27,744 research outputs found

    Two-mode heterodyne phase detection

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    We present an experimental scheme that achieves ideal phase detection on a two-mode field. The two modes aa and bb are the signal and image band modes of an heterodyne detector, with the field approaching an eigenstate of the photocurrent Z^=a+b\hat{Z}=a+b^{\dag}. The field is obtained by means of a high-gain phase-insensitive amplifier followed by a high-transmissivity beam-splitter with a strong local oscillator at the frequency of one of the two modes.Comment: 3 pages, 1 figur

    Automatic structures, rational growth and geometrically finite hyperbolic groups

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    We show that the set SA(G)SA(G) of equivalence classes of synchronously automatic structures on a geometrically finite hyperbolic group GG is dense in the product of the sets SA(P)SA(P) over all maximal parabolic subgroups PP. The set BSA(G)BSA(G) of equivalence classes of biautomatic structures on GG is isomorphic to the product of the sets BSA(P)BSA(P) over the cusps (conjugacy classes of maximal parabolic subgroups) of GG. Each maximal parabolic PP is a virtually abelian group, so SA(P)SA(P) and BSA(P)BSA(P) were computed in ``Equivalent automatic structures and their boundaries'' by M.Shapiro and W.Neumann, Intern. J. of Alg. Comp. 2 (1992) We show that any geometrically finite hyperbolic group has a generating set for which the full language of geodesics for GG is regular. Moreover, the growth function of GG with respect to this generating set is rational. We also determine which automatic structures on such a group are equivalent to geodesic ones. Not all are, though all biautomatic structures are.Comment: Plain Tex, 26 pages, no figure

    Generic Quantum Ratchet Accelerator with Full Classical Chaos

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    A simple model of quantum ratchet transport that can generate unbounded linear acceleration of the quantum ratchet current is proposed, with the underlying classical dynamics fully chaotic. The results demonstrate that generic acceleration of quantum ratchet transport can occur with any type of classical phase space structure. The quantum ratchet transport with full classical chaos is also shown to be very robust to noise due to the large linear acceleration afforded by the quantum dynamics. One possible experiment allowing observation of these predictions is suggested.Comment: 4 pages, 4 figure

    Spin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method

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    In this paper, we calculate properties of the spin polarized asymmetrical nuclear matter and neutron star matter, using the lowest order constrained variational (LOCV) method with the AV18AV_{18}, Reid93Reid93, UV14UV_{14} and AV14AV_{14} potentials. According to our results, the spontaneous phase transition to a ferromagnetic state in the asymmetrical nuclear matter as well as neutron star matter do not occur.Comment: 21 pages, 11 figure

    Participation of the hypophyseal-adrenal cortex system in thrombin clearance during immobilization stress

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    Thrombin marked with I-131 resulted in a considerable increase of the thrombined clearance rate in healthy male rats during stress caused by an immobilization lasting 30 minutes, and in an increase of thrombin clearance occurred by a combination of immobilization and administration of adrenocorticotropin (ACTH). Contrary to ACTH, the thrombin clearance is not stimulated in healthy animals by hydrocortisone. The results of the examination are presented

    Classical-Wigner Phase Space Approximation to Cumulative Matrix Elements in Coherent Control

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    The classical limit of the Wigner-Weyl representation is used to approximate products of bound-continuum matrix elements that are fundamental to many coherent control computations. The range of utility of the method is quantified through an examination of model problems, single-channel Na_2 dissociation and multi-arrangement channel photodissociation of CH_2IBr. Very good agreement with the exact quantum results is found for a wide range of system parameters.Comment: 17 pages, 12 figures, to appear in Journal of Chemical Physic

    The Equation of State of Dense Matter : from Nuclear Collisions to Neutron Stars

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    The Equation of State (EoS) of dense matter represents a central issue in the study of compact astrophysical objects and heavy ion reactions at intermediate and relativistic energies. We have derived a nuclear EoS with nucleons and hyperons within the Brueckner-Hartree-Fock approach, and joined it with quark matter EoS. For that, we have employed the MIT bag model, as well as the Nambu--Jona-Lasinio (NJL) and the Color Dielectric (CD) models, and found that the NS maximum masses are not larger than 1.7 solar masses. A comparison with available data supports the idea that dense matter EoS should be soft at low density and quite stiff at high density.Comment: 8 pages, 5 figures, invited talk given at NPA3, Dresden, March 200

    The Born and Lens-Lens Corrections to Weak Gravitational Lensing Angular Power Spectra

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    We revisit the estimation of higher order corrections to the angular power spectra of weak gravitational lensing. Extending a previous calculation of Cooray and Hu, we find two additional terms to the fourth order in potential perturbations of large-scale structure corresponding to corrections associated with the Born approximation and the neglect of line-of-sight coupling of two foreground lenses in the standard first order result. These terms alter the convergence (κκ\kappa\kappa), the lensing shear E-mode (ϵϵ\epsilon\epsilon), and their cross-correlation (κϵ\kappa\epsilon) power spectra on large angular scales, but leave the power spectra of the lensing shear B-mode (ββ\beta\beta) and rotational (ωω\omega\omega) component unchanged as compared to previous estimates. The new terms complete the calculation of corrections to weak lensing angular power spectra associated with both the Born approximation and the lens-lens coupling to an order in which the contributions are most significant. Taking these features together, we find that these corrections are unimportant for any weak lensing survey, including for a full sky survey limited by cosmic variance.Comment: Added references, minor changes to text. 9 pages, 2 figure
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