Collisional Hardening of Compact Binaries in Globular Clusters

Details Collisional Hardening of Compact Binaries in Globular Clusters Collisional Hardening of Compact Binaries in Globular Clusters

2006-09-29

arxiv.org/abs/astro-ph/0609816v1

Mon.Not.Roy.Astron.Soc.373:1188-1194,2006

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures. Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2006.11112.x

We consider essential mechanisms for orbit-shrinkage or "hardening" of compact binaries in globular clusters to the point of Roche-lobe contact and X-ray emission phase, focussing on the process of collisional hardening due to encounters between binaries and single stars in the cluster core. The interplay between this kind of hardening and that due to emission of gravitational radiation produces a characteristic scaling of the orbit-shrinkage time with the single-star binary encounter rate $\gamma$ in the cluster which we introduce, clarify, and explore. We investigate possible effects of this scaling on populations of X-ray binaries in globular clusters within the framework of a simple "toy" scheme for describing the evolution of pre-X-ray binaries in globular clusters. We find the expected qualitative trends sufficiently supported by data on X-ray binaries in galactic globular clusters to encourage us toward a more quantitative study.

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