Absorption Studies in Sapphire

Slides:



Advertisements
Similar presentations
SPATIAL CORRELATION OF INFRARED AND PL OPTICAL CENTERS IN HYDROGEN-RICH DIAMONDS Troy Ardon and Sally Eaton-Magaña Gemological Institute of America Carlsbad,
Advertisements

November 29-30, 2001 LIGO-G Z Talk at PAC-11, LHO 1 Proposal Thermal and Thermoelastic Noise Research for Advanced LIGO Optics Norio Nakagawa.
What experiments should we be doing? Dion L. Heinz University of Chicago.
Member of the Helmholtz Association Takeshi Hirai | Institute of Energy Research | Association EURATOM – FZJ Cracking of a tungsten material exposed to.
RADIATIVE PROPERTIES OF REAL MATERIALS Electromagnetic Theory: ▪ ideal, optically smooth surface ▪ valid for spectral range larger than visible Real Materials:
Ultraviolet and Visible Spectroscopy Chemical Ideas 6.8.
Silicon Oxidation ECE/ChE 4752: Microelectronics Processing Laboratory Gary S. May January 15, 2004.
Ruby Laser Crystal structure of sapphire: -Al2O3 (aluminum oxide). The shaded atoms make up a unit cell of the structure. The aluminum atom inside the.
Large sapphire substrate absorption measurements for LIGO S.M.A.- VIRGO Université Claude Bernard LYON I IPNL - IN2P3 – CNRS 22, Boulevard Niels Bohr
Spatial profiles of copper atom density in a Cu/Ne hollow cathode discharge P. Hartmann*, T.M. Adamowicz**, E. Stoffels and W.W. Stoffels, Department of.
Heat Transfer Physics 202 Professor Lee Carkner Lecture 14.
Thermal Compensation Review David Ottaway LIGO Laboratory MIT.
Prometheus-L Reactor Building Layout. Two Main Options for the Final Optic (2) Grazing incidence metal mirror (1) SiO 2 or CaF 2 wedges.
Thermo-elastic properties characterization by photothermal microscopy J.Jumel,F.Taillade and F.Lepoutre Eur. Phys. J. AP 23, Journal Club Presentation.
Dublin/July'04 1 BLTS interferometers: Big, Low-temperature Transparent Silicon Interferometers Warren Johnson Louisiana State University LIGO-G Z.
Nonlinear Optics Lab. Hanyang Univ. Chapter 3. Classical Theory of Absorption 3.1 Introduction Visible color of an object : Selective absorption, Scattering,
4-1 Chap. 7 (Optical Instruments), Chap. 8 (Optical Atomic Spectroscopy) General design of optical instruments Sources of radiation Selection of wavelength.
Defects & Impurities BW, Ch. 5 & YC, Ch 4 + my notes & research papers
Fiber Optics Communications Lecture 11. Signal Degradation In Optical Fibers We will look at Loss and attenuation mechanism Distortion of optical signals.
PREPARATION OF ZnO NANOWIRES BY ELECTROCHEMICAL DEPOSITION
Trace element content comparison for high-loss and low-loss sapphire* S. C. McGuireG. P. Lamaze and E. A. Mackey Department of PhysicsChemical Sciences.
The contribution from The contribution from photoluminescence (PL) Gordon Davies, King’s College London.
Influence of oxygen content on the 1.54 μm luminescenceof Er-doped amorphous SiO x thin films G.WoraAdeola,H.Rinnert *, M.Vergnat LaboratoiredePhysiquedesMate´riaux.
Thermal noise from optical coatings Gregory Harry Massachusetts Institute of Technology - on behalf of the LIGO Science Collaboration - 25 July
Recent advances in intercalation compounds physics.
Piezoelectric Spectroscopy of the Defects States on the Surfaces of Semiconducting Samples M. Maliński 1, J. Zakrzewski 2, K. Strzałkowski 2, F. Firszt.
Absorption in bulk crystalline silicon and in the crystal surfaces Aleksandr Khalaidovski 1 Alexander Khalaidovski 1, Jessica Steinlechner 2, Roman Schnabel.
Photoacoustic Spectroscopy of Surface Defects States of Semiconductor Samples 1) M.Maliński, 2) J.Zakrzewski, 2) F.Firszt 1) Department of Electronics.
Ultrafast Carrier Dynamics in Graphene M. Breusing, N. Severin, S. Eilers, J. Rabe and T. Elsässer Conclusion information about carrier distribution with10fs.
Gravitational Wave Detection Using Precision Interferometry Gregory Harry Massachusetts Institute of Technology - On Behalf of the LIGO Science Collaboration.
Absorption in bulk crystalline silicon and in the crystal surfaces Aleksandr Khalaidovski 1 Alexander Khalaidovski 1, Jessica Steinlechner 2, Roman Schnabel.
NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.
Tunable, resonant heterodyne interferometer for neutral hydrogen measurements in tokamak plasmas * J.J. Moschella, R.C. Hazelton, M.D. Keitz, and C.C.
Doping and Crystal Growth Techniques. Types of Impurities Substitutional Impurities Substitutional Impurities –Donors and acceptors –Isoelectronic Defects.
LIGO-G Z Thermal noise in sapphire - summary and plans Work carried out at: Stanford University University of Glasgow Caltech MIT.
IMPERFECTIONS IN SOLIDS
Quenching of Fluorescence and Broadband Emission in Yb 3+ :Y 2 O 3 and Yb 3+ :Lu 2 O 3 3rd Laser Ceramics Symposium : International Symposium on Transparent.
Coating Program Update Gregory Harry LIGO/MIT on behalf of the Coating Working Group March 22, 2006 LSC Meeting – LHO G R.
Thermoelastic dissipation in inhomogeneous media: loss measurements and thermal noise in coated test masses Sheila Rowan, Marty Fejer and LSC Coating collaboration.
Nanoscale Cr 4+ Doped Olivine Crystallites Used In Optical Amplifiers and Lasers Presentation by: Victor Ortiz Mentor: Dr. Alexei Bykov Mentor: Dr. Alexei.
Studies of Thermal Loading in Pre-Modecleaners for Advanced LIGO Amber Bullington Stanford University LSC/Virgo March 2007 Meeting Optics Working Group.
Status of Modeling of Damage Effects on Final Optics Mirror Performance T.K. Mau, M.S. Tillack Center for Energy Research Fusion Energy Division University.
TCS and IFO Properties Dave Ottaway For a lot of people !!!!!! LIGO Lab Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of.
LIGO Laboratory1 Thermal Compensation in LIGO Phil Willems- Caltech Baton Rouge LSC Meeting, March 2007 LIGO-G Z.
Sapphire for the LCGT project Eiichi Hirose ICRR, University of Tokyo Kyohei Watanabe, Norikatsu Mio PSC, University of Tokyo GT Advanced Technology, Sep.
LOSSES IN FIBER BY:Sagar Adroja.
Chapter 1 Diffusion in Solids. Diffusion - Introduction A phenomenon of material transport by atomic migration The mass transfer in macroscopic level.
1.1 What’s electromagnetic radiation
Influence of deposition conditions on the thermal stability of ZnO:Al films grown by rf magnetron sputtering Adviser : Shang-Chou Chang Co-Adviser : Tien-Chai.
LIGO-G D LIGO Laboratory1 Advanced LIGO Test Mass Material Selection Status GariLynn Billingsley LSC 20 March 2003.
J.Vaitkus et al. PC spectra. CERN RD50 Workshop, Ljubljana, "Analysis of deep level system transformation by photoionization spectroscopy"
LIGO-G Z Silicon as a low thermal noise test mass material S. Rowan, R. Route, M.M. Fejer, R.L. Byer Stanford University P. Sneddon, D. Crooks,
Heinert et al Properties of candidate materials for cryogenic mirrors 1 Properties of candidate materials for cryogenic mirrors D. Heinert,
LIGO-G R 1 Gregory Harry and COC Working Group Massachusetts Institute of Technology - Technical Plenary Session - March 17-20, 2003 LSC Meeting.
LIGO Scientific Collaboration
Imperfections in Solids
LIGO-G Z 1 Report of the Optics Working Group to the LSC David Reitze University of Florida March 20, 2003.
The coating thermal noise R&D for the 3rd generation: a multitechnique investigation E. Cesarini 1,2), M.Prato 3), M. Lorenzini 2) 1)Università di Urbino.
1 4.1 Introduction to CASTEP (1)  CASTEP is a state-of-the-art quantum mechanics-based program designed specifically for solid-state materials science.
Material Downselect Rationale and Directions Gregory Harry LIGO/MIT Kavli Institute for Astrophysics and Space Technology On behalf of downselect working.
High-temperature ferromagnetism
S. Rowan, M. Fejer, E. Gustafson, R. Route, G. Zeltzer
Overview of Advanced LIGO Coating Status
LIGO Scientific Collaboration
Main Efforts of the Core Optics WG
OPTICAL PROPERTIES K L University Department of Physics.
Modeling of Advanced LIGO with Melody
LIGO Scientific Collaboration
Defects & Impurities BW, Ch. 5 & YC, Ch 4 + my notes & research papers
Part 1: Earth’s Dynamic Interior
Presentation transcript:

