74 research outputs found

    Ramanujan and Extensions and Contractions of Continued Fractions

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    If a continued fraction Kn=1an/bnK_{n=1}^{\infty} a_{n}/b_{n} is known to converge but its limit is not easy to determine, it may be easier to use an extension of Kn=1an/bnK_{n=1}^{\infty}a_{n}/b_{n} to find the limit. By an extension of Kn=1an/bnK_{n=1}^{\infty} a_{n}/b_{n} we mean a continued fraction Kn=1cn/dnK_{n=1}^{\infty} c_{n}/d_{n} whose odd or even part is Kn=1an/bnK_{n=1}^{\infty} a_{n}/b_{n}. One can then possibly find the limit in one of three ways: (i) Prove the extension converges and find its limit; (ii) Prove the extension converges and find the limit of the other contraction (for example, the odd part, if Kn=1an/bnK_{n=1}^{\infty}a_{n}/b_{n} is the even part); (ii) Find the limit of the other contraction and show that the odd and even parts of the extension tend to the same limit. We apply these ideas to derive new proofs of certain continued fraction identities of Ramanujan and to prove a generalization of an identity involving the Rogers-Ramanujan continued fraction, which was conjectured by Blecksmith and Brillhart.Comment: 16 page

    Exactly solvable model of three interacting particles in an external magnetic field

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    The quantum mechanical problem of three identical particles, moving in a plane and interacting pairwise via a spring potential, is solved exactly in the presence of a magnetic field. Calculations of the pair--correlation function, mean distance and the cluster area show a quantization of these parameters. Especially the pair-correlation function exhibits a certain number of maxima given by a quantum number. We obtain Jastrow pre-factors which lead to an exchange correlation hole of liquid type, even in the presence of the attractive interaction between the identical electrons.Comment: 8 pages 3 figure

    Pairing symmetry and long range pair potential in a weak coupling theory of superconductivity

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    We study the superconducting phase with two component order parameter scenario, such as, dx2y2+eiθsαd_{x^2-y^2} + e^{i\theta}s_{\alpha}, where α=xy,x2+y2\alpha = xy, x^2+y^2. We show, that in absence of orthorhombocity, the usual dx2y2d_{x^2-y^2} does not mix with usual sx2+y2s_{x^2+y^2} symmetry gap in an anisotropic band structure. But the sxys_{xy} symmetry does mix with the usual d-wave for θ=0\theta =0. The d-wave symmetry with higher harmonics present in it also mixes with higher order extended ss wave symmetry. The required pair potential to obtain higher anisotropic dx2y2d_{x^2-y^2} and extended s-wave symmetries, is derived by considering longer ranged two-body attractive potential in the spirit of tight binding lattice. We demonstrate that the dominant pairing symmetry changes drastically from dd to ss like as the attractive pair potential is obtained from longer ranged interaction. More specifically, a typical length scale of interaction ξ\xi, which could be even/odd multiples of lattice spacing leads to predominant s/ds/d wave symmetry. The role of long range interaction on pairing symmetry has further been emphasized by studying the typical interplay in the temperature dependencies of these higher order dd and ss wave pairing symmetries.Comment: Revtex 8 pages, 7 figures embeded in the text, To appear in PR

    Orbital structure of the GJ876 extrasolar planetary system, based on the latest Keck and HARPS radial velocity data

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    We use full available array of radial velocity data, including recently published HARPS and Keck observatory sets, to characterize the orbital configuration of the planetary system orbiting GJ876. First, we propose and describe in detail a fast method to fit perturbed orbital configuration, based on the integration of the sensitivity equations inferred by the equations of the original NN-body problem. Further, we find that it is unsatisfactory to treat the available radial velocity data for GJ876 in the traditional white noise model, because the actual noise appears autocorrelated (and demonstrates non-white frequency spectrum). The time scale of this correlation is about a few days, and the contribution of the correlated noise is about 2 m/s (i.e., similar to the level of internal errors in the Keck data). We propose a variation of the maximum-likelihood algorithm to estimate the orbital configuration of the system, taking into account the red noise effects. We show, in particular, that the non-zero orbital eccentricity of the innermost planet \emph{d}, obtained in previous studies, is likely a result of misinterpreted red noise in the data. In addition to offsets in some orbital parameters, the red noise also makes the fit uncertainties systematically underestimated (while they are treated in the traditional white noise model). Also, we show that the orbital eccentricity of the outermost planet is actually ill-determined, although bounded by 0.2\sim 0.2. Finally, we investigate possible orbital non-coplanarity of the system, and limit the mutual inclination between the planets \emph{b} and \emph{c} orbits by 5155^\circ-15^\circ, depending on the angular position of the mutual orbital nodes.Comment: 36 pages, 11 figures, 3 tables; Accepted to Celestial Mechanics and Dynamical Astronom

