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Measurements of Measurements of 260 260- 262 262 Rf produced in Rf produced in 22 22 Ne + Ne + 244 244 Pu fusion reaction at Pu fusion reaction at TASCA TASCA Alexander Gorshkov, 12 October 2009 Alexander Gorshkov, 12 October 2009 SEVENTH WORKSHOP ON THE SEVENTH WORKSHOP ON THE CHEMISTRY OF THE HEAVIEST ELEMENTS CHEMISTRY OF THE HEAVIEST ELEMENTS

22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

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Page 1: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

Measurements ofMeasurements of 260260--262262Rf produced inRf produced in2222Ne +Ne + 244244Pu fusion reaction atPu fusion reaction at

TASCATASCA

Alexander Gorshkov, 12 October 2009Alexander Gorshkov, 12 October 2009SEVENTH WORKSHOP ON THESEVENTH WORKSHOP ON THE CHEMISTRY OF THE HEAVIEST ELEMENTSCHEMISTRY OF THE HEAVIEST ELEMENTS

Page 2: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

22

Commissioning phase was successfully accomplishedCommissioning phase was successfully accomplished:

•• wide knowledge about separator settingswide knowledge about separator settings

•• 2 types of focal plane detectors2 types of focal plane detectors

•• 2 different chemical interfaces2 different chemical interfaces ––Recoil Transfer Chambers (Recoil Transfer Chambers (RTCsRTCs))for HTM and SIMfor HTM and SIM

•• final experiment of the commissioning phasefinal experiment of the commissioning phasewith first transactinide element Rfwith first transactinide element Rf

261Rf2.7 s 68 s

8.51SF 8.28

Page 3: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

33

After 2002After 2002BeforeBefore 20022002

265Sg7 s 15 s

8.94;8.84;8.76 8.69

265Sg7 s

8.94;8.84;8.76; 8.69

261Rf68 s 2.7 s

8.518.28 SF

261Rf78 s

8.28

269Hs9.7 s

8.95; 9.129.23

270Hs~4 s

9.16

266Sg21 s

8.52; 8.77

262Rf1.2, 2.1 s

or47 ms

SF

248Cm(22Ne,xn)270-xSgLazarev et al. (1994)

Lazarev et al. (1994), Lane et al. (1996)

Somerville et al. (1985)S. Hofmann et al., New results on elements

111 and 112. (2002)

J. Dvorak et al., (2006)

MotivationMotivation

270Hs23* s

8.888.67 – 8.92

266Sg

359 msSF

262Rf

?SF

?

J. Dvorak et al., (2008)

* Calculated value

Page 4: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

44

Experimental approachesExperimental approaches

244244Pu(Pu(2222Ne,6n)Ne,6n)260260RfRf andand 244244Pu(Pu(2222Ne,4n)Ne,4n)262262RfRf

SShorthort--lived SF decaying Rf isotopes could belived SF decaying Rf isotopes could bedetected in a Focal Plain Detector.detected in a Focal Plain Detector.

244244Pu(Pu(2222Ne,5n)Ne,5n)261261RfRfTo reduce background from Target Like FragmentsTo reduce background from Target Like FragmentsHTM RTC + ROMA combination was used.HTM RTC + ROMA combination was used.

Page 5: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

55

244244Pu target wheelPu target wheel•• A rotating target wheel with three bananaA rotating target wheel with three banana--shaped segments was holding threeshaped segments was holding three

244244Pu targets (thickness:Pu targets (thickness:339900 µµgg/cm/cm22, 481, 481 µµgg/cm/cm22 andand 505022 µµgg//cmcm22).).•• The target material was deposited on 2.2The target material was deposited on 2.2-- m thick Ti backing foils.m thick Ti backing foils.

•• The target wheel rotated synchronously with the beamThe target wheel rotated synchronously with the beam macropulsemacropulse structure.structure.•• The beam energy in the center of the target was 109, 116, andThe beam energy in the center of the target was 109, 116, and 125125 MeVMeV..

