1 A formulation for the long-term evolution of EMRIs with linear order conservative self-force Takahiro Tanaka (Kyoto university) Gravitational waves in.

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1 A formulation for the long-term evolution of EMRIs with linear order conservative self-force Takahiro Tanaka (Kyoto university) Gravitational waves in collaboration with R. Fujita, S. Isoyama, A. Le Tiec, H. Nakano, N. Sago

2 Order of  in wave form Energy balance argument is sufficient. Wave form for quasi-circular orbits, for example. leading order ( O (  -1 ) phase) linear perturbation only up to here next leading order ( O (  ) phase)

3 Particle’s trajectory h~  / r Perturbation is everywhere small outside the world tube “tube radius” >>  Unavoidable ambiguity in the perturbed trajectory of O (  ) “Self-force is gauge dependent” Source trajectory has unnecessary information. While, “long term orbital evolution is gauge invariant” There must be a concise description keeping only the gauge invariant information Gauge invariance

4 H (0) =u 2 /2, and hence X  is  and X i ( i =1,2,3 ) are all constant for background geodesics. Use of canonical transformation It is natural to change the variables to the constants of motion in the background and their conjugates X . Generating fn: Interaction Hamiltonian …

5 Radiation reaction to the constants of motion “retarded” = “radiative” + ”symmetric” Geodesic preserving transformation (Mino transformation): t → -t,  → - ,  → -  Only radiative part contributes to the change of “constants of motion” except for resonance orbits. (last Capra) no need for regularization X  → -X , G (ret)  → G (adv) For resonance orbits, X 3 =  has physical meaning. which means “Orbits with different values of X are basically equivalent.”  (Mino’s time)  r 

6 { X } is not a good set of variables to see the orbital phase evolution. Small change of P, with fixed X, at a late time large variation of x Further canonical transformation: ( X,P ) → ( q,J ) action-angle variables Second canonical transformation

7 t  q t is a periodic function w.r.t. q r,q . After n r and n  cycles, q r = 2  n r, q  = 2  n , irrespective of. q  is gauge invariant in the context of long term evolution. which allows an O (  ) error at each time, but the error should not accumulate. Physical meaning of the angle variables Small change in J (or in P ) with fixed X i small variation of x

8 Mino transformation J  → J  “averaged change rate of q  ” = “phase velocity” Here, not but. almost directly related to the phase of observed GWs Phase velocity averaged after force calculation differentiation of a fn of J  X i ( i =1,2,3 ) are all constant for the background geodesic. This term should be removed Can we insist ? ?

9 The same transformation can be achieved by Yes! “ J  =constant” can be realized by an appropriate gauge transformation, x  → x  –  , without secular growth of  . Additional  W makes J  constant. Perturbation of generating function L.h.s. is gauge inv. (   q caused by  W is purely oscillatory) while r.h.s. may look a gauge-independent fn. of J. ~ ∵ J was originally gauge dependent but must be gauge invariant. ~

10 Why does fix the gauge completely? Let’s consider the above gauge transformation at the reflection point of Mino transformation, where. From the symmetry, at the reflection point. Normalization condition By considering two approximate reflection points corresponding to r min and r max, we can conclude that constant shift of J  is not allowed.

11 We discussed the effect of long-term evolution due to first order self-force. Conclusion Radiative part requires no regularization. The contribution of symmetric part is concisely encoded in gauge- invariant interaction Hamiltonian: Instead of the direct computation of the self-force, alternative simple regularization based on H int might be handy. Scalar quantity. Lower order differentiation. Time integral can be performed first. Evolution of Q in the resonance case can be also described by a similar quantity: {