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1 Introduction
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2 The stellar system
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3 Tidal interaction of a white dwarf with the central black hole
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4 Gravitational wave emission/non-linear effects, characteristic time scales
and mode amplitude limitation
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5 Conditions for safe circularisation or tidal disruption
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6 The rate of tidal capture by the black hole
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7 Probability of detection of a source of gravitational radiation
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8 Discussion
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Appendix A: Conditions for the transition from stochastic instability
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References
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