High-resolution study of Gamow- Teller transitions in pf-shell nuclei. Tatsuya ADACHI
|
|
- Ezra Taylor
- 5 years ago
- Views:
Transcription
1 High-resolution study of Gamow- Teller transitions in pf-shell nuclei Tatsuya ADACHI
2 Type II supernova Electron Capture (EC) & β decay Neutrino induced reaction A Z-1X N+1 daughter EC β A ZX N parent (A,Z) + e - (A,Z) + e + (A,Z-1) +ν e (A,Z+1) +ν e Fermi (τ) B(F) = N-Z Gamow-Teller (στ) 1 B(GT) = 2Ji C GT 2T f +1 J f T f A 2 Σ j=1 (σ j τ j ) J i T i
3 GT transitions from T z =+1 to T z =0 by ( 3 He,t) reactions (n,p) (p,p ) g.s. 0 + ( 3 He,t) g.s. T=0 βdecay 0 + g.s. 0 + T=1 T=1 IAS T z =+2 T z =+1 T z = 0 T z =-1 T z =-2 T=2 V Mn Cr Fe Mn Co Fe Ni Co Cu
4 B(GT) Measurement in Charge Exchange Reactions Cross Section for L=0 Max At 0 deg. στ Dominant An incident beam energy E i >100MeV/u One-Step Reaction Dominant σ(0 ) = K GT N GT J στ 2 B(GT) ^ σ GT : Unit Cross Section T.N. Taddeucci et. al., NPA469 (1987) 125. Cross section Relative B(GT) values are obtained. In order to obtain absolute B(GT) values ^ σ GT standard B(GT) value from β decay (a) 1 (b) + (c) 1/2,3/2,5/2 1/2,3/2,5/2 σ^ g.s. GT 0 + g.s. Tz ^σ GT Tz -1 3/2 3/2 T z =+1/2 T z =-1/2 σ GT 0 + g.s. 0 + IAS 0 + g.s. σ F B(F) B(GT) T z = +1 T z =0 T z =-1
5 WS Beam Line Grand-Raiden Spectrometer at θ lab = 0 T. Wakasa et al., NIM A482 (2002) 79. High-Dispersive WS beam line Ring Cyclotron E 3He = 140MeV/u
6 Dispersion Matching Techniques Achromatic Beam Transportation focal plane Y. Fujita et. al., NIM B126 (1997) 274. H. Fujita et. al., NIM A484 (2002) 17. Dispersive Beam Transportation Magnetic Spectrometer target ΔE ~ 200 kev for 3 He 420 MeV ΔE ~ 35 kev Hori. Angle Resolution θ ~ 5mrad
7 High-resolution ( 3 He,t) spectra Ca( 3 He,t) 42 Sc ΔE=60 kev Counts Ti( 3 He,t) 46 V ΔE=33 kev Cr( 3 He,t) Mn ΔE=29 kev g.s(ias) g.s.(ias) g.s (IAS) Fe( 3 He,t) Co g.s.(ias) ΔE=21 kev F g.s N g.s. 12 N T. Adachi et. al., PRC 73, (2006) Y. Fujita et. al., PRL (2005) E x in daughter nuclei (MeV)
8 β decay from T z = -1 to T z =0 nuclei T=2 g.s. 0 + ( 3 He,t) σ GT T=0 βdecay B(GT) g.s. 0 + g.s. 0 + T=1 T=1 IAS T z =+2 T z =+1 T z = 0 T z =-1 T z =-2 V Cr Mn Fe Co V.T. Koalowsky et. al., NPA624 (1997) 293. Mn Fe Co Ni Cu I. Reusen et. al., PRC59 (1999) 2416.
