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--- ondesgravitationnelles [2023/03/08 15:01] – daniele.steer
+++ ondesgravitationnelles [2023/03/08 15:08] (current) – daniele.steer
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         * developments to higher PN, with spins and tidal effects, all needed for future detectors especially LISA. Computation of both conservative equations of motion plus effects of gravitational radiation reaction. Computation of waveforms (modes, especially the dominant quadrupole mode 22) and flux balance equations for secular evolution of the binary.
         * Inclusion of eccentricity to higher PN, unbound hyperbolic orbits etc. Relation between unbound and bound (elliptical) orbits including tail effects.
-        * Effective Field theory techniques, amplitudes. These, together with ``classical'' PN approach, will probably develop together. Develop dictionary between the two approaches. [e.g. Asymptotic symmetries: synergy between these symmetries at null infinity and the waveform. Important for non-linear- and spin- memory effects + tails. ]
+        * Effective Field theory techniques, amplitudes. These, together with ``classical'' PN approach, will probably develop together. Develop dictionary between the two approaches. [e.g. Analysis of asymptotic symmetries: synergy between these symmetries at null infinity and the waveform. Important for non-linear- and spin- memory effects + tails. ]
         * Effective one body: under-developed in France, but crucial to match inspiral to ringdown waveforms and for practical implementation of data analysis.
         * Numerical relativity. Tremendous progress over the last decades. A field which is under-developed in France. Connection with the community working of neutron star equations of state.