GAMMA-RAY STRENGTH-FUNCTION MEASUREMENTS AT ELBE
|
|
- Scot Farmer
- 6 years ago
- Views:
Transcription
1 GAMMA-RAY STRENGTH-FUNCTION MEASUREMENTS AT ELBE R.Schwengner 1, G.Rusev 1,2, N.Tsoneva 3, N.Benouaret 1,4, R.Beyer 1, F.Dönau 1, M.Erhard 1, S.Frauendorf 1,5, E.Grosse 1,6, A.R.Junghans 1, J.Klug 1, K.Kosev 1, H.Lenske 3, C.Nair 1, K.D.Schilling 1, A.Wagner 1 1 Institut für Strahlenphysik, Forschungszentrum Dresden-Rossendorf, 1314 Dresden, Germany 2 Dept. of Physics, Duke University and Triangle Universities Nuclear Laboratory, Durham, NC Institut für Theoretische Physik, Universität Gießen, Gießen, Germany 4 Faculté de Physique, Université des Sciences et de la Technologie d Alger, Bab-Ezzouar, Algerie 5 Department of Physics, University of Notre Dame, Notre Dame, IN Institut für Kern- und Teilchenphysik, Technische Universität Dresden, 162 Dresden, Germany - The bremsstrahlung facility - Photon-scattering experiments - Data analysis and results - QRPA and QPM calculations - Photoactivation experiments Supported by Deutsche Forschungsgemeinschaft Ronald Schwengner Institut für Strahlenphysik Mitglied der Leibniz-Gemeinschaft
2 Dipole strength close to the particle-separation energy Understanding of astrophysical processes: Influence on (γ,n) reaction rates in the p-process. Influence on (n,γ) reaction rates in the s-process Sr (γ,n) Studies for transmutation: Analysis of (n,γ) reactions. Open problems: Precise knowledge of the E1 strength on the low-energy tail of the Giant Dipole Resonance. Properties of the E1 strength functions at varying proton and neutron numbers: shell effects, deformation etc. σ (mb) 1 1 S n
3 Dipole strength close to the particle-separation energy Understanding of astrophysical processes: Influence on (γ,n) reaction rates in the p-process. Influence on (n,γ) reaction rates in the s-process Sr (γ,n) Studies for transmutation: Analysis of (n,γ) reactions. Open problems: Precise knowledge of the E1 strength on the low-energy tail of the Giant Dipole Resonance. Properties of the E1 strength functions at varying proton and neutron numbers: shell effects, deformation etc. σ (mb) 1 1 S n Lorentz E = 16.8 MeV Γ = 4. MeV
4 Dipole strength close to the particle-separation energy Understanding of astrophysical processes: Influence on (γ,n) reaction rates in the p-process. Influence on (n,γ) reaction rates in the s-process Sr (γ,n) Studies for transmutation: Analysis of (n,γ) reactions. Open problems: Precise knowledge of the E1 strength on the low-energy tail of the Giant Dipole Resonance. Properties of the E1 strength functions at varying proton and neutron numbers: shell effects, deformation etc. σ (mb) 1 1 S n Lorentz E = 16.8 MeV Γ = 4. MeV RIPL
5 Dipole strength close to the particle-separation energy Understanding of astrophysical processes: Influence on (γ,n) reaction rates in the p-process. Influence on (n,γ) reaction rates in the s-process Sr (γ,n) Studies for transmutation: Analysis of (n,γ) reactions. Open problems: Precise knowledge of the E1 strength on the low-energy tail of the Giant Dipole Resonance. Properties of the E1 strength functions at varying proton and neutron numbers: shell effects, deformation etc. σ (mb) 1 1? S n Lorentz E = 16.8 MeV Γ = 4. MeV RIPL
6 The radiation source ELBE Electron Linear accelerator of high Brilliance and low Emittance
7 The bremsstrahlung facility at the electron accelerator ELBE dipole quadrupole R.S. et al., NIM A 555 (25) 211 Accelerator parameters: dipole quadrupoles Be-window steerer electronbeam dump radiator dipole quartz-window beamhardener collimator Pb accelerator hall Maximum electron energy: 18 MeV polarisation monitor Pb HPGe detector + BGO shield Maximum average current: 1 ma Micro-pulse rate: 13 MHz Micro-pulse length: 5 ps cluster detector experimental cave 1 m target photonbeam dump PE Pb door
8 Detector setup
9 Nuclides under investigation in photon-scattering experiments Z nuclide S n E kin e MeV ELBE 92 Mo a, 13.2 b,c,d Mo d 96 Mo d 98 Mo 8.6 (3.3, 3.8) a,e, (8.5, 13.2) b,c,d 1 Mo 8.3 (3.2, 3.4, 3.8) a, (7.8, 13.2) b,c,d 4 9 Zr , 9., Y f, 9.5, Sr g, (9., 13.2, 16.) h N 87 Rb i, Kr a G. Rusev et al., PRC 73 (26) 4438 b R. Schwengner et al., NPA 788 (27) 331c c G. Rusev et al., PRC 77 (28) d A. Wagner et al., JPG 35 (28) 1435 e G. Rusev et al., PRL 95 (25) 6251 f J. Reif et al., NPA 62 (1997) 1 g L. Käubler et al., PRC 7 (24) 6437 h R. Schwengner et al., PRC 76 (27) i L. Käubler et al., PRC 65 (22) 54315
10 Problem of feeding and branching Measured intensity of a γ transition: I γ (E γ, Θ) = I s ( ) Φ γ ( )ǫ(e γ ) N at W (Θ) Ω E e E, x Γ Scattering cross section integral: I s = σ γγ de = 2J ( x + 1 π hc 2J + 1 ) 2 Γ Γ Γ Γ f branching Absorption cross section: Γ Γ 1 E1 strength: σ γ = σ γγ ( Γ Γ ) 1 B(E1) Γ /E 3 γ
11 Problem of feeding and branching Measured intensity of a γ transition: I γ (E γ, Θ) > I s ( ) Φ γ ( ) ǫ(e γ ) N at W (Θ) Ω E e feeding E, x Γ Scattering cross section integral: I s = σ γγ de = 2J ( x + 1 π hc 2J + 1 ) 2 Γ Γ Γ Γ f branching Absorption cross section: Γ Γ 1 E1 strength: σ γ = σ γγ ( Γ Γ ) 1 B(E1) Γ /E 3 γ
12 Absolute detector efficiency and photon flux ε (%) E γ (kev) Φ γ ((evs) 1 ) E e kin = 13.2 MeV E γ (kev) Absolute efficiency of two detectors at 127 deduced from 22 Na, 6 Co, 133 Ba, (filled circles) and simulated with GEANT3 (solid line). Relative efficiencies deduced from 56 Co (open circles), 11 B (open triangles) and 16 O (open square). Absolute photon flux deduced from transitions in 11 B using the calculated efficiency shown in the left panel and relative photon flux calculated according to G. Roche et al. Code by E. Haug, Rad. Phys. Chem. 77 (28) 27.