9 Ratio of the GT and Fermi Unit Cross Section Proportionality for GT and Fermi σ GT (0 ) = K GT N GT J στ 2 σ F (0 ) = K F N τ J τ 2 B(GT) =σ ^ GT B(GT) B(F) =σ^ F B(F) T.N. Taddeucci et. al., NPA 469 (1987) 125. (p,n) experiment Definition of R 2 value R 2 = σ ^ GT σ^ F Fermi Unit Cross Section σ ^ F = σ F B(F) All Fermi Strengths Concentrate to IAS B(F) = N-Z If mass systematics of R 2 values is studied, σ ^ GT = R 2 σ^ F
10 Derivations of R 2 values for various nuclei 1/2,3/2,5/2 1/2,3/2,5/2 0 + g.s. 0 + IAS g.s. T z Tz Ni 64 Ni 68 Zn 78 Se 118 Sn 120 Sn 140 Ce 178 Hf σ^ F ^σ GT 62 Cu 64 Cu 68 Ga 78 Br 118 Sb 120 Sb 140 Pr 178 Ta 3/2 3/2 T z =+1/2 σ F +σ GT T z =-1/2 7 Li 23 Na 27 Al ^ σ GT 7 Be 23 Mg 27 Si 0 + g.s. 0 + IAS 0 + g.s. B(F) T z = +1 T z =0 T z =-1 18 O 26 Mg 34 S σ GT σ F 18 F 26 Al 34 Cl B(GT) 18 Ne 26 Si 34 Ar
11 Nuclear Mass Dependence of R Na 64 Ni 68 Zn 78 Se 118 Sn 120 Sn 140 Ce 178 Hf R 2 ^ ^ = σ GT /σ F 6 7 Li 18 O 34 S 4 26 Mg Nuclear Mass
12 B(GT) Derivation in Mn & 42 Sc Y. Fujita et. al., PRL (2005). β decay Fe Mn 42 Ti 42 Sc T 1/2 (msec) 155(12) 199(6) 1 = T 1/2 tf Σ 1 i=gt t i K K B(F) = (g ff t v /g A ) 2 B(GT) = F fi t i R 2 = σ ^ GT σ^ F B(GT) = σ GT B(GT) = σf B(F) σ GT 1 σ F B(F) R 2 1 = Σ T 1/2 B(F) (g v /g A ) [ff σ F + 2 f R 2 i σ i ] K σ F i=gt K : 6145(6) g v /g A : (4) B(F) : N-Z =2
13 Y. Fujita et. al., PRL (2005) Ex (MeV) T z = +1 T z = 0 T z = Ex (MeV) Estimation of f F σ F & f GT σ GT F-factor normalized Cr( 3 He,t) Mn Fe Mn Expected βdecay spectrum Assuming isospin symmetry (IAS) Cr Mn Fe 42 Ca 42 Sc 42 Ti f GT σ GT f F σ F (IAS) counts counts
14 Nuclear Mass Dependence of R 2 values (9) 8 7.8(9) 6 7 Li 23 Na 18 O 26 Mg 34 S 58 Ni 62 Ni 64 Ni 68 Zn Cr 42 Ca 118 Sn 78 Se 7.6± ± Sn 140 Ce 178 Hf R 2 ^ ^ = σ GT /σ F Nuclear Mass
15 Comparison between B(GT) s in Mn Exp. and Shell Model counts S p = 4.6 MeV Cr( 3 He,t) Mn Cr( 3 He,t) Mn B(GT) distribution 0.2 B(GT) Shell Model By M. Honma and T. Otsuka 0.2 Σ B(GT) Cumulative Sum Red :Exp Blue: SM Green: Continuous Region Included E x in Mn (MeV)
16 counts Comparison between B(GT) s in Co Exp. and Shell Model Sp = 4.4 MeV Fe( 3 He,t) Co B(GT) Fe( 3 He,t) Co Shell Model Preliminary B(GT) distribution By M. Honma and T. Otsuka 0.2 Σ B(GT) Cumulative Sum Red :Exp Blue: SM Green: Continuous Region Included E x in Co (MeV)
17 Isospin symmetry structure in A= nuclei and analogous transitions (n,p) (p,p ) ( 3 He,t) B(GT + ) B(GT - ) g.s. 0 + g.s. T z =+2 T z =+1 T z = 0 25 Mn Fe Co T=2 T=1 T=0 T=1 (IAS) (p,p ) experiment Scattering angle at 0 incident beam energies (more than 100 MeV/u) IE IE σ(0 ) = K N στ J στ 2 B(σ)
18 Identification of the isospin values 1 B(GT) = 2Ji +1 J f T f 1 B(σ) = 2Ji Analogous transitions Σ A 2 (σ j τ j ) J i T i j=1 j=1 2 C GT 2 2T f +1 C M1 2 B(σ) C M1 <f στ i> 2 = 2 B(GT) C GT <f στ i> 2 2 C M1 1/2 1/2 T z =+1 T z = 0 26Fe 28 3 : 1 1 : 1 2 C GT 1/6 1/2 27Co 27 T=2 T= T f +1 ( 3 1/3 J f T f Σ A 2 (p,p ) He,t) T=0 (σ j τ j ) J i T i g.s. g.s. T=1 (IAS)
19 Fe( 3 He,t) Co & Fe(p,p ) Fe spectra counts T = 2 Fe( 3 He,t) Co T = 0 counts Instrumental Background Fe(p,p ) Fe E p = 160 MeV at 0 at IUCF T = 2 C. Djalali et. al., PRC 35, 1201 (1987) E x (MeV)
20 Identification of Isospin values B(GT) T = 0 T = 1 T = 2 Fe( 3 He,t) Co B(σ) T = 1 T = 2 Fe(p,p ) Fe B(GT) B(σ) T = 1 T = E x (MeV)
21 Summary 1. GT transitions from T z =+1 ( 42 Ca, 46 Ti, Cr, Fe) to T z =0 ( 42 Sc, 46 V, Mn, Co) pf-shell nuclei were measured by high-resolution ( 3 He,t) experiments. 2. B(GT) values were derived from the β decay data. Nuclear mass dependence of R 2 values were systematically studied. 3. Experimental distributions were compared with those of Shell Model calculation. 4. Fe( 3 He,t) Co and Fe(p,p ) Fe spectra were compared. Isospin values T= 0, 1 and 2 of GT and M1 states were identified.
