Embodiments of the present invention may be generally related to methods, devices, and systems which measure a gravitational field. The methods and devices may utilize an interferometer to measure tilt of a pendulum, where the tilt of the pendulum is due to a gravitational force associated with a target object. In some embodiments, the interferometer may be a displaced, even parity, Sagnac interferometer. Additionally, the interferometer may be operated in the inverse weak value domain. In some embodiments, the pendulum and interferometric readout may measure relative gravitational fields that are transverse to Earth's gravitational field. In at least some embodiments, methods and devices may have shot noise limited sensitivity sufficient to detect one kilogram 25 meters away and may have a 1 nGal resolution after mere seconds of integration. Embodiments disclosed may be used to gravitationally map density fluctuations in a target object, including the human body.

A device and method for improved geodetic and seismic measurements are disclosed. The device comprises a triaxial accelerometer assembly, mounted to a reference structure, having full scale ranges greater than +/1 G on three orthogonal axes and a mechanism for rotating the triaxial accelerometer assembly on the reference structure. The triaxial acceleration assembly is calibrated with an internal alignment matrix such that measurements of Earth's gravity vector are rotationally invariant with respect to the direction of Earth's 1 G static gravity vector irrespective of the orientation of the triaxial assembly on the reference structure. In-situ calibrations are performed by rotating the axes of the triaxial acceleration assembly in the direction of Earth's static gravity vector. Drift of the triaxial accelerometer assembly is compensated for by measuring changes in the values of the invariant static gravity vector for each axis and correcting for the drift with new calibration coefficients.

A device and method for improved geodetic and seismic measurements are disclosed. The device comprises a triaxial accelerometer assembly, mounted to a reference structure, having full scale ranges greater than +/1 G on three orthogonal axes and a mechanism for rotating the triaxial accelerometer assembly on the reference structure. The triaxial acceleration assembly is calibrated with an internal alignment matrix such that measurements of Earth's gravity vector are rotationally invariant with respect to the direction of Earth's 1 G static gravity vector irrespective of the orientation of the triaxial assembly on the reference structure. In-situ calibrations are performed by rotating the axes of the triaxial acceleration assembly in the direction of Earth's static gravity vector. Drift of the triaxial accelerometer assembly is compensated for by measuring changes in the values of the invariant static gravity vector for each axis and correcting for the drift with new calibration coefficients.

Aspects of the present disclosure relate to testing apparatus and methods for measuring forces between objects. The apparatus and methods are used to detect a change in the local gravitational constant resulting from non-Newtonian effects of General Relativity and/or a novel radial dilation influence. Detection is facilitated by measuring a force difference between a stationary state and a spinning state of attractive forces between objects. The apparatus and methods are used to detect a change in electromechanical influence of forces due to the Barnett affect and other anomalous electromagnetic force contributors. A testing apparatus includes a central target arrangement. The central target arrangement includes a pair of masses, and a target coupled to the pair of masses. The testing apparatus includes a detector configured to recognize the target, and a first rotatable mass. The first rotatable mass is supported independently of the target and the pair of target masses.

Aspects of the present disclosure relate to testing apparatus and methods for measuring forces between objects. The apparatus and methods are used to detect a change in the local gravitational constant resulting from non-Newtonian effects of General Relativity and/or a novel radial dilation influence. Detection is facilitated by measuring a force difference between a stationary state and a spinning state of attractive forces between objects. The apparatus and methods are used to detect a change in electromechanical influence of forces due to the Barnett affect and other anomalous electromagnetic force contributors. A testing apparatus includes a central target arrangement. The central target arrangement includes a pair of masses, and a target coupled to the pair of masses. The testing apparatus includes a detector configured to recognize the target, and a first rotatable mass. The first rotatable mass is supported independently of the target and the pair of target masses.