13 Unresolved strength in the continuum spectrum 9 Zr 9 Zr =.2 MeV Counts per 1 kev atomic background E γ σ γγ (mb) peaks + cont. peaks Experimental spectrum of 9 Zr (corrected for room background, detector response, efficiency, measuring time) and simulated spectrum of atomic background. Scattering cross sections in 9 Zr averaged over energy bins of.2 MeV, not corrected for branching, derived from the difference of the experimental spectrum and the atomic background (triangles) and from the resolved peaks only (circles).
14 Problem of feeding and branching Correction of the strength function by using statistical methods (G. Rusev, Dissertation): Monte Carlo simulations of γ-ray cascades from groups of levels in 1 kev bins over the whole energy range. Level scheme of J =, 1 and 2 states constructed using: Backshifted Fermi-Gas Model with level-density parameters given in: T. v. Egidy, D. Bucurescu, PRC 72 (25) Wigner level-spacing distributions Partial decay widths calculated by using: Photon strength functions approximated by Lorentzian parametrisations. E1: parameters determined from a fit to (γ,n) data M1: global parametrisation of M1 spin-flip resonances E2: global parametrisation of E2 isoscalar resonances (www-nds.iaea.org/ripl-2) Porter-Thomas distributions of decay widths. Feeding intensities subtracted and intensities of g.s. transitions corrected with calculated branching ratios Γ /Γ.
15 Simulations of γ-ray cascades Zr 1 9 Zr I γ (arb. units).5 Branching transitions Ground state transitions b (%) E γ Simulated intensity distribution of transitions depopulating levels in a 1 kev bin around 9 MeV. Subtraction of intensities of branching transitions. Distribution of branching ratios b = Γ /Γ versus the excitation energy as obtained from the simulations of γ-ray cascades for 9 Zr. Estimate of Γ and σ γ.
16 Test of simulated branching ratios Zr 8 b (%) Measurement with monochromatic photons at HIγS ( E 2 kev). Black: Population of + 2 neglected. Red: Assumption that b + 2 = b G. Rusev, A.P. Tonchev et al., priv. comm. Distribution of branching ratios b = Γ /Γ versus the excitation energy as obtained from the simulations of γ-ray cascades for 9 Zr.
17 Test of E1 strength functions 1 2 Lorentzian δ = 1 σ γ (mb) Lorentzian δ = σ γ ( ) = 2S TRK 3π 3 i=1 Ex 2 Γ i ( ) (Ei 2 Ex 2 ) 2 + Ex 2 Γi 2 ( ) Γ i ( ) = Γ S ( /E i ) δ ; Γ S = 4 MeV; σ γ (mb) 1 1 f 1 = σ γ /[3(π hc) 2 E γ ] Constant S TRK = σ γ (E) de = 6 NZ A MeV mb σ γ (mb) 1 1 E i = hω (1 2 3 ǫ 2 cos ( γ 2πi ))
18 Absorption cross section in 9 Zr 9 Zr Present (γ, γ) data 1 σ γ (mb) 1 (γ,γ ) uncorr 1 S n
19 Absorption cross section in 9 Zr 9 Zr Present (γ, γ) data 1 (γ,γ ) corr σ γ (mb) 1 (γ,γ ) uncorr 1 S n
20 Absorption cross section in 9 Zr Present (γ, γ) data 1 9 Zr (γ,γ ) corr (γ,p) (γ, p) calculated ADNDT 88 (24) 1 σ γ (mb) 1 1 S n
21 Absorption cross section in 9 Zr Present (γ, γ) data σ γ (mb) Zr (γ,γ ) corr (γ,p) (γ,n) (γ, p) calculated ADNDT 88 (24) 1 (γ, n) data PR 162 (1967) 198 S n
22 Absorption cross section in 9 Zr 9 Zr Present (γ, γ) data + (γ, p) + (γ, n) data 1 σ γ (mb) 1 1 S n
23 Absorption cross section in 9 Zr 9 Zr Present (γ, γ) data + (γ, p) + (γ, n) data σ γ (mb) 1 1 Lorentz curve: E = 16.8 MeV Γ = 4. MeV π 2 σ Γ = 6 NZ A MeV mb 1 S n
24 Absorption cross section in 9 Zr 9 Zr Present (γ, γ) data + (γ, p) + (γ, n) data σ γ (mb) 1 1 Lorentz curve: E = 16.8 MeV Γ = 4. MeV π 2 σ Γ = 6 NZ A MeV mb RIPL-2 (S. Goriely, E. Khan, NPA 76 (22) 217) 1 S n
25 Absorption cross section in 9 Zr 9 Zr Present (γ, γ) data + (γ, p) + (γ, n) data σ γ (mb) 1 1 Lorentz curve: E = 16.8 MeV Γ = 4. MeV π 2 σ Γ = 6 NZ A MeV mb RIPL-2 (S. Goriely, E. Khan, NPA 76 (22) 217) S n QRPA Woods-Saxon basis Γ = 3.2 MeV
26 Absorption cross section in 88 Sr 88 Sr Present (γ, γ) data + (γ, n) data σ γ (mb) 1 1 Lorentz curve: E = 16.8 MeV Γ = 4. MeV π 2 σ Γ = 6 NZ A MeV mb RIPL-2 (S. Goriely, E. Khan, NPA 76 (22) 217) QRPA Woods-Saxon basis: Γ = 3.2 MeV
27 Absorption cross section in 89 Y 89 Y Present (γ, γ) data + (γ, p) + (γ, n) data σ γ (mb) 1 1 Lorentz curve: E = 16.8 MeV Γ = 4. MeV π 2 σ Γ = 6 NZ A MeV mb RIPL-2 (S. Goriely, E. Khan, NPA 76 (22) 217) 1 S n QRPA Woods-Saxon basis: Γ = 3.2 MeV
28 One-phonon QPM calculations for 88 Sr and 9 Zr Transition densities of neutrons and protons: Sr.5 r 2 ρ(r) (fm 1 ) < 9 MeV.5 = MeV = 9 22 MeV 9 Zr.5 Energy range below 9 MeV: Oscillations at the surface by neutrons only Indication for a PDR r (fm) 5 1
29 Absorption cross sections in Mo isotopes σ γ ( ) = 2S TRK 3π 3 i=1 Ex 2 Γ i ( ) (Ei 2 Ex 2 ) 2 + Ex 2 Γi 2 ( ) Γ i ( ) = Γ S ( /E i ) δ ; Γ S = 4 MeV; δ S TRK = σ γ (E) de = 6 NZ A E i = hω (1 2 3 ǫ 2 cos MeV mb ( γ 2πi )) 3
