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Mechanical Loss

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lightbulbAbout this topic
Mechanical loss refers to the energy dissipation in a mechanical system due to non-conservative forces, such as friction, damping, or material deformation. It quantifies the reduction in mechanical energy as a system undergoes motion, impacting efficiency and performance in various engineering applications.
lightbulbAbout this topic
Mechanical loss refers to the energy dissipation in a mechanical system due to non-conservative forces, such as friction, damping, or material deformation. It quantifies the reduction in mechanical energy as a system undergoes motion, impacting efficiency and performance in various engineering applications.

Key research themes

1. What are the physical mechanisms and modeling approaches for mechanical losses in turbomachines and gear systems?

This research theme focuses on identifying, understanding, and modeling the fundamental physical origins of mechanical losses in turbomachines and mechanical transmissions such as planetary gearsets. It covers various sources of mechanical loss, including fluid viscous effects, frictional interactions, and energy dissipation mechanisms at operating conditions. Understanding these mechanisms is critical to improving the performance and efficiency of turbomachinery and gear transmissions, which have wide applicability in aerospace, automotive, and energy sectors.

Key finding: This paper identifies key physical loss sources in turbomachines arising from entropy increases due to viscous boundary layers, mixing processes, shock waves, and heat transfer. It emphasizes that while some losses, such as... Read more
Key finding: Introduces an analytical mechanical power loss model for planetary gearsets separating unloaded losses (fluid churning, fluid shear in gaps, stator-rotor fluid shear) and loaded losses (gear mesh friction, bearing, seal... Read more
Key finding: Combines analytical and empirical descriptions of rotor-fluid interaction losses in turbocharger rotors to identify parameters affecting mechanical losses and proposes geometric design modifications. Experimental verification... Read more

2. How do mechanical stresses influence loss components, particularly excess loss, in magnetic electrical steel materials?

This area investigates how the application of mechanical stress affects magnetic losses in electrical steels, specifically focusing on the excess loss component as derived from statistical loss theory. Understanding this stress-dependence is important for the design and performance prediction of electrical machines, where mechanical forces from shrink-fitting, magnetic and centrifugal loads are significant. Precise modeling of magnetic losses under realistic stress states helps improve efficiency and reliability of electric machines.

Key finding: This study experimentally demonstrates a strong correlation between hysteresis loss variations under different compressive and tensile stresses and the excess loss component in electrical steel sheets. Using a modified single... Read more
Key finding: Utilizes machine learning, specifically random forest algorithms, to accurately predict energy losses in nonoriented electrical steel materials over varying frequencies and induction levels, including rotational flux... Read more
Key finding: Develops an area-based model to approximate core sheet losses in electrical steel materials considering the degradation effects caused by mechanical punching (guillotine cutting) and laser cutting. By linking material... Read more

3. How can mechanical loss and efficiency of electrical machines be modeled and characterized across operational regimes including torque, speed, and frequency?

This theme addresses the modeling and characterization of mechanical and magnetic losses in electrical machines, employing analytical, numerical, and data-driven methods to capture loss variations with respect to machine operating conditions such as torque and rotor speed. Improved loss function modeling enhances the construction and analysis of efficiency maps critical for machine design, control, and performance optimization, including in emerging high-performance applications such as electric traction and cryogenic conditions.

Key finding: Presents a novel approach modeling machine losses as sums of terms proportional to torque and speed powers (T^m ω^n), enabling decomposition of stator and rotor copper, iron, and magnet losses across operating points. The... Read more
Key finding: Demonstrates that heat-treated ion-beam sputtered (IBS) hafnium dioxide (HfO2) coatings exhibit mechanical loss values below amorphous tantala below ~100 K, with loss dependent on heat treatment and onset of crystallization.... Read more
Key finding: Shows that doping tantala (Ta2O5) with titania (TiO2) reduces mechanical loss and hence thermal noise in multilayer SiO2/Ta2O5 coatings used for advanced gravitational-wave detectors. Coatings with titania doping maintain low... Read more
Key finding: Provides direct experimental observation of broadband thermal noise arising from silica/tantala coatings on high-sensitivity Fabry-Perot interferometers, confirming predictions from indirect mechanical loss measurements. The... Read more