Page 6: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

66

Target station

Quadrupoles:Q1 – horisontal,

Q2 - vertical

Q1 Q2

Differentialpumping

RTC +ROMA

Dipole, 300

D

TransActinideTransActinide Separator and Chemistry Apparatus,Separator and Chemistry Apparatus,High Transmission Mode; July 2008High Transmission Mode; July 2008Pulsed

22Ne5+

beam(5 ms on/15 ms off)

with energies5.18,5.51and5.92

MeV/nucleonFocalplane

Page 7: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

77

Detection of shortDetection of short--livedlived 2222Ne(Ne(244244Pu,4n)Pu,4n)262262Rf andRf and2222Ne(Ne(244244Pu,6n)Pu,6n)260260Rf in the focal planeRf in the focal plane

• No veto detectors in TASCA were installed during the commissioning phase.• A relative high counting rate from Target Like Fragments originated a high

background, which negatively affected search limits for time- and position-correlatedEVR-SF decay chains, especially during beam pulses.

• The recoil energy of separated complete fusion products was below 8 MeV, whichmade distinguishing between an EVR and an alpha within a beam pulse also notpossible.

• To reduce background from target-like fragments TASCA was filled with 1.5 mbarof a He:H2 = 2:1 gas mixture.

BeamBeam

Focal Plane Detector(FPD)(FPD)

Page 8: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

88

•• (80 x 35) mm(80 x 35) mm22 1616--stripstrip Position Sensitive silicon Detector (PSD)(PSD) made by CANBERRA•• (58 x 58) mm(58 x 58) mm22 4848--stripstrip Double-Sided Silicon Strip Detector (DSSSD)(DSSSD) made in

Zelenograd, Russia.PSDPSD DSSSDDSSSD

Two types of the focal plane detectorTwo types of the focal plane detector

Thickness = 300 m.Bias = 40 V.

-35 oC

Thickness = 300 m.Bias = 50 V.

Room temperature.

Energy resolution FWHM for 5.8 MeV alpha particles 24 keV for the both detectors

80 mm

16 strips

35 mm

Page 9: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

99

•• Beam energy = 125Beam energy = 125 MeVMeV in thein the centercenter of the target.of the target.•• Nominal vertical position resolution isNominal vertical position resolution is 0.2 mm.0.2 mm.•• During search for position correlated chain members limits areDuring search for position correlated chain members limits are 1 mm1 mm

pixel size area about (5 x 2) mmpixel size area about (5 x 2) mm22..

Detection of shortDetection of short--livedlived 2222Ne(Ne(244244Pu,6n)Pu,6n)260260RfRfin thein the Position Sensitive DetectorPosition Sensitive Detector

The relatively large pixel size of the PSDThe relatively large pixel size of the PSDdidndidn’’t allow detection of EVRt allow detection of EVR--SF decaySF decaychains with a correlation time longer thanchains with a correlation time longer than250 ms under the experimental conditions.250 ms under the experimental conditions.

The detection efficiencies are:

• for an EVR near 100%• for an alpha particle 50-55%• for a SF fragment 100%.

Page 10: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1010

1E-3 0,01 0,1

1

2

3

4

5 Ec.o.t.

=125 MeV+7.3 -4.3

Cou

nts

T(EVR - SF), s

260Rf (T1/2=21 ms)

Time distribution of observed EVRTime distribution of observed EVR--SF correlations fromSF correlations from 260260RfRf

• T½ is in good agreement with the half-life published by Somerville et all.,(1985).

• 15 time and position correlated EVR-SF events• Time window of t 250 ms and a position window 1 mm.• EVR-SF events with correlation time > 250 ms in the PSD could not be found,

because of high probability to observe a random correlation.

Page 11: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1111

• Beam energy was 109 MeV in the center of the target.• Each two of 16 first and last strips on each side are connected to one channel.• 3 different pixel sizes: (1.2 x 1.2) mm2, (1.2 x 2.4) mm2 , (2.4 x 2.4) mm2 .

Detection of shortDetection of short--livedlived 2222Ne(Ne(244244Pu,4n)Pu,4n)262262RfRfin thein the DoubleDouble--Sided Silicon Stripe DetectorSided Silicon Stripe Detector

The detection efficiencies are:

• for an EVR near 100%• for an alpha particle 50-55%• for a SF fragment 100%.

However, the largest pixel size in theDSSSD was only a half of the pixelsize of the PSD.

