14,412 research outputs found

    Entitled to a sustainable career? Motherhood in science, engineering and technology

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    Sustaining careers and motherhood is particularly challenging in highly masculinised science, engineering and technology (SET) sectors. We explore this issue using a social comparison theory perspective, drawing on interviews with professional engineers and scientists from four companies, located in Italy, France and the Netherlands. We examine how decisions to reduce working hours are influenced by perceived ideological, normative and policy contexts. Despite contextual differences in opportunities and perceived entitlements and supports for family-friendly working hours, we found that sense of entitlement to do so without forfeiting career progression is limited across all the contexts. This attests to the enduring power of gendered organizational assumptions about ideal SET careers. Nevertheless we present examples of three women who achieved senior roles despite working reduced hours and discuss combinations of conditions which may facilitate sustainable careers and caring roles

    On CrC^r-closing for flows on 2-manifolds

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    For some full measure subset B of the set of iet's (i.e. interval exchange transformations) the following is satisfied: Let X be a CrC^r, 1r1\le r\le \infty, vector field, with finitely many singularities, on a compact orientable surface M. Given a nontrivial recurrent point pMp\in M of X, the holonomy map around p is semi-conjugate to an iet E:[0,1)[0,1).E :[0,1) \to [0,1). If EBE\in B then there exists a CrC^r vector field Y, arbitrarily close to X, in the CrC^r-topology, such that Y has a closed trajectory passing through p.Comment: 7 pages, 1 figur

    Ytterbium-doped tantalum pentoxide waveguide lasers

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    We have demonstrated a Yb:Ta2O5 waveguide laser fabricated by RF magnetron sputtering on oxidised silicon. The waveguide laser was end-pumped with a laser diode at 977 nm and lasing was observed between 1015 and 1020 nm. The launched pump power threshold and slope efficiency were measured to be ~25 mW and 1.78 %, respectively

    Around The Map

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    https://digitalcommons.library.umaine.edu/mmb-ps/1370/thumbnail.jp

    Here Comes Tootsi

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    https://digitalcommons.library.umaine.edu/mmb-vp/1452/thumbnail.jp

    My Waltz Queen: Waltz Song

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    https://digitalcommons.library.umaine.edu/mmb-vp/2249/thumbnail.jp

    A CrC^{r} Closing Lemma for a Class of Symplectic Diffeomorphisms

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    We prove a CrC^r closing lemma for a class of partially hyperbolic symplectic diffeomorphisms. We show that for a generic CrC^r symplectic diffeomorphism, r=1,2,...,r =1, 2, ...,, with two dimensional center and close to a product map, the set of all periodic points is dense

    Removing black-hole singularities with nonlinear electrodynamics

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    We propose a way to remove black hole singularities by using a particular nonlinear electrodynamics Lagrangian that has been recently used in various astrophysics and cosmological frameworks. In particular, we adapt the cosmological analysis discussed in a previous work to the black hole physics. Such analysis will be improved by applying the Oppenheimer-Volkoff equation to the black hole case. At the end, fixed the radius of the star, the final density depends only on the introduced quintessential density term ργ\rho_{\gamma} and on the mass.Comment: In this last updated version we correct two typos which were present in Eqs. (21) and (22) in the version of this letter which has been published in Mod. Phys. Lett. A 25, 2423-2429 (2010). In the present version, both of Eqs. (21) and (22) are dimensionally and analytically correc

    Revealing the Dusty Warm Absorber in MCG--6-30-15 with the Chandra HETG

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    We present detailed evidence for a warm absorber in the Seyfert 1 galaxy MCG--6-30-15 and dispute earlier claims for relativistic O line emission. The HETG spectra show numerous narrow, unresolved (FWHM < 200 km/s) absorption lines from a wide range of ionization states of N, O, Mg, Ne, Si, S, Ar, and Fe. The O VII edge and 1s^2--1snp resonance line series to n=9 are clearly detected at rest in the AGN frame. We attribute previous reports of an apparently highly redshifted O VII edge to the 1s^2--1snp (n > 5) O VII resonance lines, and a neutral Fe L absorption complex. The shape of the Fe L feature is nearly identical to that seen in the spectra of several X-ray binaries, and in laboratory data. The implied dust column density agrees with that obtained from reddening studies, and gives the first direct X-ray evidence for dust embedded in a warm absorber. The O VIII resonance lines and weak edge are also detected, and the spectral rollover below 2 keV is explained by the superposition of numerous absorption lines and edges. We identify, for the first time, a KLL resonance in the O VI photoabsorption cross section, giving a measure of the O VI column density. The O VII (f) emission detected at the systemic velocity implies a covering fraction of ~5% (depending on the observed vs. time-averaged ionizing flux). Our observations show that a dusty warm absorber model is not only adequate to explain all the spectral features > 0.48 keV (< 26 \AA) the data REQUIRE it. This contradicts the interpretation of Branduardi-Raymont et al. (2001) that this spectral region is dominated by highly relativistic line emission from the vicinity of the black hole.Comment: 4.5 pages, 1 color figure, accepted (April 2001) for publication in ApJL, not many changes from the initial submission - updated/added some measuements for the O VII resonance series, and added a discussion about FeO2 grain
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