LISA sources in globular clusters

M. J. Benacquista*, S. Portegies Zwart, F. A. Rasio

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

24 Scopus citations


Globular clusters house a population of compact binaries that will be interesting gravitational wave sources for LISA. We provide estimates for the numbers of sources of several categories and discuss the sensitivity of LISA to detecting these sources. The estimated total number of detectable sources ranges from ∼ 10 to ∼ 10 3 - Hubble Fellow. with gravitational wave frequencies above 1 mHz. These sources are typically undetectable by any other means and thus offer an opportunity for doing true gravitational-wave astronomy. The detection of these sources would provide information about both binary star evolution and the dynamics of globular clusters.

Original languageEnglish (US)
Pages (from-to)4025-4031
Number of pages7
JournalClassical and Quantum Gravity
Issue number19
StatePublished - Oct 7 2001

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)


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