Compound-Nuclear Reactions
portes grátis
Compound-Nuclear Reactions
Proceedings of the 6th International Workshop on Compound-Nuclear Reactions and Related Topics CNR*18
Bernstein, Lee A.; Talou, Patrick; Escher, Jutta; Brown, David; Froehlich, Carla; Younes, Walid; Alhassid, Yoram
Springer Nature Switzerland AG
02/2022
329
Mole
Inglês
9783030596408
15 a 20 dias
528
Descrição não disponível.
Part1. Modeling Compound-Nuclear Reactions.- Chapter1. Towards more predictive nuclear reaction modelling.- Chapter2. Modelling compound nuclear reactions with EMPIRE.- Chapter3. CoH3: The Coupled-Channels and Hauser-Feshbach Code.- Part2. Beyond Statistical Descriptions.- Chapter4. Recent advances in R-matrix data analysis.- Chapter5. The transition from isolated resonances to the continuum.- Chapter6. Cross section correlation functions and deviations from the Porter-Thomas distribution.- Chapter7. Moldauer's sum rule implies superradiance in compound nuclear reactions 48.- Chapter8. Multi-step direct reaction models including collectivity in nucleon induced reactions.- Chapter9. New symmetry-adapted ab initio approach to nuclear reactions for intermediate-mass nuclei.- Part3. Optical Models.- Chapter10. Linking nuclear reactions and nuclear structure to study exotic nuclei using the dispersive optical model.- Chapter11. Microscopic optical potential from chiral effective field theory.- Part4. Level Densities.- Chapter12. Nuclear level densities: from empirical models to microscopic methods.- Chapter13. Problem of level densities in compound nuclear reactions.- Chapter14. Nuclear shell model and level density.- Chapter15. Constraining level densities using spectral data.- Chapter16. Rotational enhancement factor for nuclear level density.- Chapter17. Role of fluctuations on the pairing properties of nuclei in the random spacing model.- Part5. Gamma-ray Strength Functions.- Chapter18. Gamma strength functions and the Brink-Axel hypothesis.- Chapter19. Gamma-ray strength functions and GDR cross sections in the IAEA photonuclear data project.- Chapter20. Neutron capture on actinides studied with DANCE.- Chapter21. Deconvolution of the photon strength function.- Part6. Oslo Method.- Chapter22. Attempting to close the loop on the Oslo technique at 198Au: constraining the nuclear spin distribution.- Chapter23. Impact of restricted spin-ranges in the Oslo method: The example of (d,p)240Pu.- Chapter24. Systematics of gamma-ray strength functions within the shell model.- Part7. Surrogate Nuclear Reactions.- Chapter25. Future perspectives for surrogate-reaction studies at storage rings.- Chapter26. Prospects for surrogate neutron capture measurements with radioactive ion beams and GODDESS.- Chapter27. Surrogate reaction method for neutron capture and other reactions on unstable nuclei.- Chapter28. Neutron capture cross sections from surrogate reaction data and theory: connecting the pieces with a Markov-Chain Monte Carlo approach.- Chapter29. Neutron transfer reactions for deformed nuclei using a Sturmian basis.- Part8. Fusion, Isotope Production, and Superheavy Nuclei.- Chapter30. PCN calculations for Z=111 to Z=118.- Chapter31. On the role of the curvature corrections in the surface tension coefficient upon the orientation effects in the fusion reactions.- Chapter32. Excitation function measurements of alpha-induced reaction on naturalcopper and titanium up to 46 MeV.- Chapter33. Measurement of the excitation function of 96Zr(alpha,x)99Mo reaction up to 32 MeV.- Part9. Fission.- Chapter34. A grand tour of nuclear fission physics.- Chapter35. Microscopic calculation of fission mass distributions at increasing excitation energies.- Chapter36. Microscopic description of fission for the r-process in neutron star mergers 242.- Chapter37. Event-by-event modeling with FREYA.- Chapter38. Capabilities of the NIFFTE FissionTPC.- Part10. Experimental Techniques and Facilities.- Chapter39. Resonance measurements at Rensselaer Polytechnic Institute.- Chapter40. Experimental facilities at iThemba LABS and measurements to constrain astrophysical processes.- Chapter41. Late gamma rays from neutron-induced fission and capture from 235U.
