Production of new neutron rich heavy and superheavy nuclei...136Xe+208Pb: productions of heavy...

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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

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    350

       

     

     

    50 100 150 200 250100

    150

    200

    250

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    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