Absorption Studies in Sapphire LIGO-G010152-00-Z A. Alexandrovski, R. K. Route, M. M. Fejer E. L. Ginzton Laboratory Stanford University fejer@leland.stanford.edu

Why Do We Care? Imperfect materials  absorption Absorption  inhomogeneous temperature rise Temperature rise  thermal expansion, change in refractive index Distorted optic  distorted wavefront Implications for IF design limits allowable power on various elements influences cavity stability through power range Options transmissive optics low loss materials clever IF design active thermal compensation reflective designs e.g. Beyersdorf talk

Temperature Rise in Absorbing Medium Absorbed optical power inhomogeneously heats crystal produces radially varying temperature produces optical distortion due to photothermal effects r T Pavg DT Temperature rise across beam independent of spot size Leads to radially varying index: Leads to radially varying phase on optical beam: Similarly get a bump on surface:  = thermal expansion coeff.

Requirements Intrinsic and extrinsic material properties combine to determine distortion transmission FOM: reflection from absorbing substrate: For LIGO II ~10 ppm/cm  OK ~40 ppm/cm  with active thermal compensation Currently: 40 ppm/cm in large samples isolated observations at 10 ppm/cm level

Outline Absorption characteristics in sapphire Absorption measurements Crystal Growth Sample Sets growth studies annealing studies Observations and Trends Status and Plans

Absorption in Sapphire Intrinsic conduction to valence band in UV multiphonon in mid-IR only cure is different material expectation and existence proofs indicate this isn’t the problem Extrinsic native defects vacancies, antisites, interstitials, impurities e.g. transition metals: Cr, Ti, Fe, … l log(a) ~10-6 cm-1 ~3 m-1 Ti3+ Cr3+

Characteristics of Absorbing Species Allowed transitions large cross sections  ppm concentrations significant Broad spectral features identification difficult off “resonant” absorption significant sum of several species can contribute to absorption at given l Redox state important e.g. a[Ti3+]  a[Ti4+] annealing alters absorption without altering impurity concentrations Impurities do not necessarily act independently Al : Al :Ti3+ : Ti4+ : Al : Al  Al : Ti3+ : Al : Al : Ti4+ : Al absorption spectra at high concentrations not always same as low complicates correlations to known spectra Ti4+ Ti3+

