3,734 research outputs found

    Being, doing, and play: A theoretical and clinical exploration

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    This paper explores the metonymy of the following aphorism, delivered by Winnicott in a 1967 lecture: “From being comes doing, but there can be no do before be.” (1970, p. 25, emphasis in original). This aphorism has been little discussed or explored in the literature, but Winnicott articulated similar ideas in his more academic papers (e.g., 1965, 1970). These similar communications about being and doing will be examined alongside more contemporary thinking about the ideas to which Winnicott alludes in this aphorism; works by Benjamin (1988) and Akhtar (2000) in particular will be brought to bear on the subject. Two case studies will then be discussed, in order to examine the clinical implications of the theoretical discussion. Ultimately, such exploration will substantiate the claim that, through the metonymy of being and doing, Winnicott was alluding to a “statement of human nature” that he published just 3 years later (1970, p. 2). Winnicott’s own concept of play will then be posited as a critical, third element comprising “the life of a human being,” which will serve to situate the discussion within a contemporary, relational framework (1970, p. 2)

    The Spin Distribution of Fast Spinning Neutron Stars in Low Mass X-Ray Binaries: Evidence for Two Sub-Populations

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    We study the current sample of rapidly rotating neutron stars in both accreting and non-accreting binaries in order to determine whether the spin distribution of accreting neutron stars in low-mass X-ray binaries can be reconciled with current accretion torque models. We perform a statistical analysis of the spin distributions and show that there is evidence for two sub-populations among low-mass X-ray binaries, one at relatively low spin frequency, with an average of ~300 Hz and a broad spread, and a peaked population at higher frequency with average spin frequency of ~575 Hz. We show that the two sub-populations are separated by a cut-point at a frequency of ~540 Hz. We also show that the spin frequency of radio millisecond pulsars does not follow a log-normal distribution and shows no evidence for the existence of distinct sub-populations. We discuss the uncertainties of different accretion models and speculate that either the accreting neutron star cut-point marks the onset of gravitational waves as an efficient mechanism to remove angular momentum or some of the neutron stars in the fast sub-population do not evolve into radio millisecond pulsars.Comment: Submitted to Ap

    Diet distribution and life history of an invasive opossum shrimp (Neomysis mercedis) in John Day Reservoir Columbia River

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    Actions for Death by Wrongful Act

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    Plumbing at the Highlands, Fort Washington, Pennsylvania, 1845-1904

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    Dynamical mean-filed approximation to small-world networks of spiking neurons: From local to global, and/or from regular to random couplings

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    By extending a dynamical mean-field approximation (DMA) previously proposed by the author [H. Hasegawa, Phys. Rev. E {\bf 67}, 41903 (2003)], we have developed a semianalytical theory which takes into account a wide range of couplings in a small-world network. Our network consists of noisy NN-unit FitzHugh-Nagumo (FN) neurons with couplings whose average coordination number ZZ may change from local (ZNZ \ll N ) to global couplings (Z=N1Z=N-1) and/or whose concentration of random couplings pp is allowed to vary from regular (p=0p=0) to completely random (p=1). We have taken into account three kinds of spatial correlations: the on-site correlation, the correlation for a coupled pair and that for a pair without direct couplings. The original 2N2 N-dimensional {\it stochastic} differential equations are transformed to 13-dimensional {\it deterministic} differential equations expressed in terms of means, variances and covariances of state variables. The synchronization ratio and the firing-time precision for an applied single spike have been discussed as functions of ZZ and pp. Our calculations have shown that with increasing pp, the synchronization is {\it worse} because of increased heterogeneous couplings, although the average network distance becomes shorter. Results calculated by out theory are in good agreement with those by direct simulations.Comment: 19 pages, 2 figures: accepted in Phys. Rev. E with minor change

    Criminal Law and It\u27s Enforcement

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