Sensitivity curves beyond the Advanced detectors

Slides:



Advertisements
Similar presentations
Albert-Einstein-Institute Hannover ET filter cavities for third generation detectors ET filter cavities for third generation detectors Keiko Kokeyama Andre.
Advertisements

Bragg’s Law nl=2dsinΘ Just needs some satisfaction!! d Θ l
‘Wet’ Chemical Techniques
Thermally Deformable Mirrors: a new Adaptive Optics scheme for Advanced Gravitational Wave Interferometers Marie Kasprzack Laboratoire de l’Accélérateur.
III. Analytical Aspects Summary Cheetham & Day, Chapters 2, 3 Chemical Characterization of Solid-State Materials Chemical Composition: Bulk, Surface, …
NanotechnologyNanoscience Modeling and Simulation Develop models of nanomaterials processing and predict bulk properties of materials that contain nanomaterials.
‘Wet’ Chemical Techniques One technique to analyze the chemistry of a mineral is to dissolve it –Water, Strong acids/bases, hydrofluoric acid, oxidants,
Masters Course: Experimental Techniques Detection of molecular species (with lasers) Techniques Direct absorption techniques Cavity Ring Down Cavity Enhanced.
Alban REMILLIEUX3 rd ILIAS-GW Annual General Meeting. London, October 26 th -27 th, New coatings on new substrates for low mechanical loss mirrors.
Optical Configuration Advanced Virgo Review Andreas Freise for the OSD subsystem.
Test mass dynamics with optical springs proposed experiments at Gingin Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin.
A. Bunkowski Nano-structured Optics for GW Detectors 1 A.Bunkowski, O. Burmeister, D. Friedrich, K. Danzmann, and R. Schnabel in collaboration with T.
Overview of coatings research and recent results at the University of Glasgow M. Abernathy, I. Martin, R. Bassiri, E. Chalkley, R. Nawrodt, M.M. Fejer,
1 An overview of work in Glasgow relevant to the design study Stuart Reid 1 SUPA, University of Glasgow Glasgow University – 22 July 2010.
LIGO Coating Project Gregory Harry LIGO/MIT - On Behalf of the Coating Working Group - LIGO/Virgo Thermal Noise Workshop October 7, 2006 Pisa, Italy LIGO-G R.
DFG-NSF Astrophysics Workshop Jun 2007 G Z 1 Optics for Interferometers for Ground-based Detectors David Reitze Physics Department University.
Optical Coatings R&D Status Gregory Harry Massachusetts Institute of Technology - On Behalf of the Coating Working Group - August, 2004 LSC Meeting Hanford.
Low temperature dissipation in coating materials S. Reid 1, I. Martin 1, H. Armandula 3, R. Bassiri 1, E. Chalkley 1 C. Comtet 4, M.M. Fejer 5, A. Gretarsson.
Center for Materials for Information Technology an NSF Materials Science and Engineering Center Scattering Techniques Lecture 17 G.J. Mankey
NANO 225 Intro to Nano/Microfabrication
Experimental investigation of dynamic Photothermal Effect
Research Topic 5 Computations Using Density Functional Theory MnO 4 AlO HF / 6-31G* (O 2 )MnO 4 AlO HF G Projects – Intermediates in oxidation of.
Parametric Instabilities In Advanced Laser Interferometer Gravitational Wave Detectors Li Ju Chunnong Zhao Jerome Degallaix Slavomir Gras David Blair.
Effect of Temperature on Coating Thermal Noise in Advanced LIGO
Coating Program Update Gregory Harry LIGO/MIT on behalf of the Coating Working Group March 22, 2006 LSC Meeting – LHO G R.
Janyce Franc-Kyoto-GWADW1 Simulation and research for the future ET mirrors Janyce Franc, Nazario Morgado, Raffaele Flaminio Laboratoire des Matériaux.
Janyce Franc Effect of Laguerre Gauss modes on thermal noise Janyce Franc, Raffaele Flaminio, Nazario Morgado, Simon Chelkowski, Andreas Freise,
Updates of Iowa State University S. Dumpala, S. Broderick and K. Rajan Sep – 18, 2013.
ACIGA High Optical Power Test Facility
Ion Beam Analysis of the Composition and Structure of Thin Films
Cavity Based Medium Resolution Spectroscopy Satyakumar Nagarajan, Frank C. De Lucia, Christopher Neese The 70 th International Symposium on Molecular Spectroscopy.
Optics related research for interferometric gravitational wave detectors S. Rowan for the Optics working group of the LIGO Scientific Collaboration SUPA,
Radiation Damage Quick Study Edward Cazalas 3/27/13.
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,
Optical Coatings for Gravitational Wave Detection Gregory Harry Massachusetts Institute of Technology - On Behalf of the LIGO Science Collaboration - August.
Studies of materials to reduce coating thermal noise K. Craig 1, I.W. Martin 1, S. Reid 2, M. Abernathy 1, R. Bassiri 1,4, K. Borisenko 3, A. Cumming 1,
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.
Low temperature dissipation in coating materials S. Reid 1, I. Martin 1, E. Chalkley 1, H. Armandula 3, R. Bassiri 1, C. Comtet 4, M.M. Fejer 5, A. Gretarsson.
1 Cascina – October 19, 2011 ASPERA Forum Laurent Pinard Substrates, Polishing, Coatings and Metrology for the 2 nd generation of GW detector Laurent PINARD.
Presentation on.  There are many methods for measuring of fiber structure. Such as:  The absorption of infrared radiation  Raman scattering of light.
STREGA WP4 coating development GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
Ab Initio Property Prediction with Density Functional Theory (DFT) Relevant to Coating Thermal Noise Laser Interferometer Gravitational-Wave Observatory.
Polarization Dependence in X-ray Spectroscopy and Scattering
2SUPA, Institute for Gravitational Research, University of Glasgow
Effects of sintering temperature on the physical and
Sanghamitra Mukhopadhyay Peter. V. Sushko and Alexander L. Shluger
UV-Curved Nano Imprint Lithography
Synopsis by Maria Ruiz-Gonzalez 12/8/16
Mirror thermal noises and its implications on the mirror design
Electric Grid Technology Energy Storage Technology
L. Glover(1,3), R. DeSalvo(1,3), B. Kells(2), I. Pinto(3)
Department of Electronics
Current status of coating research in Glasgow
The atomic structure and properties of heat-treated Ta2O5 coatings
Thermal noise reduction through LG modes
NANOCHEMISTRY.
Characterizing Multilayer Thin films
‘Wet’ Chemical Techniques
Flat-Top Beam Profile Cavity Prototype: design and preliminary tests
Introduction to thermal noise workshop and goals
Riccardo DeSalvo (Cal State LA)
Radiation tolerant fibres for LHC controls and communications
Ge nanostressors on silicon-on-insulator (SOI)
Flat-Top Beam Profile Cavity Prototype
Pierre Favier Laboratoire de l’Accélérateur Linéaire
Planck’s law: E=hn =hc/l
R&D in Glasgow MATERIALS ACTIVITY AIM Silica
Fig. 2 Materials and designs for bioresorbable PC microcavity-based pressure and temperature sensors. Materials and designs for bioresorbable PC microcavity-based.
Presentation transcript:

