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Marko Robnik

Publications and source records attributed to Marko Robnik.

At least 73 records · Page 4Linked to original sources

High order WKB prediction of the energy splitting in the symmetric double well potential

The accuracy of the WKB approximation when predicting the energy splitting of bound states in a double well potential is the main subject of this paper. The splitting of almost degenerate energy levels below the top of the barrier results from the tunneling and is thus supposed to be exponentially small. By using the standard WKB quantization we deduce an analytical formula for the energy splitting, which is the usual Landau formula with additional quantum corrections. We also examine the accuracy of our and Landau formula numerically for the case of the symmetric double well quartic potential.

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Relevance of Chaos in Numerical Solutions of Quantum Billiards

In this paper we have tested several general numerical methods in solving the quantum billiards, such as the boundary integral method (BIM) and the plane wave decomposition method (PWDM). We performed extensive numerical investigations of these two methods in a variety of quantum billiards: integrable systens (circles, rectangles, and segments of circular annulus), Kolmogorov-Armold-Moser (KAM) systems (Robnik billiards), and fully chaotic systems (ergodic, such as Bunimovich stadium, Sinai billiard and cardiod billiard). We have analyzed the scaling of the average absolute value of the systematic error $ΔE$ of the eigenenergy in units of the mean level spacing with the density of discretization $b$ (which is number of numerical nodes on the boundary within one de Broglie wavelength) and its relationship with the geometry and the classical dynamics. In contradistinction to the BIM, we find that in the PWDM the classical chaos is definitely relevant for the numerical accuracy at a fixed density of discretization $b$. We present evidence that it is not only the ergodicity that matters, but also the Lyapunov exponents and Kolmogorov entropy. We believe that this phenomenon is one manifestation of quantum chaos.

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Energy level statistics in the transition regime between integrability and chaos for systems with broken antiunitary symmetry

Energy spectra of a particle with mass $m$ and charge $e$ in the cubic Aharonov-Bohm billiard containing around $10^4$ consecutive levels starting from the ground state have been analysed. The cubic Aharonov-Bohm billiard is a plane billiard defined by the cubic conformal mapping of the unit disc pervaded by a point magnetic flux through the origin perpendicular to the plane of the billiard. The magnetic flux does not influence the classical dynamics, but breaks the antiunitary symmetry in the system, which affects the statistics of energy levels. By varying the shape parameter $\lam$ the classical dynamics goes from integrable ($\lam =0$) to fully chaotic ($\lam = 0.2$; Africa billiard). The level spacing distribution $P(S)$ and the number variance $Σ^{2}(L)$ have been studied for 13 different shape parameters on the interval ($0\le\lam\le0.2$). GUE statistics has proven correct for completely chaotic case, while in the mixed regime the fractional power law level repulsion has been observed. The exponent of the level repulsion has been analysed and is found to change smoothly from 0 to 2 as the dynamics goes from integrable to ergodic. Further on, the semiclassical Berry-Robnik theory has been examined. We argue that the semiclassical regime has not been reached and give an estimate for the number of energy levels required for the Berry-Robnik statistics to apply.

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WKB corrections to the energy splitting in double-well potentials

By using the WKB quantization we deduce an analytical formula for the energy splitting in a double-well potential which is the usual Landau formula with additional quantum corrections. Then we analyze the accuracy of our formula for the double square well potential and the parabolic double-well potential.

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New Universal Aspects of Diffusion in Strongly Chaotic Systems

We study some new universal aspects of diffusion in chaotic systems, especially such having very large Lyapunov coefficients on the chaotic (indecomposable, topologically transitive) component. We do this by discretizing the chaotic component on the Surface-of-Section in a (large) number $N$ of simplectically equally big cells (in the sense of equal relative invariant ergodic measure, normalized so that the total measure of the chaotic component is unity). By iterating the transition of the chaotic orbit through SOS, where $j$ counts the number of iteration (discrete time), and assuming complete lack of correlations even between consecutive crossings (which can be justified due to the very large Lyapunov exponents), we show the universal approach of the relative measure of the occupied cells, denoted by $ρ(j)$, to the asymptotic value of unity, in the following way: $ρ(j) = 1 - (1-\frac{1}{N})^j$, so that in the limit of big $N$, $N\to \infty$, we have, for $j/N$ fixed, the exponential law $ρ(j) \approx 1 - \exp (-j/N)$. This analytic result is verified numerically in a variety of specific systems: For a plane billiard (Robnik 1983, $λ=0.375$), for a 3-D billiard (Prosen 1997, $a=-1/5, b=-12/5$), for ergodic logistic map (tent map), for standard map ($k=400$) and for hydrogen atom in strong magnetic field ($ε=-0.05$) the agreement is almost perfect (except, in the latter two systems, for some long-time deviations on very small scale), but for Hénon-Heiles system ($E=1/6$) and for the standard map ($k=3$) the deviations are noticed although they are not very big (only about 1%). We have tested the random number generators (Press et al 1986), and confirmed that some are almost perfect (ran0 and ran3), whilst two of them (ran1 and ran2) exhibit big deviations.

