Add to ORKGA search for the {beta}{plus} decay of {sup 56}Ni has established an upper limit on the branching ratio of 7.2 {times} 10{sup {minus} 7} for the most likely such transition. This provides a lower limit of 2.3 {times} 10{sup 4} years for the cosmic ray half life of {sup 56}Ni. 2 refs., 2 figs
Radioactive ^(54)Mn, suggested as a clock for measuring the lifetime of heavy cosmic rays, has a po...
Measurements of the cosmic-ray ratio are compared with predictions from an inhomogeneousp/p disk-di†...
X-ray bursts have been suggested as a possible site for the astrophysical rp-process. The time scale...
A search for the {beta}{sup +} decay of {sup 54}Mn has established an upper limit of 4.4 {times} 10{...
A measurement of the 56Ni cosmic ray abundance has been discussed as a possible tool to determine th...
Supernovae should produce the radioactive nuclide ^(59)Ni, and in the ejecta of the explosions these...
Radionuclides in the galactic cosmic rays serve as chronometers for measuring the characteristic tim...
Measurements of the abundances of cosmic-ray ^(59)Ni and ^(59)Co are reported from the Cosmic-Ray Is...
The ratio Be/B depends on whether the confinement time of cosmic rays in the Galaxy is long or shor...
The most reliable method to estimate the residence time of cosmic rays in the Galaxy is based on the...
The proton-rich isotope Cu-56 was produced at the GSI On-Line Mass Separator by means of the Si-28(S...
Information on the origin, age and propagation of cosmic ray nuclei can be obtained from a detailed ...
\textsc{Gerda} published the best limit on $^{76}$Ge $0\nu\beta\beta$ decay's half-life of $T_{1/2}^...
The beta decay of Ni-53,Ni-54, Co-52,Co-53, Fe-51, and Mn-50 was investigated via the fragmentation ...
Journals published by the American Physical Society can be found at http://publish.aps.org/We measur...
Radioactive ^(54)Mn, suggested as a clock for measuring the lifetime of heavy cosmic rays, has a po...
Measurements of the cosmic-ray ratio are compared with predictions from an inhomogeneousp/p disk-di†...
X-ray bursts have been suggested as a possible site for the astrophysical rp-process. The time scale...
A search for the {beta}{sup +} decay of {sup 54}Mn has established an upper limit of 4.4 {times} 10{...
A measurement of the 56Ni cosmic ray abundance has been discussed as a possible tool to determine th...
Supernovae should produce the radioactive nuclide ^(59)Ni, and in the ejecta of the explosions these...
Radionuclides in the galactic cosmic rays serve as chronometers for measuring the characteristic tim...
Measurements of the abundances of cosmic-ray ^(59)Ni and ^(59)Co are reported from the Cosmic-Ray Is...
The ratio Be/B depends on whether the confinement time of cosmic rays in the Galaxy is long or shor...
The most reliable method to estimate the residence time of cosmic rays in the Galaxy is based on the...
The proton-rich isotope Cu-56 was produced at the GSI On-Line Mass Separator by means of the Si-28(S...
Information on the origin, age and propagation of cosmic ray nuclei can be obtained from a detailed ...
\textsc{Gerda} published the best limit on $^{76}$Ge $0\nu\beta\beta$ decay's half-life of $T_{1/2}^...
The beta decay of Ni-53,Ni-54, Co-52,Co-53, Fe-51, and Mn-50 was investigated via the fragmentation ...
Journals published by the American Physical Society can be found at http://publish.aps.org/We measur...
Radioactive ^(54)Mn, suggested as a clock for measuring the lifetime of heavy cosmic rays, has a po...
Measurements of the cosmic-ray ratio are compared with predictions from an inhomogeneousp/p disk-di†...
X-ray bursts have been suggested as a possible site for the astrophysical rp-process. The time scale...