1 Introduction

 1.1 Overview of BH-NS binaries
 1.2 Tidal problem around a BH: Effects of BH spin and the NS EOS
 1.3 Why is the merger of BH-NS binaries important?
 1.4 General relativistic study of BH-NS binaries in quasi-equilibrium states
 1.5 Non-relativistic simulation for the merger
 1.6 Stable mass transfer occurs or not
 1.7 General relativistic study of late inspiral and merger
 1.8 Outline and notation

  Go to previous page Go up Go to next page