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MARA recoil-mass separator at JYFL – status, instrumentation and performance modelling MARA recoil-mass separator at JYFL – status, instrumentation and performance modelling

MARA recoil-mass separator at JYFL – status, instrumentation and performance modelling - PowerPoint Presentation

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MARA recoil-mass separator at JYFL – status, instrumentation and performance modelling - PPT Presentation

Jan Sarén K Auranen M Leino J Partanen J Tuunanen J Uusitalo and RituGamma research group 662013 INPC2013 Firenze Jan Sarén 2 Outline Overview of MARA M ass A nalysing ID: 815343

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Slide1

MARA recoil-mass separator at JYFL – status, instrumentation and performance modelling

Jan Sarén

, K. Auranen, M. Leino, J. Partanen, J. Tuunanen, J. Uusitalo and Ritu-Gamma -research group

Slide2

6.6.2013INPC2013, Firenze, Jan Sarén

2Outline

Overview of MARA (Mass Analysing Recoil Apparatus)

Position of MARA at JYFL accelerator laboratory

Motivation to build MARA

Optics of charged particles

MARA working principle and its optical elements

Instrumentation

Vacuum system,

Slits and apertures,

Control system

Performance modelling

Simplified modelling scheme

Example of a fusion reaction simulated

Current status and conclusions

Slide3

6.6.2013INPC2013, Firenze, Jan Sarén

3Position of MARA at JYFL accelerator laboratory

K130 Cyclotron

MARA

RITU

Slide4

6.6.2013INPC2013, Firenze, Jan Sarén

4MARA (Mass Analysing Recoil Apparatus)

RITU

gas-filled

separator

MARA

Slide5

6.6.2013INPC2013, Firenze, Jan Sarén

5Motivation to build MARA

The gas-filled separator RITU has been used extensively over almost 2 decades to study heavy elements produced in

fusion-evaporation reactions

close to the proton drip-line and transfermium nuclei.

In recent years interest has been increasingly pointed to the lighter nuclei in the

100

Sn region and below.

RITU gas-filled separator

Problems with gas-filled separator in lighter mass region:

beam is difficult to separate in symmetric reactions (impossible in inverse kinematics)

no mass resolution -> needs often a tag (alpha, beta, isomer,...)

high counting rates at a focal plane due to other evaporation channels

Slide6

6.6.2013INPC2013, Firenze, Jan Sarén

6Optics of charged particles

In a presence of an electric and magnetic field the force acting on a charged particle (mass

m

, momentum

p

, velocity

v

and kinetic energy

E

k

) is the Lorentz force:

A rigidity is the product of a field strength and a bending radius. Thus it tells how strong field is needed to bend charged particle with given radius of curvature. The electric rigidity and the magnetic rigidity of an ion describes the trajectory of the ion through the spectrometer.

Electric rigidity:

Magnetic rigidity:

The electric and magnetic field can be designed so that the energy dispersion cancels (

E

k

in both

E

and

B

) and only the mass dispersion remains (

m

only in

B

) → RECOIL MASS SPECTROMETER (FMA, EMMA, CAMEL, HIRA, MARA, ...)

Slide7

6.6.2013INPC2013, Firenze, Jan Sarén

7MARA (Mass Analysing Recoil Apparatus)

Quadrupole triplet

scalable angular magnification

Electrostatic deflector

split anode, beam dump

effect of the gap on the field homogeneity

Arriving JYFL in late summer 2013!

