Abstract
We present an extension of a previously suggested test of all modified theories of gravity that would reproduce MOND at low accelerations. In a class of models, called "dark matter emulators", gravitational waves and other particles couple to different metrics. This leads to a detectable time lag between their detection at Earth from the same source. We calculate this time lag numerically for any event that occurs in our galaxy up to 400 kpc, and present a graph of this possible time lag. This suggests that, gravitational wave observers might have to consider the possibility of extending their analysis to non-coincident gravitational and electromagnetic signals, and the graph that we present might be a useful guideline for this effort.
Original language | English |
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Pages (from-to) | 291-295 |
Number of pages | 5 |
Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
Volume | 701 |
Issue number | 3 |
DOIs | |
Publication status | Published - 11 Jul 2011 |
Externally published | Yes |
Funding
I am grateful to Richard Woodard and Shantanu Desai for stimulating discussions. I would like to thank Szabi Marka for suggesting this problem to me. I also would like to thank Hongsheng Zhao and Anatoly Klypin for illuminating comments and discussions. I am also grateful for the hospitality of the Physics Department of Koç University. This work was partially supported by DFG-Research Training Group “Quantum and Gravitational Fields” GRK 1523/1 , by Marie Curie Grant IRG-247803 .
Funders | Funder number |
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DFG-Research | GRK 1523/1 |
Seventh Framework Programme | 247803 |
Marie Curie | IRG-247803 |
Keywords
- Cold dark matter
- Gravitational waves
- MOND
- Modified gravity models