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Comment on Energy Level Statistics in the Mixed Regime

We comment on the recent paper by Abul-Magd (J.Phys.A: Math.Gen. 29 (1996) 1) concerning the energy level statistics in the mixed regime, i.e. such having the mixed classical dynamics where regular and chaotic regions coexist in the phase space. We point out that his basic assumption on the additive property of the level-repulsion function $r(S)$ (conditional probability density) in the sense of dividing it linearly into the regular and chaotic part in proportion to the classical fractional phase space volumes $ρ_1$ and $ρ_2=q$ is not justified, since among other things, it relies on the type of Berry's ergodic assumption, which however is right only in a homogeneous ensemble of ergodic systems, but not in the neighbourhood of an integrable system. Thus his resulting distribution cannot be regarded as a theoretically well founded object. We point out that the semiclassical limiting energy level spacing distribution must be of Berry-Robnik (1984) type, and explain what transitional behaviour of the Brody-type (with fractional power-law energy level repulsion) we observe in the near semiclassical regime where effective $\hbar$ is not yet small enough. Thus we refer to the derivation, arguments and conclusions in our paper (Prosen and Robnik, J.Phys.A: Math.Gen. 26 (1994) 8059), and explain again the behaviour in this double transition region.

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Supersymmetric quantum mechanics based on higher excited states II: a few examples of isospectral partner potentials

We apply the generalized formalism and the techniques of the supersymmetric (susy) quantum mechanics to the cases where the superpotential is generated/defined by higher excited eigenstates (Robnik 1997, paper I). The generalization is technically almost straightforward but physically quite nontrivial since it yields an infinity of new classes of susy-partner potentials, whose spectra are exactly identical except for the lowest $n+1$ states, if the superpotential is defined in terms of the $(n+1)$-st eigenfunction, with $n=0$ reserved for the ground state. First we show that there are practically no possibilities for shape invariant potentials based on higher excited states. Then we calculate the isospectral partner potentials for the following 1-dim potentials (after separation of variables where appropriate): (i) 3-dim (spherically symmetric) harmonic oscillator, (ii) 3-dim (isotropic) Kepler problem, (iii) Morse potential, (iv) Pöschl-Teller type I potential, and (v) the 1-dim box potential. In all cases except in (v) we get new classes of solvable potentials. In (v) the partner potential to the box potential is a special case of Pöschl-Teller type I potential. potentials. In this paper we present results of a straightforward further application of this formalism to a few most important exactly solvable 1-dim potentials, namely (i) spherically symmetric 3-dim harmonic oscillator, (ii) 3-dim isotropic (spherically symmetric) Kepler potential, (iii) Morse potential, (iv) Pöschl-Teller type I potential, and (v) 1-dim box potential. PACS numbers: 03.65.-w, 03.65.Ge, 03.65.Sq

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Supersymmetric quantum mechanics based on higher excited states

We generalize the formalism and the techniques of the supersymmetric (susy) quantum mechanics to the cases where the superpotential is generated/defined by higher excited eigenstates. The generalization is technically almost straightforward but physically quite nontrivial since it yields an infinity of new classes of susy-partner potentials, whose spectra are exactly identical except for the lowest m+1 states, if the superpotential is defined in terms of the (m+1)-st eigenfunction, with m=0 reserved for the ground state. It is shown that in case of the infinite 1-dim potential well nothing new emerges (the partner potential is still of Pöschl-Teller type I, for all m), whilst in case of the 1-dim harmonic oscillator we get a new class of infinitely many partner potentials: for each m the partner potential is expressed as the sum of the quadratic harmonic potential plus rational function, defined as the derivative of the ratio of two consecutive Hermite polynomials. These partner potentials of course have m singularities exactly at the locations of the nodes of the generating (m+1)-st wavefunction. The susy formalism applies everywhere between the singularities. A systematic application of the formalism to other potentials with known spectra would yield an infinitely rich class of "solvable" potentials, in terms of their partner potentials. If the potentials are shape invariant they can be solved at least partially and new types of analytically obtainable spectra are expected. PACS numbers: 03.65.-w, 03.65.Ge, 03.65.Sq

