large -delayed neutron emission probabilities in the 78ni ... · j. a. winger et al., phys. rev....

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Large -Delayed Neutron Emission Probabilities in the 78 Ni Region Prof. Jeff Allen Winger Mississippi State University Background Recent Experiments The Future Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

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  • Large -Delayed Neutron EmissionProbabilities in the 78Ni Region

    Prof. Jeff Allen WingerMississippi State University

    Background

    Recent Experiments

    The Future

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

  • Why is -delayed neutron emission important?

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    r-process nucleosyntheis

    Old t1/2 and Pn valuesNew t1/2 and Pn values

    Decay properties are among important input data for the analysis of processes

    occurring in nuclear fuels : half-lives, -delayed neutron branching

    ratios, and total decay energy release (total decay heat)

    Understanding of the fission yields and the properties of neutron-rich fission products

    is important for the safe and efficient operation of current and future power

    reactors as well as for nuclear fuel/waste (re)processing

    *

    0.1 1 10 10010-6

    10-5

    10-4

    10-3

    10-2

    Del

    ayed

    neu

    tron

    yiel

    d (n

    /s/fi

    ssio

    n)

    Time after fission (s)

    ORIGEN Keepin (IAEA 6 group)

    Application of -delayed neutron emissionin nuclear power simulations

    Ian C. Gauld (2010)ORNL, Reactor and Nuclear Safety Division, Reactor Physics Group

    Integral βn measurementsused for reactor analysis

    -n isotopic decay data

    ORIGEN is missing data for very short-lived

    fission products

    *Oak Ridge Isotope Generation and Decay Code

    *

  • Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    (N-1,Z+1)0

    Energy

    (N,Z)

    Sn

    S2n

    What factors into determining the Pn value?

    Pygmy GTR

    GTR

    Strength Function

    f(Z+1,E*)

    Fermi Integral

    Feeding Intensity

    decay

    2n decay

    n decay

  • Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    The devil is in the details!77 77 * 76Cu Zn Zn

    n

    77 1 2 77 2 35 72 25/2 9/2 5/2 9/2Cu: ( 1 ) ( 1 ) Zn: ( 1 ) ( 1 )f g f g

    3 5 7, , Allowed2 2 2

    5 3 5 7, , First Forbidden2 2 2 2

    1 9, First Forbidden Unique2 2

    N Z

    9/ 21g

    5/ 21 f

    3/ 22 p

    1/ 22 p 9/ 21g

    Key Factors:1. Available energy for decay.2. Ordering and energy of the single-

    particle orbitals.3. Composition of the states

    70 72 74 76 78 80 82 84 86 88

    0

    20

    40

    60

    80

    100

    P n [

    %]

    A

    GT+FF GT GT, Moeller 97

    I.N. Borzov, Phys. Rev. C71, 065801 (2005).

    Ni isotopes

  • How do you measure -delayed neutron emission?

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    1. Direct detection of neutron

    1 corrn nb imp corr nd

    nn imp

    N r N NP

    N e

    NERO/NSCL P. Hosmer et al., Phys. Rev. C82, 025806 (2010)

    Neutron Detector

    Detector

    ImplantationDetector

    1 1 2 2

    1 1 1 1 2 2 2 2

    21 2

    1 2

    coincicence summing correction

    absolute branching ratio

    saturation fraction

    n

    s

    BR

    SF

    A s A sNP N NN N BR SF BR SF

    2. Indirect determination using rays

    1 2

    2 2

    2 2 2 2

    nmp

    A sP

    N BR SF

    HRBIF

    J. A. Winger et al., Phys. Rev. Lett. 102, 142502 (2009)S. V. Ilyushkin et al., Phys. Rev. C80, 054304 (2009)J. A. Winger et al., Phys. Rev. C81, 044303 (2010)S. Padgett et al., Phys. Rev. C82, 064314 (2010)

  • Holifield Radioactive Ion Beam Facility

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    +/-40 keV +/-160 keV

    Mass separatorM/ΔM ~ 600

    fission fragments

    charge exchange cell (removes Zn)

    Positiveions

    IRIS-1

    UCx54 MeV protons

    ORIC

    Ranging outexperiment

    LeRIBSSexperiment

    Isobar separatorM/ΔM ~ 10000

    2-3 MeV/u

    200 keV

    Positive or negative ions

    Tandem accelerator(negative ions only)

    IRIS-2

  • Ranging Out Detector Station

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    Particle Identification Energy (1 keV/chn)

    624 keV

    84Ga

    76Cu

    76Ga76Ge

    203 torr

    76Cu 76Ga76Ge

    76Cu598 keV

    76Ga 563 keV

    161 torr

    Energy (0.5 keV/chn)

    Ene

    rgy

    6th

    Ano

    de

    Total Energy

    76Ga 563 keV

    76Cu598 keV

    Excellent system for the direct measurement of absolute branching ratios.

