A method has been developed to calculate (n, xn) cross-sections (x=2, 3, 4), taking into account pre-equilibrium emission of the first particle. Emission of subsequent particles is considered to be entirely due to the equilibrium mode. Based on this model the cross-sections have been calculated and compared for a number of nuclei in the mass region A=89 to 238 for incident energies from threshold to 28 MeV. Using the squared matrix element of Kalbach we found that the preequilibrium contribution was considerable at incident energy higher than 16 MeV. In general, agreement between the measured and the calculated cross-sections is within 10 to 15%. Cross-section for (n, 4n) reaction is also calculated and compared with the available data. The...
In this study, experimental neutron-emission spectra produced by (n, xn) reactions on nuclei 232Th h...
WOS: 000256885600036In this study, we investigate the pre-equilibrium effect by using new evaluated ...
In this study, a new version EMPIRE 3.2 code was used in the cross section calculations of (n,p) rea...
WOS: 000271863900006In this present study, by using equilibrium and pre-equilibrium reaction mechani...
WOS: 000289040300005Using pre-equilibrium reaction mechanisms, the neutron-emission spectra produced...
In this study, a new version EMPIRE 3.2 code was used in the cross section calculations of (n,p) rea...
WOS: 000225509800009The (n, 2n) reaction cross section calculations for some neighbouring target nuc...
WOS: 000245671800012In this study, the (n, p) reaction cross-sections of some target nuclei in the r...
In order to calculate unmeasured data, a new semi-empirical formula for the calculation of the (n,p)...
WOS: 000220785900011The (n,2n) reaction cross-section calculations for some neighbor deformed target...
WOS: 000314975600006In this study, the pre-equilibrium and equilibrium calculations of cross-section...
In this study, the pre-equilibrium and equilibrium calculations of cross-sections of 89Y(p, xn), 90Z...
During the last 10 years, in the general context of nuclear energy applications and future reactors ...
A recently developed model that combines compound and precompound reactions with conservation of ang...
Empirical formulas in determining the cross-sections play an important role at the energies of which...
In this study, experimental neutron-emission spectra produced by (n, xn) reactions on nuclei 232Th h...
WOS: 000256885600036In this study, we investigate the pre-equilibrium effect by using new evaluated ...
In this study, a new version EMPIRE 3.2 code was used in the cross section calculations of (n,p) rea...
WOS: 000271863900006In this present study, by using equilibrium and pre-equilibrium reaction mechani...
WOS: 000289040300005Using pre-equilibrium reaction mechanisms, the neutron-emission spectra produced...
In this study, a new version EMPIRE 3.2 code was used in the cross section calculations of (n,p) rea...
WOS: 000225509800009The (n, 2n) reaction cross section calculations for some neighbouring target nuc...
WOS: 000245671800012In this study, the (n, p) reaction cross-sections of some target nuclei in the r...
In order to calculate unmeasured data, a new semi-empirical formula for the calculation of the (n,p)...
WOS: 000220785900011The (n,2n) reaction cross-section calculations for some neighbor deformed target...
WOS: 000314975600006In this study, the pre-equilibrium and equilibrium calculations of cross-section...
In this study, the pre-equilibrium and equilibrium calculations of cross-sections of 89Y(p, xn), 90Z...
During the last 10 years, in the general context of nuclear energy applications and future reactors ...
A recently developed model that combines compound and precompound reactions with conservation of ang...
Empirical formulas in determining the cross-sections play an important role at the energies of which...
In this study, experimental neutron-emission spectra produced by (n, xn) reactions on nuclei 232Th h...
WOS: 000256885600036In this study, we investigate the pre-equilibrium effect by using new evaluated ...
In this study, a new version EMPIRE 3.2 code was used in the cross section calculations of (n,p) rea...