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WKB to all orders and the accuracy of the semiclassical quantization

We perform a systematic WKB expansion to all orders for a one-dimensional system with potential $V(x)=U_0/\cos^2{(αx)}$. We are able to sum the series to the exact energy spectrum. Then we show that at any finite order the error of the WKB approximation measured in the natural units of the mean energy level spacing does not go to zero when the quantum number goes to infinity. Therefore we make the general conclusion that the semiclassical approximations fail to predict the individual energy levels within a vanishing fraction of the mean energy level spacing.

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WKB to all orders and accuracy of the semiclassical quantization

We perform a systematic WKB expansion to all orders for a one--dimensional system with potential $V(x)=U_0/\cos^2{(αx)}$. We are able to sum the series to the exact energy spectrum. Then we show that any finite order WKB approximation fails to predict the individual energy levels within a vanishing fraction of the mean energy level spacing.

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Semiclassical Expansion for the Angular Momentum

After reviewing the WKB series for the Schrödinger equation we calculate the semiclassical expansion for the eigenvalues of the angular momentum operator. This is the first systematic semiclassical treatment of the angular momentum for terms beyond the leading torus approximation.

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WKB expansion for the angular momentum and the Kepler problem: from the torus quantization to the exact one

We calculate the WKB series for the angular momentum and the non--relativistic 3-dim Kepler problem. This is the first semiclassical treatment of the angular momentum for terms beyond the leading WKB approximation. We explain why the torus quantization (the leading WKB term) of the full problem is exact, even if the individual torus quantization of the angular momentum and of the radial Kepler problem separately is not exact. PACS numbers: 03.65.-w, 03.65.Ge, 03.65.Sq

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Quantum corrections to the semiclassical quantization of a nonintegrable system

We study the semiclassical behaviour of a two--dimensional nonintegrable system. In particular we analyze the question of quantum corrections to the semiclassical quantization obtaining up to the second order of perturbation theory an explicit analytical formula for the energy levels, which is the usual semiclassical one plus quantum corrections. We compare the "exact" levels obtained numerically to the semiclassical levels studying also the effects of quantum corrections.

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Practical and algorithmical manifestations of quantum chaos

Quantum chaos manifests itself also in algorithmical complexity of methods, including the numerical ones, in solving the Schrödinger equation. In this contribution we address the problem of calculating the eigenenergies and the eigenstates by various numerical methods applied to 2-dim generic billiard systems. In particular we analyze the dependence of the accuracy (errors) on the density of discretization of the given numerical method. We do this for several different billiard shapes, especially for the Robnik billiard. We study the numerical error of the boundary integral method and the plane wave decomposition method as a function of the discretization parameter $b$ which by definition is the number of discretization nodes on the boundary per one de Broglie wavelength (arclength) interval. For boundary integral method, we discover that at each $λ$ the error scales as a power law $<|ΔE|> = A b^{-α}$, where $α$ is a strong function of $λ$: In the KAM-like regime $0\le λ\le 1/4$ it is large and close to 3.5, but close to $λ= 1/4$ it changes almost discontinuously becoming hardly any larger than zero. This is because the billiard becomes nonconvex beginning at $λ=1/4$. For the plane wave decomposition method, we found at a fixed $b$ that the average absolute value of the error $<|ΔE|>$ correlates strongly with the classical chaos, where the error $<|ΔE|>$ does increase sharply with increasing classical chaos. This property is valid also for Bunimovich stadium and the Sinai billiard.

