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F. d’Acapito LTD-10 Conference 1 The GILDA CRG at ESRF Application of LTDs to Synchrotron Radiation F. d’Acapito INFM – OGG c/o ESRF GILDA CRG B.P.220 F-38043 Grenoble (France)

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  • F. d’Acapito LTD-10 Conference 1

    The GILDA CRG at ESRF

    Application of LTDs to Synchrotron Radiation

    F. d’AcapitoINFM – OGG c/o ESRF GILDA CRG B.P.220 F-38043 Grenoble (France)

  • F. d’Acapito LTD-10 Conference 2

    The GILDA CRG at ESRF

    Layout

    • Introduction & comparison • Present & near future applications

    – X-ray Absorption Spectroscopy– X-Ray Fluorescence analysis

    • Future applications– X-ray emission spectroscopy– Resonant Inelastic X-ray scattering– X-ray Raman Scattering

    • Conclusion

  • F. d’Acapito LTD-10 Conference 3

    The GILDA CRG at ESRF

    + and - of LTD detectors

    + Low energy resolution+ Absence of geometrical constraints (scattering angles, beam size, ..)+ No critical mechanical alignment+ In vacuum operation

    - Low count rate- Reduced solid angle- Applicability to hard X-rays ?

  • F. d’Acapito LTD-10 Conference 4

    The GILDA CRG at ESRF

    Energy–resolving x-ray detectors

    LTD (STJ) SemiconductorSolid State

    Crystalanalyzers

  • F. d’Acapito LTD-10 Conference 5

    The GILDA CRG at ESRF

    Energy–resolving x-ray detectors

    106cps

    103 cps

    104 cps

    105 cps

    Count Rate

    10-4 sr0-1020TES *

    10-3 sr0.1-100.2Bragg/Grating

    10-4 sr0 - 1?10STJ *

    10-2 sr0.3-120150-300HP-Ge, Si:Li

    Solid angle

    E (keV)

    ∆E (eV)

    Type

    * Couple high resolution to no geometrical constraints

  • F. d’Acapito LTD-10 Conference 6

    The GILDA CRG at ESRF

    Application fields

    -X-ray emission spectroscopy-Resonant Raman Scattering-Non resonant Raman scattering

    00.5

    11.5

    22.5

    33.5

    4

    0 5 10 15 20 25 30 35 40

    K le

    vel N

    atur

    al W

    idth

    (eV)

    Atomic number Z

    Xtalspectrometer

    resol.

    -X-ray absorption spectroscopy-X-ray fluorescence analysis

    0

    200

    400

    600

    800

    1000

    0 10 20 30 40 50

    Kαααα line spacing

    Ekα

    (Z+1

    ) - E

    k α(Z

    ) (eV

    )

    Atomic Number Z

    2 FWHM

    Physical parameters defining the energy resolution

  • F. d’Acapito LTD-10 Conference 7

    The GILDA CRG at ESRF

    Present & near futureapplications

  • F. d’Acapito LTD-10 Conference 8

    The GILDA CRG at ESRF

    X-ray Absorption Spectroscopy

    0

    500

    1000

    1500

    2000

    18000 20000 22000 24000 26000 28000

    Fluo

    resc

    ence

    Yie

    ld (c

    ps)

    Energy (eV)

    Pd Kα

    PdKβ +

    Compton Elastic

    -0.1

    0

    0.1

    0.2

    0.3

    0.4

    0.5

    24000 24250 24500 24750 25000Abs

    orpt

    ion

    Coe

    ffici

    ent (

    Arb.

    Uni

    ts)

    Energy E (eV)

    Monochromatic X-raysof energy E

    Sample

    X-ray spectrum coming from the sample

    EXAFS spectrum

    Local Structure

    ( ) [ ]∑ −−•∝f

    if hEEirifw νδε2

    exp v)

  • F. d’Acapito LTD-10 Conference 9

    The GILDA CRG at ESRF

    Fluorescence flux

    X-ray beam: Intensity=1012 ph/s @ 6540 eV

    Sample: concentration=1015 Mn / cm2

    Detector: Collection solid angle=10-3 sr

    K fluorescence Flux: 104 ph/s

    (Neglecting elastic + compton)

  • F. d’Acapito LTD-10 Conference 10

    The GILDA CRG at ESRF

    Soft X-ray region - XAS

    STJ detector for soft x-ray fluorescence(Friedrich et al. RSI 73 (2002), 1629.)

    XAS experiment (InGaAsN at the N k edge)Lordi et al. PRL 90 (2003), 145505

  • F. d’Acapito LTD-10 Conference 11

    The GILDA CRG at ESRF

    Hard X-ray region -fluorescence

    Fluorescence spectrum of a Re foilF. Gatti et al SRN 3 (2003), in press.

    See also Poster F03

    TES detector300*400*25 µm3 Sn absorber

    TES sensor an Al/Ag multilayerCount rate ≈ 100cps

    Ω ≈ 10-8 sr

  • F. d’Acapito LTD-10 Conference 12

    The GILDA CRG at ESRF

    Cu Kα

    Co Kα&

    Fe Kβ

    Fe KαMn Kα

    Ni Kα

    Ni KβCoKβ

    FWHM = 70 eV

    Fluorescence analysis

    4000 5000 6000 7000 8000 90000

    2000

    4000

    6000

    8000

    10000

    12000

    14000

    elastico

    Ca Kα1

    Ni Kα1Co K

    α1

    Fe Kα1

    Cu Kα1

    D52_rosso D78_oro

    Cou

    nts

    Energy (eV)HP-Ge detector

    Sample of XVI centuryitalian pottery.

