221870
20180913063916.0
0021-3640
10.1134/S0021364016100040
doi
000381661200003
ISI
ARTICLE
On constraining the speed of gravitational waves following GW150914
New York
2016
Springer Verlag
2016
3
Journal Articles
We point out that the observed time delay between the detection of the signal at the Hanford and Livingston LIGO sites from the gravitational wave event GW150914 places an upper bound on the speed of propagation of gravitational waves, c (gw) ae(2) 1.7 in the units of speed of light. Combined with the lower bound from the absence of gravitational Cherenkov losses by cosmic rays that rules out most of subluminal velocities, this gives a model-independent double-sided constraint 1 ae(2) c (gw) ae(2) 1.7. We compare this result to model-specific constraints from pulsar timing and cosmology.
Blas, D.
CERN, Dept Theoret Phys, CH-1211 Geneva, Switzerland
184736
244357
Ivanov, M. M.
Ecole Polytech Fed Lausanne, LPPC, IPHYS, FSB, CH-1015 Lausanne, Switzerland
242812
248971
Sawicki, I.
Univ Geneva, Dept Phys Theor, Quai E Ansermet 24, CH-1211 Geneva, Switzerland
Sibiryakov, S.
CERN, Dept Theoret Phys, CH-1211 Geneva, Switzerland
184235
244356
624-626
10
Jetp Letters
103
LPPC
252301
U10869
oai:infoscience.tind.io:221870
article
SB
126010
EPFL-ARTICLE-221870
EPFL
PUBLISHED
REVIEWED
ARTICLE