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Sensitivity of the eigenfunctions and the level curvature distribution in quantum billiards

In searching for the manifestations of sensitivity of the eigenfunctions in quantum billiards (with Dirichlet boundary conditions) with respect to the boundary data (the normal derivative) we have performed instead various numerical tests for the Robnik billiard (quadratic conformal map of the unit disk) for 600 shape parameter values, where we look at the sensitivity of the energy levels with respect to the shape parameter. We show the energy level flow diagrams for three stretches of fifty consecutive (odd) eigenstates each with index 1,000 to 2,000. In particular, we have calculated the (unfolded and normalized) level curvature distribution and found that it continuously changes from a delta distribution for the integrable case (circle) to a broad distribution in the classically ergodic regime. For some shape parameters the agreement with the GOE von Oppen formula is very good, whereas we have also cases where the deviation from GOE is significant and of physical origin. In the intermediate case of mixed classical dynamics we have a semiclassical formula in the spirit of the Berry-Robnik (1984) surmise. Here the agreement with theory is not good, partially due to the localization phenomena which are expected to disappear in the semiclassical limit. We stress that even for classically ergodic systems there is no global universality for the curvature distribution, not even in the semiclassical limit.

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Is there relevance of chaos in numerical solutions of quantum billiards?

In numerically solving the Helmholtz equation inside a connected plane domain with Dirichlet boundary conditions (the problem of the quantum billiard) one surprisingly faces enormous difficulties if the domain has a problematic geometry such as various nonconvex shapes. We have tested several general numerical methods in solving the quantum billiards. Following our previous paper (Li and Robnik 1995) where we analyzed the Boundary Integral Method (BIM), in the present paper we investigate systematically the so-called Plane Wave Decomposition Method (PWDM) introduced and advocated by Heller (1984, 1991). In contradistinction to BIM we find that in PWDM the classical chaos is definitely relevant for the numerical accuracy at fixed density of discretization on the boundary $b$ ($b$ = number of numerical nodes on the boundary within one de Broglie wavelength). This can be understood qualitatively and is illustrated for three one-parameter families of billiards, namely Robnik billiard, Bunimovich stadium and Sinai billiard. We present evidence that it is not only the ergodicity which matters, but also the Lyapunov exponents and Kolmogorov entropy. Although we have no quantitative theory we believe that this phenomenon is one manifestation of quantum chaos. PACS numbers: 02.70.Rw, 05.45.+b, 03.65.Ge, 03.65.-w

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Boundary integral method applied in chaotic quantum billiards

The boundary integral method (BIM) is a formulation of Helmholtz equation in the form of an integral equation suitable for numerical discretization to solve the quantum billiard. This paper is an extensive numerical survey of BIM in a variety of quantum billiards, integrable (circle, rectangle), KAM systems (Robnik billiard) and fully chaotic (ergodic, such as stadium, Sinai billiard and cardioid billiard). On the theoretical side we point out some serious flaws in the derivation of BIM in the literature and show how the final formula (which nevertheless was correct) should be derived in a sound way and we also argue that a simple minded application of BIM in nonconvex geometries presents serious difficulties or even fails. On the numerical side we have analyzed the scaling of the averaged absolute value of the systematic error $ΔE$ of the eigenenergy in units of mean level spacing with the density of discretization ($b$ = number of numerical nodes on the boundary within one de Broglie wavelength), and we find that in all cases the error obeys a power law $ <|ΔE|> = A b^{-α}$, where $ α$ (and also $A$) varies from case to case (it is not universal), and is affected strongly by the existence of exterior chords in nonconvex geometries, whereas the degree of the classical chaos seems to be practically irrelevant. We comment on the semiclassical limit of BIM and make suggestions about a proper formulation with correct semiclassical limit in nonconvex geometries.

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SUPPLEMENT TO THE PAPER: Separating the regular and irregular energy levels and their statistics in Hamiltonian system with mixed classical dynamics

As a technical supplement to the above mentioned paper we present 192 consecutive eigenstates for the Robnik billiard with the shape parameter $λ=0.15$ from 10,001st to 10,192nd, by showing the plots in the configuration space and in the phase space. The latter is smoothed projection of the Wigner function onto the surface of section. By comparison with the classical SOS plots we thus examine all eigenstates and classify them in regular and irregular: There are 70 regular states and 122 irregular states, thus giving the estimate of the relative measure of the regular component $ρ_1=0.365$, which is in excellent agreement with the classical value $ρ_1=0.360$ calculated and reported by Prosen and Robnik (1993).

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