High-resolution Study of Gamow-Teller Transitions
High-resolution Study of Gamow-Teller Transitions Yoshitaka Fujita, Osaka Univ. @CNS-SS, 04.Aug.17-20 Nucleus : 3 active interactions out of 4 Strong, Weak, EM Comparison of Analogous Transitions High
More informationStudies of Gamow-Teller transitions using Weak and Strong Interactions
Studies of Gamow-Teller transitions using Weak and Strong Interactions High-resolution Spectroscopy & Tensor Interaction @ Nakanoshima, Osaka Nov. 16 Nov. 19, 2015 Yoshitaka FUJITA RCNP, Osaka Univ. Neptune
More informationGamow-Teller Transitions studied by (3He,t) reactions and the comparison with analogous transitions
Gamow-Teller Transitions studied by (3He,t) reactions and the comparison with analogous transitions Yoshitaka FUJITA (Osaka Univ.) Spin-Isospin excitations probed by Strong, Weak and EM interactions ECT*,
More informationIsospin symmetry structure of J π =1 + states in 58 Ni and 58 Cu studied by high-resolution 58 Ni( 3 He,t) and 58 Ni(p,p ) measurements
Workshop at ECT*, Torento, 27/09/09-02/10/09 Strong, Weak and Electromagnetic Interactions to probe Spin-Isospin Excitations Isospin symmetry structure of J π =1 + states in 58 Ni and 58 Cu studied by
More informationCharge Exchange and Weak Strength for Astrophysics
Charge Exchange and Weak Strength for Astrophysics Sam Austin STANfest-July 16 2004 Charge Exchange and Weak Strength for Astrophysics Interesting phenomena Electron capture strength (GT) (Langanke talk)
More informationQRPA calculations of stellar weak-interaction rates
QRPA calculations of stellar weak-interaction rates P. Sarriguren Instituto de Estructura de la Materia CSIC, Madrid, Spain Zakopane Conference on Nuclear Physics: Extremes of Nuclear Landscape. August
More informationSpin-isospin responses by charge-exchange reactions and implications for astrophysics
Spin-isospin responses by charge-exchange reactions and implications for astrophysics Muhsin N. Harakeh KVI, Groningen & GANIL, Caen The 4 th International Symposium on Neutrinos and Dark Matter in Nuclear
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 informationBeta-decay. studies with proton-rich. rich nuclei. Bertram Blank. Université Bordeaux 1 / CENBG
Beta-decay studies with proton-rich rich nuclei Super-allowed Fermi transitions Mirror decays proton-rich nuclei in the calcium-to-nickel region branching ratios, half-lives, decay schemes, masses isospin
More informationNeutrino Nuclear Responses For Double Beta Decays And Supernova Neutrinos
Neutrino Nuclear Responses For Double Beta Decays And Supernova Neutrinos Hidetoshi Akimune Konan University INPC016 Collaborators Hidetoshi Akimune Konan University Hiro Ejiri RCNP, Osaka Dieter Frekers
More informationNeutrino-Nucleus Reactions Based on Recent Progress of Shell Model Calculations
Neutrino-Nucleus Reactions Based on Recent Progress of Shell Model Calculations Toshio Suzuki (Nihon University) New shell model calculations in p-shell modified shell model Hamiltonian (SFO) with improved
More informationIsospin symmetry of T z =±3/2\ ±1/2 Gamow-Teller transitions in A=41 nuclei
PHYSICAL REVIEW C 70, 054311 (2004) Isospin symmetry of T z =±3/2\ ±1/2 Gamow-Teller transitions in A=41 nuclei Y. Fujita, 1, * Y. Shimbara, 1, T. Adachi, 1 G. P. A. Berg, 2,3 B. A. Brown, 4 H. Fujita,
More informationI. 2. Reduction of the Gamow-Teller Matrix Element for the β-decay in 70 Ga- 70 Zn by the 35-MeV (p,n) Reaction on 70 Zn
CYRIC Annual Report 2003 I. 2. Reduction of the Gamow-Teller Matrix Element for the β-decay in Ga- Zn by the 35-MeV (p,n) Reaction on Zn Orihara H., Terakawa A. *, Suzuki H. *, Kikuchi Y. *, Kumagai K.
More informationExtracting information from charge exchange reactions the tools we have--what we need Sam Austin 28 September 2009, ECT
Extracting information from charge exchange reactions the tools we have--what we need Sam Austin 28 September 2009, ECT Contexts: Type Ia (Thermonuclear) Supernovae: SN1006 Arizona Petroglyph Core Collapse
More informationShell-model description for beta decays of pfg-shell nuclei
Shell-model description for beta decays of pfg-shell nuclei Workshop on New Era of Nuclear Physics in the Cosmos the r-process nucleosynthesis Sep. 25-26, 2008 @RIKEN M. Honma (Univ. of Aizu) T. Otsuka
More informationD. Frekers. Charge-exchange reactions GT-transitions, bb-decay b b. and things beyond. n n 13 N 15 O 17F. 7Be. pep. hep
Flux @ 1 AU [cm-1 s-1 MeV-1)] for lines [cm -1 s-1 ] D. Frekers n n Charge-exchange reactions GT-transitions, bb-decay b b and things beyond 10 1 10 10 10 8 10 6 10 4 10 pp 13 N 15 O 17F 7Be pep 0.1 0.
