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“Nuclear structure” from TOF measurements
Milan Krtička Charles University in Prague
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Outline Photon (g-ray/radiative) strength functions and level density from TOF measurements Measurements of g-ray spectra from radiative neutron capture with 4p balls Needed for calculation of cross section in reactions involving photons Influence of “non-statistical” effects observed in neutron capture on the decay of nucleus (on level density, calculated cross sections) Observed effect for neutron widths Measurement of intensities of primary transitions with Ge detectors Needed for calculation of cross section Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Introduction Main problems with description of atomic nucleus: Interaction (nuclear Hamiltonian) is not known precisely “Many body” problem How do we describe the nucleus? At low excitation energies – well separated levels – people try to describe the nucleus with “microscopic” models (nuclear structure) At higher excitation energies – “statistical approaches” use of average quantities and fluctuation properties Niels Bohr - Nature (1936) Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Photon Strength Functions
} Average quantities – level density (LD) and photon strength functions (PSFs) for different types of transitions (E1, M1, E2,…) PSFs give the average probability of photon emission from “highly-excited” states or photoexcitation (in absolute units) needed in all cases where one deals with g decay/photoexcitation a b Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Photon Strength Functions
Above neutron separation energy measured in (g,xn) experiments in many nuclei Experiment does not distinguish multipolarity, dominance of E1 assumed Giant Dipole Electric Resonance is observed (and predicted) in all nuclei The shape seems to be well described by single, or double (or triple?) Lorentzian What is the PSF shape below neutron separation energy and for transitions between excited states? From B.L. Berman, S.C. Fultz, Rev. Mod. Phys. 47 (1975) 713 Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Brink hypothesis n,g Brink hypothesis: generalization “g.s.” “f” n,g
A target in photonuclear/photoabsorption experiment is in the ground state i g.s. γ n,g “equivalent to” Quasicontinuum Identical ! Brink hypothesis: generalization “g.s.” “f” i f γ n,g “equivalent to” Fictitious (γ,γ‘) and (γ,x) experiments g.s. NRF experiments Photoexcitation pattern of an excited target nucleus Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Brink hypothesis The energy dependence of the photoeffect is independent of the detailed structure of the initial state dependence on g-ray energy but not on excit. energy (T), Jp,… validity of the hypothesis? at least approximately - from (n,g) reaction and hot nuclei some weak signs of temperature (excitation energy) dependence LANL, June 27, 2012 Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Different PSFs shapes from different reactions
Main unresolved problems Exact shape of E1 at low energy tail of GDER Dependence of low-energy tail of GDER on temperature (excitation energy) Inconsistency of PSFs derived from different experiments Contribution of M1 strength … Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
How to process data? Spectra of photons usually given by a complicated interplay of PSFs for different types of transitions (E1, M1, E2,…) and LD A problem with “disentanglement” of PSFs and LD also in (n,g) Probably the only solution (at the moment) is a comparison of experimental spectra with outcome of simulations We use the DICEBOX code for making these simulations Simulates gamma decay of a compound nucleus within extreme statistical model Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Simulation of cascades - DICEBOX algorithm
Main assumptions: For nuclear levels below certain “critical energy” spin, parity and decay properties are known from experiments Energies, spins and parities of the remaining levels are assumed to be a random discretization of an a priori known level-density formula A partial radiation width if (XL), characterizing a decay of a level i to a level f, is a random realization of a chi-square-distributed quantity the expectation value of which is equal to f (XL)(Eγ) Eγ2L+1/(Ei), where f (XL) and ρ are also a priori known Selection rules governing the decay are taken into account Any pair of partial radiation widths if (XL) is statistically uncorrelated Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Modelling within ESM Simulation of the decay: “nuclear realization” (106 levels Ţ 1012 Glgf) “precursors” are introduced fluctuations originating from nuclear realizations cannot be suppressed Deterministic character of random number generators is exploited Outcomes from modelling are compared with experimental data Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Main features of DICEBOX
There exists infinite number of artificial nuclei (nuclear realizations) obtained with the same set of LD and PSFs models that differ in exact number of levels and intensities of transitions between each pair of them leads to different predictions from different nuclear realizations (NRs) DICEBOX allows to treat predictions from different NRs – fluctuations can be treated correctly The size of fluctuations from different nuclear realizations depend on the (observable) quantity and nucleus Due to fluctuations only “integral” quantities can be compared Simulation of detector response must be applied (GEANT simulations for DANCE,…) Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Spectra from 4p ball – MSC spectra
Eg1 Eg2 Eg3 Eg4 Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Spectra from 4p ball BaF2 detector arrays used so far “The only” problem might be due to a background from neutron capture on Ba isotopes in crystals Background is small for strong resonances and often can be subtracted Spectra from isolated neutron resonances (DANCE, n_TOF) Spins and parities of initial states known Spectra from unresolved resonance region (Karlsruhe, FRANZ,…) A mixture of different spins (and parities) – can be reasonably estimated at low neutron energies (up to several hundred keV of En - neutron strength functions must be known) Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Spectra from 4p ball – unresolved resonances
Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Resolved resonances TOF spectrum from 95Mo(n,g) from DANCE Only events corresponding to strong resonances are used Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Spectra from 4p ball – resolved resonances
In some cases – isotope dependent Different shapes (multiplicity distributions) of MSC spectra for different Jp Can be used for Jp assignment / Jp needed in simulations Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Spectra from 4p ball – resolved resonances
Another illustration of difference of spectra from resonances with different Jp Experiment Simulations Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Spectra from 4p ball – resolved resonances
Experiment Predicted fluctuations from simulations Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
151Eu spectra M=1 M=2 M=3 M=4 M=5 M=6 M=7 M=2 M=1 M=3 M=4 M=5 M=6 M=7 Predicted shapes from all s-wave resonances (2+ and 3+) identical The same for simulations Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Results Only restricted regions of nuclei have been/are planed to be probed Rare-earth nuclei (mainly deformed) Actinides (deformed) Presence of so-called scissors mode tested Mo region Test of the presence of enhancement of PSF at low Eg – proposed from Oslo method in A< nuclei Sn/Cd region In addition to the enhancement, tests of presence of pygmy resonance Pt/Au region Shape of PSF is probably very different from other regions (pygmy) Almost all results obtained at DANCE Some results for actinides at n_TOF – only sum-energy spectra published, MSC spectra are processed Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Results Only restricted regions of nuclei have been/are planed to be probed Rare-earth nuclei (mainly deformed) Actinides (talks of J. Ullmann and C. Guerrero) Presence of so-called scissors mode tested Mo region Test of the presence of enhancement of PSF at low Eg – proposed from Oslo method in A< nuclei Sn/Cd region In addition to the enhancement, tests of presence of pygmy resonance Pt/Au region Shape of PSF is probably very different from other regions (pygmy) Almost all results obtained at DANCE Some results for actinides at n_TOF – only sum-energy spectra published, MSC spectra are processed Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Fe, Mo + other light nuclei – softpole
Data from Oslo strong enhancement of PSF at low g-ray energies In the case of Fe a support from TSC measurements arbitrary normalization of exp. data Prospects of TOF, Darmstadt, Mar 18-20, 2013
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MSC spectra of 96Mo (2+ resonaces)
Strong PSF enhancement at low Eg leads to strong change in predicted MSC spectra – shift in multiplicity distribution, spectral shape Prospects of TOF, Darmstadt, Mar 18-20, 2013
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MSC spectra of 96Mo (3- resonaces)
Strong PSF enhancement at low Eg leads to strong change in predicted MSC spectra – shift in multiplicity distribution, spectral shape Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
MSC spectra of 96Mo 2+ 3- Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
(n,g) data on 96Mo Predicted MSC spectra similar for T-dependent PSFs from the figures But correct statistical analysis of TSC spectra excludes the model on right figure at 99.8 % confidence level Krticka et al., PRC (2008) the enhancement is “very weak” if any Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
A mode observed in (e,e’) and (g,g’) at excitation energy near 3 MeV In (g,g’) problems with exp. threshold relation between exp. and actual strength? – important especially in odd nuclei Data from two-step cascades (TSC) in 163Dy and Oslo data, (3He,a), on several isotopes indicated that the strength at similar energy is needed also for transitions between excited states – a mode in a PSF TSC spectra clearly showed that the excitation is in M1 M1 strength is “comparable to/ stronger than” E1 near 3 MeV H. Maser et al., PRC 53 (1995) 2749 Ge detectors: allows to resolve individual GS transitions (in even-even nuclei) Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
Neutron separation energy in odd products makes the bumps more pronounced than in even-even products No resonance structure in PSF postulated Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
Resonance structure postulated in E1 PSF Confirms conclusion from TSC spectra Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
Resonance structure postulated in M1 PSF only on states with excitation energy of lower than 3 MeV Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
Resonance structure postulated in M1 PSF only on states with excitation energy of lower than 3 MeV Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
Resonance structure postulated in M1 PSF on all states Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
Resonance structure must be postulated in M1 PSF at all energies (we are sensitive up to about 4 MeV) – Brink hypothesis valid Odd-even effect seems to be seen in the strength of the mode - strength reproducing 157,159Gd is about 3x higher than in 156,158Gd Energy near 3 MeV in rare-earth nuclei (what is the energy in other regions (actinides)?) Half-width is about 1 MeV Some inconsistencies in parameters between Oslo and (n,g) Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
3-MeV bumps in spectra seen also in even-even nuclei Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Rare-earth region – “scissors mode”
One can make additional gates on spectra – a peak in 156Gd comes from decay of about 5 states with excitation MeV transitions to these states can be checked gated MSC spectra Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Pygmy resonance in 198Au data obtained before 1980 ?