Page 12: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1212

Time distribution of EVRTime distribution of EVR--SF correlations fromSF correlations from 262262RfRf

••15 EVR15 EVR--SF correlations withSF correlations with tt 2 ms and EVR energies of 7.52 ms and EVR energies of 7.5 5.05.0 MeVMeV..They were attributed to the decay of Am fission isomers:They were attributed to the decay of Am fission isomers:244m244mAm:Am: TT1/21/2 = 0.9 ms (Nuclear Data Sheets 99, 197 (2003)= 0.9 ms (Nuclear Data Sheets 99, 197 (2003)246m246mAm:Am: TT1/21/2 = 73= 73 s (Nuclear Data Sheets 84, 901 (1998).s (Nuclear Data Sheets 84, 901 (1998).

1E-3 0,01 0,1 1 10 100 1000 100000

1

2

3

4

5

6

7 Ec.o.t.= 109 MeV

246mAm3 events

244mAm12 events

Cou

nts

Time, ms

262Rf10 events

•• 10 correlated EVR10 correlated EVR--SF events ofSF events of 262262Rf (EVRRf (EVR –– 11÷÷3.53.5 MeVMeV, SF > 90, SF > 90 MeVMeV))TT½½ ((262262Rf) = ms,Rf) = ms, in contradiction with values from Lane et al.in contradiction with values from Lane et al.(1996) and Somerville et al. (1985)(1996) and Somerville et al. (1985)

10050190

Page 13: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1313

10050190

Am SF isomersAm SF isomers

262262RfRf

Observed EVRObserved EVR--SF events and random event analysisSF events and random event analysis

Number of random events in DSSSD withinNumber of random events in DSSSD within t of 1 st of 1 s

Page 14: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1414

Preseparation and detection of long-lived 261Rf in ROMADetection of longDetection of long--livedlived 261261RfRf

TASCA filling gas - pure He (pressure 0.4 mbar)

Page 15: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1515

OvenHe gas

Pressure ~1.2 barFlow rate: 3.45 l/min

• Mylar window - 1.2 µm thick (140 x 40) mm2

• 17 mm-deep RTC flushed with He jet

KCl aerosol producedby sublimation of KCl at 650 °C.

4 m PTFE capillary(inner diameter: 2 mm)

Detection of longDetection of long--livedlived 261261Rf in ROMARf in ROMA

Page 16: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1616

• The particles were deposited on 40- g/cm2 thick polyethylene foils.• ROMA wheel diameter = 85 cm.• The wheel periodically stepped and transported the sample from collection position to eight

counting positions equipped with (20 x 10)-mm2 large PIN diodes.

Rotating wheel OnRotating wheel On--lineline MultidetectorMultidetector Analyzer (ROMA)Analyzer (ROMA)

• For measurements of 261aRf, a stepping time was 35 s.• For 261bRf experiments were performed with a stepping time 1.5 s.

Page 17: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1717

261261Rf was produced in the 5n channel atRf was produced in the 5n channel at EEc.o.tc.o.t =116=116 MeVMeV,, ttstepstep = 35 s.= 35 s.149 single149 single --particles (Eparticles (E = 7.8= 7.8 –– 8.58.5 MeVMeV) from) from 261a261aRf andRf and 257257No were registered;No were registered;among these 28among these 28 -- correlationscorrelations.

2222Ne(Ne(244244Pu,5n)Pu,5n)261a261aRf in ROMARf in ROMA

1 10 1000

5

10

15

20

25

30 Ec.o.t.

=116 MeVC

ount

s

Measurement time, s

261aRf + 257No

-6 T1/2 = 90 s+8

Time analysis of single alphaTime analysis of single alpha--particles and correlations confirmed, that detectedparticles and correlations confirmed, that detectedevents originated fromevents originated from 261a261aRf.Rf.

Page 18: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1818

0,1 1 100,0

0,5

1,0

1,5

2,0

2,5

3,0

3,5

4,0

4,5C

ount

s

Measurement time, s

Ec.o.t.=116 MeV

-0,5261bRf (T1/2 = 2,2 s)+1,0

At the same beam energy 11 SF-events were registered and are attributed to261bRf. The time analysis revealed T1/2(261bRf) of s. ttstepstep = 1.5 s.= 1.5 s.

2222Ne(Ne(244244Pu,5n)Pu,5n)261b261bRf in ROMARf in ROMA

The SF activity assigned in Lane et al.(1996) to 262Rf most likely originatedfrom then unknown 261bRf.

