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Detecting beyond-Einstein polarizations of continuous gravitational waves
The direct detection of gravitational waves with the next-generation detectors, like Advanced LIGO, provides the opportunity to measure deviations from the predictions of general relativity. One such departure would be the existence of alternative polarizations. To measure these, we study a single d...
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Published in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2015-04, Vol.91 (8), Article 082002 |
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container_title | Physical review. D, Particles, fields, gravitation, and cosmology |
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creator | Isi, Maximiliano Weinstein, Alan J. Mead, Carver Pitkin, Matthew |
description | The direct detection of gravitational waves with the next-generation detectors, like Advanced LIGO, provides the opportunity to measure deviations from the predictions of general relativity. One such departure would be the existence of alternative polarizations. To measure these, we study a single detector measurement of a continuous gravitational wave from a triaxial pulsar source. We develop methods to detect signals of any polarization content and distinguish between them in a model-independent way. We present LIGO Science Run 5 sensitivity estimates for 115 pulsars. |
doi_str_mv | 10.1103/PhysRevD.91.082002 |
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subjects | Cosmology Detectors Deviation Gravitation Gravitational waves Mathematical models Polarization Pulsars |
title | Detecting beyond-Einstein polarizations of continuous gravitational waves |
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