Using (4+1) split and energy conditions to study the induced matter in 5D Ricc-flat cosmology

Using binary stars to bound the mass of the graviton

Using clocks to determine the entropy of black holes and other space-time singularities

Using curvature invariants for wave extraction in numerical relativity

Using Early Data to Illuminate the Pioneer Anomaly

Using Energy Conditions to Distinguish Brane Models and Study Brane Matter

Using FEMLAB for Gravitational problems: numerical simulations for all

Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit

Using generalized PowerFlux methods to estimate the parameters of periodic gravitational waves

Using global positioning systems to test extensions of General Relativity

Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes

Using long-baseline interferometric gravitational waves detectors for high precision measures of the gravitational acceleration

Using Markov chain Monte Carlo methods for estimating parameters with gravitational radiation data

Using Muonic Hydrogen in Optical Spectroscopy Experiment to Detect Extra Dimensions

Using polarized maser to detect high-frequency relic gravitational waves

Using pulsars to define space-time coordinates

Using Simulation, Comparison and Grid Search To Find all Possible Binary Black Hole Source Parameters For Extreme Mass-Ratio Inspiral Gravitational Wave Signals

Using strictly isospectral unbroken nonrelativistic supersymmetry as a toy model

Using the etalon effect for in-situ balancing of the Advanced Virgo arm cavities

Using the INSPIRAL program to search for gravitational waves from low-mass binary inspiral