Experimental Study of Crackling Noise as Micro-mechanics of Flow Kla Karava Mentors: Xiaoyue Ni, Julia Greer, and Rana Adhikari Part of the LIGO SURF programme 2015 California Institute of Technology LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 1 Form F0900041-v1 Motivation for Crackling Noise Barkhausen noise in magnetisation Wikimedia Commons Stochastic LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 2 Form F0900041-v1 Crackling Noise in aLIGO LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 3 Form F0900041-v1 Potential Source? LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 4 Form F0900041-v1 Potential Source? Non-linear collective behaviour of pinned dislocations Orowan Bowing X. Ni ,What is Crackling Noise: a Study of Micro-mechanics of Flow in Metals (2015) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 5 Form F0900041-v1 Then, how to study? Pure Copper > Maraging Steel fcc > bcc Well-defined slip planes {111} {110} MSM Part IA Course D Handout, University of Cambridge (2014) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 6 Form F0900041-v1 Then, how to study? Monocrystalline Cu nanopillars: 500x1500 nm (1:3) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 7 Form F0900041-v1 Why Nanopillars? Nanopillar Bulk MSM Part IA Course D Handout, University of Cambridge (2014) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 8 Form F0900041-v1 Focused Ion Beam (FIB) X. Ni, What is Crackling Noise: a Study of Micro-mechanics of Flow in Metals (2015) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 9 Form F0900041-v1 Focused Ion Beam (FIB) FEI® Versa 3D LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 10 Form F0900041-v1 Well, what’s the problem? Too much noise LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 11 Form F0900041-v1 Alternative approach? Energy dissipation Dynamic Mechanical Analysis (DMA) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 12 Form F0900041-v1 Dynamic Mechanical Analysis (DMA) 𝜎 𝑡 = 𝜎0 sin(𝜔𝑡) 𝜀 𝑡 = 𝜀0 sin(𝜔𝑡 − 𝜙) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 13 Form F0900041-v1 Dynamic Mechanical Analysis (DMA) Continuous DMA LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 14 Form F0900041-v1 Dynamic Mechanical Analysis (DMA) X. Ni , What is Crackling Noise: a Study of Micro-mechanics of Flow in Metals (2015) LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 15 Form F0900041-v1 Dynamic Mechanical Analysis (DMA) Hysitron® Triboindenter LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 16 Form F0900041-v1 Dynamic Moduli 𝐸 = 𝐸𝑠𝑡𝑜𝑟𝑎𝑔𝑒 + 𝑖𝐸𝑙𝑜𝑠𝑠 𝜎0 𝐸 ≡ (cos𝜙 + 𝑖sin𝜙) 𝜀0 LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 17 Form F0900041-v1 Standard Linear Model of Solids Frame Stiffness 𝑘1 Indenter Stiffness Machine Damping Contact Stiffness Material Stiffness Leaf Spring Stiffness Contact Damping LIGO-G09xxxxx-v1 LIGO Scientific Collaboration A.R. Maloney & W.D. Nix , An Improved Analysis for Viscoelastic Damping in Dynamic Nanoindentation (2007) 18 Form F0900041-v1 Results for Cu 500nm Theoretical results 1 Hz 10 Hz 200 Hz Experimental results 1 Hz 10 Hz 200 Hz LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 19 Form F0900041-v1 But…how can we be sure? Machine artefacts: thermal drift? Calibration? Are machine parameters actually constant? LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 20 Form F0900041-v1 Fused Silica Nanopillars Amorphous No dislocation LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 21 Form F0900041-v1 Result for Fused Silica 1 Hz LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 22 Form F0900041-v1 Size Effect Cu 1 µm nanopillars LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 23 Form F0900041-v1 Comparing Results 500 nm 1 Hz 10 Hz 200 Hz 1 µm 1 Hz 10 Hz 200 Hz LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 24 Form F0900041-v1 Conclusion Non-constant loss moduli in the elastic regime Not from machine artefacts Non-trivial microstructure evolution Existence of crackling noise? Need a theoretical model to confirm Further experiments LIGO-G09xxxxx-v1 LIGO Scientific Collaboration 25 Form F0900041-v1