Absorption Measurement Spectrophotometer broad continuous wavelength coverage (UV – IR) difficult to resolve below 10-3 absorption reflections and interference also influence transmission especially for broad features no spatial resolution gives line-integrated absorption Common-path photothermal interferometry (Alexometry) spatially resolved (< 0.5 mm ) sensitive (~ 1 ppm/cm absorption) requires laser, so wavelength coverage not continuous 1.06 m, 0.532 m, 0.514 m, 0.488 m, … CPPI Perkin-Elmer Pump Probe Sample

Typical Spectra longitudinal scan in Al2O3 Various Al2O3 Samples 25 ppm >200 ppm 100 um Scan through electroded Al2O3 ·       trace 1: 100A-thick electrode ·       trace 2: 1200A-thick electrode

HEM Crystal Growth Heat Exchanger Method Starting materials He-gas cools bucket of melt solidification outwards from bottom Starting materials typically “craquelle” sapphire ppm levels of some transition metals purity   $  Segregation impurities rejected (k < 1) into melt segregate into outer regions of crystal (last to crystallize) can expect different behavior top/middle/bottom of boule can remelt outer portion to concentrate impurities remelt inner portion to reduce impurity concentration opposite argument for k >1 impurities

Samples Experimental design Growth Studies Annealing Studies anticipated mechanisms: impurity concentration, intrinsic defects, redox state two main control methods: growth and annealing Growth Studies ~ 30 CSI White, 1 cm cubes primarily expected to influence impurity concentration starting materials virgin material from 5 different vendors/purity remelted boules samples cut from top/middle/bottom of boule explore impurity segregation effects Annealing Studies 2.5 cm dia x 1 cm thick a-axis Hemex CSI White primarily influence redox state, intrinsic defects (e.g. Oxygen vacancies) parameters: time, temperature, reducing (H2) or oxidizing (air, O2) furnace design accidental introduction of impurities, especially near surface Occasional samples large CSI samples from coating or Q tests SIOM crystals T M B

Composition Analysis (GDMS) ppm’s of everything

Example of As-Grown Sample Data and Inference Observations F+-center 255 nm F-center 203 nm 255 nm absorption correlates with 1064 nm extrapolates to limit of 40 ppm weaker correlation at high concentration No correlation of 1064 nm absorption and Ti fluor. Tentative Conclusions F-center (or correlated defect) contributes to 1064 abs. can drive this defect to negligible level remaining 40 ppm from another defect Ti not related to these defects Typical of process for other observed correlations

Other Typical Observations Absorption (ppm/cm) 1064 nm vs 532 nm, o-wave

Curious observation (Rosetta Sapphire) Single 1 cm sample region with 10 ppm/cm region with 600 ppm/cm abrupt boundary between Preparation unexceptional Tantalizing existence proof Mechanism not yet clear suggests “self-normalizing” measurements 1 cm 600 ppm/cm 10 ppm/cm

Typical Annealing results 1 cm thick window Two diffusion waves? Junk from furnace? Desired oxidation Before: 50 ppm Short Long: 25 ppm

Complicated Annealing Phenomena Bulk: 50 ppm Minimum: 10 ppm Maximum: 80 ppm surface contamination? oxidation 1064 nm absorption through cross-section of a cube

Annealed Samples Show Variety of Outcomes similar table exists for as-grown cubes

Observed Trends Annealing No strong correlation with starting material hydrogen annealing does not affect bulk absorption oxygen annealing appears to reduce bulk absorption surface contamination appears to limit final outcome two diffusion “waves”: one reduces loss, one increases it No strong correlation with starting material native defect? furnace contamination? No strong correlation with position in boule or remelt multiple impurities?

Status/ Plans Currently: Next steps: ~ 40 ppm/cm ~reproducible 25 ppm/cm observed in macroscopic volumes 10 ppm/cm in isolated regions Next steps: elimination of surface effects essential for reproducible studies new annealing furnace (CSI and SU) more careful surface prep and absorption measurement prior to annealing repeat best annealing conditions w/o surface contamination “wave” revisit impurity correlations after reproducible annealing neutron activation with Southern U. (McGuire) multiwavelength PCI “solid-state electrolysis” from General Physics Institute (Danileiko)?