Magnetic dipole

inclined and rounded effective field boundaries (EFB)

surface coils

Focal plane

after 2.0 m long drift length

slit system

two position sensitive detectors → tracking

Target

beam from K130 cyclotron

Schematic view of MARA

Adjustable aperture in

x

and

y

directions

Adjustable aperture in x direction

Slide8

6.6.2013INPC2013, Firenze, Jan Sarén

8MARA (Mass Analysing Recoil Apparatus)

Realistic view of MARA

Slide9

6.6.2013INPC2013, Firenze, Jan Sarén

9The MARA working principle

Quadrupole triplet

:

point-to-parallel focus from target to the deflector

point-to-point focus from target to the focal plane

Deflector

:

separates primary beam and products

separates according to energy (per charge)

Magnetic dipole

separates masses and cancels the energy dispersion at the focal plane

Different

energies

Different

masses

Slide10

6.6.2013INPC2013, Firenze, Jan Sarén

10MARA specification

Some comparison to other RMS with physical mass separation:

MARA has asymmetric ion optical configuration with one electrostatic deflector (E): QQQEM

Fixed energy focus (due to missing second deflector)

Heavily tilted m/q focal plane

Shorter than other recoil mass separators

Typical angular acceptance of 10 msr

Typical m/q and energy acceptance

Typical resolving power

Slide11

6.6.2013INPC2013, Firenze, Jan Sarén

11MARA specification

Slide12

6.6.2013INPC2013, Firenze, Jan Sarén

12Transmission and acceptance studies of MARA

MARA has about 20% larger solid angle acceptance than RITU.

Angular acceptance is almost symmetric: ~45x55 mrad

2

while RITU acceptance is asymmetric ~25x85 mrad

2

.

MARA can collect only 2 or 3 charge states representing 30-45% of total.

The figure below shows transmission as a function of the width of the angular distribution of products. Real transmission is smaller due to energy spread and charge distribution.

MARA

and

RITU

Transmission with central energy and charge state

Slide13

6.6.2013INPC2013, Firenze, Jan Sarén

13Transmission and acceptance studies of MARA

No strong coupling between horizontal and vertical angles (

A

and

B

in the figure)

Strong coupling between energy deviation and angle in both x and y

horizontal “angle”: A = p

x

/p

z

(~rad),

vertical “angle”: B = p

y

/p

z

(~rad)

Slide14

6.6.2013INPC2013, Firenze, Jan Sarén

14Instrumentation: vacuum system

Gate valves (x3): after target, between deflector and the dipole and before focal plane chamber.

The high voltages of the deflector requires high vacuum. Since there are very limited space between Q

3

and the deflector the triplet and the deflector will form one vacuum section. The second section is formed by the dipole and part of the tube towards the focal plane. Turbo molecular pumps and a cryo pump will be used for pumping.

Slide15

6.6.2013INPC2013, Firenze, Jan Sarén

15Instrumentation: apertures and slits

m/q slits

±10 cm from the FP

Adjustable apertures (RED)

Fixed shadowing plates (MAGENTA)

Baffle structure in the dipole vacuum chamber and in the drift tube.

Slide16

6.6.2013INPC2013, Firenze, Jan Sarén

16Instrumentation: Apertures and slits

Due to tilted focal plane in MARA it is preferable to have two m/q slit systems before and after the focal plane.

Slide17

6.6.2013INPC2013, Firenze, Jan Sarén

17Control system

Key notes about MARA control system

Control system can be used to control vacuum components (pressure meters and gate valves), magnet power, deflector HV, apertures and slits

Implemented using programmable logic control (PLC) system

Automatic conditioning of the deflector HV

Uses local cyclotron control system infrastructure (Alcont)

Software and hardware interlocks

Manual operation can be switched on

Control panel of slits and apertures

MARA control system is designed and

built by J. Partanen

Slide18

6.6.2013INPC2013, Firenze, Jan Sarén

18Possible target area detectors

In principle all detector setups used or planned to be used with RITU could be used also in conjunction with MARA. These are for example:

JUROGAM Ge-detector array and SAGE electron spectrometer

UoY

96 CsI crystals (20x20mm

2

)

Can be used simultaneously with JUROGAM

Can be used to veto charged particle channels

which enhances sensitivity in pure neutron evaporation channel.

