22,883 research outputs found

    Semi-Bounded Restrictions of Dirac Type Operators and the Unique Continuation Property

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    Let M be a connected Riemannian manifold and let D be a Dirac type operator acting on smooth compactly supported sections in a Hermitian vector bundle over M. Suppose D has a self-adjoint extension A in the Hilbert space of square-integrable sections. We show that any L2L^2-section Ļ•\phi contained in a closed A-invariant subspace onto which the restriction of A is semi-bounded has the unique continuation property: if Ļ•\phi vanishes on a non-empty open subset of M, then it vanishes on all of M.Comment: 10 pages, LaTeX, minor corrections, reference adde

    Form factors in Bā†’Ļ€Ļ€ā„“Ī½Ė‰ā„“B\to \pi\pi\ell\bar\nu_\ell from QCD light-cone sum rules

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    The form factors of the semileptonic Bā†’Ļ€Ļ€ā„“Ī½Ė‰B\to \pi\pi\ell\bar\nu decay are calculated from QCD light-cone sum rules with the distribution amplitudes of dipion states. This method is valid in the kinematical region, where the hadronic dipion state has a small invariant mass and simultaneously a large recoil. The derivation of the sum rules is complicated by the presence of an additional variable related to the angle between the two pions. In particular, we realize that not all invariant amplitudes in the underlying correlation function can be used, some of them generating kinematical singularities in the dispersion relation. The two sum rules that are free from these ambiguities are obtained in the leading twist-2 approximation, predicting the BĖ‰0ā†’Ļ€+Ļ€0\bar{B}^0\to \pi^+\pi^0 form factors FāŠ„F_{\perp} and Fāˆ„F_{\parallel} of the vector and axial bā†’ub\to u current, respectively. We calculate these form factors at the momentum transfers 0<q2ā‰²120<q^2\lesssim 12 GeV2^2 and at the dipion mass close to the threshold 4mĻ€24m_\pi^2. The sum rule results indicate that the contributions of the higher partial waves to the form factors are suppressed with respect to the lowest PP-wave contribution and that the latter is not completely saturated by the Ļ\rho-meson term.Comment: 17 pages, 4 figures, a few comments and references added, version to be published in Nucl.Phys.

    Optimal choice and beliefs with ex ante savoring and ex post disappointment

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    We propose a new decision criterion under risk in which people extract both utility from anticipatory feelings ex ante and disutility from disappointment ex post. The decision maker chooses his degree of optimism, given that more optimism raises both the utility of ex ante feelings and the risk of disappointment ex post. We characterize the optimal beliefs and the preferences under risk generated by this mental process and apply this criterion to a simple portfolio choice/insurance problem. We show that these preferences are consistent with the preference reversal in the Allaisā€™ paradoxes and predict that the decision maker takes on less risk compared to an expected utility maximizer. This speaks to the equity premium puzzle and to the preference for low deductibles in insurance contracts. Keywords: endogenous beliefs, anticipatory feeling, disappointment, optimism, decision under risk, portfolio allocation

    DeepPose: Human Pose Estimation via Deep Neural Networks

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    We propose a method for human pose estimation based on Deep Neural Networks (DNNs). The pose estimation is formulated as a DNN-based regression problem towards body joints. We present a cascade of such DNN regressors which results in high precision pose estimates. The approach has the advantage of reasoning about pose in a holistic fashion and has a simple but yet powerful formulation which capitalizes on recent advances in Deep Learning. We present a detailed empirical analysis with state-of-art or better performance on four academic benchmarks of diverse real-world images.Comment: IEEE Conference on Computer Vision and Pattern Recognition, 201

    Mutual versus stock insurers : fair premium, capital, and solvency

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    Mutual insurance companies and stock insurance companies are different forms of organized risk sharing: policyholders and owners are two distinct groups in a stock insurer, while they are one and the same in a mutual. This distinction is relevant to raising capital, selling policies, and sharing risk in the presence of financial distress. Up-front capital is necessary for a stock insurer to offer insurance at a fair premium, but not for a mutual. In the presence of an owner-manager conflict, holding capital is costly. Free-rider and commitment problems limit the degree of capitalization that a stock insurer can obtain. The mutual form, by tying sales of policies to the provision of capital, can overcome these problems at the potential cost of less diversified owners

    Diachronic and synchronic thesauruses

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    Per capita income and the extensive margin of bilateral trade

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    This paper quantitatively explores the role of the demand structure in explaining the relationship between an importer's per capita income and the extensive margin of bilateral trade. The underlying mechanism is based on the fact that agents expand the set of goods they consume with income. This in turn affects the structure of a country's import demand and therewith the extensive margin of trade. We formalize this intuition by incorporating preferences that allow for binding non-negativity constraints into an otherwise standard Ricardian multi-country model. We quantify the model using the data on US consumer expenditures and aggregate values of bilateral trade flows and find that the behavior of the model's extensive margin of bilateral trade is consistent with the data (as opposed to the standard model). Two popular counterfactual experiments - lower trade costs and the rise of China and India - demonstrate that the mechanism outlined in this paper is indeed quantitatively important

    Suitable Initial Conditions for Newtonian Simulations with Massive Neutrinos

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    Initial conditions for cosmological N-body simulations are usually calculated by rescaling the present day linear power spectrum obtained from an Einstein-Boltzmann solver to the initial time employing the scale-independent matter growth function. For the baseline Lambda-CDM model, this has been shown to be consistent with General Relativity (GR) even in the presence of relativistic species such as photons. We show that this approach is not feasible in cosmologies with massive neutrinos and present an alternative method employing the Newtonian motion gauge framework.Comment: 10 pages, 4 figure
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