30 Absorption cross sections in Mo isotopes σ γ ( ) = 2S TRK 3π 3 i=1 Ex 2 Γ i ( ) (Ei 2 Ex 2 ) 2 + Ex 2 Γi 2 ( ) Γ i ( ) = Γ S ( /E i ) δ ; Γ S = 4 MeV; δ S TRK = σ γ (E) de = 6 NZ A E i = hω (1 2 3 ǫ 2 cos MeV mb ( γ 2πi )) 3
31 Comparison with other experiments Present (γ, γ) data (γ, n) data H. Beil et al., NPA 227 (1974) 427 ( 3 He, 3 He γ) data M. Guttormsen et al., PRC 71 (25) 4437 (n, γ) data J. Kopecky and M. Uhl, Bologna 1994
32 QRPA calculations for deformed nuclei Hamiltonian for 1 states: - Nilsson or Woods-Saxon mean field plus monopole pairing - isoscalar and isovector dipole-dipole and octupole-octupole interactions F. Dönau, PRL 94 (25) 9253 F. Dönau et al., PRC 76 (27) Total energy as a function of the quadrupole deformation ε 2 and the triaxiality γ: γ 3 γ 3 γ 3 γ 3 γ ε ε ε ε ε 2 92 Mo 5 94 Mo Mo Mo 56 1 Mo 58 ε 2 =. ε 2 =.2 ε 2 =.1 ε 2 =.18 ε 2 =.21 γ = 6 γ = 37 γ = 32 TAC model with shell-correction method: S. Frauendorf, NPA 557 (1993) 259c, NPA 667 (2) 115
33 QRPA calculations in a deformed basis for Mo isotopes / TRK (%) / TRK (%) / TRK (%) Mo 94 Mo 96 Mo 98 Mo 1 Mo Experiment 92 Mo 94 Mo 96 Mo 98 Mo 1 Mo QRPA with WS 92 Mo 94 Mo 96 Mo 98 Mo 1 Mo Talys N N N Σ TRK = Σ( ) = i σ γ (E i ) E σ γ (E) de = 6 NZ A MeV mb
34 Summary Study of dipole-strength distributions at high excitation energy and high level density via photon scattering. Comparison of measured spectrum with calculated atomic background: 3 4% of the total dipole strength in resolved peaks and 7 6% in continuum. Simulations of statistical γ cascades: Estimate of intensities of inelastic transitions. Deduced σ γ connect smoothly with (γ,n) data. (i) Correct determination of σ γ up to the (γ,n) threshold. (ii) Information on the photoabsorption cross section over the whole energy range from low excitation energy up to the GDR. (iii) Observation of extra strength in the range from 6 to 12 MeV not described in current approximations of dipole-strength functions. QPM calculations: (i) Qualitative description of the observed extra strength. (ii) Extra strength below 9 MeV caused by oscillations of the excessive neutrons. (iii) Increase of dipole strength below the neutron-threshold toward the heavier Mo isotopes is correlated with increasing deformation.
35 Photodissociation Photodissociation reactions: (γ, n) (γ, p) (γ, α) Method: photoactivation (A, Z) + γ (A, Z 1) + p Measure decay rate of (A, Z 1) N act (E e ) = N tar Ee E thr σ (γ,x) Φ γ (E, E e ) de N act (E e ) = I γ (E γ ) ε 1 (E γ ) p 1 (E γ ) κ corr
36 Photoactivation of 92 Mo Photoactivation process γ transitions Electron capture (EC) and β decay + + β 5% + β 64.6 s 93% 1/2 9/ min 48.2% Mo kev kev Sn kev 1/ ps 1% (2.9%) kev EC 2.9% EC 4% 1/ d 9/2 + EC 93% ( β + <.2%) 68 y.58% Nb 14.5 kev kev not to scale Sp 7456 kev 5/2 + stable kev + stable kev 91 4Zr A = 91 A = Mo N act (E e ) = N tar Ee E thr σ (γ,x) Φ γ (E, E e ) de N act (E e ) = I γ (E γ ) ε 1 (E γ ) p 1 (E γ ) κ corr
37 Setup for photoactivation experiments Pneumatic delivery Accelerator hall Bremsstrahlung cave Low level counting setup Graphite Photoactivation target Aluminium collimator Photo activation target HPGe detectors Photon beam dump Lead housing Lead castle Photoactivated target HPGe detector Electron beam Electron beam dump (rotated by 9 ) Steel Iron Lead wall PE blocks Dewar Depot
38 Activation yield Solid lines: NON-SMOKER, T. Rauscher and F.-K. Thielemann, ADNDT 88 (24) 1 Dashed lines: TALYS, A. Koning et al., AIP Conf. Proc. 769 (25) 1154 Activation yields of Mo isotopes normalised to the activation yield of the 197 Au(γ, n) reaction.
39 Activation yield 144 Sm(γ,n) 143 Sm 144 Sm(γ,n) 143m Sm Solid lines: NON-SMOKER, T. Rauscher and F.-K. Thielemann, ADNDT 88 (24) Sm(γ, α) 14 Nd Dashed lines: TALYS, A. Koning et al., AIP Conf. Proc. 769 (25) 1154 Activation yields of 144 Sm normalised to the activation yield of the 197 Au(γ, n) reaction.
40 Activation yield low-background measurement Spectra of the decay of 14 Nd 14 Pr 14 Ce following the 144 Sm(γ, α) reaction. Measured in ELBE building Measured in underground lab Felsenkeller in Dresden
41 Summary Photodissociation of Mo isotopes and of 144 Sm studied via photoactivation at the ELBE accelerator. Determination of the photon flux in the electron-beam dump by means of the 197 Au(γ, n) reaction. Measurement of weak decay rates in an underground lab. 92 Mo(γ, α) 88 Zr and 144 Sm(γ, α) 14 Nd reactions observed for the first time at astrophysically relevant energies. Rough agreement with predictions of Hauser-Feshbach models for (γ, n) and (γ, p) reactions. Predictions differ for (γ, α) reactions.
