Details
Original language | English |
---|---|
Article number | 124020 |
Journal | Physical Review D |
Volume | 97 |
Issue number | 12 |
Publication status | Published - 15 Jun 2018 |
Externally published | Yes |
Abstract
In the general theory of relativity, gravitational waves have two possible polarizations, which are transverse and traceless with helicity ±2. Some alternative theories contain additional helicity 0 and helicity ±1 polarization modes. Here, we consider a hypothetical "pure vector" theory in which gravitational waves have only two possible polarizations, with helicity ±1. We show that if these polarizations are allowed to rotate as the wave propagates, then for certain source locations on the sky, the strain outputs of three ideal interferometric gravitational wave detectors can exactly reproduce the strain outputs predicted by general relativity.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Physics and Astronomy (miscellaneous)
Cite this
- Standard
- Harvard
- Apa
- Vancouver
- BibTeX
- RIS
In: Physical Review D, Vol. 97, No. 12, 124020, 15.06.2018.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Can a pure vector gravitational wave mimic a pure tensor one?
AU - Allen, Bruce
N1 - Publisher Copyright: © 2018 authors. Published by the American Physical Society.
PY - 2018/6/15
Y1 - 2018/6/15
N2 - In the general theory of relativity, gravitational waves have two possible polarizations, which are transverse and traceless with helicity ±2. Some alternative theories contain additional helicity 0 and helicity ±1 polarization modes. Here, we consider a hypothetical "pure vector" theory in which gravitational waves have only two possible polarizations, with helicity ±1. We show that if these polarizations are allowed to rotate as the wave propagates, then for certain source locations on the sky, the strain outputs of three ideal interferometric gravitational wave detectors can exactly reproduce the strain outputs predicted by general relativity.
AB - In the general theory of relativity, gravitational waves have two possible polarizations, which are transverse and traceless with helicity ±2. Some alternative theories contain additional helicity 0 and helicity ±1 polarization modes. Here, we consider a hypothetical "pure vector" theory in which gravitational waves have only two possible polarizations, with helicity ±1. We show that if these polarizations are allowed to rotate as the wave propagates, then for certain source locations on the sky, the strain outputs of three ideal interferometric gravitational wave detectors can exactly reproduce the strain outputs predicted by general relativity.
UR - http://www.scopus.com/inward/record.url?scp=85049524689&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.97.124020
DO - 10.1103/PhysRevD.97.124020
M3 - Article
AN - SCOPUS:85049524689
VL - 97
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 12
M1 - 124020
ER -