The reaction 12C(α,γ)16O is of paramount importance for the nucleosynthesis of heavier elements in stars. It takes place during helium burning and determines the abundance of 12C and 16O at the end of this burning stage and therefore influences subsequent nuclear reactions. Currently the cross section at astrophysically relevant energies is not known with satisfactory precision. Due to the low cross section of the reaction, low background, high beam intensities and target thicknesses are necessary for experiments. Therefore a new laboratory hosting a 5 MV ion accelerator, was built in the shallow-underground tunnels of Felsenkeller. The main background component in such laboratories was investigated with a muon telescope in this thesis. It ...
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies t...
International audienceThe production of intense beams of light radioactive nuclei can be achieved at...
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies t...
The relevant interaction energies for astrophysical radiative capture reactions are very low, much b...
Low-background experiments with stable ion beams are an important tool for putting the model of stel...
The 13C(α, n)16O reaction determines the dominant neutron source of the sprocess in thermally pulsin...
Since understanding and quantifying cosmic ray induced radioactive backgrounds in copper and germani...
The 13C(α, n)16O reaction determines the dominant neutron source of the sprocess in thermally pulsin...
The 12C(p,γ) and 13C(p,γ) reaction cross sections are currently under investigation in the low-backg...
A muon collider represents the ideal machine to reach very high center-of-mass energies and luminosi...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
Low-background experiments with stable ion beams are an important tool for putting the model of stel...
The fusion reactions 12C(12C,a)20Ne and 12C(12C,p)23Na have been studied from E = 2.10 to 4.75 MeV b...
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to...
Favored by the low background in underground laboratories, low-background accelerator-based experime...
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies t...
International audienceThe production of intense beams of light radioactive nuclei can be achieved at...
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies t...
The relevant interaction energies for astrophysical radiative capture reactions are very low, much b...
Low-background experiments with stable ion beams are an important tool for putting the model of stel...
The 13C(α, n)16O reaction determines the dominant neutron source of the sprocess in thermally pulsin...
Since understanding and quantifying cosmic ray induced radioactive backgrounds in copper and germani...
The 13C(α, n)16O reaction determines the dominant neutron source of the sprocess in thermally pulsin...
The 12C(p,γ) and 13C(p,γ) reaction cross sections are currently under investigation in the low-backg...
A muon collider represents the ideal machine to reach very high center-of-mass energies and luminosi...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
Low-background experiments with stable ion beams are an important tool for putting the model of stel...
The fusion reactions 12C(12C,a)20Ne and 12C(12C,p)23Na have been studied from E = 2.10 to 4.75 MeV b...
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to...
Favored by the low background in underground laboratories, low-background accelerator-based experime...
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies t...
International audienceThe production of intense beams of light radioactive nuclei can be achieved at...
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies t...