Sensitivity curves beyond the Advanced detectors 3

Mirror coatings thermal noise: setting the goal for ET aLIGO ET-HF ET-LF Mirrors (Coatings) 1/5.5 from T 1/1.7 from beam diameter 1/√x from j Reduction: times @ 300 K times @ 10 K 2.8 8.2 For the ET requirements: x > 2.7 @ 300K x > 0.8 @ 10k The 1.7 factor may increase further if the LG33 mode replaces the TEM00 in the cavities

Parameters for the different generations of GWD 300 K 10 K 20 K

Strategies to reduce the losses in coatings Optimum annealing Blending of oxides (TiO2, Ta2O5, SiO2, HfO2, ZrO2) Nano-layering Oxygen free amorphs (silicon... But absorption is high) Structural investigation: searching for the relaxation mechanisms and a way to deactivate them

Structural investigation tools - 1 Atomic distribution, small and medium range order X-ray and electron diffraction (length scale up to ~1 nm) Extended x-ray Absorption Fine Structure (EXAFS) (length scale up to ~1 nm) Scanning diffraction using 2 nm x-ray beam size (length scale 0.5 nm to 3 nm) Structure dynamics Raman scattering spectrometry: [0.1, 5] THz (vibration of structures with dimensions in the range [0.1, 1] nm) Brillouin scattering spectrometry: [5, 100] GHz (medium range order)

Structural investigation tools - 2 Chemical state and stoichiometry X-ray Photoelectron spectroscopy (XPS) Nuclear Magnetic Resonance (NMR) Rutherford Back Scattering (RBS) Modelling So far the simulation is the only way to “see” the relaxing structures Prediction of mechanical losses are based on barrier height distribution g(V) and on the deformation potential g. Structural data can be used to check the simulation

Open questions (not an exhaustive list!) Does annealing increase or reduce losses? And does it at any temperature? What are the relaxing structures in the different optical coatings? Why does fused silica have a very deep minimum of losses at room temperature? And why the other oxides don’t? How close to reality are the barrier heights distributions simulated by molecular dynamics?