Yu. Oganessian FLNR (JINR) PAC–meeting, June 22, 2009, Dubna
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Transcript of Yu. Oganessian FLNR (JINR) PAC–meeting, June 22, 2009, Dubna
Yu. Oganessian
FLNR (JINR)
PAC–meeting, June 22, 2009, Dubna
Dubna
JINR
Experimental activities and main results of the researches at FLNR (JINR)
Theme: Synthesis of new nuclei and study of nuclear properties and heavy-ion reaction mechanism 03-05-1004-1994/2009
A&MA&M
ANLANL ORNLORNL IPNIPN INFN
Heavy ion accelerators
RIKENRIKEN
GANILGANILGSIGSI
MSUMSU
INFNINFN
Heavy Ion National Laboratories
Pioneers
LBLLBL
JINRJINR
BNLBNL CERNCERN
GSIGSI
Heavy Ion Colliders
Heavy ion physics: from the beginning to now…
RIB-FactoryRIB-FactoryRIBRIB
RIBRIB RIBRIB
RIBRIB
RIBRIB
Nuclei close to and beyond the border line
Light nuclei
neutrons
prot
ons
Heaviest nuclei
p/n - transfer & fragmentation p/n - transfer & fragmentation 2
50
50
50
82
28
28
20
208
82
/radioactive ion beams
beams of the neutron-rich projectiles: 3H(12.3y), 6He(0.8s) and 8He(0.12s)...
& target nuclei: 1,2H,3H(12.3y),3,4He
n
B
0
0
5
5
10
10
15
15
20
20 25 30 35
Z=2
Z=20
Z=2
Z=8Z=8
N=
2
N=
8
S ta b le Iso to p es
D ou b le M a g ic N uc le i
K no w n Iso to pe s
U nkn ow n Iso to p es
Pro
ton
Nu
mb
er
Neutron Num ber
N=
20
N=
28
36
N=
20
N=
28
28O
10He
n
B
0
0
5
5
10
10
15
15
20
20 25 30 35
Z=2
Z=20
Z=2
N=
28
N=
26
Z=8Z=8
N=
2
N=
8
N=
20
N=
16
S ta b le Iso to p es
D ou b le M a g ic N uc le i
K no w n Iso to pe s
U nkn ow n Iso to p es
Pro
ton
Nu
mb
er
Neutron Num ber
N=
20
N=
28
36
?
?
?
?
Shells in the light nucleiShells in the light nuclei
beams0.8s 0.1s
Radioactive ion beams
DIRECT
10m
0
R IB
400-cm cyclotron
400-cm cyclotron
low energy beam line
stable ion beams now 7Li
radioactive ion beams
DubnaRadioactive IonBeams
now 6He
Electronaccelerator
ISOL
now 8He
DIRECT
8He
d4H
6 8He + tHe and , d, p reactions
4n
n4
8He
t
t
7H
5H
5H
2n
2n
2nn
nn4
6He
tt
4He
4He
6He
d
t
4H
4H
t
tt
t
3H - target
t -
pro
jec
tile
s6
He
- p
roje
cti
les
8He
- p
roje
cti
les
2H - target H - target
d
p pt t
6He
8He
p
6He
p
tp
pt
t
t
4He
4He
2n
6He4He
4He
Neutron correlationsNeutron correlations
Strangely enough, but all the combinations:
3H, 6He, 8He (beams) + 1H, 2H, 3H (targets)
have been studied.
n
Be
B
C
B
N
F
Ne
10
12
6
6
4
4
2
20
8
8
O
He
Li
no shell effectwas observed
Unbound
strong shell effect in the “doubly-magic” nucleus
structure
discovery “di-neutron”
in halo-nucleus 6HeFLNR 2001
core
2n- halo
superheavyhydrogen
Be2p-emission
evidence of shell structure
5730y
n
Be
B
C
B
N
F
Ne
10
12
6
6
4
4
2
20
8
8
O
He
Li
discovery “di-neutron”
in halo-nucleus 6HeFLNR 2001
core
2n- halo
Be2p-emission
core
2p- halo?
Neβ+-2p emission
15O2p- halo?
0.11s
4He
PbSub-barrier fusion of halo nucleusSub-barrier fusion of halo nucleus
6He
6He
neutrontransfer
Pb
targets: Au, Pb
ECM - EB (MeV)
Cro
ss s
ectio
ns (
mb)
6He-neutrontransfer
4He-neutrontransfer6He-fusion
4He-fusion
Nuclear reactions induced by halo nucleiNuclear reactions induced by halo nuclei “of-line” gammameasurements
Experimental scheme & conditions “in-beam” gammaspectroscopy
Ю.Ц. Оганесян. «Тяжелые ионы в ЛЯР». Семинар, ЛЯР ОИЯИ, Дубна, 28 апреля 2008г.