More informationBertram Blank CEN Bordeaux-Gradignan. Germanium detector calibration experimental studies: decay mirror decay future work
Bertram Blank CEN Bordeaux-Gradignan Germanium detector calibration experimental studies: 0 + -0 + decay mirror decay future work 20 th Colloque de GANIL, Amboise, October 15th 20th, 2017 Nuclear beta
More information* On leave from FLNR / JINR, Dubna
* On leave from FLNR / JINR, Dubna 1 Introduction: Keywords of this experimental program Search for new isotopes The limits of nuclear stability provide a key benchmark of nuclear models The context of
More informationCharge Exchange reactions with Unstable Nuclei
Charge Exchange reactions with Unstable Nuclei Sam Austin and Remco Zegers Sam Austin, Daniel Bazin, Alex Brown, Christian Diget, Alexandra Gade, Carol Guess, Marc Hausmann, Wes Hitt, Meredith Howard,
More informationQRPA calculations of stellar weak decay rates
QRPA calculations of stellar weak decay rates P. Sarriguren Instituto de Estructura de la Materia CSIC, Madrid, Spain E. Moya de Guerra, R. Alvarez-Rodriguez, O. Moreno Universidad Complutense Madrid International
More informationD. Frekers. Putting together the pieces of the puzzle in bb-decay n. TRIUMF May Gentle Touch: q tr = 0 l = 0.
D. Frekers Putting together the pieces of the puzzle in bb-decay n b TRIUMF May-2016 n b GT? Gentle Touch: q tr = 0 l = 0 dσ dσ 5 10 0 hω excitation σ n n The pieces of the puzzle Chargex-reactions ( 3
More informationDouble-beta decay matrix elements and charge exchange reactions
Double-beta decay matrix elements and charge exchange reactions M. Sasano, Spin-Isospin Laboratory, RIKEN Nishina Center K. Yako, Center for Nuclear Physics, University of Tokyo E Double beta decay Double
More information5 questions, 3 points each, 15 points total possible. 26 Fe Cu Ni Co Pd Ag Ru 101.
Physical Chemistry II Lab CHEM 4644 spring 2017 final exam KEY 5 questions, 3 points each, 15 points total possible h = 6.626 10-34 J s c = 3.00 10 8 m/s 1 GHz = 10 9 s -1. B= h 8π 2 I ν= 1 2 π k μ 6 P
More informationConstraining Astrophysical Reaction Rates with Transfer Reactions at Low and Intermediate Energies
Constraining Astrophysical Reaction Rates with Transfer Reactions at Low and Intermediate Energies Christoph Langer (JINA/NSCL) INT Workshop: Reactions and Structure of Exotic Nuclei March 2015 1 Understanding
More informationnp Spin-Correlation in the Ground State Studied by Spin-M1 Transitions
np Spin-Correlation in the Ground State Studied by Spin-M1 Transitions Atsushi Tamii Research Center for Nuclear Physics (RCNP) Osaka University, Japan for RCNP-E299 Collaborations 2nd International Workshop
More informationD. Frekers. Novel approaches to the nuclear physics of bb-decay: INT chargex reactions, mass-measurements,m-capture
D. Frekers Novel approaches to the nuclear physics of bb-decay: chargex reactions, mass-measurements,m-capture b n n INT- 2018 b GT? Gentle Touch: q tr = 0 l = 0 dσ dσ 5 10 0 hω excitation σ n n Where
More informationSpin-isospin correlation in 8 He and 12 Be(p,n)
Mini-workshop 18 November 2014 Spin-isospin correlation in 8 He and Be(p,n) H. Sakai 1, H. Sagawa 1,2, M. Kobayashi 3, S. Shimoura 3, T. Suzuki 4 and K. Yako 3 For the SHARAQ Collaboration 1 RIKEN Nishina
More informationSpin Cut-off Parameter of Nuclear Level Density and Effective Moment of Inertia
Commun. Theor. Phys. (Beijing, China) 43 (005) pp. 709 718 c International Academic Publishers Vol. 43, No. 4, April 15, 005 Spin Cut-off Parameter of Nuclear Level Density and Effective Moment of Inertia
More informationThe Periodic Table. Periodic Properties. Can you explain this graph? Valence Electrons. Valence Electrons. Paramagnetism
Periodic Properties Atomic & Ionic Radius Energy Electron Affinity We want to understand the variations in these properties in terms of electron configurations. The Periodic Table Elements in a column
More informationThis work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract
This work was performed under the auspices of the U.S. Department of Energy by under contract DE-AC52-7NA27344. Lawrence Livermore National Security, LLC The ITER tokamak Tungsten (W) is attractive as
More informationContents / Key words. Self-consistent deformed pnqrpa for spin-isospin responses
Contents / Key words Self-consistent deformed pnqrpa for spin-isospin responses Self-consistency: T=1 pairing and IAS Collectivity of GT giant resonance Possible new type of collective mode: T= proton-neutron
More informationCHEM 130 Exp. 8: Molecular Models
CHEM 130 Exp. 8: Molecular Models In this lab, we will learn and practice predicting molecular structures from molecular formulas. The Periodic Table of the Elements IA 1 H IIA IIIA IVA VA VIA VIIA 3 5
More informationRadioactivity at the limits of nuclear existence
Radioactivity at the limits of nuclear existence Zenon Janas Institute of Experimental Physics University of Warsaw Chart of nuclei - stable - β + - β - - α - fission - p p and 2p radioactivty proton radioactivity
More informationShape coexistence and beta decay in proton-rich A~70 nuclei within beyond-mean-field approach
Shape coexistence and beta decay in proton-rich A~ nuclei within beyond-mean-field approach A. PETROVICI Horia Hulubei National Institute for Physics and Nuclear Engineering, Bucharest, Romania Outline
More informationRadiometric Dating (tap anywhere)
Radiometric Dating (tap anywhere) Protons Neutrons Electrons Elements on the periodic table are STABLE Elements can have radioactive versions of itself called ISOTOPES!! Page 1 in your ESRT has your list!
