A test of Lorentz invariance using a torsion pendulum
Lorentz invariance test using bar magnet on torsion fiber, analyzing preferred reference frame in space assuming earth velocity coupled to electron spin through specific term
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Lorentz invariance test using bar magnet on torsion fiber, analyzing preferred reference frame in space assuming earth velocity coupled to electron spin through specific term
Invariant set existence inside submanifold convex to flow established from vector field properties on submanifold boundary
Compton-Getting effect for cosmic ray particles and photons and Lorentz-invariance of distribution functions, discussing thermal background radiation, proton spectra, etc
Cramer-Rao efficiencies of best linear invariant estimators, using Weibull distribution in model for survival populations connected with life testing
Invariance conditions and state transition matrix of linear systems
Turbulent chemical reactions invariance preservation for zero diffusivity
Determining optimal time-invariant output feedback controllers for linear dynamic systems
Input-output properties of feedback systems based on linear time invariate systems
Developmental history of adiabatic invariance including contributors to radiation energy transfer and celestial mechanics concepts
Feedback compensator for linear-time invariant system insensitive to parameter variations
Empirical approach to third-invariant violation for radial diffusion of outer zone electrons
Stability of linear time invariant discrete systems including multiple poles
Flows on 3-manifolds near isolated invariant sets
Closed invariant sets of smooth flow on compact manifold involving homoclinic or heteroclinic point theory of Poincare
Thermoelastic stability as function of thermodynamic properties of elastic materials, applying invariance principle to dynamical systems on Banach space
Lorentz invariant theory for relativistic gravity testing, deriving conservation laws and parameter constraints from parametrized post-Newtonian equations of motion
Theoretical work designed to bridge the gap between celestial mechanics and the motion of charged particles in magnetic fields is presented. Attempts are made to devise a simple uninvolved method to solve adiabatic invariant motion problems. The method is illustrated by solving a problem involving the motion of a slowly perturbed harmonic oscillator.
The development of an invariant model designed expressly for the computation of shear flows is discussed. The model for incompressible layers seeks a second-order closure of the equations for the mean and fluctuating fields. The development of a method for computing the behavior of shear layers in compressible forces is described. The complexity of the analysis is restrained by limiting the consideration to a flat plate boundary layer where the mean pressure can be taken to be constant.