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    Rights statement: Copyright 2019 American Institute of Physics. The following article appeared in Physical Review D, 91, 2015 and may be found at https://doi.org/10.1103/PhysRevD.91.082002 This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.

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Detecting beyond-Einstein polarizations of continuous gravitational waves

Research output: Contribution to Journal/Magazine › Journal article › peer-review

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Detecting beyond-Einstein polarizations of continuous gravitational waves. / Isi, M.; Weinstein, Alan J.; Mead, C. et al.
In: Physical Review D, Vol. 91, No. 8, 082002, 01.04.2015.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Isi, M, Weinstein, AJ, Mead, C & Pitkin, M 2015, 'Detecting beyond-Einstein polarizations of continuous gravitational waves', Physical Review D, vol. 91, no. 8, 082002. https://doi.org/10.1103/PhysRevD.91.082002

APA

Isi, M., Weinstein, A. J., Mead, C., & Pitkin, M. (2015). Detecting beyond-Einstein polarizations of continuous gravitational waves. Physical Review D, 91(8), Article 082002. https://doi.org/10.1103/PhysRevD.91.082002

Vancouver

Isi M, Weinstein AJ, Mead C, Pitkin M. Detecting beyond-Einstein polarizations of continuous gravitational waves. Physical Review D. 2015 Apr 1;91(8):082002. doi: 10.1103/PhysRevD.91.082002

Author

Isi, M. ; Weinstein, Alan J. ; Mead, C. et al. / Detecting beyond-Einstein polarizations of continuous gravitational waves. In: Physical Review D. 2015 ; Vol. 91, No. 8.

Bibtex

@article{4a82ae46532c4678bbebe6c106dd2e14,
title = "Detecting beyond-Einstein polarizations of continuous gravitational waves",
abstract = "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.",
keywords = "Experimental tests of gravitational theories, Wave propagation and interactions, Modified theories of gravity, Gravitational wave detectors and experiments",
author = "M. Isi and Weinstein, {Alan J.} and C. Mead and M. Pitkin",
note = "Copyright 2019 American Institute of Physics. The following article appeared in Physical Review D, 91, 2015 and may be found at https://doi.org/10.1103/PhysRevD.91.082002 This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.",
year = "2015",
month = apr,
day = "1",
doi = "10.1103/PhysRevD.91.082002",
language = "English",
volume = "91",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "8",

}

RIS

TY - JOUR

T1 - Detecting beyond-Einstein polarizations of continuous gravitational waves

AU - Isi, M.

AU - Weinstein, Alan J.

AU - Mead, C.

AU - Pitkin, M.

N1 - Copyright 2019 American Institute of Physics. The following article appeared in Physical Review D, 91, 2015 and may be found at https://doi.org/10.1103/PhysRevD.91.082002 This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.

PY - 2015/4/1

Y1 - 2015/4/1

N2 - 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.

AB - 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.

KW - Experimental tests of gravitational theories

KW - Wave propagation and interactions

KW - Modified theories of gravity

KW - Gravitational wave detectors and experiments

U2 - 10.1103/PhysRevD.91.082002

DO - 10.1103/PhysRevD.91.082002

M3 - Journal article

VL - 91

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 8

M1 - 082002

ER -