Study of negative ion surface production in caesium-free H 2 plasma PhD student: Kostiantyn Achkasov...

Post on 26-Dec-2015

217 views 1 download

Tags:

Transcript of Study of negative ion surface production in caesium-free H 2 plasma PhD student: Kostiantyn Achkasov...

Study of negative ion surface production in caesium-free H2 plasma

PhD student:• Kostiantyn Achkasov

Tutors:• Gilles Cartry and Alain Simonin

3rd FUSENET PhD Eventin Fusion Science and Engineering 

University of York, 23rd - 26th of July 2013

2

Fundamentals

3rd FUSENET PhD Event in York: 26th of June 2013

Controlled thermonuclear fusion is one of the most promising future energy sources

3

Fundamentals

Controlled thermonuclear fusion is one of the most promising future energy sources

3rd FUSENET PhD Event in York: 26th of June 2013

4

Fundamentals

ITER is the world's largest experimental tokamak nuclear fusion reactor being built at the south of France

Controlled thermonuclear fusion is one of the most promising future energy sources

3rd FUSENET PhD Event in York: 26th of June 2013

5

Fundamentals

ITER is the world's largest experimental tokamak nuclear fusion reactor being built at the south of France

Required electron temperature: 10 – 20 keV (~108 °C)

only 1 keV can be achieved with Ohmic heating

Controlled thermonuclear fusion is one of the most promising future energy sources

3rd FUSENET PhD Event in York: 26th of June 2013

6

Fundamentals

ITER is the world's largest experimental tokamak nuclear fusion reactor being built at the south of France

Required electron temperature: 10 – 20 keV (~108 °C)

only 1 keV can be achieved with Ohmic heating

Controlled thermonuclear fusion is one of the most promising future energy sources

one needs additional heating methods!3rd FUSENET PhD Event in York: 26th of June 2013

7

NBI for ITERNBI - neutral beam injection

3rd FUSENET PhD Event in York: 26th of June 2013

5.3 m

4.7 m

15 m

8

NBI for ITER

17 MW &1 MeV of neutrals

Total weight > 900 tons

Calorimeter

Bushing

RID Neutralizer Ion source and accelerator

NBI - neutral beam injection

3rd FUSENET PhD Event in York: 26th of June 2013

9

Why to use i- ?

neutrals of 1 MeV are needed to heat the ITER plasma core and ignite the fusion reactions

3rd FUSENET PhD Event in York: 26th of June 2013

10

neutrals of 1 MeV are needed to heat the ITER plasma core and ignite the fusion reactions

At such an energy:D+ → 0%D- → 56% of neutralisation efficiency

Ion neutralization

Why to use i- ?

0

10

20

30

40

50

60

70

80

90

100

0 200 400 600 800 1000

Energy of D+ or D- (keV)

Fra

ctio

n (

%)

D-

D+

3rd FUSENET PhD Event in York: 26th of June 2013

11

Ion neutralization

Necessary D- current: ~ 50 A (250 A∙m-2)

Why to use i- ?

0

10

20

30

40

50

60

70

80

90

100

0 200 400 600 800 1000

Energy of D+ or D- (keV)

Fra

ctio

n (

%)

D-

D+

neutrals of 1 MeV are needed to heat the ITER plasma core and ignite the fusion reactions

At such an energy:D+ → 0%D- → 56% of neutralisation efficiency

3rd FUSENET PhD Event in York: 26th of June 2013

0

10

20

30

40

50

60

70

80

90

100

0 200 400 600 800 1000

Energy of D+ or D- (keV)

Fra

ctio

n (

%)

D-

D+

12

new large i- source has to be developed!

Ion neutralization

Necessary D- current: ~ 50 A (250 A∙m-2)

Why to use i- ?

neutrals of 1 MeV are needed to heat the ITER plasma core and ignite the fusion reactions

At such an energy:D+ → 0%D- → 56% of neutralisation efficiency

3rd FUSENET PhD Event in York: 26th of June 2013

Present i– source

13

i- source conceptRF Driver

3rd FUSENET PhD Event in York: 26th of June 2013

• i- surface production with Cs deposition

• has many drawbacks like diffusion of Cs inside the accelerator

• is presently the only way to meet ITER requirements

14

RF Driver

Present i– sourcei- source concept

3rd FUSENET PhD Event in York: 26th of June 2013

Alternative solutions to the use of Cswould be highly valuable for the future fusion i- sources!

