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Production of new neutron rich heavy and superheavy nuclei Valeriy Zagrebaev, Mikhail Itkis , Alexander Karpov for “SHE-2015”, March 31, 2015, A&M University, USA JINR (Dubna) Fusion reactions Elements 119 and 120 are on the way. What’s the next? Radioactive ion beams? Multinucleon transfer reactions Shell effects in damped collisions of heavy ions? Production of new neutron rich SH nuclei in transfer reactions Production of new neutron rich Heavy nuclei in transfer reactions Separation of the products of transfer reaction (GALS setup)
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  • Production of new neutron rich heavy and superheavy nuclei

    Valeriy Zagrebaev, Mikhail Itkis, Alexander Karpov

    for “SHE-2015”, March 31, 2015, A&M University, USA

    JINR (Dubna)

    •  Fusion reactions •  Elements 119 and 120 are on the way. What’s the next? •  Radioactive ion beams?

    •  Multinucleon transfer reactions •  Shell effects in damped collisions of heavy ions? •  Production of new neutron rich SH nuclei in transfer reactions •  Production of new neutron rich Heavy nuclei in transfer reactions •  Separation of the products of transfer reaction (GALS setup)

  • We are still far from the Island of Stability

    2

  • What is beyond 118 element?

    Ø  Heavier projectiles (50Ti, 54Cr, 58Fe, 64Ni) Ø  Heavier targets (251Cf, 254Es -???); Ø  Symmetric reactions: 136Xe+136Xe, 136Xe+150Nd, 150Nd+150Nd; Ø  Multi–Nucleon–Exchange - Reactions with RIB (??, or colliders –

    technique – (K4-K10)): Ø  Nucleon transfer reactions (136Xe+208Pb, 238U+248Cm).

    Sufficient increasing of overall experiment efficiency is needed!

    Heaviest target: 249Cf → Zmax= 118 ↓

  • New elements 119 and 120 are coming !

    4

  • Mass-energy distributions of binary reaction fragments

    Driving potentials are calculated with the NRV code (nrv.jinr.ru)

    150

    200

    250

    300

    350

    36S+238U→274Hs*

    E*=46 MeV

    Mass (u)

    64Ni+238U→302120*

    E*=31 MeV

    48Ca+238U→286Cn*

    E*=35 MeV

    Yie

    lds

    (arb

    .u.)

     

     

     

    TK

    E (

    MeV

    )

    Z=28

     

     

     

     

     

     

    50 100 150 200 250

    1

    2

    3

    Z=28

    Z=82N=126N=50Z=28

    Z=82N=126N=50

     

     

    M=200 u M=208 u M=215 u

    50 100 150 200 250

    1

    2

    3

     

     

    50 100 150 200 250

    1

    2

    3

    4

    Z=82N=126N=50

     

    210

    220

    230

    240

    250

    260poten

    tial energ

    y (M

    eV)

    • G.N. Knyazheva, I. Itkis, E.M. Kozulin. The time scale of quasifission process in the reactions with heavy ions. International Symposium Entrance Channel Effect on the Reaction Mechanism in Heavy Ion Collisions, Messina (Italy) - November 6-8, 2013, Journal of Physics: Conference Series 515 (2014) 012009.

  • 100

    150

    200

    250

    300

    350

       

     

     

    50 100 150 200 250100

    150

    200

    250

    300

    35064Ni+238U→302120

     

     

    Mass (u)

    58Fe+244Pu→302120

    0

    1

    2

    3

    4

     

       

    50 100 150 200 2500123456  

       

    Mass (u)

    100

    150

    200

    250

    300

    35048Ca+238U→286Cn

     

     

     

    TK

    E (

    MeV

    )

    0.0

    0.5

    1.0

    1.5

    2.0

    2.5  

     

     

    Yie

    ld (

    arb. u

    nit

    s)

    150 200 250 3000

    100200300400500600700800

     

     

     

    Co

    un

    ts

    200 250 300 3500

    20406080

    100120  

     

     

    200 250 300 3500

    2

    4

    6

    8

    10  

     

    TKE (MeV)

    Y(ACN/2±20)=12%

    Y(ACN/2±20)=8%

    Y(ACN/2±20)=4%

    1840

    2444

    2576

    Zt Zp

    34 u

    22 u

    11 u

    70%

    ≤2%

    ≤0.2%

    for ACN/2±20

    E*CN≈45MeV

    E.M. Kozulin et al., Dynamics of the 64Ni+238U reaction as a possible tool for synthesis of element with Z=120. Phys. Lett. B686, (2010), 227-232.

  • Influence of entrance channel

    Z1Z2=980 1472 2132 2660

    • E.M.Kozulin, G.N.Knyazheva, I.M.Itkis, E.M.Gazeeva, N.I.Kozulina, T.A.Loktev, K.V.Novikov, I.Harca. Shell effects in fission, quasi-fission and in multi-nucleon transfer reactions. International Symposium Entrance Channel Effect on the Reaction Mechanism in Heavy Ion Collisions, Messina (Italy) - November 6-8, 2013, Journal of Physics: Conference Series 515 (2014) 012010.