DIPOLE-STRENGTH IN N=50 NUCLEI STUDIED IN PHOTON-SCATTERING EXPERIMENTS AT ELBE
DIPOLE-STRENGTH IN N=50 NUCLEI STUDIED IN PHOTON-SCATTERING EXPERIMENTS AT ELBE R.Schwengner 1, G.Rusev 1, N.Benouaret 1,2, R.Beyer 1, F.Dönau 1, M.Erhard 1, E.Grosse 1,3, A.R.Junghans 1, K.Kosev 1, J.Klug
More informationPhoton-scattering experiments at γelbe and at HIγS Data analysis Results Comparison of experimental results with model predictions
Text optional: Institutsname Prof. Dr. Hans Mustermann www.fzd.de Mitglied der Leibniz-Gemeinschaft Pygmy dipole strength in 86 Kr and systematics of N = 5 isotones R. Schwengner 1, R. Massarczyk 1,2,
More informationNew Phenomena in Gamma-Ray Strength Functions
Text optional: Institutsname Prof. Dr. Hans Mustermann www.fzd.de Mitglied der Leibniz-Gemeinschaft Ronald Schwengner Institut für Strahlenphysik http://www.hzdr.de New Phenomena in Gamma-Ray Strength
More informationInstantaneous Shape Sampling for Calculating the Electromagnetic Dipole Strength in Transitional Nuclei S. Frauendorf
Instantaneous Shape Sampling for Calculating the Electromagnetic Dipole Strength in Transitional Nuclei S. Frauendorf Department of Physics University of Notre Dame, USA Institut fuer Strahlenphysik, Forschungszentrum
More informationElectromagnetic Dipole Strength distribution in 124,128,134 Xe below the neutron separation energy
Electromagnetic Dipole Strength distribution in 124,128,134 Xe below the neutron separation energy Ralph Massarczyk Helmholtz-Zentrum Dresden-Rossendorf 29.05.2013 R.Massarczyk (HZDR) dipole strength in
More informationMeasuring Neutron Capture Cross Sections on s-process Radioactive Nuclei
Measuring Neutron Capture Cross Sections on s-process Radioactive Nuclei 5th Workshop on Nuclear Level Density and Gamma Strength Oslo, May 18-22, 2015 LLNL-PRES-670315 LLNL-PRES-XXXXXX This work was performed
More informationInvestigation of dipole strength at the ELBE accelerator in Dresden-Rossendorf
EPJ Web of Conferences 21, 04006 (2012) DOI: 10.1051/ epjconf/ 20122104006 C Owned by the authors, published by EDP Sciences, 2012 Investigation of dipole strength at the ELE accelerator in Dresden-Rossendorf
More information5th Workshop on Nuclear Level Density and Gamma Strength. Oslo, May 18-22, Nuclear microscopic strength functions in astrophysical applications
5th Workshop on Nuclear Level Density and Gamma Strength Oslo, May 18-22, 2015 Nuclear microscopic strength functions in astrophysical applications N. Tsoneva Institut für Theoretische Physik, Universität
More informationThe decay of 1 + states as a new probe of the structure of 0 + shape isomers
The decay of 1 + states as a new probe of the structure of 0 + shape isomers G. Rusev 1, R. Schwengner 1, F. Dönau 1, S. Frauendorf 1,2, L. Käubler 1, L. K. Kostov 3, S. Mallion 1,4, K. D. Schilling 1,
More informationPhoton strength functions in Mo region. Milan Krtička
Photon strength functions in Mo region Milan Krtička Outline 1. MSC spectra in 98 Mo (DANCE measurement) 2. Discussion of PSF in Mo region 98 Mo Part 1 MSC spectra in 98 Mo M. Krtička 1, C.L. Walker 2,3,
More informationMissing Dipole Excitation Strength below the Particle Threshold
Missing Dipole Excitation Strength below the Particle Threshold A.P. Tonchev a, C. Angell b, M. Boswell b, C.R. Howell a, H.J. Karwowski b, J.H. Kelley c, W. Tornow a, N. Tsoneva d a Duke University and
More informationInstantaneous shape sampling - a model for the electromagnetic dipole strength in transitional nuclei
Instantaneous shape sampling - a model for the electromagnetic dipole strength in transitional nuclei I. Bentley, 1 S. Brant, 2 F. Dönau, 3 S. Frauendorf, 1 S. Q. Zhang, 4 B. Kämpfer, 3 and R. Schwengner
More informationInvestigation of radiative proton-capture reactions using high-resolution g-ray spectroscopy
Investigation of radiative proton-capture reactions using high-resolution g-ray spectroscopy P. Scholz, F. Heim, J. Mayer, M. Spieker, and A. Zilges Institute for Nuclear Physics, University of Cologne
More informationDipole Response of Exotic Nuclei and Symmetry Energy Experiments at the LAND R 3 B Setup
Dipole Response of Exotic Nuclei and Symmetry Energy Experiments at the LAND R 3 B Setup Dominic Rossi for the LAND collaboration GSI Helmholtzzentrum für Schwerionenforschung GmbH D 64291 Darmstadt, Germany
More informationTest of the Brink-Axel Hypothesis with Gamma Strength Functions from Forward Angle Inelastic Proton Scattering
Test of the Brink-Axel Hypothesis with Gamma Strength Functions from Forward Angle Inelastic Proton Scattering Peter von Neumann-Cosel Institut für Kernphysik, Technische Universität Darmstadt Gamma strength
More informationExperimental study of the 14 N(p,γ) 15 O reaction
Experimental study of the 14 N(p,γ) 15 O reaction Michele Marta FZ Dresden - Rossendorf Institute for Radiation Physics Nuclear Physics Division International School of Nuclear Physics (32nd Course) Erice
More informationRecent developments in neutron capture on actinides using the DANCE detector
Recent developments in neutron capture on actinides using the DANCE detector J.L. Ullmann Los Alamos National Laboratory Sixth Workshop on Nuclear Level Density and Gamma Strength. Oslo, Norway, May 8
More informationLow-lying gamma-strength within microscopic models
Low-lying gamma-strength within microscopic models Elena Litvinova 1,2 1 GSI Helmholtzzentrum für Schwerionenforschung mbh, Darmstadt, Germany 2 Institut für Theoretische Physik, Goethe Universität, Frankfurt
More informationBeyond mean-field study on collective vibrations and beta-decay
Advanced many-body and statistical methods in mesoscopic systems III September 4 th 8 th, 2017, Busteni, Romania Beyond mean-field study on collective vibrations and beta-decay Yifei Niu Collaborators:
More informationAndreas Zilges. Newest results on pygmy resonances in atomic nuclei. Institut für Kernphysik Universität zu Köln. (ZI 510/4-1 and INST 216/544-1)
Newest results on pygmy resonances in atomic nuclei Andreas Zilges Institut für Kernphysik Universität zu Köln supported by (ZI 510/4-1 and INST 216/544-1) Giant Dipole Resonance (GDR) 1937: Z. Phys. 106
More informationStatistical-Model and Direct-Semidirect-Model Calculations of Neutron Radiative Capture Process
New Era of Nuclear Physics in the Cosmos, the r-process Nucleo-Synthesis RIKEN, Japan, Sep. 25,26, 2008 Statistical-Model and Direct-Semidirect-Model Calculations of Neutron Radiative Capture Process T.
