[1209.5731] Extreme-mass-ratio bursts from the Galactic Centre

Authors: Christopher P. L. Berry, Jonathan R. Gair

Date: 25 Sep 2012

Abstract: An extreme-mass-ratio burst (EMRB) is a gravitational wave signal emitted when a compact object passes through periapsis on a highly eccentric orbit about a much more massive body, in our case a stellar mass object about the 4.31 \times 10ˆ6 M_sol massive black hole (MBH) in the Galactic Centre. We investigate how EMRBs could constrain the parameters of the Galaxy's MBH. EMRBs should be detectable if the periapsis is r_p < 65 r_g for a \mu = 10 M_sol orbiting object, where r_g = GM/cˆ2 is the gravitational radius. The signal-to-noise ratio \rho scales like log(\rho) = -2.7 log(r_p/r_g) + log(\mu/M_sol) + 4.9. For periapses smaller than ~ 10 r_g, EMRBs can be informative, providing good constraints on both the MBH's mass and spin.

abs pdf

Sep 28, 2012

1209.5731 (/preprints)
2012-09-28, 09:53 [edit]

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© M. Vallisneri 2012 — last modified on 2010/01/29

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