    Decoherence as Decay of the Loschmidt Echo in a Lorentz Gas

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    Classical chaotic dynamics is characterized by the exponential sensitivity to initial conditions. Quantum mechanics, however, does not show this feature. We consider instead the sensitivity of quantum evolution to perturbations in the Hamiltonian. This is observed as an atenuation of the Loschmidt Echo, M(t)M(t), i.e. the amount of the original state (wave packet of width σ\sigma) which is recovered after a time reversed evolution, in presence of a classically weak perturbation. By considering a Lorentz gas of size LL, which for large LL is a model for an {\it unbounded} classically chaotic system, we find numerical evidence that, if the perturbation is within a certain range, M(t)M(t) decays exponentially with a rate 1/τϕ1/\tau_{\phi} determined by the Lyapunov exponent λ\lambda of the corresponding classical dynamics. This exponential decay extends much beyond the Eherenfest time tEt_{E} and saturates at a time tsλ1ln(N~)t_{s}\simeq \lambda^{-1}\ln (\widetilde{N}), where N~(L/σ)2\widetilde{N}\simeq (L/\sigma)^2 is the effective dimensionality of the Hilbert space. Since τϕ\tau _{\phi} quantifies the increasing uncontrollability of the quantum phase (decoherence) its characterization and control has fundamental interest.Comment: 3 ps figures, uses Revtex and epsfig. Major revision to the text, now including discussion and references on averaging and Ehrenfest time. Figures 2 and 3 content and order change

    Hidden Order in the Cuprates

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    We propose that the enigmatic pseudogap phase of cuprate superconductors is characterized by a hidden broken symmetry of d(x^2-y^2)-type. The transition to this state is rounded by disorder, but in the limit that the disorder is made sufficiently small, the pseudogap crossover should reveal itself to be such a transition. The ordered state breaks time-reversal, translational, and rotational symmetries, but it is invariant under the combination of any two. We discuss these ideas in the context of ten specific experimental properties of the cuprates, and make several predictions, including the existence of an as-yet undetected metal-metal transition under the superconducting dome.Comment: 12 pages of RevTeX, 9 eps figure

    Vortex structure in d-density wave scenario of pseudogap

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    We investigate the vortex structure assuming the d-density wave scenario of the pseudogap. We discuss the profiles of the order parameters in the vicinity of the vortex, effective vortex charge and the local density of states. We find a pronounced modification of these quantities when compared to a purely superconducting case. Results have been obtained for a clean system as well as in the presence of a nonmagnetic impurity. We show that the competition between superconductivity and the density wave may explain some experimental data recently obtained for high-temperature superconductors. In particular, we show that the d-density wave scenario explains the asymmetry of the gap observed in the vicinity of the vortex core.Comment: 8 pages, 10 figure

    Dispersion of Ordered Stripe Phases in the Cuprates

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    A phase separation model is presented for the stripe phase of the cuprates, which allows the doping dependence of the photoemission spectra to be calculated. The idealized limit of a well-ordered array of magnetic and charged stripes is analyzed, including effects of long-range Coulomb repulsion. Remarkably, down to the limit of two-cell wide stripes, the dispersion can be interpreted as essentially a superposition of the two end-phase dispersions, with superposed minigaps associated with the lattice periodicity. The largest minigap falls near the Fermi level; it can be enhanced by proximity to a (bulk) Van Hove singularity. The calculated spectra are dominated by two features -- this charge stripe minigap plus the magnetic stripe Hubbard gap. There is a strong correlation between these two features and the experimental photoemission results of a two-peak dispersion in La2x_{2-x}Srx_xCuO4_4, and the peak-dip-hump spectra in Bi2_2Sr2_2CaCu2_2O8+δ_{8+\delta}. The differences are suggestive of the role of increasing stripe fluctuations. The 1/8 anomaly is associated with a quantum critical point, here expressed as a percolation-like crossover. A model is proposed for the limiting minority magnetic phase as an isolated two-leg ladder.Comment: 24 pages, 26 PS figure
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