More informationMonte Carlo Simulation for Statistical Decay of Compound Nucleus
CNR20, Prague, Czech Republic, Sep. 9 23, 20 Monte Carlo Simulation for Statistical Decay of Compound Nucleus T. Kawano, P. Talou, M.B Chadwick Los Alamos National Laboratory Compound Nuclear Reaction,
More informationDevelopment of a neutron time-of-flight source at the ELBE accelerator
Development of a neutron time-of-flight source at the ELBE accelerator *,1, E. Altstadt 2, C. Beckert 2, R. Beyer 1, H. Freiesleben 3, V. Galindo 2, M. Greschner 3, E. Grosse 1,3, A. R. Junghans 1, D.
More informationNuclear Resonance Fluorescence with. NRF with monoenergetic photons and fundamental experiments at ELI-NP. Julius Wilhelmy
Nuclear Resonance Fluorescence with monoenergetic photons and fundamental experiments at ELI-NP Julius Wilhelmy Institute for Nuclear Physics, University of Cologne g BMBF Verbund 05P2015 Darmstadt Köln
More informationFast neutron inelastic scattering Roland Beyer, Forschungszentrum Dresden-Rossendorf
Fast neutron inelastic scattering Roland Beyer, Forschungszentrum Dresden-Rossendorf Institute of Radiation Physics Roland Beyer www.fzd.de Member of the Leibniz Association Data needs for transmutation
More informationMass and energy dependence of nuclear spin distributions
Mass and energy dependence of nuclear spin distributions Till von Egidy Physik-Department, Technische Universität München, Germany Dorel Bucurescu National Institute of Physics and Nuclear Engineering,
More informationMICROSCOPIC NATURE OF THE PHOTON STRENGTH FUNCTION: STABLE AND UNSTABLE Ni AND Sn ISOTOPES
MICROSCOPIC NATURE OF THE PHOTON STRENGTH FUNCTION: STABLE AND UNSTABLE Ni AND Sn ISOTOPES O. Achakovskiy 4, A. Avdeenkov 4, S. Goriely 2, S. Kamerdzhiev 1, S. Krewald 3, D. Voitenkov 4 1. Institute for
More informationSymmetries and collective Nuclear excitations PRESENT AND FUTURE EXOTICS IN NUCLEAR PHYSICS In honor of Geirr Sletten at his 70 th birthday
Symmetries and collective Nuclear excitations PRESENT AND FUTURE EXOTICS IN NUCLEAR PYSICS In honor of Geirr Sletten at his 70 th birthday Stefan Frauendorf, Y. Gu, Daniel Almehed Department of Physics
More informationSUPPLEMENTARY INFORMATION
SUPPLEMENTARY INFORMATION doi:10.1038/nature143 1. Supplementary Methods A. Details on the experimental setup Five 3 3 LaBr 3 :Ce-detectors were positioned 22 cm away from a 13 Cs gamma-ray source, which
More informationIsospin Character of Low-Lying Pygmy Dipole States via Inelastic Scattering of 17 O ions
14 th International Conference on Nuclear Reaction Mechanisms Varenna, June 15-19, 2015 Isospin Character of Low-Lying Pygmy Dipole States via Inelastic Scattering of 17 O ions Fabio Crespi Università
More informationGamma-ray strength functions obtained with the Oslo method
Gamma-ray strength functions obtained with the Oslo method Ann-Cecilie Larsen July 8, 2008 DEPARTMENT OF PHYSICS UNIVERSITY OF OSLO Collaborators Oslo: A. Bürger, M. Guttormsen, S. Messelt, F. Ingebretsen,
More informationGiant Resonances Wavelets, Scales and Level Densities
Giant resonances Damping mechanisms, time and energy scales Fine structure Wavelets and characteristic scales Application: GQR TU DARMSTADT Many-body nuclear models and damping mechanisms Relevance of
More informationBjörn Lehnert. Search for double beta decays of palladium isotopes into excited states
Search for double beta decays of palladium isotopes into excited states INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 35th Course Erice 23/09/2013 Björn Lehnert Institut für Kern- und Teilchenphysik Outline
More informationShell model description of dipole strength at low energy
Shell model description of dipole strength at low energy Kamila Sieja Institut Pluridisciplinaire Hubert Curien, Strasbourg 8-12.5.217 Kamila Sieja (IPHC) 8-12.5.217 1 / 18 Overview & Motivation Low energy
More informationInvestigation of the Pygmy Dipole Resonance in particle- coincidence experiments
Investigation of the Pygmy Dipole Resonance in particle- coincidence experiments V. Derya 1*, J. Endres 1, M. N. Harakeh 2,3, D. Savran 4,5, M. Spieker 1*, H. J. Wörtche 2, and A. Zilges 1 1 Institute
More informationRelativistic Radioactive Beams as a Tool for Nuclear Astrophysics
Relativistic Radioactive Beams as a Tool for Nuclear Astrophysics Thomas Aumann December 11 th 2013 27 th Texas Symposium on Relativistic Astrophysics Dallas, Texas Supported by the BMBF under contract
More informationHigh precision neutron inelastic cross section measurements
High precision neutron inelastic cross section measurements A. Olacel, C. Borcea, M. Boromiza, A. Negret IFIN-HH, DFN Outline The experimental setup GELINA GAINS Data analysis algorithm. Monte Carlo simulations
More informationTEST OF CLOSED-FORM GAMMA-STRENGTH FUNCTIONS. Vladimir Plujko. Taras Shevchenko National University; Institute for Nuclear Research, Kyiv, Ukraine
TEST OF CLOSED-FORM GAMMA-STRENGTH FUNCTIONS Vladimir Plujko Taras Shevchenko National University; Institute for Nuclear Research, Kyiv, Ukraine 1. Radiative (photon, gamma) strength functions (RSF)- definitions.
