Soft X-ray multilayer mirrors by ion assisted sputter...
Transcript of Soft X-ray multilayer mirrors by ion assisted sputter...
V. RIGATO 1Source: INFN-LNL-2009 SIF- Bologna September 21, 2010
Soft X-ray multilayer mirrors by ion assisted sputter deposition
Valentino Rigato
INFN Laboratori Nazionali di Legnaro
Bologna, September 21, 2010
V. RIGATO 2Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
OUTLINE
Laboratory Facilities at INFN-Laboratori Nazionali di Legnaro (LNL)
Multilayers with nanometer periodicity for ultra-violet and X-ray mirror technology
EUV – soft X-ray multilayersPreparation & results
X-Ray astronomy multilayers
Summary
V. RIGATO 3Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
The laboratory activity is supported by the experiments submitted and approved by INFN National Commissions and by external projects
The LNL Materials Laboratory
The LNL Materials Laboratory fields
ion–surface interaction processes(ion beam analysis, ion implantation, ion assisted film growth, irradiation )
thin films synthesis by PVD and hybrid CVD-PVD technologies
nanostructured, multilayer and advanced thin films materials
ion plasma diagnostics
electron and atomic force microscopy
electrical mechanical properties of coatings
structural properties of coatings
Publications&
Know how
V. RIGATO 4Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
The Materials LaboratoryAdvanced materials process development and synthesis
Reactive Plasma Sputtering Deposition
Plasma Diagnostics
Ion-solid interaction
Low Friction, High HardnessNanoscaled Materials and Multilayers
Soft X-ray multilayers
High Performance Plastics
Passivating layers
Scintillator materials
Research activity of the Laboratory 1) Advanced materials preparation2) Process development
V. RIGATO 5Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Characterization of materials with advanced methods1) Composition, stoichiometry, microstructure, morphology, surface topography2) Electrical, optical and mechanical properties
The Materials LaboratoryCharacterization of Physical Properties
Composition / depth profile / structureIon Beam Analysis (RBS, NRA, ERD, PIXE)Micro-PIXE 2-D trace element analysisFT-IRNuclear cross section measurement
Other physical propertiesNano-Hardness, Elastic modulusAdhesion (Micro-Scratch)Residual StressAtomic Force Microscopy & SEM
Ca Si K Fe
Ca Si K Fe
2*2 mm2
V. RIGATO 6Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Soft-X ray Multilayer MirrorsEUV and X-Ray High Reflectivity Multilayer mirrors are deposited on flat and curved substrates forapplications in X-ray astronomy, EUV lithography , “water-window” microscopy, Free Electron Laser Optics
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B4C
Rifle
ttivit
à
Energia (eV)
SiO2/(B4C/Si/B4C/Mo)×40/SiBombardamento ionicoa bassa energia (~15eV)
SiO2/(B4C/Si/B4C/Mo)×40/SiBombardamento ionico modulatoper ogni strato 5/25/75eV
Mo
Si
B4C
~3 nm
struttura del periodo
EUV Bragg High Reflectivity
Mirror design for GI hard X-ray telescopes
Multilayer Technology
Low energy ion bombardment Modulated ion bombardment
V. RIGATO 7Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
NORMAL INCIDENCE SOFT X-RAY MIRRORS
MATERIALS
absorberspacer ddnm +=Λ )(
Λ=Γ absorberd
NUMBER OF LAYERS
INTERFACE ROUGHNESS
ATOMIC INTERMIXING
V. RIGATO 8Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Soft X-Ray Multilayer Materials combinations
EUV-lithography (6 – 15 nm) (95 – 206 eV)
Astrophysics (17 – 30 nm) (41 – 73 eV)
Biology (water window 2.35 – 4.5 nm) (528 – 276 eV)
V. RIGATO 9Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
INTERFACE ATOMIC CONTROL
Sharp interfaces
Controlled intermixing
Ultra-Low interface roughness
LOW REFLECTIVITYHIGHEST REFLECTIVITY
HIGHEST REFLECTIVITY
V. RIGATO 10Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
HOW TO CONTROL INTERFACE QUALITYMultilayer are deposited by rf sputtering in Ar or Xe plasma
Ion bombardment energy and flux are controlled by plasma diagnosticsLangmuir probe with position controlPlasma potential + substrate DC BIAS (Ion Energy)Plasma density, electron temperature (Ion Flux)
Plasma is confined magnetically near substrate to increase the density of plasma facing the substrate
Variable magnetic field (0-100 Gauss) implies variable plasma density hence flux to substratePlasma density: 1010 ions/cm3 is typical
Low pressure radio frequency sputtering is preferredAbout 10-3 mBar pressure
The ion/atom ratio is calculated by using the microbalance and by using Nucler Techniques to determine the impingement rate
WHAT ION ENERGY IS BETTER ?
