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Cited by 14 publications
(2 citation statements)
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“…Other sources of systematic errors concern the experimental conditions. Some of the most important problems there involve inefficient neutron-γ discrimination (often done by time-of-flight techniques as in [30], or by simply considering γ rays only at backward angles as in [49]), contamination of highenergy γ spectra by cosmic rays (which can be greatly reduced by coincidence measurements as in [50]), target impurities, pile-up (see, e.g., [51] for a thorough investigation of these two effects), and add-back issues. Add back is a technique often used for an array of small detectors where for high-energy γ rays one observes a significant amount of (i) Compton scattering from one detector into a neighboring one, and (ii) pair production with subsequent annihilation γ rays being detected in neighboring detectors.…”
Section: Statistical-model Calculations and Comparison To Experimenta...mentioning
confidence: 99%
“…Other sources of systematic errors concern the experimental conditions. Some of the most important problems there involve inefficient neutron-γ discrimination (often done by time-of-flight techniques as in [30], or by simply considering γ rays only at backward angles as in [49]), contamination of highenergy γ spectra by cosmic rays (which can be greatly reduced by coincidence measurements as in [50]), target impurities, pile-up (see, e.g., [51] for a thorough investigation of these two effects), and add-back issues. Add back is a technique often used for an array of small detectors where for high-energy γ rays one observes a significant amount of (i) Compton scattering from one detector into a neighboring one, and (ii) pair production with subsequent annihilation γ rays being detected in neighboring detectors.…”
Section: Statistical-model Calculations and Comparison To Experimenta...mentioning
confidence: 99%
“…A number of measurements have been reported on the J-dependence of the GDR width in different mass regions [9][10][11][12][13][14][15][16][17][18][19] utilizing the heavy ion fusion reactions. However, there are not many such measurements covering a wide range of T for the same nucleus.…”
Section: Introductionmentioning
confidence: 99%