More informationAn Introduction to the Ion-Optics of Magnet Spectrometers
An Introduction to the Ion-Optics of Magnet Spectrometers U. Tokyo, RIKEN The 14 th RIBF Nuclear Physics Seminar Series of Three Lectures CNS, University of Tokyo February 27, 2006 Georg P. Berg University
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 informationCorrelations between magnetic moments and β decays of mirror nuclei
PHYSICAL REVIEW C, (8) Correlations between magnetic moments β decays of mirror nuclei S. M. Perez,, W. A. Richter, B. A. Brown, M. Horoi Department of Physics, University of Cape Town, Private Bag, Rondebosch,
More informationIsoscalar spin-triplet pairing and tensor correla1ons on Spin-Isospin response Osaka,Japan, November 16-19,
Isoscalar spin-triplet pairing and tensor correla1ons on Spin-Isospin response ------------- Osaka,Japan, November 16-19, 2015 ----------------- Hiroyuki Sagawa RIKEN/University of Aizu Skyrme tensor interac1ons
More informationNuclear Structure in Astrophysics Recent Examples from the S-DALINAC
TU DARMSTADT 2007 Nuclear Structure in Astrophysics Recent Examples from the S-DALINAC S-DALINAC and research program an overview Selected examples: Deuteron electrodisintegration under 180 and its importance
More informationCLASS TEST GRADE 11. PHYSICAL SCIENCES: CHEMISTRY Test 4: Matter and materials 1
CLASS TEST GRADE PHYSICAL SCIENCES: CHEMISTRY Test 4: Matter and materials MARKS: 45 TIME: hour INSTRUCTIONS AND INFORMATION. Answer ALL the questions. 2. You may use non-programmable calculators. 3. You
More informationRare Isotope productions from Projectile Fragmentation. Ca + Be. Betty Tsang March 27, 2008
Rare Isotope productions from Projectile Fragmentation 48 Ca + Be Betty Tsang March 27, 2008 Acknowledgement Collaborators: Michal Mocko (thesis) M. Andronenko, L. Andronenko, N. Aoi, J. Cook, F. Delaunay,
More informationRemarks about weak-interaction processes
Remarks about weak-interaction processes K. Langanke GSI Darmstadt and TUD, Darmstadt March 9, 2006 K. Langanke (GSI and TUD, Darmstadt)Remarks about weak-interaction processes March 9, 2006 1 / 35 Nuclear
More informationPresentation at the 10th RIBLL Collaboration Symposium, Beijing, 2017/1/7
Presentation at the 10th RIBLL Collaboration Symposium, Beijing, 2017/1/7 Outline 1. Background 1.1 Decay for proton-rich nuclei 1.2 Astrophysical implications 2. Experiments 2.1 Introduction 2.2 Experimental
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 informationDouble Charge-Exchange Reactions and Double Beta- Decay. N. Auerbach, Tel Aviv University and Michigan State University
Double Charge-Exchange Reactions and Double Beta- Decay N. Auerbach, Tel Aviv University and Michigan State University D.C. Zheng, L. Zamick and NA, Annals of Physics 197, 343 (1990). Nuclear Structure
More informationI. 1. Nuclear Structure Study of 50 Mn by Charge-exchange (p,n) Reaction on 50 Cr
CYRIC Annual Report 2002 I. 1. Nuclear Structure Study of 50 Mn by Charge-exchange (p,n) Reaction on 50 Cr Kamurai G., Orihara H., Terakawa A., Yamamoto A., Suzuki H., Mizuno H., Kikuchi Y., Kumagai K.,
More informationORBITAL DIAGRAM - A graphical representation of the quantum number "map" of electrons around an atom.
