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2016

Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter

Muñoz, Julian B., Kovetz, Ely D., Dai, Liang et al.

Understand

The possibility that part of the dark matter is made of massive compact halo objects (MACHOs) remains poorly constrained over a wide range of masses, and especially in the $20-100\, M_\odot$ window.

We show that strong gravitational lensing of extragalactic fast radio bursts (FRBs) by MACHOs of masses larger than $\sim20\,M_\odot$ would result in repeated FRBs with an observable time delay.
Strong lensing of an FRB by a lens of mass $M_L$ induces two images, separated by a typical time delay $\sim$ few $\times(M_L/30\, M_\odot)$ milliseconds.
Considering the expected FRB detection rate by upcoming experiments, such as CHIME, of $10^4$ FRBs per year, we should observe from tens to hundreds of repeated bursts yearly, if MACHOs in this window make up all the dark matter.

Built on

B. J. Carr and S. W. Hawking, Mon. Not. Roy. Astron. Soc. 168, 399 (1974)
1974
Earlier work this paper cites.
B. J. Carr, Astrophys. J. 201, 1 (1975)
1975
Earlier work this paper cites.
K. Griest, Astrophys. J. 366
1991
Earlier work this paper cites.
A. Gould, Astrophys. J. 386
1992
Earlier work this paper cites.
R. A. Allsman et al
2001
Earlier work this paper cites.
B. M. S. Hansen and M. Lyutikov, Mon. Not. Roy. Astron. Soc. 322
2001
Earlier work this paper cites.
S. Cole et al
2001
Earlier work this paper cites.
R. Takahashi and T. Nakamura, Astrophys. J. 595
2003
Earlier work this paper cites.
A. M. Hopkins and J. F. Beacom, Astrophys. J. 651
2006
Earlier work this paper cites.
P. Tisserand et al
2007
Earlier work this paper cites.
D. R. Lorimer, M. Bailes, M. A. McLaughlin, D. J. Narkevic and F. Crawford, Science 318
Original
2007
Earlier work this paper cites.
M. A. W. Verheijen, T. A. Oosterloo, W. A. van Cappellen, L. Bakker, M. V. Ivashina and J. M. van der Hulst, AIP Conf. Proc. 1035
Original
2008
Earlier work this paper cites.
D. P. Quinn, M. I. Wilkinson, M. J. Irwin, J. Marshall, A. Koch and V. Belokurov, Mon. Not. Roy. Astron. Soc. 396
Original
2009
Earlier work this paper cites.