For the study of astrophysically relevant capture reactions in the underground laboratory LUNA a new setup of high sensitivity has been implemented. The setup includes a windowless gas target, a 4p BGO summing crystal, and beam calorimeters. The setup has been recently used to measure the d(p,g)3He cross-section for the first time within its sola
LUNA is an experimental approach for the study of nuclear fusion reactions based on an underground a...
Direct measurements of small nuclear reaction cross sections require a low background in the signal ...
Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it i...
For the study of astrophysically relevant capture reactions in the underground laboratory LUNA a new...
The electron screening effect has been studied by measuring the cross section of the reaction D(3He,...
A compact high-current 50 kV ion accelerator facility including a windowless gas target system, a be...
The goal of nuclear astrophysics is to measure cross-sections of nuclear physics reactions of intere...
The aim of experimental nuclear astrophysics is to provide information on the nuclear processes invo...
The reaction 3He(3He,2p)4He has been studied for the first time over the whole thermal energy region...
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 ...
Cross section measurements for quiescent stellar H-burning are hampered mainly by extremely low coun...
Accurate knowledge of thermonuclear reaction rates is important in understanding the generation of e...
Accurate knowledge of thermonuclear reaction rates is important in understanding the generation of e...
Abstract Accurate knowledge of thermonuclear reaction rates is important in understanding the genera...
LUNA is an experimental approach for the study of nuclear fusion reactions based on an underground a...
Direct measurements of small nuclear reaction cross sections require a low background in the signal ...
Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it i...
For the study of astrophysically relevant capture reactions in the underground laboratory LUNA a new...
The electron screening effect has been studied by measuring the cross section of the reaction D(3He,...
A compact high-current 50 kV ion accelerator facility including a windowless gas target system, a be...
The goal of nuclear astrophysics is to measure cross-sections of nuclear physics reactions of intere...
The aim of experimental nuclear astrophysics is to provide information on the nuclear processes invo...
The reaction 3He(3He,2p)4He has been studied for the first time over the whole thermal energy region...
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 ...
Cross section measurements for quiescent stellar H-burning are hampered mainly by extremely low coun...
Accurate knowledge of thermonuclear reaction rates is important in understanding the generation of e...
Accurate knowledge of thermonuclear reaction rates is important in understanding the generation of e...
Abstract Accurate knowledge of thermonuclear reaction rates is important in understanding the genera...
LUNA is an experimental approach for the study of nuclear fusion reactions based on an underground a...
Direct measurements of small nuclear reaction cross sections require a low background in the signal ...
Accurate knowledge of thermonuclear reaction rates is a key issue in nuclear astrophysics since it i...