z>92 (heaviest element in nature) and upto z=100-101

47
March, 2006 SERC Course 1 Z>92 (Heaviest Element in Nature) and upto Z=100-101 achieved by n irradiation or p, and d bombardment in Cyclotron (1940-1955) (LBL) Z=102-106 by Light or Heavy-ion induced Fusion -evaporation using heavy element targets (1958-1974) Z=107-112 Heavy ion inuced fusion 208 Pb, 209 Bi targets (GSI) Identified by recoil separation technique and connecting Search for Superheavy element and Role of Fission Dynamics

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Search for Superheavy element and Role of Fission Dynamics. Z>92 (Heaviest Element in Nature) and upto Z=100-101 achieved by n irradiation or p, a, and d bombardment in Cyclotron (1940-1955) (LBL) Z=102-106 by Light or Heavy-ion induced Fusion - PowerPoint PPT Presentation

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Page 1: Z>92 (Heaviest Element in Nature) and upto Z=100-101

March, 2006 SERC Course 1

Z>92 (Heaviest Element in Nature) and upto Z=100-101 achieved by n irradiation or p, and d bombardment in Cyclotron (1940-1955) (LBL)

Z=102-106 by Light or Heavy-ion induced Fusion -evaporation using heavy element targets (1958-1974) Z=107-112 Heavy ion inuced fusion 208Pb,209Bi targets (GSI) Identified by recoil separation technique and connecting to known daughter decay after implanting into Si strip detectors. Z=112-116 48Ca+Pu,Am,Cm,Cf (JINR, Dubna) Identified by gas filled separators and Si strip setectors

Search for Superheavy element and Role of Fission Dynamics

Page 2: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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Page 3: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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Page 5: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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Cross-section data and extrapolated values for cold-fusionReactions (1n -evaporation channel)

Cross-section increases with increasing isospin

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48Ca+242Pu->287114+3n 48Ca+244Pu-

>288114+4n

48Ca+244Pu->289114+3n

E*~33 MeVE*~34-38 MeV

Page 9: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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Yury Ts. OganessianPure Appl. Chem., Vol. 76, No. 9, pp. 1715–1734, 2004.

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48Ca+244Pu

Page 12: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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The flight time of the reaction products through SHIP is 2 ms.

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∙ Cold Fusion 208Pb and 209Bi targets bombarded by the following projectiles: 48Ca, 50Ti, 54Cr,58Fe, 62Ni, 64Ni, 70Zn, 76Ge, 82Se, and 86Kr.

∎ Hot Fusion 48Ca projectiles bombarded targets of 238U, 244Pu, 243Am, 245Cm, 248Cm, and 249Cf,

Page 17: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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BLDf gradually disappears

Spherical

Deformed

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Fission barrier calculations of Smolanzuk et al.

106Sg has highest barrier with half life of 3 hrs

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Extra push energies Swiatecki

For Z1Z2>1000 to 1650 depending on the value of the charge asymmetry, Zp/ZT.

Page 21: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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Onset of fusion limitationDue to Extra push energies

No hindrance

Effective fissility : weighted mean of mono-nuclear and binaryWith weight for binary taken as 1/3

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Injection direction

Fusion area inside Saddle point

Difference in energyBetween touchingPoint and saddle pointSmall due to shell structureOf Ca and Pb

All trajectories reaches fusion

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Quasi-fission isdominant

Extra pocket in massSymmetric region Deep

Quasi-fission

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The curve V (Z,L = 0) (for the value of R corresponding to

the pocket) has a few local minima, which reflect the shell

structure in the interacting nuclei.

Evgeni A. CherepanovBrazilian Journal of Physics, vol. 34, no. 3A, September, 2004

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48Ca+208PbEX=50 MeV

Aritomo and OhtaPre-print

Nuclear Physics A 744 (2004) 3–14

Mass asymm fluctuatesaround 0.5 and then relaxes quickly andTrajectory move to main pocket

Page 27: Z>92 (Heaviest Element in Nature) and upto Z=100-101

March, 2006 SERC Course 2748Ca+244PuEx=50 MeV

Critical stage

Turning stage

For FF massAsymmetrieslarge

For QF neck developsand speeds up fissionkeeping mass asymm.

For deep QF mass asymmRelaxed in sub-pocketAt TS

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The smaller formation probability due to inhibition of fusion by competing mechanism:DIC,QF,FF,PEF Asymmetric channels: higher E* and unfavourable for survival

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Transition fromFF to QF

QF

Mass distribution forFF is asymmetric in shapeWith peak around 132

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Measurements at LNL,Legnaro (Italy)Measurements at LNL,Legnaro (Italy)

470-630 MeV 80Se + 208Pb

372 MeV 56Fe+232Th

288116

Measurement of fragment mass and kinetic energy and neutron correlations

80Se + 232Th 312124470-630 MeV

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Schematics of the setup for Se+Pb,Th experiment

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80Se+232Th 470 MeV80Se+208Pb 470 MeV

DIC dominates but significant events around symmetry

Page 34: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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Mass (amu)

50 100 150 200 25010-1

100

101

102

103470 MeV510 MeV550 MeV630 MeV

Z = 50 N = 82

Mass (amu)

50 100 150 200 250101

102

103

Z = 50 N = 82

d/d

M (a

rb. u

nits

)

80Se+232Th 470 MeV80Se+208Pb 470 MeV

Se+Pb more asymmetric compared to Se+Th

QF is expected to be more for Se+Th

Page 35: Z>92 (Heaviest Element in Nature) and upto Z=100-101

March, 2006 SERC Course 35Ecm-VB (MeV)

0 20 40 60 80 100 120 140 160 180 200

cros

s se

ctio

nsX

Ecm

(arb

. un

its)

0

2000

4000

6000

8000

80Se+208Pb (gated region)80Se+232Th (gated region)Fit to Se+Pb dataFit to Se+Th data

higher extra-push energyin the case of 80Se+232Th

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80Se+208Pb 288116

ExCN (MeV)

0 50 100 150 200 250

tot

0

10

20

30

40

50

80Se+232Th 312124

ExCN (MeV)

0 50 100 150 200 250

tot

0

10

20

30

40

50

ν sf tot =10±2 for Se+Pb

12±1 for Fe+Th

=17±2 for Se+Th

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on average of about 0.6 neutron per unit Z

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an increase of about 0.54 neutron per unit Z

excitation energy gained by the system in its transition from the saddle to the scission point (the term ΔEx by Hilscher) that is known to show a strong mass and Z dependence.

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JINR,Dubna

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41 detectors of DEMON at DubnaT. Materna et al. Nuclear Physics A734 (2004) 184-l 87

The pre-scission neutron multiplicity distribution simulated

using backtracing procedure show two components for Ca+Pu

Whereas for Ca+Pb only one component is seen

FF

QF

A/2±30

208±20

Page 41: Z>92 (Heaviest Element in Nature) and upto Z=100-101

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??

Connectecd withknown species

Self-consistent

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Change fromHot fusion toCold fusionFor higher N-Z

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Survival probability Depends on fissionfission delaydelayAnd speed of coolingMainly by neutron neutron evaporationevaporation

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Expected intensities s-1 for neutron-rich radioactive beams

SPIRAL 24Ne 7 x 107

HI based 44Ar 5 x 107

PIAFE 78Zn 108

84Ge 2 x 108

94Kr 2 x 109

Region beyond Z= 114 needs beam intensities in excess of 1014 s-1.

Reactor based

With MAFF and spallation facility with 100μA proton of 1GeVIntensities may go up by 3 to 4 orders of magnitude

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