  • 88Sr+176Yb: shell effects in damped collisions

    170 175 180 185 190 195 200 20510-4

    10-3

    10-2

    10-1

    100

    101

    102

    Z=82

    Yie

    ld (

    mb

    /(sr

    u))

    Fragment mass (u)

    88Sr +176Yb

    Z=28

    60 80 100 120 140 160 180 2000102030405060708090100

    Fragment mass (u)

    Exci

    tati

    on

    ener

    gy (

    MeV

    )

    40 60 80 100 120 140 160 180 200 220250

    260

    270

    280

    290

    300

    310

    208Pb58Fe

    N=50

    Z=50N=82

    N=126Z=82

    Z=28

    176Yb

    Pote

    nti

    al ener

    gy (

    MeV

    )

    Fragment mass (u)

    88Sr

    140120100806040200-20-40-60

    60 80 100 120 140 160 180 200

    160180200220240260280300320340360

    Fragmet mass (u)

    TK

    E (

    MeV

    )

    100 3x100 101 3x101 102 3x102 103 3x103 104

    TK

    EL

    (M

    eV)

    • E.M. Kozulin, G.N. Knyazheva, S.N. Dmitriev, I.M. Itkis, M.G. Itkis, T.A. Loktev, K.V. Novikov, A. Baranov, W.H. Trzaska, E. Vardaci, S. Heinz, O. Beliuskina, S.V.Khlebnikov. Shell effects in damped collisions of 88Sr with 176Yb at the Coulomb barrier energy. Phys. Rev. C89, 014614 (2014).

  • Fusion reactions with Radioactive Ion Beams for the production of neutron rich superheavy nuclei ?

    No chances today and in the nearest future 9

  • Multinucleon transfer reactions for synthesis of heavy and

    superheavy nuclei

  • Production of superheavies in multi-nucleon transfers (choice of reaction is very important)

    11

  • Shell effects: Pb valley normal (symmetrizing) quasi-fission

    inverse (anti-symmetrizing) quasi-fission

    12

  • U-like beams give us more chances to produce neutron rich SH nuclei in “inverse quasi-fission” reactions

    experiment is scheduled for March at GSI (we want to see Pb+x, then Pb+Ca+Pb) 13

  • 238U + 248Cm. Primary fragments

    14

  • Production of transfermium nuclei along the line of stability looks quite possible (only if there are shell effects!?)

    Rather wide angular distribution of reaction fragments: a new kind of separators is needed

    experiments on Au+Th and U+Th are currently going on in Texas (without separators) 15

  • Test (surrogate) reaction aimed on a search for the shell effects

    in low-energy multi-nucleon transfer reactions

    The experiment was performed (September 2014) at the Flerov Laboratory (Dubna)

  • New heavy nuclei in the region of N=126

    “blank spot”

  • Test experiment on 136Xe + 208Pb collisions (Dubna, 2011)

    18 Experiment with Z identification of PLF was performed in Legnaro last summer

  • 136Xe+208Pb: productions of heavy neutron-rich nuclei in multinucleon transfer reaction

    30 0

    40 0

    50 0

    60 0

    TK

    E (

    MeV

    )

    100 12 0 1 40 160 180 20 0 2 20 24010

    -3

    10-2

    10-1

    1 00

    1 01

    208Pb

    Mass (u)

    Yie

    ld (

    mb)

    136Xe+208Pb(Ec.m.

    =526 MeV)

    136Xe 200 205 210 215 220 225 230

    10-3

    10-2

    10-1

    100

    101

    Z=88

    Z=84

    Z=86

    136Xe+208Pb (Ec.m.=514MeV)

    cro

    ss s

    ecti

    on (

    mb

    )

    Mass (u)

    Cross  sec(on  for  210Po,  222Rn,  224Ra  (Ac(va(on  analysis)  

    • E.M.Kozulin, E.Vardaci, G.N.Knyazheva, A.A.Bogachev, S.N.Dmitriev, I.M.Itkis, M.G.Itkis, A.G.Knyazev, T.A.Loktev, K.V.Novikov, E.A.Razinkov, O.V.Rudakov, S.V.Smirnov, W.Trzaska, V.I.Zagrebaev. Mass distributions of the 136Xe + 208Pb at laboratory energies around the Coulomb barrier: a candidate reactions for production neutron-rich nuclei at N=126. Phys. Rev. C86, 044611 (2012).

  • Production of new neutron rich heavy nuclei located along the last “waiting point” of astrophysical nucleosynthesis:

    Choice of reaction ?

  • How to separate a given nucleus from all the other transfer reaction products ?

    Fusion reactions

    Transfer reactions

    Available separators are not applicable !

  • New setup for selective laser ionization and separation of multi-nucleon transfer reaction products stopped in gas

    (project GaLS, to be realized in Dubna in 2015)

  • New setup for selective laser

    ionization (FLNR, Dubna)

    two pumping lasers Nd: YAG and three DYE lasers (+ Ti: Sapphire laser)

  • Summary

    •  Elements 119 and 120 can be really synthesized in the Ti and/or Cr fusion reactions with cross sections of about 0.05 - 0.02 pb.

    •  Multi-nucleon transfer reactions can be really used for synthesis of neutron enriched long-living SH nuclei located along the beta-stability line. U-like beams are needed as well as new kind of separators.

    •  Shell effects in production of trans-target nuclei (inverse quasi-fission) should be proved experimentally at last.

    •  Transfer reactions give a unique possibility for synthesis of heavy neutron-rich nuclei with N=126 – the last “waiting point” of astrophysical nucleosynthesis.

    •  Selective laser-ionization technique (GALS setup being developed at FLNR) is a powerful method of separation of the products of transfer reactions.

    24


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