astro-ph.SR2017

Constraining the Be()B -factor with the new precise Be solar neutrino flux from Borexino

Marcell P. Takács, Daniel Bemmerer, Arnd R. Junghans +1

Among the solar fusion reactions, the rate of the Be()B reaction is one of the most difficult to determine rates. In a number of previous experiments, its astrophysica…

astro-ph.SR2017

Origin of meteoritic stardust unveiled by a revised proton-capture rate of O

M. Lugaro, A. I. Karakas, C. G. Bruno +34

Stardust grains recovered from meteorites provide high-precision snapshots of the isotopic composition of the stellar environment in which they formed. Attributing their origin to…

astro-ph.SR2016★ 49 cited

Ne and Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for Ne(p,)Na

A. Slemer, P. Marigo, D. Piatti +36

We investigate the impact of the new LUNA rate for the nuclear reaction NeNa on the chemical ejecta of intermediate-mass stars, with particular focus on the ther…

astro-ph.SR2016★ 32 cited

The impact of the revised ON reaction rate on O stellar abundances and yields

O. Straniero, C. G. Bruno, M. Aliotta +33

Context. Material processed by the CNO cycle in stellar interiors is enriched in 17O. When mixing processes from the stellar surface reach these layers, as occurs when stars become…

astro-ph.SR2012★ 58 cited

First Direct Measurement of the ^{17}O(p,γ)^{18}F Reaction Cross-Section at Gamow Energies for Classical Novae

D. A. Scott, A. Caciolli, A. DiLeva +29

Classical novae are important contributors to the abundances of key isotopes, such as the radioactive ^{18}F, whose observation by satellite missions could provide constraints on n…