More informationNuclear Astrophysics Research at HIγS
Nuclear Astrophysics Research at HIγS Selected Examples of Work in Progress Werner Tornow Duke University & TUNL Outline A. What is HIγS? B. Few-Body Physics (see T. Shima) C. Nuclear Astrophysics 4 9
More informationPhotonuclear Reaction Cross Sections for Gallium Isotopes. Serkan Akkoyun 1, Tuncay Bayram 2
Photonuclear Reaction Cross Sections for Gallium Isotopes Serkan Akkoyun 1, Tuncay Bayram 2 1 Cumhuriyet University, Vocational School of Healt, Sivas, Turkey 2 Sinop University, Department of Physics,
More informationInvestigation of Pygmy Dipole Resonance in neutron rich exotic nuclei
Investigation of Pygmy Dipole Resonance in neutron rich exotic nuclei R.Avigo 1,2, O.Wieland 1, A.Bracco 1,2, F.Camera 1,2 on behalf of the AGATA and DALI2 collaborations 1 INFN, sezione di Milano 2 Università
More informationImportance of nuclear triaxiality for electromagnetic strength, level density and neutron capture cross sections in heavy nuclei
Importance of nuclear triaxiality for electromagnetic strength, level density and neutron capture cross sections in heavy nuclei E. Grosse b, A.R. Junghans a and R. Massarczyk a,b a Institute of Radiation
More informationBeta decay for neutron capture
Beta decay for neutron capture Sean Liddick ICNT, June 7th, 2016 r-process calculations neutron star merger hot wind cold wind Abundance pattern is different for the different astrophysical scenarios.
More informationanti-compton BGO detector
1 2 3 Q β - measurements with a total absorption detector composed of through-hole HPGe detector and anti-compton BGO detector 4 5 Hiroaki Hayashi a,1, Michihiro Shibata b, Osamu Suematsu a, Yasuaki Kojima
More informationNuclear Reaction Rates for Astrophysical Nucleosynthesis
Nuclear Reaction Rates for Astrophysical Nucleosynthesis Department of Physics, Central Michigan University, Mt. Pleasant, MI 48859, USA E-mail: palum1a@cmich.edu D. Galaviz Centro de Fisica Nuclear da
More informationThe Effect of Pygmy Resonances in p-process Nucleosynthesis
The Effect of Pygmy Resonances in p-process Nucleosynthesis by Christoper T. Angell A dissertation submitted to the faculty of the The University of North Carolina at Chapel Hill in partial fulfillment
More informationStatistical Model Calculations for Neutron Radiative Capture Process
Statistical Nuclear Physics and its Applications in Astrophysics, Jul. 8-, 2008 Statistical Model Calculations for Neutron Radiative Capture Process T. Kawano T-6 Nuclear Physics Los Alamos National Laboratory
More informationStatistical Theory for the Beta-Delayed Neutron and Gamma-Ray Emission
Statistical Theory for the Beta-Delayed Neutron and Gamma-Ray Emission T. Kawano, P Möller Theoretical Division, Los Alamos National Laboratory LA-UR-13-21895 Slide 1 Combining QRPA Calculation and Statistical
More informationWarm superdeformed nuclei:
S. Leoni University of Milano and INFN Warm superdeformed nuclei: Probes of Nuclear Structure and Tunneling Processes At the Onset of Chaos Oslo WS May 29 Outline: 1- INTRO: Warm Superdeformed Nuclei 2-
More information1 Geant4 to simulate Photoelectric, Compton, and Pair production Events
Syed F. Naeem, hw-12, Phy 599 1 Geant4 to simulate Photoelectric, Compton, and Pair production Events 1.1 Introduction An Aluminum (Al) target of 20cm was used in this simulation to see the eect of incoming
More informationSome results obtained with Gogny force included in HFB, QRPA as well as in configuration mixing GCM like approach
Some results obtained with Gogny force included in HFB, QRPA as well as in configuration mixing GCM like approach Sophie Péru M. Dupuis, S. Hilaire, F. Lechaftois (CEA, DAM), M. Martini (Ghent University,
More informationCharge exchange reactions and photo-nuclear reactions
Charge exchange reactions and photo-nuclear reactions σ( 7 Li, 7 Be) and σ(γ,n) S. Nakayama (Univ of Tokushima) Determination of σ(γ,n) from CE reactions (CE reaction = Charge Exchange reaction) Application
More informationFAST NEUTRON CROSS-SECTION MEASUREMENTS WITH THE NELBE NEUTRON TIME-OF-FLIGHT FACILITY. Postfach D Dresden, Germany
FAST NEUTRON CROSS-SECTION MEASUREMENTS WITH THE NELBE NEUTRON TIME-OF-FLIGHT FACILITY A. Wagner 1*, D. Bemmerer 1, R. Beyer 1, E. Birgersson 1, A. Ferrari 1, E. Grosse 1,3, R. Hannaske 1, A. R. Junghans
More informationMeasurement of the inelastic neutron scattering cross section of 56 Fe
EPJ Web of Conferences 8, 07007 (2010) DOI: 10.1051/epjconf/20100807007 c Owned by the authors, published by EDP Sciences, 2010 Measurement of the inelastic neutron scattering cross section of 56 Fe R.
More informationPrompt γ-rays from Neutron Inelastic
Prompt γ-rays from Neutron Inelastic Scattering at FaNGaS: Benchmark Spectrum Analysis T.H. Randriamalala, M. Rossbach Institute of Energy and Climate Research, Nuclear Waste Management and Reactor Safety,
More informationMagnetic rotation past, present and future
PRAMANA c Indian Academy of Sciences Vol. 75, No. 1 journal of July 2010 physics pp. 51 62 Magnetic rotation past, present and future A K JAIN and DEEPIKA CHOUDHURY Department of Physics, Indian Institute
More informationExperimental Initiatives in Nuclear Astrophysics
Experimental Initiatives in Nuclear Astrophysics Carl Brune Astrophysics: H and He burning, S process Facilities: neutron and gamma beams, underground accelerators, ICF plasmas Joint DNP Town Meetings
More informationNuclear astrophysics of the s- and r-process
Nuclear astrophysics of the s- and r-process René Reifarth Goethe University Frankfurt Ecole Joliot Curie School on Neutrons and Nuclei Frejus, France, Sep-28 Oct-3 2014 Nucleosynthesis tales from the
More informationThe two-step (and multiple-step) γ cascade method as a tool for studying γ-ray strength functions. Milan Krtička
The two-step (and multiple-step) γ cascade method as a tool for studying γ-ray strength functions Milan Krtička Outline The method of two-step γ-cascades following thermal neutron capture (setup at Rez
More informationInstitut für Kernphysik, Universität zu Köln, Germany 2. Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest, Romania 3
High-Resolution Study of Low-Spin States in Mark Spieker 1,*, Dorel Bucurescu 2, Janis Endres 1, Thomas Faestermann 3, Ralf Hertenberger 4, Sorin Pascu 1,2, Hans-Friedrich Wirth 4, Nicolae-Victor Zamfir
More informationRadiative Capture Reaction
A New Decay Path in the C+16O Radiative Capture Reaction Institut Pluridisciplinaire Hubert Curien, Strasbourg, France Outline Narrow Resonances, C +16O Detailed study of the C(16O,γ)28Si resonant radiative
More informationMicroscopic cross sections : an utopia? S. Hilaire 1, A.J. Koning 2 & S. Goriely 3.
