activity
20112021
most citedAstrophysical S-factor of the reaction at 0.4 -- 1.3\,MeV

34 citations · 138 across the 9 of their papers we have counts for

collaborators

10 papers

nucl-ex20218 cited

Measurement of the 91Zr(p,gamma)92mNb cross section motivated by type Ia supernova nucleosynthesis

Gy. Gyürky, Z. Halász, G. G. Kiss +6

The synthesis of heavy, proton rich isotopes is a poorly understood astrophysical process. Thermonuclear (type Ia) supernova explosions are among the suggested sites and the abunda…

nucl-ex20204 cited

Determination of luminosity for in-ring reactions: A new approach for the low-energy domain

Y. M. Xing, J. Glorius, L. Varga +59

Luminosity is a measure of the colliding frequency between beam and target and it is a crucial parameter for the measurement of absolute values, such as reaction cross sections. In…

physics.acc-ph2018

The new Felsenkeller 5 MV underground accelerator

Daniel Bemmerer, Thomas E. Cowan, Alexander Domula +18

The field of nuclear astrophysics is devoted to the study of the creation of the chemical elements. By nature, it is deeply intertwined with the physics of the Sun. The nuclear rea…

nucl-ex201734 cited

Astrophysical S-factor of the reaction at 0.4 -- 1.3\,MeV

L. Wagner, S. Akhmadaliev, M. Anders +18

The reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning and thus determines its rate. The precise knowl…

astro-ph.CO201528 cited

Constraining Big Bang lithium production with recent solar neutrino data

Marcell P. Takács, Daniel Bemmerer, Tamás Szücs +1

The 3He(α,γ)7Be reaction affects not only the production of 7Li in Big Bang nucleosynthesis, but also the fluxes of 7Be and 8B neutrinos from the Sun. This double role is exploited…

nucl-ex201520 cited

Measurement of (alpha,n) reaction cross sections of erbium isotopes for testing astrophysical rate predictions

G. G Kiss, T. Szücs, T. Rauscher +5

The -process in core-collapse and/or type Ia supernova explosions is thought to explain the origin of the majority of the so-called nuclei (the 35 proton-rich isotopes betwe…