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Peculiarities of Modeling LPP Source at 6.X nm V.Novikov, V.Ivanov, K.Koshelev, V.Krivtsun, A.Grushin, R.Kildiyarova, A.Solomyannaya EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011
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Challenges of modeling of Sn, Gd and Tb EUV sources

Jan 22, 2023

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Page 1: Challenges of modeling of Sn, Gd and Tb EUV sources

Peculiarities of Modeling LPP Source

at 6.X nm

V.Novikov,

V.Ivanov, K.Koshelev, V.Krivtsun, A.Grushin,

R.Kildiyarova, A.Solomyannaya

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Page 2: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Outline

• Theoretical base

• Optimal plasma parameters

• Band position

• Scaling CE by RZLINE modeling

• Laser types: Nd YAG vs CO2

• Conclusion

2

Page 3: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Fuel at ~ 6.5-6.7 nm

3

S S Churilov, R R Kildiyarova, A N Ryabtsev and S V Sadovsky Phys. Scr. 80 (2009) 045303

Gd

Tb

Page 4: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

THERMOS_BELINE code

4

• Main purpose:

- to get CRE tables with arbitrary radiation field;

- obtaining the realistic emission spectra;

- in-line version for radiative hydro-dynamics;

Method:

- special averaging with given photon energy grid;

- usage the stored data prepared beforehand.

The code makes possible self-consistent calculation

of level kinetics and radiation transport for arbitrary

plasma configurations.

The code includes:

radiation transport of overlapped spectral lines with

arbitrary optical thickness and realistic line profiles;

verified atomic database for low-Z materials (H, He, C,

N,O) and also for Xe, Sn, W, Tb, Gd.

COMPUTING OF LEVEL KINETICS & RADIATION TRANSPORT

Sn

Gd

Page 5: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011 5

Gd XVII - XXII (4dm4fn)

Mirror 6.6 - 6.8 nm

Gd & Tb ions emission

Tb XXIII - XXX (4pk4dm4fn)

Page 6: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011 6

Sn (13.5) vs Gd (6.x)

6

Material Sn Gd

Band 2% at 13.5 nm 0.6% at 6.x

Ions VIII - XIV XVII - XXII

Temperature ~ 35 eV ~ 100 eV

Size ~ 200 um ~ 200 um

Optical thickness

Electron density

CE

Page 7: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Sn ionization: T=32.5 eV

7

Saha

transparent plasma

optically thick

in the interval 13-14 nm

Page 8: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Gd ionization at T=90 eV

8

D=200um

Page 9: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Gd absorption in band

9

D = 0.02 cm

tau = 10

Page 10: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Sn (13.5) vs Gd (6.x)

10

Material Sn Gd

Band 2% at 13.5 nm 0.6% at 6.x

Ions VIII - XIV XVII - XXII

Temperature ~ 35 eV ~ 100 eV

Size ~ 200 um ~ 200 um

Optical thickness ~ 1 ~ 1

Electron density ~ 1019 1/cm3 ~ 1020 1/cm3

CE

Page 11: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Position of band

11

13.5 6.746

Sn Gd

Page 12: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Detailed spectrum

12

Gd

Page 13: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Influence of broadening

13

Gd Sn vs

Page 14: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

14

Gd D = 200 um

Ne=1020 1/cm3

Page 15: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

15

Gd D = 200 um

Ne=1020 1/cm3

Page 16: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

16

Gd D = 200 um

Ne=1020 1/cm3

Page 17: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

17

Gd D = 200 um

Ne=1020 1/cm3

Page 18: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

18

Gd D = 200 um

Ne=1020 1/cm3

Page 19: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

19

Gd D = 200 um

Ne=1020 1/cm3

Page 20: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

20

Gd D = 200 um

Ne=1020 1/cm3

Page 21: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

21

Gd D = 200 um

Ne=1020 1/cm3

Page 22: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Temperature dependence

22

Gd D = 200 um

Ne=1020 1/cm3

Page 23: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Dependence on plasma size

23

Gd Tb

T = 110 eV

Ne = 1020 1/cm3 T = 90 eV

Ne = 1020 1/cm3

Page 24: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Dependence on plasma size

24

Tb Gd

T = 110 eV

Ne = 1020 1/cm3 T = 90 eV

Ne = 1020 1/cm3

Page 25: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Dependence on plasma size

25

Tb Gd

T = 110 eV

Ne = 1020 1/cm3 T = 90 eV

Ne = 1020 1/cm3

Page 26: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Sn (13.5) vs Gd (6.x)

26

Material Sn Gd

Band 2% at 13.5 nm 0.6% at 6.x

Ions VIII - XIV XVII - XXII

Temperature ~ 35 eV ~ 100 eV

Size ~ 200 um ~ 200 um

Optical thickness ~ 1 ~ 1

Electron density ~ 1019 1/cm3 ~ 1020 1/cm3

CE ~ 7% ~ 3%

More realistic modeling is based

on RHD calculations with the code

RZLINE

Page 27: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

2D Eulerian RMHD code

Laser tracing,

absorption and reflection of laser pulse,

energy fluxes to and from target,

electron and ion thermo-conductivity,

radiative transfer in ~100 spectral groups,

evaporation and condensation of target,

ionization and recombination of plasma.

Diffusion-like spectral radiation transport,

calculation of EUV source size,

detailed spectra,

anisotropy of EUV radiation,

fast ions.

Nonhomogeneous grid ~ 105 r,z cells

Calculation time ~ 2 hours on PC

RZLINE code

RZLINE works with two types of tables:

1.Transparent case table

2.Optically thick case table

(nontrasparent in band)

Temperature 1 – 500 eV

Electron density 1014 – 1023 1/cm

Photon energy range 1 – 1000 eV

Page 28: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

CE scaling

28

flat target

Nd YAG laser

t = 2 ns

D = 160 um

Gd

Page 29: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

CE scaling

Nd YAG laser

E = 1 J

D = 100 um

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

1e+013 1e+014

flat target

Gd

Page 30: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

1e+010 1e+011 1e+012

CE

, %

Power density, W/cm^2

Experiment

CE scaling

30

CO2 laser

t = 60 ns

D = 200 um

Gd

flat target

including anisotropy

w/o including anisotropy

Page 31: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Comparison with experiment

31

CO2 laser

E = 0.8 J

t = 60 ns

D = 200 um

flat target Gd

Page 32: Challenges of modeling of Sn, Gd and Tb EUV sources

EUV and Soft X-ray Source Workshop, Dublin, November 7-10, 2011

Conclusion

32

Comparison of Gd & Sn plasma

LPP source was fulfilled

Optimal plasma for homogeneous Gd ball with size

D ~ 200 um,T ~ 90 eV, Ne ~ 1020 1/cm3

gives CE ~ 3 % in 0.6% band at 6.746 nm

Modeling by using the code RZLINE gives

for plate Gd target CE ~ 1 % for CO2 laser