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PhD thesis in English

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2. Diagonalization of Transition AmplitudesTo address this, <strong>in</strong> pr<strong>in</strong>ciple one can use Monte Carlo simulations [57, 58] tocalculate amplitudes A to high precision. Although this can effectively resolve theproblem <strong>in</strong> many cases, it is often numerically very expensive. More importantly,resort<strong>in</strong>g to the use of Monte Carlo practically limits further analytical approaches.We will <strong>in</strong>stead use the recently <strong>in</strong>troduced effective action approach [44, 10, 45, 46,11] that gives closed-form analytic expressions A (p) (x, y; t) for transition amplitudeswhich converge much faster,A (p) (x, y; t) = A(x, y; t) + O(t p+1 /t d/2 ) , (2.25)where p is an <strong>in</strong>teger number correspond<strong>in</strong>g to the order of the effective actionused. For a general many-body theory effective actions up to p = 10 have beenderived, while for a specific models much higher values can be obta<strong>in</strong>ed, e.g. for theanharmonic oscillator and other polynomial <strong>in</strong>teractions, for which effective actionshave been calculated up to p = 144. So, if p is high enough, it is sufficient that thetime of evolution is less than the radius of convergence of the above series (t < τ c ∼ 1)and errors <strong>in</strong> calculated values of transition amplitudes will be negligible. This isillustrated <strong>in</strong> Fig. 2.7 for the case of a quartic anharmonic oscillator. The use ofhigh-order expansion <strong>in</strong> the time of propagation of amplitudes will allow us to usetimes of evolution up to τ c , which are much longer than the typical times one canuse with the naive (p = 1) amplitudes. At the same time, the expansion up to veryhigh orders substantially decreases the errors associated with t, and may practicallyelim<strong>in</strong>ate them.The analytic expressions for higher-order approximations for transition amplitudesare based on the notion of effective actions, which are <strong>in</strong>troduced by cast<strong>in</strong>gthe solution of the time dependent Schröd<strong>in</strong>ger equation for the transition amplitude<strong>in</strong> the formA(x, y; t) =1√(2πt)d e−(x−y)2 2t −tW( x+y ,x−y;t) 2 , (2.26)where W(x, δ; t) is the effective potential, with the follow<strong>in</strong>g boundary behavior:lim W(x, δ; t) = V (x) . (2.27)t→0As shown previously, the effective potential W(x, δ; t) is regular <strong>in</strong> the vic<strong>in</strong>ity oft = 0, enabl<strong>in</strong>g us to represent it <strong>in</strong> the form of a power series <strong>in</strong> short time ofpropagation t. The coefficients <strong>in</strong> this series are functions of the potential and34

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