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PhD thesis in English

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2. Diagonalization of Transition Amplitudes∆-dependence of errors with<strong>in</strong> our calculation scheme highly outperforms the polynomialdependence <strong>in</strong> ∆ 2 obta<strong>in</strong>ed by the direct diagonalization of the Hamiltonian.This is true even for short times of propagation t. Although <strong>in</strong>teraction terms <strong>in</strong>the potential affect the numerical values of errors, diagonalization of the transitionamplitudes still substantially outperforms diagonalization of the Hamiltonian, andis the preferred method. This success is a consequence of the non-perturbative behaviorof the spatial discretization error with<strong>in</strong> this calculation scheme. This leadsus to the key conclusion that discretization parameters can be always optimized sothat presented approach of solv<strong>in</strong>g eigenvalue problem of space-discretized transitionamplitudes highly outperforms direct diagonalization of the space-discretizedHamiltonian. The cont<strong>in</strong>uum limit ∆ → 0 is far more easily approached <strong>in</strong> thefirst case and the correspond<strong>in</strong>g discretization errors are substantially smaller forthe same discretization coarseness. From the numerical po<strong>in</strong>t of view, as the valueof parameter ∆ directly determ<strong>in</strong>es the size of the matrix to be diagonalized, thecomputational cost for the same precision is significantly reduced.Further analysis of various errors <strong>in</strong> the ground energy calculation for parametersk 2 = 1, k 4 = 48 of the anharmonic potential (2.29) is given <strong>in</strong> Fig. 2.9. Thedependence of the error related to the <strong>in</strong>troduction of the space cutoff L is illustrated<strong>in</strong> Fig. 2.9(top), while Fig. 2.9(bottom) gives the dependence of ground energy errorson the time of propagation parameter t for various values of the discretization step ∆.On both graphs we see the results obta<strong>in</strong>ed with effective actions of different levelsp. Fig. 2.9(bottom) clearly shows that the errors due to the time of propagationare proportional to t p , as expected when we use the effective action of the level p.The errors <strong>in</strong> eigenvalues are of the same order as errors <strong>in</strong> calculation of <strong>in</strong>dividualmatrix elements, and for this reason we see the typical t p behavior of ground andhigher energy eigenvalues. It is already now evident that the use of higher-ordereffective actions <strong>in</strong>creases the accuracy of numerically calculated energy eigenstatesfor many orders of magnitude.The L-dependence of the error is analytically known [55, 56]. The saturation oferrors on the top graph for a given level p corresponds to a maximal precision thatcan be achieved with that p, i.e. denotes the value of L for which errors <strong>in</strong>troduced byother sources become larger than the error due to the f<strong>in</strong>ite value of the space cutoff.This can be easily seen if we comb<strong>in</strong>e the data from both graphs. For example, thelevel p = 9 effective action has the saturated value of the error of the order of10 −14 . For t = 0.02 we f<strong>in</strong>d that the error due to the time of propagation is of the38

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