Balance Laws as Test of Gravitational Waveforms
Lavinia Heisenberg

TL;DR
This paper introduces a new method based on balance laws derived from full non-linear general relativity to evaluate the accuracy and consistency of gravitational waveforms, addressing systematic errors in current models.
Contribution
It develops a novel approach to derive and apply balance laws directly from non-linear GR for testing gravitational waveform quality and internal consistency.
Findings
Balance laws can effectively evaluate waveform accuracy.
The method detects weaknesses in approximate waveform models.
Balance laws serve as a consistency check for gravitational waveforms.
Abstract
Gravitational waveforms play a crucial role in comparing observed signals to theoretical predictions. However, obtaining accurate analytical waveforms directly from general relativity remains challenging. Existing methods involve a complex blend of post-Newtonian theory, effective-one-body formalism, numerical relativity, and interpolation, introducing systematic errors. As gravitational wave astronomy advances with new detectors, these errors gain significance, particularly when testing general relativity in the non-linear regime. A recent development proposes a novel approach to address this issue. By deriving precise constraints - or balance laws - directly from full non-linear GR, this method offers a means to evaluate waveform quality, detect template weaknesses, and ensure internal consistency. Before delving into the intricacies of balance laws in full non-linear general…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Relativity and Gravitational Theory