178 (MAGNETIC) SPIN QUANTUM NUMBER: "spin down" or "spin up" - An ORBITAL (region with fixed "n", "l" and "ml" values) can hold TWO electrons. ORBITAL DIAGRAM - A graphical representation of the quantum
More information1 of 5 14/10/ :21
X-ray absorption s, characteristic X-ray lines... 4.2.1 Home About Table of Contents Advanced Search Copyright Feedback Privacy You are here: Chapter: 4 Atomic and nuclear physics Section: 4.2 Absorption
More informationSupernovae from massive stars
Supernovae from massive stars Events in which heavy elements are made that enrich the interstellar medium from which later stars form Alak K. Ray, TIFR, Mumbai A core collapse Supernova: Death of a massive
More informationNuclear Physics and Supernova Dynamics. Karlheinz Langanke GSI Helmholtzzentrum Darmstadt Technische Universität Darmstadt
Nuclear Physics and Supernova Dynamics Karlheinz Langanke GSI Helmholtzzentrum Darmstadt Technische Universität Darmstadt Tribute to Gerry - Stony Brook, November 26, 2013 Hans Bethe s Centennial at Caltech
More informationSelected Topics in Physics a lecture course for 1st year students by W.B. von Schlippe Spring Semester 2007
Selected Topics in Physics a lecture course for 1st year students by W.B. von Schlippe Spring Semester 2007 Lecture 11 1.) Determination of parameters of the SEMF 2.) α decay 3.) Nuclear energy levels
More informationMagnetic Dipole and Quadrupole Transitions in Nuclei Open Problems
TU DARMSTADT Magnetic Dipole and Quadrupole Transitions in Nuclei Open Problems Qualitative nature of the M1 response Orbital M1 scissors mode: low and high Spin M1 resonance in heavy deformed nuclei Quenching
More informationGANIL / SPIRAL1 / SPIRAL2
Nuclear Structure, Reaction and Dynamics GANIL / SPIRAL1 / SPIRAL2 A huge discovery potential Exotic Nuclei Proton number Z Which force? 3-body, tensor, spin-orbit, Isospin dependence, Continuum coupling
More informationRich Opportunities for Astrophysics
Rich Opportunities for Astrophysics A flood of new observations and more to come with INTEGRAL, JWST, Constellation-X, Growing computational capability Problems ripe for solution: How supernovae explode,
More informationElement Cube Project (x2)
Element Cube Project (x2) Background: As a class, we will construct a three dimensional periodic table by each student selecting two elements in which you will need to create an element cube. Helpful Links
More informationLast 4 Digits of USC ID:
Chemistry 05 B Practice Exam Dr. Jessica Parr First Letter of last Name PLEASE PRINT YOUR NAME IN BLOCK LETTERS Name: Last 4 Digits of USC ID: Lab TA s Name: Question Points Score Grader 8 2 4 3 9 4 0
More informationObservation of the Giant monopole resonances in the Sn isotopes via (α,α ) reactions at 400 MeV at RCNP - Latest results and implications -
Observation of the Giant monopole resonances in the isotopes via (α,α ) reactions at 400 MeV at RCNP - Latest results and implications - Collaborators: S. Okumura, U. Garg, M. Fujiwara, P.V. Madhusudhana
More informationCh. 9 NOTES ~ Chemical Bonding NOTE: Vocabulary terms are in boldface and underlined. Supporting details are in italics.
Ch. 9 NOTES ~ Chemical Bonding NOTE: Vocabulary terms are in boldface and underlined. Supporting details are in italics. I. Review: Comparison of ionic and molecular compounds Molecular compounds Ionic
More informationAtomic Physics. Chapter 6 X ray. Jinniu Hu 24/12/ /20/13
Atomic Physics Chapter 6 X ray 11/20/13 24/12/2018 Jinniu Hu 1!1 6.1 The discovery of X ray X-rays were discovered in 1895 by the German physicist Wilhelm Roentgen. He found that a beam of high-speed electrons
More informationProbing the Symmetries of Isobaric Analogue States M.A.Bentley University of York, UK. in collaboration with. Dave Warner
DDW Symposium CCLRC Daresbury February 2006 1 Probing the Symmetries of Isobaric Analogue States M.A.Bentley University of York, UK in collaboration with Dave Warner Overview Overview DDW Symposium CCLRC
More informationSilvia M. Lenzi University of Padova and INFN. Silvia Lenzi, 10th Int. Spring Seminar on Nuclear Physics, Vietri sul Mare, May 21-25, 2010
Structure of Neutron-Rich Nuclei near N=40 Silvia M. Lenzi University of Padova and INFN 10th International Spring Seminar on Nuclear Physics Vietri sul Mare, May 21-25, 2010 Collaboration Theory: F. Nowacki,
More informationThe Ring Branch. Nuclear Reactions at. Mass- and Lifetime Measurements. off Exotic Nuclei. Internal Targets. Electron and p. Experiments: Scattering
stochastic cooling Exotic nuclei from Super-FRS Degrader for fast slowing down The Ring Branch TOF Detector MCPs E anode ion B CR Electron cooler NESR secondary electrons Experiments: Mass- and Lifetime
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 informationproton-neutron pairing vibrations
proton-neutron pairing vibrations Outline of this lecture: Basics of the vibrational modes of excitation in nuclei surface vibration, like-particle pairing vibration, and then Microscopic framework to
More informationPART 1 Introduction to Theory of Solids
Elsevier UK Job code: MIOC Ch01-I044647 9-3-2007 3:03p.m. Page:1 Trim:165 240MM TS: Integra, India PART 1 Introduction to Theory of Solids Elsevier UK Job code: MIOC Ch01-I044647 9-3-2007 3:03p.m. Page:2
More informationApplications of nuclear physics in neutrino physics
Applications of nuclear physics in neutrino physics Emanuel Ydrefors E. Ydrefors (KTH) Neutrino physics 1 / 16 Outline of lecture Brief introduction to neutrinos Nuclear beta decay Neutrino-nucleus scattering
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 informationNeutrino Nuclear Responses for ββ ν & Charge Exchange Reactions. Hiro Ejiri RCNP Osaka & CTU Praha
Neutrino Nuclear Responses for ββ ν & Charge Exchange Reactions Hiro Ejiri RCNP Osaka & CTU Praha Nuclear responses (matrix elements) for ββ ν and charge exchange reactions H. Ejiri, Phys. Report 338 (2000)
More informationTHE STRUCTURE OF ATOMS. ATOMS Atoms consist of a number of fundamental particles, the most important ones are...
