Frequency space derivation of linear and non-linear memory gravitational wave signals from eccentric binary orbits
Arpan Hait, Subhendra Mohanty, Suraj Prakash

TL;DR
This paper derives frequency space templates for linear and non-linear gravitational wave memory signals from eccentric binary orbits, using a field-theoretic approach, aiding future GW data analysis.
Contribution
It introduces a novel frequency domain calculation of GW memory signals from eccentric orbits using scattering amplitudes, highlighting new features like log(ω) terms.
Findings
Derived GW waveforms in frequency space for eccentric orbits
Identified log(ω) terms in hyperbolic orbit memory signals
Compared results with existing literature and highlighted novel features
Abstract
The memory effect in gravitational wave (GW) signals is the phenomenon, wherein the relative position of two inertial GW detectors undergoes a permanent displacement owing to the passage of GWs through them. Measurement of the memory signal is an important target for future observations as it establishes a connection between observations with field-theoretic results like the soft-graviton theorems. Theoretically, the memory signal is predicted at the leading order quadrupole formula for sources like binaries in hyperbolic orbits. This can be in the realm of observations by Advanced LIGO, Einstein-Telescope, or LISA for black-holes with masses ) scattered by the super-massive black-hole at the galactic center. Apart from the direct memory component there is a non-linear memory signal in the secondary GW emitted from the primary GW chirp-signals emitted by…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Geophysics and Sensor Technology