Microscopic cross sections : an utopia? S. Hilaire 1, A.J. Koning 2 & S. Goriely 3 www.talys.eu 1 CEA,DAM,DIF - France 2 Nuclear Research and Consultancy Group, Petten, The Netherlands 3 Institut d Astronomie
More informationBeta decay for neutron capture Sean Liddick
Beta decay for neutron capture Sean Liddick 6 th Oslo Workshop on Strength and Level Density, May 8-12, 2017 Nuclear Physics Uncertainties for r-process: (n,γ) (n,γ) uncertainties Monte-Carlo variations
More informationPhotofission of 238-U Nuclei
Photofission of 238-U Nuclei International Thorium Energy Conference - ThEC18, 29-31st of October 2018, Belgium İsmail Boztosun This research has been supported by TÜBİTAK with grant number 114F220 Motivations
More informationStudies involving discrete spectroscopy. Studies involving total absorption or calorimetry
11/8/2016 1 Two general themes Studies involving discrete spectroscopy Typically involving high resolution Ge detectors Ex. 8p/GRIFFIN at TRIUMF-ISAC Studies involving total absorption or calorimetry Typically
More informationNuclear Reactions with light ion and photon beams; Contributions to Neutrino Astrophysics
Nuclear Reactions with light ion and photon beams; Contributions to Neutrino Astrophysics 1. Incompressibility and Giant Resonances (ISGMR, ISGDR) 2. Charge exchange reactions 3. Photon Beams for (g,g
More informationMeasurement of γ Strength Function and Level Density of 138. La at oooooo
Measurement of γ Strength Function and Level Density of 138 La at oooooo Vincent Kheswa PhD Student ithemba LABS, Somerset West, South Africa 27 May 2013 Outline» Introduction» Experimental Setup» Preliminary
More informationPhoton Strength Functions and Nuclar Level Densities in Gd Nuclei from Neutron Capture Experiments
Photon Strength Functions and Nuclar Level Densities in Gd Nuclei from Neutron Capture Experiments J. Kroll 1,, B. Baramsai 3, G. E. Mitchell 1, C. Arnold 3, F. Bečvář, T. Bredeweg 3, A. Couture 3, R.
More informationarxiv:nucl-th/ v1 14 Nov 2005
Nuclear isomers: structures and applications Yang Sun, Michael Wiescher, Ani Aprahamian and Jacob Fisker Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre
More informationSystematics of Scissors Mode in Gd Isotopes from experiment with DANCE Detector. Jiří Kroll. for DANCE collaboration
Systematics of Scissors Mode in Gd Isotopes from experiment with DANCE Detector Jiří Kroll for DANCE collaboration Faculty of Mathematics and Physics, Charles University, Prague Outline Motivation SM observed
More informationThe intense, pulsed positron source EPOS at the Research Centre Dresden-Rossendorf
The intense, pulsed positron source EPOS at the Research Centre Dresden-Rossendorf The EPOS Team and R. Krause-Rehberg Martin-Luther University, Halle-Wittenberg, Dept. of Physics, 06099 Halle / Germany
More informationRole of (a,n) reactions in the nucleosynthesis of light r-elements in neutrino-driven winds
Role of (a,n) reactions in the nucleosynthesis of light r-elements in neutrino-driven winds Jorge Pereira, Fernando Montes National Superconducting Cyclotron Laboratory, MSU, USA Joint Institute for Nuclear
More informationStructure of the Low-Lying States in the Odd-Mass Nuclei with Z 100
Structure of the Low-Lying States in the Odd-Mass Nuclei with Z 100 R.V.Jolos, L.A.Malov, N.Yu.Shirikova and A.V.Sushkov JINR, Dubna, June 15-19 Introduction In recent years an experimental program has
More informationProbing the Nuclear Symmetry Energy and Neutron Skin from Collective Excitations. N. Paar
Calcium Radius Experiment (CREX) Workshop at Jefferson Lab, March 17-19, 2013 Probing the Nuclear Symmetry Energy and Neutron Skin from Collective Excitations N. Paar Physics Department Faculty of Science
More informationTowards first-principle description of electromagnetic reactions in medium-mass nuclei
Canada s National Laboratory for Particle and Nuclear Physics Laboratoire national canadien pour la recherche en physique nucléaire et en physique des particules Towards first-principle description of
More informationMeasurement of the photodissociation of the deuteron at energies relevant to Big Bang nucleosynthesis
Journal of Physics: Conference Series PAPER OPEN ACCESS Measurement of the photodissociation of the deuteron at energies relevant to Big Bang nucleosynthesis To cite this article: R Hannaske et al 2016
More informationNew half-live results on very long-living nuclei
Fakultät Mathematik und Naturwissenschaften, Institut für Kern- und Teilchenphysik New half-live results on very long-living nuclei 29.9. 2016, NNR 2016 Osaka Institut für Kern- und Teilchenphysik Contents
More informationInvestigation of the mixed-symmetry states in Mo by means of high-resolution electron and proton scattering*
Investigation of the mixed-symmetry states in Mo by means of high-resolution electron and proton scattering* Institut für Kernphysik, Technische Universität Darmstadt Oleksiy Burda 2 1 3 2 4 5 3,4 N. Botha,
More informationRecent developments in the nuclear shell model and their interest for astrophysics
Recent developments in the nuclear shell model and their interest for astrophysics Kamila Sieja Institut Pluridisciplinaire Hubert Curien, Strasbourg FUSTIPEN topical meeting "Recent Advances in the Nuclear
More informationB. PHENOMENOLOGICAL NUCLEAR MODELS
B. PHENOMENOLOGICAL NUCLEAR MODELS B.0. Basic concepts of nuclear physics B.0. Binding energy B.03. Liquid drop model B.04. Spherical operators B.05. Bohr-Mottelson model B.06. Intrinsic system of coordinates
More informationSURROGATE REACTIONS. An overview of papers by Jason Burke from LLNL
SURROGATE REACTIONS An overview of papers by Jason Burke from LLNL Compound Nuclear Reaction cross sections Cross sections for compound-nuclear reactions are required input for astrophysical models and
More informationNuclear Photonics: Basic facts, opportunities, and limitations
Nuclear Photonics: Basic facts, opportunities, and limitations Norbert Pietralla, TU Darmstadt SFB 634 GRK 2128 Oct.17th, 2016 Nuclear Photonics 2016, Monterey Nuclear Photonics: Basic Facts Prof.Dr.Dr.h.c.