WHAT ION/ATOM IS BETTER ?
V. RIGATO 11Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
ION ENERGY -Bulk vs surface processesAr+ ion bombardment calculation (normal incidence)
Energy window for surface processes induced by Ar bombardmentSi: 20 - 50 eVMo: 40 - 100 eV
Sputtering and intermixingSi: E(Ar)>50 eVMo: E(Ar)>100 eV
* Z. Q. Ma and Y. Kido, Thin Solid Films 359, 288 (2000).
EdMo = 33eV
EdSi = 13eV
INVESTIGATED ENERGY
• E(Ar) = 25 eV• E(Ar) = 75 eV• Modulated Energy
V. RIGATO 12Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
*
ION/ATOM RATIOMolecular Dynamics calculations on metallic multi-layers indicate that for smoothing the interface appropriate combination of ion energy and ion/atom flux is necessary: the ion/atom ratio should be > 1
FOR MOLYBDENUM AND SILICON
Growth rate: 0.05 - 0.1 nm/s
Ion/atom ratio = 2
* X. W. Zhou and H. N. G. Wadley, Journal of Applied Physics 87, 2273 (2000).
V. RIGATO 13Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
High Resolution TEM & Reflectivity
Examples of Si(white)/Mo(dark) multilayer with reflectivityhigher than 60% at near normal incidence (@about 13.5nm)
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angle of normal incidence: 10°
Ref
lect
ivity
Photon Energy (eV)
% (pol s) % (pol p)
V. RIGATO 14Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Montecarlo CalculationsCalculate Silicon deposition rate
depends on under-layer and layer thickness
Interface thickness and composition
Mo
Ar+Si
20nm
INTERFACE NATURE
V. RIGATO 15Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Interface study is necessary to simulate XRR spectra
Interface widths (dSi/Mo and dMo/Si) Depend on ion bombardmentdMo/Si thickest
XRR PROBES INTERFACE NATURE
EAr=25eV
EAr=75eV
V. RIGATO 16Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Thermally stable engineered Mo/Si EUV multi-layers (…Si/B4C/Mo/B4C/Si…)
Interdiffusion between elements is controlled by deposition of blocking thin layer barriers
Nuclear Reaction Analysis is used to qualify the process and materials
Mo ≈ 2.5nm
amorphous Si(-H)BxC
BxC
Elastic scattering of α-particles(RBS, ERD) for H, Si, Mo analysis11B(p,α)8Be 11B(d,α0)9Be12C(d,p)13C
BxC interface atomic-layer
V. RIGATO 17Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
B(4.7)C monolayer at interfaces
Thickness and composition depends on under-layer
BxC on Mo – low energy (25eV)BxC on Si – low energy (25eV)BxC on Si – High energy (75eV)BxC on Mo – High energy (75eV)
Mo
Si
Mo
SiBxC
Mo
Si
Mo
Si
Mo
Si
Mo
SiBxC
B4C monolayer blocking interface
NRA
25eV vs 75eV bombardment on B4CBxC
V. RIGATO 18Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
Ar ion bomardment energy may be changed during the layer growth
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B4C
Ref
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Photon Energy (eV)
SiO2/(B4C/Si/B4C/Mo)×40/SiAr+ energy ~25eV
SiO2/(B4C/Si/B4C/Mo)×40/SiAr+ modulated energy for each layer: 5eV(~<1nm)/25eV(~1nm)/75eV(remaining)
Mo
Si
B4C
~3 nm
periodic structure
ION ENERGY MODULATION
Lowest energy (<=1nm)
E(Ar)=25eV (=1nm)
E(Ar)=75eV (reamining)G
RO
WTH
V. RIGATO 19Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
VARIABLE PERIODICITY MULTILAYERS - X-Ray Astronomy
Hard X-Ray Grazing Incidence reflectivity optimized by varying the period: ≈ 2 to 20nm
Single LayerReflectivity
Softer X-ra
ys
Hard X-rays
Low Density Material (C, Si)
High Density Material (Pt, W)
V. RIGATO 20Source: INFN-LNL 2009 SIF Bologna , September, 21 2010
SUMMARY
Multilayer coatings have been developed since many years at the INFN-LNL
In EUV and X-Ray mirrors technology nano-meter periodicity multilayerswith either constant or variable period have quite unique reflectioncapabilities
Ion bombardment of growing layers is necessary to improve and control the quality of interfaces and obtain highest reflectivity
Ar energy <100 eV, ion/atom ratio >1Best results obtained by changing the ion energy during the first stages of film growth
The method is scalable to large area and applicable to many materials