Atomic Structure THE STRUCTURE OF ATOMS ATOMS Atoms consist of a number of fundamental particles, the most important ones are... Mass / kg Charge / C Relative mass Relative Charge PROTON NEUTRON ELECTRON
More informationCOMPARATIVE STUDY OF PIGE, PIXE AND NAA ANALYTICAL TECHNIQUES FOR THE DETERMINATION OF MINOR ELEMENTS IN STEELS
COMPARATIVE STUDY OF PIGE, PIXE AND NAA ANALYTICAL TECHNIQUES FOR THE DETERMINATION OF MINOR ELEMENTS IN STEELS ANTOANETA ENE 1, I. V. POPESCU 2, T. BÃDICÃ 3, C. BEªLIU 4 1 Department of Physics, Faculty
More information02/05/09 Last 4 Digits of USC ID: Dr. Jessica Parr
Chemistry 05 B First Letter of PLEASE PRINT YOUR NAME IN BLOCK LETTERS Exam last Name Name: 02/05/09 Last 4 Digits of USC ID: Dr. Jessica Parr Lab TA s Name: Question Points Score Grader 2 2 9 3 9 4 2
More informationNucleus. Electron Cloud
Atomic Structure I. Picture of an Atom Nucleus Electron Cloud II. Subatomic particles Particle Symbol Charge Relative Mass (amu) protons p + +1 1.0073 neutrons n 0 1.0087 electrons e - -1 0.00054858 Compare
More informationMeasurement of the 14 Be(p,n) 14 B(1 + ) Reaction in Inverse Kinematics
XXVII Texas Symposium on Relativistic Astrophysics, December 8-13, 2013. Dallas, TX Measurement of the e(p,n) (1 + ) Reaction in Inverse Kinematics Y.Satou, Seoul National University e Y.Satou, et al.,
More informationNuclear Astrophysics
I. Hydrostatic burning and onset of collapse Karlheinz Langanke GSI & TU Darmstadt 15 Stellar energy source Energy comes from nuclear reactions in the core. E = mc 2 4 1 H 4 He + neutrinos + 26.7MeV The
More informationResearch Activities at the RCNP Cyclotron Facility
Research Activities at the RCNP Cyclotron Facility Kichiji Hatanaka Research Center for Nuclear Physics Osaka University International Symposium on Nuclear Physics in Asia Convention Center of Beihang
More informationErice, September, 2017,
Erice, September, 2017, Double beta (bb) decay neutrinoless double beta (0nbb) decay NME the specialties of 96 Zr/ 96 Nb for b and bb decay Mass measurements using the JYFLTRAP ion trap Results and the
More informationBeta Decay Studies in nuclear structure
Beta Decay Studies in nuclear structure Escuela de doctorado de Física Nuclear Santiago 1 de Marzo de 2007 Introducción Cómo hacer una medida Un ejemplo Berta Rubio IFIC (CSIC-Univ. Valencia) B. Rubio.
More informationElectron Configuration. The electron configuration of an atom tells us how the electrons are distributed among the various atomic orbitals.
Electron Configuration The electron configuration of an atom tells us how the electrons are distributed among the various atomic orbitals. Spin Quantum Number, m s In the 1920s, it was discovered that
More informationORBITAL DIAGRAM - A graphical representation of the quantum number "map" of electrons around an atom.
160 ORBITAL DIAGRAM - A graphical representation of the quantum number "map" of electrons around an atom. 4p 3d 4s 3p 3s 2p 2s 1s Each blank represents an ORBITAL, and can hold two electrons. The 4s subshell
More information-"l" also contributes ENERGY. Higher values for "l" mean the electron has higher energy.