Slide19

6.6.2013INPC2013, Firenze, Jan Sarén

19First stage detector system at the focal plane

Multi Wire Proportional

Counter

, MWPC,

1 mm wire pitch in x- and y-directions

gives position, time and energy loss of a recoil

Micron BB17 DSSD

128x48 mm

2

128x48 strips

cooled to ~ -20

°

C

BB17 is planned to be replaced later with a same size DSSD but having 0.67 mm strip pitch.

MARA focalplane is designed to be highly modifiable and easy to maintain.

Vacuum chamber around DSSD can be replaced to larger one in order to fit a planar Ge-detector or scintillation detectors inside chamber.

Slide20

6.6.2013INPC2013, Firenze, Jan Sarén

20Tests with Mesytech preamplifier

Micron W1-300

50x50 mm

2

16x16 strips

cooled to -20

°

C

Mesytec MPRT16 preamplifier

16 channels

4 gain settings

differential output

NIM-tricker output

2 TFA outputs (8 channels in one)

Nutaq (Lyrtech)

VHS-ADC

16 channels

moving window

convolution

tracing of

preamp signal

possible

133

Ba conversion

e

-

(FWHM ~ 11 keV)

141

Am alphas

(FWHM ~ 19 keV)

252

Cf fission fragments

Slide21

6.6.2013INPC2013, Firenze, Jan Sarén

21

Simulation of a fusion evaporation reactions

Generating a primary beam particles

Generating a primary beam particles

Slowing beam down to reaction position (TRIM/some distribution)

Generating a primary beam particles

Evaporating light particles independently and isotropically in CM frame using the kinetic energy distribution given by PACE4 code. The weight of the product is calculated from beam intensity, total number of events, target thickness, cross section and position weight

Generating a primary beam particles

Slowing and scattering products out from the target (TRIM/some distribution)

Transferring products over drift length or optical element using GICOSY matrices

Applying slits and apertures to particles

Analysing results

Development of a multipurpose graphical interface for ion-optical calculations is going on...

The code will be able to use transfer matrices and fieldmaps and can simulate also gas-filled

systems. First version should work this autumn.

Transferring products over drift length or optical element using GICOSY matrices

Applying slits and apertures to particles

Slide22

6.6.2013INPC2013, Firenze, Jan Sarén

22Example reaction: 40Ca+40Ca->78Zr+2n

Symmetric reaction

target 300

m

g/cm

2

Beam energy 117 MeV

Cross sections from PACE4

almost 40% of products in two most abundant charge states

pure neutron channel has narrower energy and angle distribution

other channels produce around 6 orders of magnitudes more fusion products in total

Slide23

6.6.2013INPC2013, Firenze, Jan Sarén

23Example reaction: 40Ca+40Ca->78Zr+2n

Most of the counting rate can be cut by one aperture (10 cm before the FP) and one barrier (10 cm after the FP)

Products (

RED

) has been multiplied by 10

4

.

Slide24

6.6.2013INPC2013, Firenze, Jan Sarén

24Example reaction: 40Ca+40Ca->78Zr+2n

m/q spectrum calculated from realistic focal plane information (scattering and limited resolution in detectors) (bottom figure)

The biggest problem is to separate isobars and other peaks which have almost the same m/q ratio

Veto detector (UoYTube) for charged channels is more than welcome...

Slide25

6.6.2013INPC2013, Firenze, Jan Sarén

25Example reaction: 40Ca+40Ca->78Zr+2n

Spatial distribution at the implantation detector 40 cm after the optical focal plane (MWPC).

The choosed DSSD size of 128x48 mm

2

seems to be suitable.

Slide26

6.6.2013INPC2013, Firenze, Jan Sarén

26Current status and conclusions

Danfysik will deliver the electrostatic deflector late summer 2013.

Minimal focal plane detection system, the 128x48 mm

2

DSSD and a MWPC, are supposed to be ready around October 2013. All vacuum chambers will be also ready that time.

Transmission-, alignment- and other ion-optical tests with an alpha source will take place end of the year and commissioning with a primary beam can be estimated to start early spring 2014.

We hope MARA can fulfil the expectations we have set and will be a complementary recoil separator to RITU gas-filled one.