Gravitational Waves from an Axi-symmetric Source in the Nonsymmetric Grav. Theory
J. W. Moffat, D. C. Tatarski

TL;DR
This paper investigates gravitational waves in an axi-symmetric Nonsymmetric Gravitation Theory (NGT), deriving solutions and analyzing mass behavior and energy flux during radiation in such systems.
Contribution
It provides exact solutions for axi-symmetric NGT systems and analyzes how mass and energy flux behave during gravitational radiation, extending understanding beyond spherical symmetry.
Findings
Mass remains constant only in static systems
Mass decreases monotonically when the system radiates
Energy flux associated with waves is positive
Abstract
We examine gravitational waves in an isolated axi--symmetric reflexion symmetric NGT system. The structure of the vacuum field equations is analyzed and the exact solutions for the field variables in the metric tensor are found in the form of expansions in powers of a radial coordinate. We find that in the NGT axially symmetric case the mass of the system remains constant only if the system is static (as it necessarily is in the case of spherical symmetry). If the system radiates, then the mass decreases monotonically and the energy flux associated with waves is positive.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · Geophysics and Gravity Measurements
