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2020

Gravitational wave background from extreme mass ratio inspirals

Bonetti, Matteo, Sesana, Alberto

Understand

Extreme mass ratio inspirals (EMRIs), i.e.

binary systems comprised by a compact stellar-mass object orbiting a massive black hole, are expected to be among the primary gravitational wave (GW) sources for the forthcoming LISA mission.
The astrophysical processes leading to the formation of such systems still remain poorly understood, resulting into large uncertainties in the predicted cosmic rate of these sources, spanning at least three orders of magnitude.
As LISA can individually resolve mostly EMRIs up to $z\gtrsim1$, the ensemble of signals below its detection threshold will add up incoherently forming an unresolved confusion noise, which can be formally described as a stochastic background.

Built on

E. Bortolas and M. Mapelli, MNRAS 485
Original
1902
Earlier work this paper cites.
D. Gerosa, S. Ma, K. W. K. Wong, E. Berti, R. O’Shaughnessy, Y. Chen, and K. Belczynski, Phys. Rev. D 99
Original
1902
Earlier work this paper cites.
A. Pound, B. Wardell, N. Warburton, and J. Miller, Phys. Rev. Lett. 124
Original
1908
Earlier work this paper cites.
E. Gallo and A. Sesana, ApJ 883
Original
1909
Earlier work this paper cites.
J. R. Gair, C. Tang, and M. Volonteri, Phys. Rev. D 81
Original
1921
Earlier work this paper cites.
P. C. Peters and J. Mathews, Physical Review 131
1963
Earlier work this paper cites.
P. C. Peters, Physical Review 136
1964
Earlier work this paper cites.
M. J. Rees, Nature 333
1988
Earlier work this paper cites.
J. G. Hills, Nature 331
1988
Earlier work this paper cites.
D. Hils and P. L. Bender, ApJ 445
1995
Earlier work this paper cites.
S. Sigurdsson and M. J. Rees, MNRAS 284
1997
Earlier work this paper cites.
L. S. Finn and K. S. Thorne, Phys. Rev. D 62
2000
Earlier work this paper cites.
S. L. Larson, W. A. Hiscock, and R. W. Hellings, Phys. Rev. D 62
2000
Earlier work this paper cites.
G. Nelemans, L. R. Yungelson, and S. F. Portegies Zwart, A&A 375
2001
Earlier work this paper cites.
E. S. Phinney, arXiv e-prints , astro-ph/0108028 (2001), arXiv:astro-ph/0108028 [astro-ph]
2001
Earlier work this paper cites.
P. Madau and M. J. Rees, ApJ 551
2001
Earlier work this paper cites.
B. J. Kavanagh, D. A. Nichols, G. Bertone, and D. Gaggero, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
Y. Levin, arXiv e-prints , astro-ph/0307084 (2003), arXiv:astro-ph/0307084 [astro-ph]
2003
Earlier work this paper cites.
M. C. Miller, M. Freitag, D. P. Hamilton, and V. M. Lauburg, ApJ 631
2005
Earlier work this paper cites.
C. Hopman and T. Alexander, ApJ 629
2005
Earlier work this paper cites.
A. Sesana, F. Haardt, P. Madau, and M. Volonteri, ApJ 623
2005
Earlier work this paper cites.