The problem of the magnitude of the S--factor of the hep process $p + {^3\mathrm{He}} \to {^4\mathrm{He}} + e^+ + \nu_e$ is one of the most important unsolved problems in nuclear astrophysics. The magnitude of $S(hep)$ has also an important impact on the interpretation of the Super-Kamiokande solar neutrino results in terms of neutrino oscillations. We point out the possiblity to determine the major hadronic contribution to $S(hep)$ from the measurement of the total cross section of the process $n + {^3\mathrm{H}} \to {^4\mathrm{He}} + e^- + \bar{\nu}_e$ in experiments with high intensity beams of thermal or cold neutrons
3 pags., 1 tab. -- Nuclear Physics in Astrophysics V 3–8 April 2011, Eilat, IsraelThe astrophysical ...
The astrophysical factor for the proton weak capture on {sup 3}He is calculated with correlated-hype...
The astrophysical factor for the proton weak capture on 3He is calculated with correlated-hyperspher...
We discuss the problem of solar hep neutrinos originating from the reaction p + 3He -> 4He + e+ + nu...
We discuss the problem of solar hep neutrinos originating from the reaction p+ 3He -> 4He + e+ + nu ...
The results of a new calculation of the astrophysical S-factor for the proton weak capture on He-3 a...
The S-factor for the {sup 3}He(p,e+ve){sup 4}He reaction has been recently calculated using realisti...
High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4He with a large end point...
Key Words solar burning, solar neutrinos, neutrino oscillations, effective field theory PACS Codes 2...
The plasma astrophysical S factor for the He3(d,p)He4 fusion reaction was measured for the first tim...
The astrophysical S factor for the proton weak capture on He-3 is calculated with correlated-hypersp...
The astrophysical factor for the proton weak capture on He-3 is calculated with correlated hypersphe...
We have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(...
The excess of highest energy solar-neutrino events recently observed by Superkamiokande can be in pr...
The astrophysical S-factor for the proton weak capture on {sup 3}He is calculated with correlated-hy...
3 pags., 1 tab. -- Nuclear Physics in Astrophysics V 3–8 April 2011, Eilat, IsraelThe astrophysical ...
The astrophysical factor for the proton weak capture on {sup 3}He is calculated with correlated-hype...
The astrophysical factor for the proton weak capture on 3He is calculated with correlated-hyperspher...
We discuss the problem of solar hep neutrinos originating from the reaction p + 3He -> 4He + e+ + nu...
We discuss the problem of solar hep neutrinos originating from the reaction p+ 3He -> 4He + e+ + nu ...
The results of a new calculation of the astrophysical S-factor for the proton weak capture on He-3 a...
The S-factor for the {sup 3}He(p,e+ve){sup 4}He reaction has been recently calculated using realisti...
High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4He with a large end point...
Key Words solar burning, solar neutrinos, neutrino oscillations, effective field theory PACS Codes 2...
The plasma astrophysical S factor for the He3(d,p)He4 fusion reaction was measured for the first tim...
The astrophysical S factor for the proton weak capture on He-3 is calculated with correlated-hypersp...
The astrophysical factor for the proton weak capture on He-3 is calculated with correlated hypersphe...
We have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(...
The excess of highest energy solar-neutrino events recently observed by Superkamiokande can be in pr...
The astrophysical S-factor for the proton weak capture on {sup 3}He is calculated with correlated-hy...
3 pags., 1 tab. -- Nuclear Physics in Astrophysics V 3–8 April 2011, Eilat, IsraelThe astrophysical ...
The astrophysical factor for the proton weak capture on {sup 3}He is calculated with correlated-hype...
The astrophysical factor for the proton weak capture on 3He is calculated with correlated-hyperspher...