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nuclear reaction mechanisms;compound-nuclear decays;Hauser-Feshbach theory;pre-equilibrium nuclear reactions;particle and gamma emission;statistical reactions;direct reactions;surrogate reactions;level densities;strength functions;fision
Part1. Modeling Compound-Nuclear Reactions.- Chapter1. Towards more predictive nuclear reaction modelling.- Chapter2. Modelling compound nuclear reactions with EMPIRE.- Chapter3. CoH3: The Coupled-Channels and Hauser-Feshbach Code.- Part2. Beyond Statistical Descriptions.- Chapter4. Recent advances in R-matrix data analysis.- Chapter5. The transition from isolated resonances to the continuum.- Chapter6. Cross section correlation functions and deviations from the Porter-Thomas distribution.- Chapter7. Moldauer's sum rule implies superradiance in compound nuclear reactions 48.- Chapter8. Multi-step direct reaction models including collectivity in nucleon induced reactions.- Chapter9. New symmetry-adapted ab initio approach to nuclear reactions for intermediate-mass nuclei.- Part3. Optical Models.- Chapter10. Linking nuclear reactions and nuclear structure to study exotic nuclei using the dispersive optical model.- Chapter11. Microscopic optical potential from chiral effective field theory.- Part4. Level Densities.- Chapter12. Nuclear level densities: from empirical models to microscopic methods.- Chapter13. Problem of level densities in compound nuclear reactions.- Chapter14. Nuclear shell model and level density.- Chapter15. Constraining level densities using spectral data.- Chapter16. Rotational enhancement factor for nuclear level density.- Chapter17. Role of fluctuations on the pairing properties of nuclei in the random spacing model.- Part5. Gamma-ray Strength Functions.- Chapter18. Gamma strength functions and the Brink-Axel hypothesis.- Chapter19. Gamma-ray strength functions and GDR cross sections in the IAEA photonuclear data project.- Chapter20. Neutron capture on actinides studied with DANCE.- Chapter21. Deconvolution of the photon strength function.- Part6. Oslo Method.- Chapter22. Attempting to close the loop on the Oslo technique at 198Au: constraining the nuclear spin distribution.- Chapter23. Impact of restricted spin-ranges in the Oslo method: The example of (d,p)240Pu.- Chapter24. Systematics of gamma-ray strength functions within the shell model.- Part7. Surrogate Nuclear Reactions.- Chapter25. Future perspectives for surrogate-reaction studies at storage rings.- Chapter26. Prospects for surrogate neutron capture measurements with radioactive ion beams and GODDESS.- Chapter27. Surrogate reaction method for neutron capture and other reactions on unstable nuclei.- Chapter28. Neutron capture cross sections from surrogate reaction data and theory: connecting the pieces with a Markov-Chain Monte Carlo approach.- Chapter29. Neutron transfer reactions for deformed nuclei using a Sturmian basis.- Part8. Fusion, Isotope Production, and Superheavy Nuclei.- Chapter30. PCN calculations for Z=111 to Z=118.- Chapter31. On the role of the curvature corrections in the surface tension coefficient upon the orientation effects in the fusion reactions.- Chapter32. Excitation function measurements of alpha-induced reaction on naturalcopper and titanium up to 46 MeV.- Chapter33. Measurement of the excitation function of 96Zr(alpha,x)99Mo reaction up to 32 MeV.- Part9. Fission.- Chapter34. A grand tour of nuclear fission physics.- Chapter35. Microscopic calculation of fission mass distributions at increasing excitation energies.- Chapter36. Microscopic description of fission for the r-process in neutron star mergers 242.- Chapter37. Event-by-event modeling with FREYA.- Chapter38. Capabilities of the NIFFTE FissionTPC.- Part10. Experimental Techniques and Facilities.- Chapter39. Resonance measurements at Rensselaer Polytechnic Institute.- Chapter40. Experimental facilities at iThemba LABS and measurements to constrain astrophysical processes.- Chapter41. Late gamma rays from neutron-induced fission and capture from 235U.
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