197Au(n,)198Au reaction Photonuclear data Isolated neutron resonances Fast n-capture, CTF Fast n-capture, BSFG Lorentzian GDR “Depressed” Lorentzian GDR ? Is there, indeed, an E1 pygmy resonance at 5.5 MeV? … or a mere deficiency and/or a redistribution of E1 photon strength? Redrawn from S. Joly, D. M. Drake and L. Nilsson, PRC 20 (1979) 2072 GSI, January 15, 2013 Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Pygmy resonance in 198Au data from the Karlsruhe 4 BaF2 calorimeter
No pygmy resonance postulated Pygmy resonance at 5.5 MeV Suppression of PSF below 5 MeV No difference in fits … but postulating a pygmy resonance leads to too large total radiation width Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Pygmy resonance in 198Au Exactly the same results obtained also from also TSC spectra Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Fluctuation properties
Inherent part of the statistical model/calculations It is assumed that wave functions at high excitation energies are “very complicated” and the distribution of their overlaps (via EM operator) <y|T(EM)|y> are “random” – create Gaussian distribution This assumption least to the Porter-Thomas distribution (PTD) (c2 distribution with one degree of freedom n) of reduced neutron widths, partial radiation widths, … Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Fluctuation properties
Recently, a strong indication of a violation of the Porter-Thomas distribution (PTD) (n = 1.0) of reduced neutron widths was found in odd Pt isotopes From analysis of neutron widths measured at ORELA P. Koehler PRL 105, (2010) Maximum-Likelihood (ML) analysis yielded: 192Pt: n = 0.57± Pt: n = 0.47± Pt: n = 0.60±0.28 No indication of the PTD violation in 232Th (target) not yet published There are more nuclei showing some problems with PTD P. Koehler, Phys. Rev. C 76, (2007), Phys. Rev. C 84, (2011) More detailed investigation needed Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
ORELA Measurements Transmission as well as capture cross section measured Resonance parameters deduced using SAMMY Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Testing the PTD Using 192,194Pt+n ORELA Data Several statistics to test the consistency with PTD used Combining them for two nuclei: PTD rejected at % confidence level Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Fluctuation properties
A violation of PTD might have “strong” consequences: If distributions were “wider” (n < 1) – there would be higher number of levels with small widths - either unobserved or difficult to be distinguished from p-wave resonances Resonance spacing can be different Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Fluctuation properties
A violation of PTD might have “strong” consequences: If distributions were “wider” (n < 1) – there would be higher number of levels with small widths - either unobserved or difficult to be distinguished from p-wave resonances Resonance spacing can be different Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Fluctuation properties
Is there any problem also with gamma widths? Primary transitions from neutron resonances can be, in principle, measured A few measurements were performed at GELINA (thesis of F. Gunsing and L. Zanini) and Dubna (F. Bečvář) Test of the PTD and/or correlations with some quantum numbers (K) would be perfect A huge amount of material needed – about 100 g Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Prospects of TOF, Darmstadt, Mar 18-20, 2013
Example: Spectra of primary transitions from several Jp = 1- resonances in 107Ag(n,g) as measured at GELINA Thesis of L. Zanini Prospects of TOF, Darmstadt, Mar 18-20, 2013
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Thank you very much for your attention!
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