261Rf68 s 2.7 s

8.518.28 SF

015022 ...

Page 19: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

1919

X coordinateX coordinate FractionFractioncoveredcovered

±±8 cm8 cm 99%99%

±±7 cm7 cm 90%90%±±6 cm6 cm 80%80%

±±5 cm5 cm 70%70%

±±4 cm4 cm 60%60%±±3 cm3 cm 53%53%

±±2 cm2 cm 33%33%±±1 cm1 cm 17%17%

Y coordinateY coordinate FractionFractioncoveredcovered

±±4 cm4 cm 99%99%

±±3 cm3 cm 97%97%±±2 cm2 cm 90%90%

±±1 cm1 cm 64%64%

2222Ne(ENe(Elablab = 115= 115 MevMev CofTCofT) +) + 244244Pu (400Pu (400 mmg/cmg/cm22)) -->> 261261Rf + 5nRf + 5n

Pressure = 0.3 mbar

TransmissionTransmission to theFocal Plane = 12.0%12.0%

* Based on TRANSPORT ion* Based on TRANSPORT ion--optic calculations (from A.optic calculations (from A. SemchenkovSemchenkov))

81% inside81% inside14 x 4 cm14 x 4 cm22 RTC windowRTC window

53% inside53% inside8 x 4 cm8 x 4 cm22 PSDPSD

MonteMonte--CarloCarlo simulationsimulation

Page 20: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2020

From measured 261aRf event number, cross section of 4.4 nb from Lazarevet al. (2000), = 80 %, = 60 % and ROMA detection efficiencytransmission of Rf through TASCAtransmission of Rf through TASCA to the Focal Plane is 10.510.5 %%..

RTC jet

detectiondecayjetRTCproduced

measuredTASCA N

NE

TASCA transmission forTASCA transmission for 2222Ne(Ne(244244Pu,xn)Pu,xn)266266--xxRfRf

81% inside81% inside140 x 40 mm140 x 40 mm22

RTC windowRTC window

53% inside53% inside80 x 35 mm80 x 35 mm22

PSDPSD

Considering MonteConsidering Monte--Carlo calculations, transmissionCarlo calculations, transmissionof Rf through TASCA:of Rf through TASCA:

•• to the RTC window 140 x 40 mmto the RTC window 140 x 40 mm22 is 8is 8..55 %.%.•• to the PSD area 80 x 35 mmto the PSD area 80 x 35 mm22 is 5is 5..33 %.%.•• to the DSSSD area 58 x 58 mmto the DSSSD area 58 x 58 mm22 is 5is 5..11 %.%.

* Based on TRANSPORT ion* Based on TRANSPORT ion--optic calculations (from A.optic calculations (from A. SemchenkovSemchenkov))

Page 21: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2121

503051 ...

4n channel: 0.75 nb @ 109 MeV5n channel: 2.5 nb @ 116 MeV6n channel: 0.55 nb @ 125 MeVCross section forCross section for 2222Ne(Ne(244244Pu,6n)Pu,6n)260260RfRf == nbnbCross section forCross section for 2222Ne(Ne(244244Pu,4n)Pu,4n)262262RfRf == pbpb..

100 105 110 115 120 125 130 135 140

0,1

1

1035 40 45 50 55 60 65 70

cros

s se

ctio

n (n

b)

ELab (MeV)

260Rf (6n)261a,bRf (5n)262Rf (4n)

E*(AME2003), MeV

Cross section forCross section for 2222Ne(Ne(244244Pu,5n)Pu,5n)261b261bRfRf == nbnb,,published cross section forpublished cross section for 2222Ne(Ne(244244Pu,5n)Pu,5n)261a261aRfRf = 4.4= 4.4 nbnb

260130500

804081 .

..

HIVAP prediction forHIVAP prediction for 2222Ne(Ne(244244Pu,xn)Pu,xn)266266--xxRfRf

Page 22: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2222

ConclusionConclusion

•• TT ½½ forfor 260260Rf = s isRf = s is in good agreement with the halfin good agreement with the half--lifelifepublished bypublished by Somerville et all.,(1985).Somerville et all.,(1985).

•• Cross section forCross section for 2222Ne(Ne(244244Pu,6n)Pu,6n)260260RfRf == nbnb.. New!New!