15

Present i– source

RF Driver• i- surface production with Cs deposition

• has many drawbacks like diffusion of Cs inside the accelerator

• is presently the only way to meet ITER requirements

i- source concept

3rd FUSENET PhD Event in York: 26th of June 2013

16

Helicon reactor PHISIS

• H2 and D2 plasma

• P = 20 – 900 W• no magnetic field• preactor = 0.2 – 2 Pa

• capacitively coupled plasma mode

Experimental set-up

Graphite samplePump

Pyrex tube

Antenna

Coils

Mass Spectrometer Hiden EQP 300

3rd FUSENET PhD Event in York: 26th of June 2013

17

Experimental set-up

Helicon reactor PHISIS

• H2 and D2 plasma

• P = 20 – 900 W• no magnetic field• preactor = 0.2 – 2 Pa

• capacitively coupled plasma mode

3rd FUSENET PhD Event in York: 26th of June 2013

18

Langmuir probe

Sample

Experimental set-up

Mass Spectrometer

3rd FUSENET PhD Event in York: 26th of June 2013

19

Measurement principle

VMS Vs Vp

Mass Spectrometer Plasma Sample

E

0

3rd FUSENET PhD Event in York: 26th of June 2013

VMS Vs Vp

Mass Spectrometer Plasma Sample

20

E

0 10 20 30 40 50 60 70 80

0.01

0.1

1 0.2 Pa H2,100 W,V

p=21V

Vs=-130V D=37mm,

H2

+90%, HOPG, WS

H- c

ou

nts

/s

Energy (eV)

0

Negative ion distribution function (NIDF)

Measurement principle

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)1 Pa H2,60 W, V

p=7V,V

s=-95V

21

Modeling of the NIDF

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)

f(E) SRIM1 Pa H

2,60 W, V

p=7V,V

s=-95V

22

Modeling of the NIDF

SRIM: the stopping and range of ions in matter

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)

f(E) SRIM1 Pa H

2,60 W, V

p=7V,V

s=-95V

23

Modeling of the NIDF

×× Plasma transmissionNIDF of i- emitted by

the surface

Surface

Mass spectrometer transmission

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)

f(E) SRIM1 Pa H

2,60 W, V

p=7V,V

s=-95V

24

Modeling of the NIDF

SRIM

×× Plasma transmissionNIDF of i- emitted by

the surface

Surface

Mass spectrometer transmission

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)

f(E) SRIM1 Pa H

2,60 W, V

p=7V,V

s=-95V

25

Modeling of the NIDF

SRIM SIMION

×× Plasma transmissionNIDF of i- emitted by

the surface

Surface

Mass spectrometer transmission

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)

f(E) SRIM f ''(E) modeling

1 Pa H2,60 W, V

p=7V,V

s=-95V

26

• good agreement between F’’(E) and Fmeasured(E)

Modeling of the NIDF

3rd FUSENET PhD Event in York: 26th of June 2013

0 10 20 300.01

0.1

1

Energy (eV)

no

rma

lis

ed

in

ten

sit

y (

arb

.u)

Fmeasured

(E)

f(E) SRIM f ''(E) modeling

1 Pa H2,60 W, V

p=7V,V

s=-95V

27

• good agreement between F’’(E) and Fmeasured(E)

• SRIM calculation: C-H layer with 30% of hydrogen on the surface

Modeling of the NIDF

3rd FUSENET PhD Event in York: 26th of June 2013

NIDF studyof different carbon materials

28

highly oriented pyrolitic graphite (HOPG)

-40 -20 0 20 40 60 80

10

100

1000

10000

100000

35 °C 200 °C 400 °C 782 °C

Vs= - 130 V

= 0°

Inte

nsity

(ar

b. u

nits

)

Energy (eV)

HOPG 50 eV

3rd FUSENET PhD Event in York: 26th of June 2013

29

-10 0 10 20 30 40 50 60 70

0.01

0.1

1

35 °C

Vs= - 130 V

= 0°

Inte

nsity

(ar

b. u

nits

)

Energy (eV)

HOPG 50 eV

NIDF studyof different carbon materials

highly oriented pyrolitic graphite (HOPG)

3rd FUSENET PhD Event in York: 26th of June 2013

30

-10 0 10 20 30 40 50 60 70

0.01

0.1

1

35 °C

Vs= - 130 V

= 0°

Inte

nsity

(ar

b. u

nits

)

Energy (eV)

HOPG 50 eV

F”(E,θ)30% H

NIDF studyof different carbon materials

highly oriented pyrolitic graphite (HOPG)

3rd FUSENET PhD Event in York: 26th of June 2013

31

0

0.01

0.1

1

35 °C 200 °C

Vs= - 130 V

= 0°

Inte

nsity

(ar

b. u

nits

)

Energy (eV)

HOPG 50 eV

F”(E,θ)30% H

NIDF studyof different carbon materials

highly oriented pyrolitic graphite (HOPG)

3rd FUSENET PhD Event in York: 26th of June 2013

32

0

0.01

0.1

1

35 °C 200 °C

Vs= - 130 V

= 0°

Inte

nsity

(ar

b. u

nits

)

Energy (eV)

HOPG 50 eV

F”(E,θ)20% H

F”(E,θ)30% H

NIDF studyof different carbon materials

highly oriented pyrolitic graphite (HOPG)

3rd FUSENET PhD Event in York: 26th of June 2013

33

H coverageon HOPG decreases with temperature

0

0.01

0.1

1

35 °C 200 °C

Vs= - 130 V

= 0°

Inte

nsity

(ar

b. u

nits

)

Energy (eV)

HOPG 50 eV

F”(E,θ)20% H

F”(E,θ)30% H

NIDF studyof different carbon materials

highly oriented pyrolitic graphite (HOPG)

