Ab Initio Property Prediction with Density Functional Theory (DFT) Relevant to Coating Thermal Noise Laser Interferometer Gravitational-Wave Observatory.

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Ab Initio Property Prediction with Density Functional Theory (DFT) Relevant to Coating Thermal Noise Laser Interferometer Gravitational-Wave Observatory Rand Dannenberg, California Institute of Technology, for the LIGO Optics Working Group LIGO in Hanford, WA. The twin detector is located in Livingston, LA. When a spacetime wave is generated by black hole or neutron star inspiral, arm lengths change in opposition as it moves though the detector, and a signal results. ΔL(wave) ~ 1/1000 of a proton. Atomic motion in the mirrors is a noise source ΔL(noise)! Goal – Loss Angle Minimization in Coatings: L material is IBS SiO2. H material is IBS Ta2O5. Seek lower φH or φL coating materials. Seek designs minimizing H volume. φL(SiO2) ~ 10-5 rad. φH (Ta2O5) ~ 10-4 rad. TiO2 doped into Ta2O5 lowers loss angle φH. Mechanism not well understood ! Fluctuation Dissipation Theorem: Brownian motion of material ↔ mechanical loss φ ↕ Brownian motion of material ↔ arm length noise Coating Thermal Noise: Limiting noise source for Advanced LIGO. Arm Cavity Mirror Coatings chief source. Mirrors are 1064 nm dielectric coatings. Arms L = 4 km Noise Inputs Predictable with DFT: Specific atomic heat capacity CV-at. Elastic Moduli B and Y. Gruneisen Parameter g. Thermal expansion α = gCV-at/3B. Ab Initio Example 1: SiO2-doped-TiO2: Basic Noise Formulae: Equations for thermal noise figure of merit S in a coating. Other Things Predictable with DFT: Refractive index dispersion. Band structure and gap. UV optical properties. IR vibrations. Quartz Anatase CASTEP Density Functional Theory calculation showing that when TiO2 rutile and anatase phases are doped with SiO2, there is a plateau in the refractive index for a broad range of bulk moduli. Green points are experimental data, all else is a DFT prediction. Noting (**), coating thermal noise could be minimized in TiO2 by SiO2 doping. (**) Thermal noise figure of merit for fixed index for a coating on fused silica for varying modulus. Ta2O5 n ~ 2.09, φ ~ 3.8x10-4, YH = 140 GPa → S = 38.13 (52.6% worse) Ti:Ta2O5 n ~ 2.09, φ ~ 2.3x10-4, YH = 140 GPa → S = 24.97 (baseline) Si:TiO2 (50-50) n ~ 2.08 (same thicknesses), φ ~ 3.1x10-4, YH = 87 GPa → S = 27.39 (9.7% worse) Si:TiO2 (65-35) n ~ 1.85 (thickness ≈ doubles!), φ ~ 1.9x10-4, YH = 73 GPa → S = 30.16 (20.7% worse) Modulus tuning in Si:TiO2 almost effective as loss angle reduction in Ti:Ta2O5 Ab Initio Example 2: Heat Capacity – Loss Correlation Ab Initio Example 3: Thermal Expansion Coefficient HfO2 TaO3 Al2O3 ZrO2 diamond CASTEP Density Functional Theory calculation showing a trend with specific (atomic) heat capacity, with measured loss angle. The magenta data uses experimental values of the heat capacity Cp, demonstrating a reasonable prediction of that property as well, Comparing the predicted ab initio CV (blue and yellow). CASTEP Density Functional Theory calculation of CTE using computed values of C, B and the expression α = gC/3B for Gruneisen parameter g=1. Conclusions & Further Work: DFT gives reasonable predictions of many properties for films, despite that the DFT input structures are crystalline, but films are amorphous. DFT cannot directly predict thermal noise, but relations between predictable parameters and thermal noise is suggested. Crown jewel of coating thermal noise Ti:Ta2O5 simulations will have to wait until more processors are available (all on 16 processors). Rand Dannenberg e-mail: rdannenb@ligo.caltech.edu Caltech Downs 313 website: http://www.ligo.caltech.edu Pasadena CA 91125 USA LIGO-G1000562-v1