•• TT1/21/2 forfor 261b261bRf = s isRf = s is in good agreement with the halfin good agreement with the half--lifelifepublished bypublished by Dvorak et all.,(2008).Dvorak et all.,(2008).

•• Cross section forCross section for 2222Ne(Ne(244244Pu,5n)Pu,5n)261b261bRfRf == nbnb.. New!New!•• The production ratio ofThe production ratio of 261a261aRfRf :: 261b261bRfRf == 2.5 : 12.5 : 1..

•• Transmission of Rf through TASCA to the Focal Plane =Transmission of Rf through TASCA to the Focal Plane = 10.510.5 %.%.

•• TT½½ forfor 262262Rf = ms,Rf = ms, in contradiction with values published byin contradiction with values published byLane et al. (1996) and Somerville et al. (1985).Lane et al. (1996) and Somerville et al. (1985). New!New!

•• Cross section forCross section for 2222Ne(Ne(244244Pu,4n)Pu,4n)262262RfRf == pbpb New!New!

015022 ...

373421 ..

10050190

804081 .

..

503051 ...

260130500

Page 23: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2323

AcknowledgmentsAcknowledgmentsA. Yakushev, R.A. Yakushev, R. GraegerGraeger,,A.A. TTüürlerrler,,

Ch. E.Ch. E. DDüüllmannllmann, M., M. SchSchäädeldel,,J.J. KhuyagbaatarKhuyagbaatar, D. Ackermann,, D. Ackermann,W.W. BrBrüüchlechle, M. Block, E., M. Block, E. JJäägerger, J., J. KrierKrier,,B.B. SchaustenSchausten, E., E. SchimpfSchimpf, D. Rudolph,, D. Rudolph,

K.K. EberhardtEberhardt, J. Even,, J. Even,J.J. BallofBallof, J.V., J.V. KratzKratz,,D.D. LiebeLiebe, P., P. ThThöörlerle,,

I.I. DragojeviDragojevi , J.M. Gates,, J.M. Gates,H.H. NitscheNitsche, L., L. StavsetraStavsetra,,

J.P.J.P. OmtvedtOmtvedt,, SabelnikovSabelnikov,,F.F. SamadaniSamadani,,

J.J. UusitaloUusitalo,,

A. Toyoshima,A. Toyoshima,

Page 24: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2424

Thank you for your attention!Thank you for your attention!

Page 25: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2525

Current working hypothesis of the decay patterns observed in theCurrent working hypothesis of the decay patterns observed in the chainchain269269HsHs 265265SgSg 261261RfRf ((257257NoNo ))

* Ch. E. Düllmann, A. Türler. Phys. Rev. C 77, 064320 (2008).

Page 26: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

2626

• Predicted values of B· of EVRs in the range of 1.90 T·m - 1.98 T·m.• Predicted magnetic rigidities for elastically scattered 244Pu nuclei recoiling

from the target with twice the momentum of the beam are about 1.86 T·m.

Charge states of slow heavy EVRs in H2 are much lower than in He -> high B· values.DGFRS can reach B· more than 3 T·m. TASCA - 2.4 T·m only, which is not enoughto bend Rf EVRs from the reaction 22Ne+244Pu. To reduce background from target-likefragments TASCA was filled with 1.5 mbar of a He:H2 = 2:1 gas mixture.As will be described in already prepared article of J. Khuyagbaatar the use of suchgas mixtures indeed combines the advantages of both gas components.

TASCA filling gasTASCA filling gas

HH22

Page 27: 22Ne + Ne + 244Pu fusion reaction at Pu fusion reaction at

27271,80 1,85 1,90 1,95 2,00 2,05 2,10

0,0

0,2

0,4

0,6

0,8

1,0

1,2

1,4

1,6

1,8

2,0

Eve

nts

/ Int

egra

l

B , T m

Used settings: D=Used settings: D= 555555 A (1.99 T m), QA (1.99 T m), Q11 = Q= Q22 == 508508 AAProbable best settings: D=Probable best settings: D= 553355 A (1.94 T m), QA (1.94 T m), Q11 = Q= Q22 = 490 A= 490 A

Measured yield dependence from magnetic rigidityMeasured yield dependence from magnetic rigidity