Add to ORKGMeasuring nuclear reactions of astrophysical interest at the relevant energies is not always possible on the Earth\u2019s surface because of the cosmic-ray background that dominates the spectra. The LUNA collaboration exploits the lowbackground enviroment of Gran Sasso National Laboratory to study these reactions at or close to the Gamow peak. The latest experimental efforts included the measurement of the 15N(p,\u3b3)16O at beam energies between 77 and 350 keV. The status of these measurements is summarised in this contribution
Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it i...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
Measuring nuclear reactions of astrophysical interest at the relevant energies is not always possibl...
Measuring nuclear reactions of astrophysical interest at the relevant energies is not always possibl...
The aim of experimental nuclear astrophysics is to provide information on the nuclear processes invo...
LUNA (Laboratory for Underground Nuclear Astrophysics) is a nuclear astrophysics experiment running ...
Precise knowledge of nuclear cross sections at stellar energies is of importance for cosmology as we...
One of the main ingredients of nuclear astrophysics is the knowledge of the thermonuclear reactions ...
One of the main ingredients of nuclear astrophysics is the knowledge of the thermonuclear reactions ...
The evolution of celestial bodies is regulated by gravitation and thermonuclear reaction rates, whil...
Nuclear astrophysics strives for a comprehensive picture of the nuclear reactions responsible for sy...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
The CNO cycle consists of a set of nuclear reactions that convert hydrogen into helium and releases ...
Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it i...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
Measuring nuclear reactions of astrophysical interest at the relevant energies is not always possibl...
Measuring nuclear reactions of astrophysical interest at the relevant energies is not always possibl...
The aim of experimental nuclear astrophysics is to provide information on the nuclear processes invo...
LUNA (Laboratory for Underground Nuclear Astrophysics) is a nuclear astrophysics experiment running ...
Precise knowledge of nuclear cross sections at stellar energies is of importance for cosmology as we...
One of the main ingredients of nuclear astrophysics is the knowledge of the thermonuclear reactions ...
One of the main ingredients of nuclear astrophysics is the knowledge of the thermonuclear reactions ...
The evolution of celestial bodies is regulated by gravitation and thermonuclear reaction rates, whil...
Nuclear astrophysics strives for a comprehensive picture of the nuclear reactions responsible for sy...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
The CNO cycle consists of a set of nuclear reactions that convert hydrogen into helium and releases ...
Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it i...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...