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- W1928562011 abstract "or small mass ratio for its formulation. This case should encompass the inspiral and possibly the plunge and merger phases of binaries with otherwise general parameters (e.g., mass ratio and relative velocity) though more investigation is needed to substantiate it. In the second part, we discuss how the mass ratio can be treated as a perturbation parameter in the post-Newtonian eective" @default.
- W1928562011 created "2016-06-24" @default.
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- W1928562011 date "2009-06-04" @default.
- W1928562011 modified "2023-09-27" @default.
- W1928562011 title "New analytical methods for gravitational radiation and reaction in binaries with arbitrary mass ratio and relative velocity" @default.
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