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Microscopic-Macroscopic Approach to Nuclear Fission Process - GSI Darmstadt

Explore the study of nuclear fission through a microscopic-macroscopic approach, highlighting mass and charge distributions, experimental information, and the GSI ABLA model. Understand the importance of fission in basic research and various applications in astrophysics, RIB production, and spallation sources. Discover challenges in studying fission properties for exotic nuclei and the need for a global description. Dive into fission competition in excited nuclei de-excitation, including fission barriers, fragment distributions, and more. Find out about high and low-energy experimental data at GSI and the macroscopic-microscopic transition. Learn about the ABLA evaporation/fission model and its components for comprehensive insights.

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Microscopic-Macroscopic Approach to Nuclear Fission Process - GSI Darmstadt

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  1. Microscopic-macroscopic approach to the nuclear fission process Aleksandra Kelić, Maria Valentina Ricciardi, Karl-Heinz Schmidt GSI – Darmstadt http://www.gsi.de/charms/

  2. Outline -Why studying fission Basic research Applications (astrophysics, RIB production, spallation sources...) • - Mass and charge distributions • Experimental information • GSI model ABLA - Fission barriers of exotic nuclei Test of isotopic trends of different models - Summary and outlook

  3. Motivation • Basic research • Fission corresponds to a large-scale collective motion where both static and dynamic properties play important role Excellent tool to study, e.g. • Nuclear structure effects at large deformations • Fluctuations in charge polarisation • Viscosity of nuclear matter

  4. Motivation • RIB production (fragmentation method, ISOL method), • Spallation sources and ADS Data measured at FRS* * Ricciardi et al, PRC 73 (2006) 014607; Bernas et al., NPA 765 (2006) 197; Armbruster et al., PRL 93 (2004) 212701; Taïeb et al., NPA 724 (2003) 413; Bernas et al., NPA 725 (2003) 213 www.gsi.de/charms/data.htm Challenge - need for consistent global description of fission and evaporation

  5. Motivation Astrophysics - r-process and nucleosynthesis -Trans-uranium elements 1) - r-process endpoint 2) - Fission cycling 3) 1) Cowan et al, Phys. Rep. 208 (1991) 267; 2) Panov et al., NPA 747 (2005) 633 3) Seeger et al, APJ 11 Suppl. (1965) S121 4) Rauscher et al, APJ 429 (1994) 49 S. Wanajo et al., NPA 777 (2006) 676 Challenge - fission properties (e.g. fission barriers, fission-fragment distributions) for nuclei not accessible in laboratory.

  6. E* What do we need? Fission competition in de-excitation of excited nuclei • • Fission barriers • Fragment distributions • • Level densities • • Nuclear viscosity • Particle-emission widths

  7. Mass and charge division in fission

  8. Experimental information - High energy In cases when shell effects can be disregarded, the fission-fragment mass distribution is Gaussian  Data measured at GSI: T. Enqvist et al, NPA 2001 (see www.gsi.de/charms/)

  9. Experimental information - Low energy • Particle-induced fission of long-lived targets and spontaneous fission • Available information: • - A(E*) in most cases • - A and Z distributions of light fission group only in the thermal-neutron induced fission on the stable targets • EM fission of secondary beams at GSI • Available information: • - Z distributions at "one" energy

  10. Experimental information - Low energy More than 70 secondary beams studied: from Z=85 to Z=92 Schmidt et al., NPA 665 (2000) 221

  11. N90 N82 Macroscopic-microscopic approach - Transition from single-humped to double-humped explained by macroscopic and microscopic properties of the potential-energy landscape near outer saddle. Macroscopic part: property of CN Microscopic part: properties of fragments* * Maruhn and Greiner, Z. Phys. 251 (1972) 431, PRL 32 (1974) 548; Pashkevich, NPA 477 (1988) 1;

  12. Basic assumptions • Macroscopic part: • Macroscopic potential is property of fissioning system ( ≈ f(ZCN2/ACN)) • Potential near saddle from exp. mass distributions at high E* (Rusanov): cAis the curvature of the potential at the elongation where the decision on the A distribution is made. cA = f(Z2/A)  Rusanov* * Rusanov et al, Phys. At. Nucl. 60 (1997) 683

  13. Basic assumptions • Microscopic part: • Microscopic corrections are properties of fragments (= f(Nf,Zf)) • Assumptions based on shell-model calculations (Maruhn & Greiner, Pashkevich) • Shells near outer saddle "resemble" shells of final fragments (but weaker) • Properties of shells from exp. nuclide distributions at low E* A  140 A  132 Calculations done by Pashkevich

