8,890 research outputs found

    EEOC v. Mcdonald\u27s Restaurants of California, Inc.

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    EEOC v. Pape Material Handling, Inc.,

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    EEOC v. American Laser Centers

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    Neutron Star Properties from an NJL Model Modified to Simulate Confinement

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    The NJL model has recently been extended with a method to simulate confinement. This leads in mean field approximation to a natural mechanism for the saturation of nuclear matter. We use the model to investigate the equation of state of asymmetric nuclear matter and then use it to compute the properties of neutron stars.Comment: 5 pages, 6 figures, to be published in the proceedings for QCD Down Under Workshop, Adelaide, March 10-19, 200

    Statistical Properties of Height of Japanese Schoolchildren

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    We study height distributions of Japanese schoolchildren based on the statictical data which are obtained from the school health survey by the ministry of education, culture, sports, science and technology, Japan . From our analysis, it has been clarified that the distribution of height changes from the lognormal distribution to the normal distribution in the periods of puberty.Comment: 2 pages, 2 figures, submitted to J. Phys. Soc. Jpn.; resubmitted to J. Phys. Soc. Jpn. after some revisio

    Addressing decision making for remanufacturing operations and design-for-remanufacture

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    Remanufacturing is a process of returning a used product to at least original equipment manufacturer original performance specification from the customers' perspective and giving the resultant product a warranty that is at least equal to that of a newly manufactured equivalent. This paper explains the need to combine ecological concerns and economic growth and the significance of remanufacturing in this. Using the experience of an international aero-engine manufacturer it discusses the impact of the need for sustainable manufacturing on organisational business models. It explains some key decision-making issues that hinder remanufacturing and suggests effective solutions. It presents a peer-validated, high-level design guideline to assist decision-making in design in order to support remanufacturing. The design guide was developed in the UK through the analysis of selections of products during case studies and workshops involving remanufacturing and conventional manufacturing practitioners as well as academics. It is one of the initial stages in the development of a robust design for remanufacture guideline

    Strong coupling in the Kondo problem in the low-temperature region

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    The magnetic field dependence of the average spin of a localized electron coupled to conduction electrons with an antiferromagnetic exchange interaction is found for the ground state. In the magnetic field range ÎŒH∌0.5Tc\mu H\sim 0.5 T_c (TcT_c is the Kondo temperature) there is an inflection point, and in the strong magnetic field range ÎŒH≫Tc\mu H\gg T_c, the correction to the average spin is proportional to (Tc/ÎŒH)2(T_c/\mu H)^2. In zero magnetic field, the interaction with conduction electrons also leads to the splitting of doubly degenerate spin impurity states

    Black hole tidal problem in the Fermi normal coordinates

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    We derive a tidal potential for a self-gravitating fluid star orbiting Kerr black hole along a timelike geodesic extending previous works by Fishbone and Marck. In this paper, the tidal potential is calculated up to the third and fourth-order terms in R/rR/r, where RR is the stellar radius and rr the orbital separation, in the Fermi-normal coordinate system following the framework developed by Manasse and Misner. The new formulation is applied for determining the tidal disruption limit (Roche limit) of corotating Newtonian stars in circular orbits moving on the equatorial plane of Kerr black holes. It is demonstrated that the third and fourth-order terms quantitatively play an important role in the Roche limit for close orbits with R/r \agt 0.1. It is also indicated that the Roche limit of neutron stars orbiting a stellar-mass black hole near the innermost stable circular orbit may depend sensitively on the equation of state of the neutron star.Comment: Correct typo
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