More informationExperimental neutron capture data of 58 Ni from the CERN n TOF facility
Introduction n TOF facility Data analysis Experimental neutron capture data of 58 Ni from the CERN n TOF facility Department of Physics, Faculty of Science, University of Zagreb 25. August 2014. Overview
More informationNovel High Performance Computational Aspects of the Shell Model Approach for Medium Nuclei
Novel High Performance Computational Aspects of the Shell Model Approach for Medium Nuclei Mihai Horoi Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA Collaborators:
More informationPositron program at the Idaho Accelerator Center. Giulio Stancari Idaho State University and Jefferson Lab
Positron program at the Idaho Accelerator Center Giulio Stancari Idaho State University and Jefferson Lab International Workshop on Positrons at Jefferson Lab Newport News, Virginia (USA), 26 March 2009
More informationThe Nuclear Equation of State
The Nuclear Equation of State Theoretical models for nuclear structure studies Xavier Roca-Maza Università degli Studi di Milano e INFN, sezione di Milano Terzo Incontro Nazionale di Fisica Nucleare LNF,
More informationNew Concept of EPOS Progress of the Mono-energetic Positron Beam (MePS) Gamma-induced Positron Spectroscopy (GiPS)
Progress of the EPOS Project: Gamma Induced Positron Spectroscopy (GiPS) R. Krause-Rehberg 1,*,W.Anwand 2,G.Brauer 2, M. Butterling 1,T.Cowan 2,M. Jungmann 1, A. Krille 1, R. Schwengner 2, A. Wagner 2
More informationRadiative-capture reactions
Radiative-capture reactions P. Descouvemont Physique Nucléaire Théorique et Physique Mathématique, CP229, Université Libre de Bruxelles, B1050 Bruxelles - Belgium 1. Introduction, definitions 2. Electromagnetic
More informationSpectroscopy of light exotic nuclei using resonance scattering in inverse kinematics.
Spectroscopy of light exotic nuclei using resonance scattering in inverse kinematics. Grigory Rogachev RESOLUT: a new radioactive beam facility at FSU Solenoid 2 Magnetic Spectrograph Magnetic Spectrograph
More informationAnalysis of Nuclear Transmutation Induced from Metal Plus Multibody-Fusion-Products Reaction
Ohta, M. and A. Takahashi. Analysis of Nuclear Transmutation Induced from Metal Plus Multibody-Fusion- Products Reaction. in Tenth International Conference on Cold Fusion. 2003. Cambridge, MA: LENR- CANR.org.
More informationDipole resonances in 4 He
Dipole resonances in He σ( 7 Li, 7 Be), σ(ν,ν ), and σ γ S. Nakayama (Univ of Tokushima) Neutrino-induced reactions (neutral current) He(ν,ν ) in SN ν-heating He( 7 Li, 7 Be) Application of the He( 7 Li,
More informationNeutron capture measurements at the CERN neutron Time Of Flight (n_tof) facility. Nuclear astrophysics aspects
Neutron capture measurements at the CERN neutron Time Of Flight (n_tof) facility Nuclear astrophysics aspects Paolo Maria MILAZZO (on behalf of the n_tof collaboration) The n_tof Collaboration CERN Technische
More informationDetermination of radiative strength functions
Determination of radiative strength functions and level density Andreas Schiller, Ohio U Motivation Discrete spectroscopy Continuous spectroscopy Energies of discrete [2 +, 3 -, etc.] levels Level density,
More informationNeutron Halo in Deformed Nuclei
Advances in Nuclear Many-Body Theory June 7-1, 211, Primosten, Croatia Neutron Halo in Deformed Nuclei Ó Li, Lulu Ò School of Physics, Peking University June 8, 211 Collaborators: Jie Meng (PKU) Peter
More informationMontecarlo simulation of the decay of warm superdeformed nuclei
Montecarlo simulation of the decay of warm superdeformed nuclei E. Vigezzi INFN Milano Understanding the dynamics in the SD well: probing γ strength functions, energy barriers, level densities, residual
More informationGAMMA-RAY STRENGTH FUNCTION METHOD: A WAY FROM PHOTONEUTRON EMISSION TO RADIATIVE NEUTRON CAPTURE
GAMMA-RAY STRENGTH FUNCTION METHOD: A WAY FROM PHOTONEUTRON EMISSION TO RADIATIVE NEUTRON CAPTURE H. UTSUNOMIYA, H. AKIMUNE, T. YAMAGATA, C. IWAMOTO Department of Physics, Konan University, Okamoto 8-9-1,
More informationSemi-Classical perturbation theory Coulomb only First-order most used
direct reactions Models for breakup Semi-Classical perturbation theory Coulomb only First-order most used TDSE (Time Dependent Schrodinger Equation) Coulomb + Nuclear Semi-classical orbit needed DWBA (Distorted
More informationImpact of Nuclear Reaction Uncertainties on AGB Nucleosynthesis Models
Impact of Nuclear Reaction Uncertainties on AGB Nucleosynthesis Models, ab R. Gallino, b F. Käppeler, c M. Wiescher, d and C. Travaglio a a INAF - Astronomical Observatory Turin, Turin, Italy b University
More informationJoint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation August Introduction to Nuclear Physics - 1
2358-19 Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation 6-17 August 2012 Introduction to Nuclear Physics - 1 P. Van Isacker GANIL, Grand Accelerateur National d'ions Lourds
More informationLow-energy nuclear response: structure and underlying mechanisms
Low-energy nuclear response: structure and underlying mechanisms Elena Litvinova National Superconducting Cyclotron Laboratory @ Michigan State University, East Lansing, USA In collaboration with: P. Ring,
More information