Abstract

The prospects for determining cross sections for compound-nuclear neutron-capture reactions from Surrogate measurements are investigated. Calculations as well as experimental results are presented that test the Weisskopf-Ewing approximation, which is employed in most analyses of Surrogate data. It is concluded that, in general, one has to go beyond this approximation in order to obtain (n, ) cross sections of su cient accuracy for most astrophysical and nuclear-energy applications. Cross sections for compound-nuclear (n, ) reactions are needed for a variety of applications, including astrophysics and nuclear energy. Modeling astrophysical processes that produce the heavy isotopes beyond iron, simulating nu- clear reactor operations, exploring alternative fuel cycles for energy generation, and studying transmutation options for radioactive waste, requires cross sections for neutron- induced reactions on isotopes from di erent regions of the nuclear chart. As many short-lived species cannot be made into targets for direct cross-section measurements, one has to rely on calculations or explore indirect approaches. The accuracies for the cross sections of inter- est, often in the range of 10% or less, can be much smaller than the theoretical uncertainties that exist when the model parameters are insu ciently constrained by data. For in- stance, standard evaluations for the (n, ) reaction on the s-process branch point nucleus 95 Zr (t1=2 = 64 d) vary from each other roughly by a factor of four 1 . Exploiting regional systematics, whenever cross sections or relevant structural data (level densities, -ray strength functions, etc.) for near- by nuclei are known, can provide valuable constraints for the calculations. In this contribution we explore the prospects for de- termining or constraining (n, ) cross sections through Sur- rogate measurements. The Surrogate nuclear reaction tech- nique combines experiment with theory to obtain cross sec- tions for compound-nuclear (CN) reactions, a+A! B ! c+C, involving targets (A) that are di cult or impossible to obtain (1-3). In the Hauser-Feshbach formalism, the cross section for this desired reaction takes the form: (Ea) = X

Highlights

  • Cross sections for compound-nuclear (n,γ) reactions are needed for a variety of applications, including astrophysics and nuclear energy

  • Motivated by the renewed interest in the Surrogate nuclear reactions approach, we have examined the prospects for determining (n,γ) cross sections for deformed rare-earth and actinide nuclei from Surrogate measurements

  • We investigated the validity of the Weisskopf-Ewing approximation, which is commonly employed when extracting (n,f) cross sections from Surrogate experiments

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Summary

Introduction

Cross sections for compound-nuclear (n,γ) reactions are needed for a variety of applications, including astrophysics and nuclear energy. Exploiting regional systematics, whenever cross sections or relevant structural data (level densities, γ-ray strength functions, etc.) for nearby nuclei are known, can provide valuable constraints for the calculations In this contribution we explore the prospects for determining or constraining (n,γ) cross sections through Surrogate measurements. For low energies (En < 1-2 MeV) the conditions for the Weisskopf-Ewing approximation are not expected to be well satisfied [3] and it becomes necessary to account for the “spin-parity mismatch,” that is differences between the spin-parity distributions of the compound nuclei produced in the desired and Surrogate reactions, respectively Introducing such corrections in the analysis of Surrogate fission data has been shown to improve the agreement with direct measurements [4, 5]. Examples include (n,f) cross sections for 237U [6] and 233Pa [7]

Gamma decay probabilities and the Weisskopf-Ewing approximation
Cross sections from Weisskopf-Ewing analyses
Findings
Summary and conclusions

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