We have measured the ɑ-particle spectrum from the decay of ^(16)N by selecting a low-energy ^(16)N beam with the TRIUMF isotope separator, TISOL, stopping the ^(16)N nuclei in a foil, and counting the α, particles and ^(12)C recoil nuclei, in coincidence, in thin surface-barrier detectors. The spectrum has been fitted by R- and K-matrix parametrizations which include the measured ^(12)C(α, y)^(16)O and ^(12)C(α,y)^(12)C cross sections. Best fit values for S_(E1)(0.3) have been derived for the El part of the ^(12)C(α,y)^(16)O reaction. These are S_(E1)(0.3)=75±20 keV·barn and S_(E1)(0.3)=62±15 keV·barn for the R- and K-matrix parametrizations, respectively
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
straints on the low-energy E1 cross section of 12C(α, γ)16O from the β-delayed α spectrum of 16N, Ph...
The ^{12}C(α,γ)^{16}O reaction plays a central role in astrophysics, but its cross section at energi...
We have measured the ɑ-particle spectrum from the decay of ^(16)N by selecting a low-energy ^(16)N b...
The shape of the low-energy part of the β-delayed α-particle spectrum of 16N is very sensitive to th...
The low-energy part of the βα-decay spectrum of ^(16)N permits the determination of the reduced α-wi...
The α spectrum following the β decay of 16N from the isotope separator TISOL has been measured by de...
The low-energy part of the βɑ-decay spectrum of ^(16)N permits the determination of the reduced ɑ-wi...
It has proven to be very difficult to determine the astrophysically important cross section for ^(12...
Radiative alpha-capture by ^(12)C is a key process occurring during the helium-burning phase in red ...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
A measurement of the β-delayed α decay of N16 using a set of twin ionization chambers is described. ...
A new measurement of the β-delayed α decay of N16 has been performed using a set of high efficiency ...
The level matrix corresponding to the scrK-matrix parametrization of a resonant nuclear reaction is ...
The low energy part of the beta delayed, alpha spectrum of ^(16)N can be used to determine the p-wav...
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
straints on the low-energy E1 cross section of 12C(α, γ)16O from the β-delayed α spectrum of 16N, Ph...
The ^{12}C(α,γ)^{16}O reaction plays a central role in astrophysics, but its cross section at energi...
We have measured the ɑ-particle spectrum from the decay of ^(16)N by selecting a low-energy ^(16)N b...
The shape of the low-energy part of the β-delayed α-particle spectrum of 16N is very sensitive to th...
The low-energy part of the βα-decay spectrum of ^(16)N permits the determination of the reduced α-wi...
The α spectrum following the β decay of 16N from the isotope separator TISOL has been measured by de...
The low-energy part of the βɑ-decay spectrum of ^(16)N permits the determination of the reduced ɑ-wi...
It has proven to be very difficult to determine the astrophysically important cross section for ^(12...
Radiative alpha-capture by ^(12)C is a key process occurring during the helium-burning phase in red ...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
A measurement of the β-delayed α decay of N16 using a set of twin ionization chambers is described. ...
A new measurement of the β-delayed α decay of N16 has been performed using a set of high efficiency ...
The level matrix corresponding to the scrK-matrix parametrization of a resonant nuclear reaction is ...
The low energy part of the beta delayed, alpha spectrum of ^(16)N can be used to determine the p-wav...
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
straints on the low-energy E1 cross section of 12C(α, γ)16O from the β-delayed α spectrum of 16N, Ph...
The ^{12}C(α,γ)^{16}O reaction plays a central role in astrophysics, but its cross section at energi...