    TES Detector

  • F. d’Acapito LTD-10 Conference 13

    The GILDA CRG at ESRF

    Wafer surface impurity analysis

    Intentionally contaminated Si wafer. Measurement done with a Si:Li detector, ∆E=140 eV.P. Pianetta et al. RSI 66 (1995), 1293

    •Control of industrial processes•Synch. Radiation source•Total reflection condition•Detection limit: 108 – 1012 at/cm2

    High resolution desirableHigh count rate (>105 cps)

  • F. d’Acapito LTD-10 Conference 14

    The GILDA CRG at ESRF

    Future applications

  • F. d’Acapito LTD-10 Conference 15

    The GILDA CRG at ESRF

    High resolution x-ray emission spectroscopy

    • Kα and (much more) Kβ lines exhibit variations linked to the chemical environment

    • Variations are greater than the natural linewidth of the K state

    •The achievement of energy resolution of the order of 1-2 eV could give access to the several exprimental techniques techniques

    Levels of x-ray fluorescence transitions

    n=1

    2

    3

    4

  • F. d’Acapito LTD-10 Conference 16

    The GILDA CRG at ESRF

    Mn K fluorescence

    Emission from Mn excited above the K edge

    U. Bergmann et al. CPL 302 (1999), 119.

    Kα1 and Kα2 transition from 2p levels: fair chemical sensitivity

    Kβ1,3 and Kβ’ transition from the 3p statesKβ2.5 and Kβ’’ transitions from the valence band

    Chemical sensitivity !

  • F. d’Acapito LTD-10 Conference 17

    The GILDA CRG at ESRF

    Mn Kβ fluorescence

    Variation of the Kβ lines for various Mn compounds. Excitation well above the edge. (Tsutsumi et al. PRB 13 (1976), 930.)

    •Simple chemical characterization

    •Data collection currently done with Crystal analyzers•Possible use of LTD detectors if ∆E=few eV•Advantage in using LTD detectors: parallel acquisition, no mechanical movement

  • F. d’Acapito LTD-10 Conference 18

    The GILDA CRG at ESRF

    Spin selective XAS

    G. Peng et al. JACS 116 (1994), 2919

    •In MnII compounds it can be shown that Kβ1,3 originates from a spin down electron, Kβ’ from a spin up electron

    •XAS spectra can be collected by separately monitoring the two lines

    •Differences are observed that reflect the different DOS for the two spin configurations.

    •Peak separation 16 eV at 6500 eV.

    ConventionalXAS

    1s->3d

  • F. d’Acapito LTD-10 Conference 19

    The GILDA CRG at ESRF

    Resonant Inelastic X-ray Scattering (RIXS)

    •1) Promotion of a K electron above Ef by photon absorption (virtual state, no energy conservation).•2) Filling of the K hole with an L electron•3) Emission of a photon

    •The energy of the global process is conserved Ein-Eout = ε - EL•The process is resonant, i.e. enhanced near the (K) edge•Access to the electronic structure

    K

    L

    Ef

    1

    2

    ε

  • F. d’Acapito LTD-10 Conference 20

    The GILDA CRG at ESRF

    RIXSDallera & Grioni STUC 14 (2003), 57

    •Data collected with grating spectrometer

    •Evidence of a Charge Transfer peak for an excitation energy on the white line

    •The CT peak disappears for higher excitation energies

    Peak separations 5-20 eV at 835 eV

  • F. d’Acapito LTD-10 Conference 21

    The GILDA CRG at ESRF

    (Non resonant) X-ray Raman Scattering, XRS

    νi, ki

    ν f, k f

    Q=kf-kiΘ

    ( ) [ ] ( )[ ]fiif hEEirQifw ννδ −−−•Θ+∝ 22 expcos1 rr

    Transition probability w

    Same operator as XAS

  • F. d’Acapito LTD-10 Conference 22

    The GILDA CRG at ESRF

    XRS

    C K edge, graphite 6 keV

    XRS

    XAS

    U. Bergmann et al.Microchem. J. 71 (2002) 221

    •Useful for obtaining bulk information on light atoms: experiment is done at high energy.

    •1eV energy resolution is OK for data collection.

    •Signal significantly smaller than Elastic / Compton

  • F. d’Acapito LTD-10 Conference 23

    The GILDA CRG at ESRF

    Energy Dispersive X-ray Diffraction (EDX)

    Bragg law: λ=2dsin Θ

    •Normally λ is fixed and Θ is varied•In EDX Θ is fixed and λ is varied

  • F. d’Acapito LTD-10 Conference 24

    The GILDA CRG at ESRF

    EDX

    Typical EDX spectra

    Used in the early days of SRfor experiments needing small sized beams (HighPressure).Limitations•Energy resolution•Count Rate

    Application of LTDdetectors to small beams

  • F. d’Acapito LTD-10 Conference 25

    The GILDA CRG at ESRF

    Conclusion

    • High resolution LT-detectors match the requirements for X-ray absorption spectroscopy &

    fluorescence analysis ⇓

    Rise the maximum count rateExtend to hard X-rays

    • Possible use for X-ray emission spectroscopy & Raman scattering

    ⇓Improve the energy resolution down to 1 eV.

    • EDX ?