65 research outputs found

    Psychometrics versus Representational Theory of Measurement

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    Erik Angner has argued that simultaneous endorsement of the representational theory of measurement (RTM) and psychometrics leads to inconsistency. His claim rests on an implicit assumption: RTM and psychometrics are full-fledged approaches to measurement. I argue that RTM and psychometrics are only partial approaches that deal with different aspects of measurement, and that therefore simultaneous endorsement of the two is not inconsistent. The argument has implications for the improvement of measurement practices. The author(s) disclosed receipt of the following financial support for the research, authorship, and/or publication of this article: gratefully acknowledges research funding from the following institutions: Cambridge AHRC (Arts and Humanities Research Council) Doctoral Training Partnership; the British Society for the Philosophy of Science; Cambridge Commonwealth, European and International Trust; and Newnham College

    Review of The Oxford Handbook of Happiness

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    The Oxford Handbook of Happiness is the most comprehensive single volume on the subject of happiness. This long-anticipated landmark collection, along with the similarly ambitious Encyclopedia of Quality of Life Research (A. Michalos, ed. 2013, Springer) shows happiness scholarship coming of age and spreading outward into new themes and disciplines as well as forward into policy and practice. The book takes a broad definition of happiness and its contents span positive psychology and interdisciplinary (but psychology-focused) happiness studies. On the whole, the handbook is a remarkable achievement in that it covers most of the basic contemporary knowledge about happiness as well as giving glimpses of more advanced and specific findings

    Проблема ада как компонент проблемы зла в христианской религиозно-философской парадигме

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    Целью данной работы выступает религиоведческое исследование темы получившей название проблема ада в ее философско-теологическом измерении. Соответственно цели автор ставит перед собой такие задания как: проследить становление традиционной концепции ада, выявить богословские и философские предпосылки формирования данного учения, провести религиоведческий и философский анализ альтернативных учений относительно загробного воздаяния

    Multi-messenger observations of a binary neutron star merger

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    On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta
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