All papers in Mechanical Loss

The worldwide effort to detect gravitational-waves uses long baseline laser interferometry. The optics in the interferometers use ion-beam deposited multilayer dielectric coatings, for high reflectivity. In addition, the coatings must... more
We have investigated by spectroscopic ellipsometry (SE) the optical properties (190 - 1700 nm) of uniform, amorphous thin films of Ta2O5 and Nb2O5 as a function of the annealing temperature and after so-called "doping" with Ti... more
.Gy abstractAbstract Current interferometric gravitational wave detectors use test masses with mirror coatings formed from multiple layers of dielectric materials, most commonly alternating layers of (silica) and (tantala). However,... more
We have investigated by spectroscopic ellipsometry (SE) the optical properties (190 - 1700 nm) of uniform, amorphous thin films of Ta2O5 and Nb2O5 as a function of the annealing temperature and after so-called "doping" with Ti... more
The understanding of how the structure rules the several properties that distinguish amorphous solids from crystals is important for a technological progress, regarding several applications. The random network structure that characterises... more
We have directly observed broadband thermal noise in silica/tantala coatings in a high-sensitivity Fabry-Perot interferometer. Our result agrees well with the prediction based on indirect, ring-down measurements of coating mechanical... more
Understanding the local atomic order in amorphous thin film coatings and how it relates to macroscopic performance factors, such as mechanical loss, provides an important path towards enabling the accelerated discovery and development of... more
We present the results of mechanical characterizations of many different high-quality optical coatings made of ion-beam-sputtered titania-doped tantala and silica, developed originally for interferometric gravitational-wave detectors. Our... more
In recent years an increasing number of devices and experiments are shown to be limited by mechanical thermal noise. In particular sub-Hertz laser frequency stabilization and gravitational wave detectors, that are able to measure... more
Gravitational waves are detected using resonant optical cavity interferometers. The mirror coatings’ inherent thermal noise and photon scattering limit sensitivity. Crystals within the reflective coating may be responsible for either or... more
Amorphous SiO2 thin films are one of the two components of the highly reflective mirror coatings of gravitational-wave detectors. For this study, layers of amorphous SiO2 on crystalline Si substrates were produced by ion-beam sputtering... more
Amorphous SiO2 thin films are one of the two components of the highly reflective mirror coatings of gravitational-wave detectors. For this study, layers of amorphous SiO2 on crystalline Si substrates were produced by ion-beam sputtering... more
Brownian thermal noise associated with highly reflective coatings is a fundamental limit for several precision experiments, including gravitational-wave detectors. Research is currently ongoing to find coatings with low thermal noise that... more
A new method of probing mechanical losses and comparing the corresponding deposition processes of metallic and dielectric coatings in 1-100 MHz frequency range and cryogenic temperatures is presented. The method is based on the use of... more
Thermal noise is a limiting factor in many high-precision optical experiments. A search is underway for novel optical materials with reduced thermal noise. One such pair of materials, gallium arsenide and aluminum-alloyed gallium arsenide... more
The aim of the work was to determine the phenomena of internal friction (mechanical losses) occurring in ferroelectric-ferromagnetic composites created based on PZT-type ferroelectric powder and ferrite. The composites were obtained using... more
We have compiled measurements of the mechanical loss in fused silica from samples spanning a wide range of geometries and resonant frequency in order to model the known variation of the loss with frequency and surface-to-volume ratio.... more
We have measured the mechanical loss of a dielectric multilayer reflective coating (ion-beam sputtered SiO2 and Ta2O5) in cooled mirrors. The loss was nearly independent of the temperature (4 K ∼ 300 K), frequency, optical loss, and... more
Amorphous SiO2 thin films are one of the two components of the highly reflective mirror coatings of gravitational-wave detectors. For this study, layers of amorphous SiO2 on crystalline Si substrates were produced by ion-beam sputtering... more
Complex multilayer thin film filters for optical applications have been designed, prepared and characterized in this work. E-beam reactive evaporation technique has been used as a deposition process. In the first stage, optimized... more
We have directly observed broadband thermal noise in silica/tantala coatings in a high-sensitivity Fabry-Perot interferometer. Our result agrees well with the prediction based on indirect, ring-down measurements of coating mechanical... more
Understanding the local atomic order in amorphous thin film coatings and how it relates to macroscopic performance factors, such as mechanical loss, provides an important path towards enabling the accelerated discovery and development of... more
We report on the effects of an electrical charge on mechanical loss of a fused silica disk. A degradation of Q was seen that correlated with charge on the surface of the sample. We examine a number of models for charge damping, including... more
Gy abstractAbstract Current interferometric gravitational wave detectors use test masses with mirror coatings formed from multiple layers of dielectric materials, most commonly alternating layers of (silica) and (tantala). However,... more