3rd FUSENET PhD Event in York: 26th of June 2013

34

yield comparison

0 100 200 300 400 500 600 700 800

10000

100000

1000000

Vs= - 130 V

= 0°

HOPG

Tot

al y

ield

(ar

b. u

nits

)

T,°C

NIDF studyof different carbon materials

3rd FUSENET PhD Event in York: 26th of June 2013

35

yield comparison

0 100 200 300 400 500 600 700 800

10000

100000

1000000

Vs= - 130 V

= 0°

HOPG

Tot

al y

ield

(ar

b. u

nits

)

T,°C

NIDF studyof different carbon materials

-10 0 10 20 30 40 50

HOPG

H- c

ount

s/s

(arb

uni

ts)

Energy (eV)

3rd FUSENET PhD Event in York: 26th of June 2013

36

yield comparison

0 100 200 300 400 500 600 700 800

10000

100000

1000000

Vs= - 130 V

= 0°

HOPG

Tot

al y

ield

(ar

b. u

nits

)

T,°C

NIDF studyof different carbon materials

% H

3rd FUSENET PhD Event in York: 26th of June 2013

37

yield comparison

0 100 200 300 400 500 600 700 800

10000

100000

1000000

Vs= - 130 V

= 0°

HOPG BDD

Tot

al y

ield

(ar

b. u

nits

)

T,°C

NIDF studyof different carbon materials

% H % H

% H

Boron-doped diamond:

BDD

3rd FUSENET PhD Event in York: 26th of June 2013

38

yield comparison

0 100 200 300 400 500 600 700 800

10000

100000

1000000

Vs= - 130 V

= 0°

HOPG BDD ID

Tot

al y

ield

(ar

b. u

nits

)

T,°C

NIDF studyof different carbon materials

% H

biasing problemsbelow 400°C

% H % H

% H

Intrinsic diamond: ID

3rd FUSENET PhD Event in York: 26th of June 2013

0 100 200 300 400 500 600 700 800

10000

100000

1000000

Vs= - 130 V

= 0°

HOPG BDD ID

Tot

al y

ield

(ar

b. u

nits

)

T,°C

39

yield comparison

% H % H

% H

% H

Raman spectroscopy:

sp3/sp2 BDD

sp3/sp2 HOPG

biasing problemsbelow 400°C

NIDF studyof different carbon materials

3rd FUSENET PhD Event in York: 26th of June 2013

40

sp3/sp2 phase ratio

J. Robertson, Materials Science and Engineering, R37 (2002)

Raman spectroscopy:

sp3/sp2 BDD

sp3/sp2 HOPG

NIDF studyof different carbon materials

3rd FUSENET PhD Event in York: 26th of June 2013

HOPG gives the highest i- yield at Troom

ID gives the highest i- yield at elevated T: 500°C

Conclusions

413rd FUSENET PhD Event in York: 26th of June 2013

HOPG gives the highest i- yield at Troom

ID gives the highest i- yield at elevated T: 500°C

proper use of MS diagnostic and modeling allows to determine H coverage on the sample surface

Conclusions

423rd FUSENET PhD Event in York: 26th of June 2013

HOPG gives the highest i- yield at Troom

ID gives the highest i- yield at elevated T: 500°C

proper use of MS diagnostic and modeling allows to determine H coverage on the sample surface

MS combined with Raman spectroscopy shows:

the phase ratio sp3/sp2 changes when increasing T which alters the H surface coverage and the i- yield

Conclusions

433rd FUSENET PhD Event in York: 26th of June 2013

HOPG gives the highest i- yield at Troom

ID gives the highest i- yield at elevated T: 500°C

proper use of MS diagnostic and modeling allows to determine H coverage on the sample surface

MS combined with Raman spectroscopy shows:

the phase ratio sp3/sp2 changes when increasing T which alters the H surface coverage and the i- yield

New materials with the optimal sp3/sp2 state have to be probed deeper understanding is crucial

Conclusions

443rd FUSENET PhD Event in York: 26th of June 2013

Perspectives

453rd FUSENET PhD Event in York: 26th of June 2013

Next steps

prove experimentally the H surface coverage change with T:• Infrared Spectroscopy• Temperature Programmed Desorption Spectroscopy

Perspectives

463rd FUSENET PhD Event in York: 26th of June 2013

Next steps

prove experimentally the H surface coverage change with T:• Infrared Spectroscopy• Temperature Programmed Desorption Spectroscopy

try out new materials:• low work-function materials (Gd, Ba, ...)• large band-gap insulators (Si, GaAs,…)

Perspectives

47

Next steps

prove experimentally the H surface coverage change with T:• Infrared Spectroscopy• Temperature Programmed Desorption Spectroscopy

try out new materials:• low work-function materials (Gd, Ba, ...)• large band-gap insulators (Si, GaAs,…)

3rd FUSENET PhD Event in York: 26th of June 2013

Final steps

Test the chosen material in a real negative ion source (Cybele) equipped with an extraction device and a particle accelerator (MANTIS) in CEA-Cadarache

The End

Thank you for your attention

and time!

483rd FUSENET PhD Event in York: 26th of June 2013