Heaviest nuclei
Light nuclei
neutrons
prot
ons
Heaviest nuclei
Pb-based fusion Pb-based fusion
48Ca-beam& actinide
target nuclei
search for magic numbers
82
126
152
162184
108
100
114
Island of Stability
shoal
peninsula
continent
New landsNew lands
Neutron number
Pro
ton
nu
mb
er
100 110 120 130 140 150 160 170 180 190
120
110
100
90
80
70
Island of Stability
New landsNew lands Microscopic theory
cold fusionPb + HI
hot fusion Act.+ 48Ca
Reaction of Synthesis
Fusion & fission
Cold fusion
208Pb+48Ca
+58Fe
+86Kr
238U+48Ca 33MeV
26MeV
21MeV
Act.+48Ca
touchingpoint
fission from the excited state
quasifissionFLNR 1998►
FLNR 1963►
neutrons
fission isomers
spontaneous fission
β-delay fission
fission modes
FLNR 1962
FLNR 1962
γ-rays
1940►
10-30
10-32
10-34
10-36
10-38
102 104 106
1n
4n
108 110 112 114 116 118 120
Atom ic num ber
Cro
ss s
ectio
ns (
cm)2
C old fus ion
H ot fus ion
208 209 48 50 70Pb, B i + C a, Ti,... Zn
Actin ides + N e , M g,... S 22 26 34
4n-3nActin ides + C a 48
SHE
Cold & hot fusion cross sectionsCold & hot fusion cross sections
fusion
survival
90
100
110
120
1 2 3 4 5 6 7 8
120 130 140 150 160 170 180 190Neutron num ber N
Calculated Barriers Heights (M eV)
P. Moller et al., Phys. Rev., C79, 064304 (2009)
Bf (MeV)
Pro
ton
num
ber
Z
226Ra
232Th238U
248Cf
252Fm
Z=120
0.20 s
SF~90%
3n
1
2 26 m s+32-9
10.74 MeV
114
120
N =179
N =177
118
287
299
295
10.03 MeV
1.1 s+1.3-0.4
9.55 MeV 7.0 s+8.3
-2.5
110
279
112
283
244 58Pu + Fe
3
116
291
3
4n
116
290 11.65 MeV 0.89 m s+1.07
-0.31
1
112
282
10.84 MeV 7.1 ms +3.2
-1.7
10.19 MeV
0.13 s +0.04-0.02
SF
2
205 MeV
120
N =178
118
298
294
114
286
The sensitivity of experiment corresponds to σ=0.4 pb for detection of one event.
Search for Element 120Search for Element 120
0 50
Z .Z / (A +A )1 2 11/3
21/3
100
10 -6
10-2
10 -4
10-8
10 -10
100 150 200 250
no hindrance
350
26 248M g+ Cm
58 208Fe+ Pb
36 238S + Ufu
sion
pro
babi
lity
300
Fusion ProbabilityFusion Probability
48Ca+226Ra
136Xe+136Xe
132Sn+176Yb
Z=108Z=108
Decay Properties
115/287
10.59
3 ms2
113/283
10.12
0. s1
111/279
10.37
0.17 s
109/2 57
10.33
9.7 ms
107/2 17
105/267
1.2 h
109/276
9.71
0.72 s
107/272
9.02
9.8 s
113/284
10.00
0.48 s
115/288
10.46
87 ms
105/268
1.2 d
111/280
9.75
3 6. s
104/268
243Am242Pu, 245Cm
226Ra
Sg/266
0.2 s
Hs/270
10 s
9.06
σ4n≈10pb
237Np
244Pu, 248Cm249Cf
DecaychainsDecaychains
34 nuclides
48Ca +
T1/2= 320d
164
104/270
105/270
107/274
109/278
111/282
113/286
115/290
117/294
103/266
102/266
107/273
109/277
105/269
111/281
113/285
115/289
117/293
104/269
249Bk
+48Ca
2009-2010
Collaboration: FLNR (Dubna) ORNL (Oak-Ridge) LLNL (Livermore)IAR (Dmitrovgrad)Vanderbilt University (Nashville)
12.0
11 .0
10 .0
110
112
Z -even
T heory :
114
116
118
108
106
9.0
8.0
7.0260 270 280 2 09 300
A tom ic m ass num ber
Alp
ha d
eca
y en
erg
y (M
eV)
Z -even
E xp:
-6
-8
-4
-2
0
2
4
6
8
10
12
14
16
18
Z=112
112
114110
106
Sg
Rf
No
Cf
N=152
N 6=1 2
N 5=1 2N 84=1
Fm
140 145 150 155 160 165 170 175 180 185N eu tron num ber
Log
T
(s)
SF
Exp.
Th.
H sD s112114
S gR fC f-N o
Spontaneous fission half-livesSpontaneous fission half-lives
Actinides
Trans-actinides Superheavy nuclei
With Z >40% larger than that of Bi, the heaviest stable element, that is an impressive extension in nuclear survival.
Although the SHN are at the limits of Coulomb stability, shell stabilization lowers: the ground-state energy, creates a fission barrier, and thereby enables the SHN to exist.