Complex multilayer thin film filters for optical applications have been designed, prepared and characterized in this work. E-beam reactive evaporation technique has been used as a deposition process. In the first stage, optimized... more
Alex Amato,∗ Silvana Terreni, Massimo Granata, Christophe Michel, Benoit Sassolas, Laurent Pinard, Maurizio Canepa, and Gianpietro Cagnoli Laboratoire des Matériaux Avancés, CNRS/IN2P3, F-69622 Villeurbanne (FR). OPTMATLAB, Dipartimento... more
Gravitational waves are a prediction of Einstein's General Theory of Relativity. Astrophysical events like supernova and binary neutron star inspirals are predicted to create potentially detectable waves. The Laser Interferometer... more
The sensitivity of current and planned gravitational wave interferometric detectors is limited, in the most critical frequency region around 100 Hz, by a combination of quantum noise and thermal noise. The latter is dominated by Brownian... more
We present the results of mechanical characterizations of many different high-quality optical coatings made of ion-beam-sputtered titania-doped tantala and silica, developed originally for interferometric gravitational-wave detectors. Our... more
To support the research effort for the third generation of gravitational wave interferometers, the Laboratoire des Matériaux Avancés (LMA) at Lyon, France has developed a new cryogenic facility to characterize optics at low temperature.... more
Gravitational-wave detectors such as Virgo and the laser interferometric gravitational-wave observatory (LIGO) use a long-baseline Michelson interferometer with Fabry-Perot cavities in the arms to search for gravitational waves. The... more
Gravitational waves are detected using resonant optical cavity interferometers. The mirror coatings' inherent thermal noise and photon scattering limit sensitivity. Crystals within the reflective coating may be responsible for either or... more
Optical coatings formed from amorphous oxide thin films have many applications in precision measurements. The Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) and Advanced Virgo use coatings of SiO 2 (silica) and TiO 2... more
Light scattered by amorphous thin-film optical coatings limits the sensitivity of interferometric gravitational-wave detectors. We describe an imaging scatterometer to assess the role that crystal growth during annealing plays in this... more
Optical coatings formed from amorphous oxide thin films have many applications in precision measurements. The Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) and Advanced Virgo use coatings of SiO 2 (silica) and TiO 2... more
V. Pierro, 2, ∗ V. Fiumara, 2 F. Chiadini, 2 V. Granata, 2 O. Durante, 2 J. Neilson, 2 C. Di Giorgio, 2 R. Fittipaldi, 2 G. Carapella, 2 F. Bobba, 2 M. Principe, 2, 7 and I. M. Pinto 2, 7 Dip. di Ingegneria, DING, Universitá del Sannio,... more
In this work we analyze coatings for gravitational wave detector mirrors obtained by sequencing dielectric layers, with fixed thicknesses, made of three different materials (ternary sequences). Two materials are chosen non-dissipative,... more
We investigated elastic loss in GaAs/AlGaAs multilayers to help determine the suitability of these coatings for future gravitational wave detectors. We measured large (≈ 70-mm diameter) substrate-transferred crystalline coating samples... more
Large optical components (diameter 350 mm), having extremely low loss at 1064 nm, are needed for the large-scale Michelson-type interferometer VIRGO. Today, ion beam sputtering is the only deposition technique able to produce optical... more
Large optical components (diameter 350 mm), having extremely low loss at 1064 nm, are needed for the large-scale Michelson-type interferometer VIRGO. Today, ion beam sputtering is the only deposition technique able to produce optical... more
We present the results of the study on the thermal conductivity of different thin film materials produced by conventional thermal evaporation. The main features of the thermal pulse method employed for the measurement of the thermal... more
The sensitivity of current and planned gravitational wave interferometric detectors is limited, in the most critical frequency region around 100 Hz, by a combination of quantum noise and thermal noise. The latter is dominated by Brownian... more
Light scattered by amorphous thin-film optical coatings limits the sensitivity of interferometric gravitational-wave detectors. We describe an imaging scatterometer to assess the role that crystal growth during annealing plays in this... more
Objective: to investigate the ideal combination of materials for tooth prosthesis. Methods: Due to achieving fast results, the axisymmetrical finite element method (FEM) was used to compare stress distribution in a maxillary second... more
The limit sensitivity of interferometric gravitational wave antennas is set by the thermal noise in the dielectric mirror coatings. These are currently made of alternating quarter-wavelength high/low index material layers with low... more
The worldwide effort to detect gravitational-waves uses long baseline laser interferometry. The optics in the interferometers use ion-beam deposited multilayer dielectric coatings, for high reflectivity. In addition, the coatings must... more
Planned, cryogenic gravitational-wave detectors will require improved coatings with a strain thermal noise reduced by a factor of 25 compared to Advanced LIGO. In this article, we present investigations of HfO2 doped with SiO2 as a new... more
Planned, cryogenic gravitational-wave detectors will require improved coatings with a strain thermal noise reduced by a factor of 25 compared to Advanced LIGO. In this article, we present investigations of HfO2 doped with SiO2 as a new... more
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