    Ion Chamber

    CARDS Ge Array

    Moving Tape Collector

    Clarion ARay for Decay Spectroscopy

  • Low-energy Radioactive Ion Beam Spectroscopy Station

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    CARDS Ge ArrayMoving Tape Collector

    MTC and CARDS frame built by Ed Zganjar (LSU)

    1. Much higher beam currents since we do not use tandem. (Factor of ~20.)

    2. The ability to use positive or negative ions.3. With positive ions, additional gain of ~10 from not

    using charge exchange cell.4. Better effective mass resolving power for the high

    resolution separator when using positive ions. Can achieve nearly pure beams.

    5. Faster MTC drive allows study of shorter lived nuclides.

    6. Higher beam intensity allows for detailed decay spectroscopy.

    7. Higher beam intensity allows us to reach further from stability.

    8. Possibility to implement tagging in the future.

  • HRIBF n-Decay Studies Near 78Ni

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    40 5045 54

    Cu

    Ni

    Ge

    Ga

    Zn

    As

    78Ni

    83Ga 84Ga

    77Cu

    81Zn

    78Cu76Cu

    HRBIF J. A. Winger et al., Phys. Rev. Lett. 102, 142502 (2009)S. V. Ilyushkin et al., Phys. Rev. C80, 054304 (2009)J. A. Winger et al., Phys. Rev. C81, 044303 (2010)S. Padgett et al., Phys. Rev. C82, 064314 (2010)

    Co

    82Zn

    74Cu 75Cu

    83Zn

    85Ga

    79Cu

    *NERO/NSCL P. Hosmer et al., Phys. Rev. C82, 025806 (2010)

    **

    * ** *

    * * *

    * *

    ***

    *

  • How it all works out.

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    Ex: 76,77 76,77 * 75,76Cu Zn Zn

    n

    Energy (0.5 keV/chn)

    76Zn199 keV

    77Zn189 keV

    75Zn228 keV

    Energy (0.5 keV/chn)

    76Zn199 keV

    76Cu

    76Ga76Ge

    RO Mode203 torr

    76Cu 76Ga

    76Ge

    PT Mode161 torrE

    nerg

    y 6t

    hA

    node

    Total Energy

    76

    6 6

    77

    3 3

    4 25

    24 23

    21 19

    78

    8

    5

    27

    8

    23 5

    83

    Old

    4.2

    1

    PT Sat. 7.3 7.0

    RO 10.2 29 29

    20.2 28 28.7

    PT 7.2 31.5 34.0

    Sat.

    Adopt

    7.

    Experiment Theory

    Nuclide Mode MTC Rel

    9.7

    New

    7

    32.1 28.5

    PT 5.2 6

    .2

    30.0

    65

    62.8

    42.6

    2

    40.4

    50.5

    . Abs

    5

    PT 20.2 6

    .

    4

    Cu

    Cu s

    s

    s

    Cu s

    Ga s

    4

    50.7

    Sat

    1 .7

    . 61

    5

  • It ain’t always that easy!

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    Major complications:1. Unknown or incorrect branching ratios.2. Unknown feeding through isomers.

    J. A. Winger et al., Phys. Rev. Lett. 102, 142502 (2009) S. V. Ilyushkin et al., Phys. Rev. C80, 054304 (2009)

  • 5/2- ground stateFlanagan et al., PRL103, 142501 (2009)

    75Zn Level Scheme

    Dr. Jeff Winger

    (421) 19(4)%BR

    1. Set limits on the absolute branching ratio.2. Identified the 1/2- isomer and the 9/2+

    excited state

    North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

  • Dr. Jeff Winger

    -decays of 83,84,85GaWinger et al., PRC81, 044303 (2010)

    624 keV

    107 keV85Ga at LeRIBSS, Feb. 2011 1. Refined the energy of the1/2+

    state and identified the second excited state in 83Ge

    2. Establish the 5/2- gs for 83Ga3. Established the energy of the

    first 2+ state in 84Ge4. Observed the decay of 85Ga for

    the first timeNorth American Workshop on Beta-Delayed Neutron Emission 5/3/2013

  • Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    Results Pn values are consistently higher than previously reported for nuclides in this region.

  • The Future

    Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013

    0

    20

    40

    60

    80

    100

    0.001 0.01 0.1 1 10

    Energy (MeV)

    Eff

    icie

    ncy

    (%)

    HRIBF

    long-counter

    NERO

    Neutron Efficiency by Ring

    0

    20

    40

    60

    80

    100

    0.001 0.01 0.1 0.5 1 2 3 5

    Energy (MeV)

    Eff

    icie

    ncy

    (%)

    Ring 4

    Ring 3

    Ring 2

    Ring 1

  • Dr. Jeff Winger North American Workshop on Beta-Delayed Neutron Emission 5/3/2013