  14. Basic assumptions • Dynamics: • Approximations based on Langevin calculations (P. Nadtochy): • τ (mass asymmetry) >> τ (saddle scission): decision near outer saddle • τ (N/Z) << τ (saddle scission) : decision near scission • Population of available states with statistical weight (near saddle or scission) Mass of nascent fragments N/Z of nascent fragments

  15. Macroscopic-microscopic approach • Fit parameters: • Curvatures, strengths and positions of two microscopic contributions as free parameters • These 6 parameters are deduced from the experimental fragment distributions and kept fixed for all systems and energies. • For each fission fragment we get: • Mass • Nuclear charge • Kinetic energy • Excitation energy • Number of emitted particles

  16. ABLA - evaporation/fission model • Evaporation stage • - Extended Weisskopf approach with extension to IMFs • - Particle decay widths • - inverse cross sections based on nuclear potential • - thermal expansion of source • - angular momentum in particle emission • - g-emission at energies close to the particle threshold (A. Ignatyuk) • Fission • - Fission decay width • - analytical time-dependent approach (B. Jurado) • - double-humped structure in fission barriers • - symmetry classes in low-energy fission • - Particle emission on different stages of the fission process

  17. Comparison with data

  18. ABLA Test of the fission part  Fission probability 235Np  Data (A. Gavron et al., PRC13 (1976) 2374) ABLA Test of the evaporation part  56Fe (1 A GeV) + 1H  Data (C. Villagrasa et al, P. Napolitani et al)  INCL4+ABLA

  19. 92U 91Pa 142 140 141 90Th 138 139 89Ac 132 131 133 134 137 135 136 Fission of secondary beams after the EM excitation Black - experiment (Schmidt et al, NPA 665 (2000)) Red - calculations With the same parameter set for all nuclei!

  20. Neutron-induced fission of 238U for En = 1.2 to 5.8 MeV Data - F. Vives et al, Nucl. Phys. A662 (2000) 63; Lines - ABLA calculations

  21. Experimental data: Model calculations (model developed at GSI): More complex scenario 238U+p at 1 A GeV

  22. Fission barriers Difficulties when extrapolating in unknown regions (e.g. r-process, super-heavies)

  23. Fission barriers - Experimental information Relative uncertainty: >10-2 Available data on fission barriers, Z ≥ 80 (RIPL-2 library)

  24. Fission barriers - Experimental information Fission barriers Relative uncertainty: >10-2 GS masses Relative uncertainty: 10-4 - 10-9 Courtesy of C. Scheidenberger (GSI)

  25. Experiment - Difficulties • Experimental sources: • Energy-dependent fission probabilities • Extraction of barrier parameters: • Requires assumptions on level densities Gavron et al., PRC13 (1976) 2374

  26. Experiment - Difficulties Extraction of barrier parameters: Requires assumptions on level densities! Gavron et al., PRC13 (1976) 2374

  27. Theory • Recently, important progress on calculating the potential surface using microscopic approach(e.g. groups from Brussels, Goriely et al; Bruyères-le-Châtel, Goutte et al; Madrid, Pèrez and Robledo; ...): • - Way to go! • - But, not always precise enough and still very time consuming • Another approach  microscopic-macroscopic models (e.g. Möller et al; Myers and Swiatecki; Mamdouh et al; ...)

  28. Bjørnholm and Lynn, Rev. Mod. Phys. 52 Theory - Difficulties Dimensionality (Möller et al, PRL 92) and symmetries (Bjørnholm and Lynn, Rev. Mod. Phys. 52) of the considered deformation space are very important! Reflection symmetric Reflection asymmetric Limited experimental information on the height of the fission barrier  in any theoretical model the constraint on the parameters defining the dependence of the fission barrier on neutron excess is rather weak.

  29. Neutron-induced fission rates for U isotopes Panov et al., NPA 747 (2005) Open problem Limited experimental information on the height of the fission barrier Kelić and Schmidt, PLB 643 (2006)

  30. Experimental saddle-point mass Macroscopic saddle-point mass Idea Predictions of theoretical models are examined by means of a detailed analysis of the isotopic trends of saddle-point masses. Usad  Empirical saddle-point shell-correction energy

  31. Very schematic! SCE Neutron number Idea What do we know about saddle-point shell-correction energy? 1. Shell corrections have local character 2. Shell-correction energyat SP should be very small (e.g Myers and Swiatecki PRC 60 (1999); Siwek-Wilczynska and Skwira, PRC 72 (2005)) 1-2 MeV If an model is realistic  Slope ofUsad as function of N should be ~ 0 Any general trend would indicate shortcomings of the model.

