VUV spectroscopy of BaF 2 :Er A.J. Wojtowicz

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A.J. Wojtowicz, FPS July 2007 1 VUV spectroscopy of BaF 2 :Er A.J. Wojtowicz Institute of Physics, N. Copernicus Univ. Toruń, POLAND FPS 2007 French-Polish Symposium on Spectroscopy of Modern Materials in Physics, Chemistry and Biology. July 15 – 18 2007, Clermont-Ferrand, France

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VUV spectroscopy of BaF 2 :Er A.J. Wojtowicz Institute of Physics, N. Copernicus Univ. Toruń, POLAND FPS 2007 French-Polish Symposium on Spectroscopy of Modern Materials in Physics, Chemistry and Biology. July 15 – 18 2007, Clermont-Ferrand, France. INTRODUCTION - PowerPoint PPT Presentation

Transcript of VUV spectroscopy of BaF 2 :Er A.J. Wojtowicz

Page 1: VUV spectroscopy of BaF 2 :Er A.J. Wojtowicz

A.J. Wojtowicz, FPS July 2007 1

VUV spectroscopy of BaF2:Er

A.J. WojtowiczInstitute of Physics, N. Copernicus Univ. Toruń, POLAND

FPS 2007French-Polish Symposium on Spectroscopy

of Modern Materials in Physics, Chemistry and Biology.

July 15 – 18 2007, Clermont-Ferrand, France

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INTRODUCTION

Why VUV spectroscopy?

Materials for UV, VUV solid state lasers

quantum cutting phosphors

scintillators

GOAL of this work:

identify various VUV excited emissions and

identify different excitation mechanisms in

BaF2:Er

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Scintillators

Ce scintillators: LSO, LYSO, LuAP, LuYAP

fn 2n31

1105.1

2

224

R

Ce: 350 nm, 15-30 ns

then Pr i Nd, emitting at 250, 190 nm,

should have 8-15 and 5-10 ns (more or less true)

Heavy lantanides have even higher energy d-levels…

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Could it be that 4d-5f emission from ions such as

Tb, Dy, Ho, Er or Tm is efficient and even faster

under excitation by ionizing radiation?

Is the oscillator strength f up to the expectations?

Is energy transfer from host to ion efficient?

NO on both questions in the case of BaF2:Er

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In general, for Ln 4fn

4fn → 5d4fn-1

for Ce just one option:

4f → 5d (no f electrons left behind)

for Pr

4f2↑↑(HS) → 5d↑4f↑(HS) or 5d↓4f↑(LS);

the second option is higher in energy and

forbidden; f almost the same

for higher n it is getting worse;

more allowed states lower f

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For n > 7 situation changes drastically.

For Tb3+:

4fn ↑↑↑↑↑↑↑↓(2S+1=7, LS) → 5d↑4fn-1 ↑↑↑↑↑↑↑

(2S+1=9, HS) spin-forbidden, lower in energy

and

5d↓4fn-1 ↑↑↑↑↑↑↑, no spin flip (2S+1=7, LS)

spin-allowed but higher in energy – Hund’s rule;

the lowest excited state will be HS and

emission transition will be spin-forbidden

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SAMPLES and EXPERIMENTS

BaF2:0.2%Er, grown by Bridgman, at Optovac,

donated by A. Lempicki of ALEM, Boston

Emission and excitation spectra:

I–beamline, Superlumi, Hasylab, Hamburg,

Germany (prof. G. Zimmerer)

U9B beamline, National Synchrotron Light Source,

Brookhaven, USA (dr J. Sutherland)

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VIS emissions; lower Er3+ levels excited

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UV emissions; higher Er3+ levels excited

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Excitation spectra of VIS emissions; RT and 5 K

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Excitation below 124 nm; STE, some VIS emission

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VIS and UV emissions competition, Er-BE and d-levels

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STE, Er-BE and d-levels

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STE emission under over the bandgap excitation

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VUV emissions under d-level excitation

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Excitation spectrum of VUV emissions

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Excitation spectrum of Ce emission in BaF2

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BaF2:Ce, crystal field splitting 10Dq, (3+2) structure, d-levels split into t and e

In BaF2:Er four bands, no single electron crystal field structure (3+2) like in BaF2:Ce

Er3+4f11 ground state 4I15/2 (LS, 2S+1=4)

Excited state 5d(e)↓ 5I8(4f10) (HS, 2S+1=6)

Excited state 5d(e)↑ 5I8(4f10) (LS, 2S+1=4)

Excited state 5d(e)↑ 5I7(4f10) (LS, 2S+1=4)

Excited state 5d(t)↓ 5I8(4f10) (HS, 2S+1=6)

10Dq ~ 12800 cm-1

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Excitation spectrum of VUV emissions

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Emission and absorption spectra; the lowest d-level

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The shape, difference between emission and absorption

Zero-phonon line, exp(-S)S, Huang Rhys factor

S ~ 1-2

Surprisingly weak electron-phonon coupling, consequently relatively narrow bands in emission and

absorption

No good match to 2F5/2 or other high 4f11 levels,transitions directly from d ?

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UNDER VUV EXCITATION THERE ARE 3 DISTINCT TYPES OF EMISSIONS:

1) VIS Er3+4f11 emission lines

2) UV and VUV 4f11, 5d-4f emission lines and bands

3) STE emisssion (no relation to Er)

SUMMARY

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UNDER VUV EXCITATION THERE ARE 3 DISTINCT CHANNELS:

1) Below 124 nm, STE emission, no transfer to Er

2) Above 124 nm, up to about 170 nm Er-BE (CT), large relaxation (F+H), subsequent transfer to lower

Er 4f11 energy levels (VIS emissions)

3) In the range 130 to 160 nm, d-levels, direct? via ? (2F(2)5/2?)

higher Er 4f11 energy levels (UV and VIS emissions)

SUMMARY

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No fast and efficient scintillator

Although there is some competition from direct VIS, VUV and UV (and consequtive VIS) emissions prevail

under selective VUV excitation into d-bands quantum cutting phosphors?

VUV, UV lasers?

Possible upconversion(reversed two photon cascade emission)

SUMMARY

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ADVICE AND EXPERTISE in VUV experimentsProf. G. Zimmerer, dr M. Kirm of Hasylab

Drs. J. Sutherland, J. Trunk, U9B Brookhaven

Help in experiments: W. Drozdowski, J. Glodo, M. Wisniewska, D.Wisniewski

Crystals of BaF2:Er and others, donatedby A. Lempicki, ALEM Assoc. Boston

ACKNOWLEDGMENT