The fundamentals of the modern theory concerning the mass limits of nuclear matter have obtained experimental verification
0
bb20 R
E
40
60
0
E (
MeV
)
5 10 15 20 25 30 35r
-40
-20
R
b
[V (r) - ] d r1 /2
E1 / Log ~T1/2 V (r )N
V C
V C+ V N 238 U
212 P o
V = V + VN C
Size of SH-nucleiSize of SH-nuclei
Geiger–Nutall relation Log Tα = C + D/√Qα
based on invariable density of nuclear matter and nuclear size:
R = r0·A1/3
perfectly works in theRegion: 212Po- 238U,where alpha-decay half-lives changed more than 1025 times!
7 8Alpha decay energy, Q (M eV)
Ha
lf-lif
e,
T (
s)
9
LogT =(a .Z+b).Q +c .Z+d-1 /2
1 0 11 1 2
106
106104
102
102Z = 100
1 0 -5
1 0 -3
1 0 -1
1 01
1 03
1 0 5
118
116
114
11 2
110
1 08
110
108106
100 -104
Cold fusion
Act.+48Ca
11 4
118
116
11 2
even
odd
available for chemical studies
Superheavy nuclei aren't exception to this rule
Chemical properties
7s
6s
5s
5d
4d4s3s2s
5fr max
rel /r
max
non-
rel
4f
Relativistic Contraction
non-
relativistic
7s
6s
5s
5d
4d4s3s2s
5f
4f
0,80
0,75
0,85
0,90
0,95
1,00
1,05
7s
6s
5s
6p5p4p
5d
4d
3p
4s3s2s
5f
0 20 40 60 80 100 120Z
1s 2p3d
4f
rm ax : principal maximum of the wave function of the outermost orbital
J.P. Desclaux, At. Data Nucl. Data Tables 12 , 311 (1973)J.P. Desclaux, At. Data . Data Tables 12 , 311 (1973)J.P. Desclaux, At. Data . Data Tables 12 , 311 (1973)
-
relativistic
SHE
112
114114
113
Atomic propertiesAtomic properties
~ Z2
Hg
PbTl
Bi
8119
121
120? ?
?
121 122 123 135
more and more inert?
H
1
Li
3
Be
4
Na
11
M g
12
K
19
Ca
20
Sc
21
104
Ti
22
V
23
Cr
24
M n
25
Fe
26
Co
27
Ni
28
Cu
29
Zn
30
1
2
3 4 6 7 8 9 10 11 12
13 14 15 16 17
18
1
2
3
4
5
6
He
B
Al Si P S
ONC F
Cl Ar
Ne
7105 106 107 108 109 110 111 112 113 115114 116 117 118
72 74 75 76 77 78 79 80 81 82 83 84 85 8655 56
87 88
37 38 39 40 42 43 44 45 46 47 48 49 50 51 52 53 54
31 32 33 34 35 36
Rf Db Sg Bh Hs M t
Rb Sr Y Zr M oNb Tc Ru Rh Pd Ag Cd In Sn Sb Tc I Xe
Cs Ba Hf WTa Re O s Ir Pt Au Hg Ti Pb Bi Po At Rn
Fr Ra
G a G e As Se Br Kr
Dar
ms-
tad
tiu
m
Ds Rg
5
73
41
?
Periodic Table of ElementsPeriodic Table of ElementsElement 112 is a noble metal – like Hg
room temperature
transport & on-line chemistry
transport & off-line chemistry
155
Neutron num ber
Hal
f-lif
e,
T
(s)
160 165 170 175
118
116114
112
112
113
113
110
110
111
111115
1801 0 -6
1 0 -4
1 0 -2
1 0 -4
1 0 0 1 s
1 m in
1 m s
102
Half-lives of nuclei with Z ≥
110
Half-lives of nuclei with Z ≥
110
Act. + 48Ca
N=162
“in
fli
gh
t”
available for chemistry & mass separation
“on
lin
e”
“gas
cat
cher
”
rotatingtarget
entrancewindow
beam
beam
RECOILS q=q eq
pumping
pumping
acceleratio
n
RF
RF+ERF
q=1+ He
H 2+B
stopping
volume
E
separatingwindow
GAS CATCHERGAS CATCHER
Guy Savardfrom Argonne National Laboratory
beam of high quality
1. Experiments on synthesis of the isotopes of element 117
in the reaction 249Bk + 48Ca. a) Gas-filled separator b) Chemistry: on-line Z=113 / off-line Z=105
up to July 2010 Cyclotron U-400
2009 / 2010
2. Studies of 2p-emission from 6Be in the charge – exchange reaction 6Li → 6Be with ACCULINA – separator
Cyclotron U-400M3. First experiments with on-line MASHA separator
Low energy beam line on Cyclotron U-400M
110 scientist
(16 doctors of science and 48 PhD)
during next 6 years will take part in the new theme
“Synthesis and properties of nuclei at the stability limits”
(2010 / 2016)