  32. Studied models 1) Droplet model (DM) [Myers 1977], which is a basis of often used results of the Howard-Möller fission-barrier calculations [Howard&Möller 1980] 2) Finite-range liquid drop model (FRLDM) [Sierk 1986, Möller et al 1995] 3) Thomas-Fermi model (TF) [Myers and Swiatecki 1996, 1999] 4) Extended Thomas-Fermi model (ETF) [Mamdouh et al. 2001] Myers, „Droplet Model of Atomic Nuclei“, 1977 IFI/Plenum Howard and Möller, ADNDT 25 (1980) 219. Sierk, PRC33 (1986) 2039. Möller et al, ADNDT 59 (1995) 185. Myers and Swiatecki, NPA 601( 1996) 141 Myers and Swiatecki, PRC 60 (1999) 0 14606-1 Mamdouh et al, NPA 679 (2001) 337

  33. Example for uranium Usadas a function of a neutron number A realistic macroscopic model should give almost a zero slope!

  34. Results Slopes of δUsadas a function of the neutron excess  Themost realistic predictions are expected from the TF model and the FRLD model  Further efforts needed for the saddle-point mass predictions of the droplet model and the extended Thomas-Fermi model Kelić and Schmidt, PLB 643 (2006)

  35. Conclusions - Good description of mass and charge division in fission based on a macroscopic-microscopic approach, which allows for robust extrapolations - According to a detailed analysis of the isotopic trends of saddle-point masses indications have been found that the Thomas-Fermi model and the FRLDM model give the most realistic predictions in regions where no experimental data are available - Need for more precise and new experimental data using new techniques and methods (e.g. R3B and ELISE at FAIR)  basis for further developments in theory

  36. Additional slides

  37. Particle emission widths Extended Weißkopf-Ewing formalism • Barriers  • based on Bass potential (empirically deduced from fusion) • Inverse cross section  • energy-dependent inverse cross sections → ingoing-wave boundary condition model • tunnelling through the barrier • Angular momentum  • change in angular momentum due to particle emission

  38. IMF Emission • All nuclei below the Businaro-Gallone maximum of the mass-asymmetry dependent barrier are taken into account in the evaporation process  natural transition between fission and evaporation picture. • The barriers are given by the Bass nuclear potential.

  39. Comparison with data - spontaneous fission Experiment Calculations (experimental resolution not included)

  40. Theory • Strutinsky-type calculations of the potential-energy landscape (e.g. P. Möller) • + Good qualitative overview on multimodal character of fission. • - No quantitative predictions for fission yields. • - No dynamics • Statistical scission-point models (e.g. Fong, Wilkins et al.) • + Quantitative predictions for fission yields. • - No memory on dynamics from saddle to scission. • Statistical saddle-point models (e.g. Duijvestijn et al.) • + Quantitative predictions for fission yields. • - Neglecting dynamics from saddle to scission. • - Uncertainty on potential energy leads to large uncertainties in the yields. • Time-dependent Hartree-Fock calculations with GCM (Goutte) • + Dynamical and microscopic approach. • - No dissipation included. • - High computational effort.

  41. Topographic theorem A. Karpov et al, in preparation Open symbols - inner barrier Closed symbols - outer barrier

  42. Fission experiments at FRS Two types of experiments Performed in inverse kinematics using relativistic (~ 1 A GeV) heavy-ion (up to 238U) beams

  43. Experimental setup 1 max = 15 mrad p/p =  1.5 % Resolution: - ()/ 5·10-4 - Z  0.4 - A / A  2.510-3 ToF   x1, x2  B E  Z But, only one fragment

  44. Nuclide identification 238U + 1H at 1 A GeV M.V. Ricciardi, PhD thesis

  45. Kinematics 238U+Pb, 1 A GeV

  46. Production mechanism Fragment kinematic properties + limited angular acceptance of the FRS  Information on reaction mechanism Enqvist et al., NPA 658 (1999) 47 As a result  for each nucleus: productions cross section, velocity and production mechanism

  47. Measured cross sections - one example Data available at: www.gsi.de/charms/data.htm Data accuracy Statistic: ~ 3% Systematic: 9 - 15 % * Ricciardi et al, PRC 73 (2006) 014607; Bernas et al., NPA 765 (2006) 197; Armbruster et al., PRL 93 (2004) 212701; Taïeb et al., NPA 724 (2003) 413; Bernas et al., NPA 725 (2003) 213 www.gsi.de/charms/data.htm

  48. Experimental setup 2 1st Production and identification of secondary beams 2nd Identification of both fission fragments - EM fission - Nuclear fission Ch. Schmitt, in preparation

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