175 - Giving the four parameters will uniquely identify an electron around an atom. No two electrons in the same atom can share all four. These parameters are called QUANTUM NUMBERS. PRINCIPAL QUANTUM
More informationIntroduction to X-ray Photoelectron Spectroscopy (XPS) XPS which makes use of the photoelectric effect, was developed in the mid-1960
Introduction to X-ray Photoelectron Spectroscopy (XPS) X-ray Photoelectron Spectroscopy (XPS), also known as Electron Spectroscopy for Chemical Analysis (ESCA) is a widely used technique to investigate
More informationGuide to the Extended Step-Pyramid Periodic Table
Guide to the Extended Step-Pyramid Periodic Table William B. Jensen Department of Chemistry University of Cincinnati Cincinnati, OH 452201-0172 The extended step-pyramid table recognizes that elements
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 informationLaser Spectroscopy on Bunched Radioactive Ion Beams
Laser Spectroscopy on Bunched Radioactive Ion Beams Jon Billowes University of Manchester Balkan School on Nuclear Physics, Bodrum 2004 Lecture 1. 1.1 Nuclear moments 1.2 Hyperfine interaction in free
More informationNuclear Astrophysics
Nuclear Astrophysics II. Core-collapse supernovae Karlheinz Langanke GSI & TU Darmstadt Aarhus, October 6-10, 2008 Karlheinz Langanke ( GSI & TU Darmstadt) Nuclear Astrophysics Aarhus, October 6-10, 2008
More informationCHEM 10113, Quiz 5 October 26, 2011
CHEM 10113, Quiz 5 October 26, 2011 Name (please print) All equations must be balanced and show phases for full credit. Significant figures count, show charges as appropriate, and please box your answers!
More informationNeutrino Nuclear Responses and Medium Energy Photons
Neutrino Nuclear Responses and Medium Energy Photons Hiro Ejiri RCNP Osaka & CTU Praha Thanks Chary for invitation Saskatchewan 4-10 1. Neutrino studies in nuclei & neutrino nuclear responses 2. Neutrino/weak
More information8. Relax and do well.
CHEM 1515 Exam II John II. Gelder October 14, 1993 Name TA's Name Lab Section INSTRUCTIONS: 1. This examination consists of a total of 8 different pages. The last two pages include a periodic table, a
More information(please print) (1) (18) H IIA IIIA IVA VA VIA VIIA He (2) (13) (14) (15) (16) (17)
CHEM 10113, Quiz 3 September 28, 2011 Name (please print) All equations must be balanced and show phases for full credit. Significant figures count, show charges as appropriate, and please box your answers!
More informationLarge scale shell model calculations for neutron rich fp-shell nuclei
Large scale shell model calculations for neutron rich fp-shell nuclei Physical Research Laboratory, Ahmedabad-380 009, India Collaborators: I. Mehrotra (Allahabad) P.Van Isacker (GANIL, France) V.K.B.
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 PowerPoint slides. in Tenth International Conference on Cold Fusion. 23. Cambridge,
More informationChapter 6 Part 3; Many-electron atoms
Chapter 6 Part 3; Many-electron atoms Read: BLB 6.7 6.9 HW: BLB 6:59,63,64,67,71b-d,74,75,90,97; Packet 6:10 14 Know: s & atoms with many electrons Spin quantum number m s o Pauli exclusion principle o
More informationUnit 1 Part 2 Atomic Structure and The Periodic Table Introduction to the Periodic Table UNIT 1 ATOMIC STRUCTURE AND THE PERIODIC TABLE
UNIT 1 ATOMIC STRUCTURE AND THE PERIODIC TABLE PART 2 INTRODUCTION TO THE PERIODIC TABLE Contents 1. The Structure of the Periodic Table 2. Trends in the Periodic Table Key words: group, period, block,
More information8. Relax and do well.
CHEM 1314 3;30 pm Theory Exam III John III. Gelder November 13, 2002 Name TA's Name Lab Section INSTRUCTIONS: 1. This examination consists of a total of 8 different pages. The last page include a periodic
More informationTwo-Proton Decay Experiments
Two-Proton Decay Experiments Robert Charity Washington University, St. Louis, USA Classification of 2p decays Goldansky (190) 2p decay (like double β decay) Intermediate state not accessible to 1p decay.
More informationMANY ELECTRON ATOMS Chapter 15
MANY ELECTRON ATOMS Chapter 15 Electron-Electron Repulsions (15.5-15.9) The hydrogen atom Schrödinger equation is exactly solvable yielding the wavefunctions and orbitals of chemistry. Howev er, the Schrödinger
More informationNuclear Physics and Astrophysics 2015 (SPA-5302), Homework 2
Nuclear Physics and Astrophysics 2015 (SPA-5302), Homework 2 2015 Teppei Katori Name: ID: Problem 1 (4 points) An acient archaeological wooden tool is excavated in China. An experimenter measures the activity
More informationCircle the letters only. NO ANSWERS in the Columns!
Chemistry 1304.001 Name (please print) Exam 5 (100 points) April 18, 2018 On my honor, I have neither given nor received unauthorized aid on this exam. Signed Date Circle the letters only. NO ANSWERS in
More informationAMD. Skyrme ( ) 2009/03/ / 22
2009 3 25 26 AMD Skyrme ( ) 2009/03/25 26 1 / 22 (?) ( ) 2009/03/25 26 2 / 22 Nuclear Matter in Nuclear Collisions and Neutron Stars 0 60 E sym [MeV] 40 20 0 0 NL3 ChPT DBHF DD ρδ DD TW var AV18+ δ V+3
More information