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  • Oxford University Press  (22)
  • American Physical Society (APS)  (5)
  • American Institute of Physics (AIP)
  • 2010-2014  (27)
  • 1
    Publication Date: 2013-10-01
    Description: Author(s): L. Caron, M. Hudl, V. Höglin, N. H. Dung, C. P. Gomez, M. Sahlberg, E. Brück, Y. Andersson, and P. Nordblad Magnetic and magnetocaloric properties of high-purity, giant magnetocaloric polycrystalline and single-crystalline Fe 2 P are investigated. Fe 2 P displays a moderate magnetic entropy change, which spans over 70 K and the presence of strong magnetization anisotropy proves this system is not fully itiner... [Phys. Rev. B 88, 094440] Published Mon Sep 30, 2013
    Keywords: Magnetism
    Print ISSN: 1098-0121
    Electronic ISSN: 1095-3795
    Topics: Physics
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  • 2
    Publication Date: 2012-04-10
    Description: Author(s): M. A. L. Capri, A. J. Gómez, M. S. Guimaraes, V. E. R. Lemes, S. P. Sorella, and D. G. Tedesco A qualitative study of the lightest glueball states in Euclidean S U (2) Yang-Mills theory quantized in the maximal Abelian gauge is presented. The analysis is done by generalizing to the maximal Abelian gauge the so-called replica model, already successfully introduced in the Landau gauge. As it will... [Phys. Rev. D 85, 085012] Published Mon Apr 09, 2012
    Keywords: Field theory, formal particle theory
    Print ISSN: 0556-2821
    Electronic ISSN: 1089-4918
    Topics: Physics
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  • 3
    Publication Date: 2012-06-22
    Description: Author(s): M. Cannoni, M. E. Gómez, M. A. Pérez-García, and J. D. Vergados We discuss the possibility that colliding dark matter particles in the form of neutralinos may be gravitationally boosted near the supermassive black hole at the Galactic center so that they can have enough collision energy to annihilate into a stau pair. Since in some phenomenologically favored sup... [Phys. Rev. D 85, 115015] Published Thu Jun 21, 2012
    Keywords: Beyond the standard model
    Print ISSN: 0556-2821
    Electronic ISSN: 1089-4918
    Topics: Physics
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  • 4
    Publication Date: 2011-05-03
    Description: Author(s): M. A. L. Capri, A. J. Gómez, M. S. Guimaraes, V. E. R. Lemes, S. P. Sorella, and D. G. Tedesco In previous work by M. A. L. Capri, A. J. Gomez, M. S. Guimaraes, V. E. R. Lemes, S. P. Sorella, and D. G. Tedesco [Phys. Rev. D 82, 105019 (2010)], we have shown that the soft breaking of the Becchi-Rouet-Stora-Tyutin (BRST) symmetry arising within the Gribov-Zwanziger framework can... [Phys. Rev. D 83, 105001] Published Mon May 02, 2011
    Keywords: D15
    Print ISSN: 0556-2821
    Electronic ISSN: 1089-4918
    Topics: Physics
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  • 5
    Publication Date: 2013-12-06
    Description: We present new deep near-infrared broad- and narrow-band imaging and low-resolution spectroscopy of the star formation region RCW 121 (IRAS 17149–3916) which we analyse in combination with Herschel (70, 160, 250, 350 and 500 μm) and Spitzer (3.6, 4.5, 5.8 and 8 μm) images. The near-infrared photometry reveals the presence of a stellar cluster of approximate size of 92 arcsec which is composed of at least 264 members, approximately 25 per cent of these showing excess emission at 〉 2.0 μm, indicative of circumstellar discs. Isochrones corresponding to ages 0.5–1.0 Myr and A V  = 7.8 fit well the position of a large fraction of likely cluster members in the K s versus H – K s diagram. We find three massive star-forming cores located in the boundaries of an expanding H ii region ionized by a central O-type star. From their far-infrared spectral energy distributions (SEDs) we derive masses and temperatures of the dense cores. When these young stellar objects (YSOs) have warm emission components, the 1.2–500 μm SEDs are fitted with Robitaille et al.'s star–disc-envelope model to obtain their physical parameters. The masses of the three YSOs are between 8 and 10 M . The youngest site (core I) is undetected at 〈 100 μm and is at the earliest evolutionary stage that can currently be detected. The other two cores (II and III) contain YSOs of similar masses and have near-infrared counterparts, which imply a more advanced evolutionary stage. The YSO at core II has been found to have associated a jet, with strong H 2 line emission, co-existing with an H 2 O maser source. RCW 121 is another example of multiple star formation being triggered by the expansion of a single H ii region.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 6
    Publication Date: 2013-10-16
    Description: Author(s): M. A. L. Capri, D. Dudal, A. J. Gómez, M. S. Guimaraes, I. F. Justo, S. P. Sorella, and D. Vercauteren We present an analytical study of continuum 4 d S U (2) gauge-Higgs models with a single Higgs field with fixed length in either the fundamental or adjoint representation. We aim at analytically probing the renowned predictions of Fradkin and Shenker on the phase diagram in terms of confinement versus ... [Phys. Rev. D 88, 085022] Published Tue Oct 15, 2013
    Keywords: Field theory, formal particle theory
    Print ISSN: 0556-2821
    Electronic ISSN: 1089-4918
    Topics: Physics
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  • 7
    Publication Date: 2014-03-30
    Description: Insertion sequences (ISs) are small transposable elements widespread in bacterial genomes, where they play an essential role in chromosome evolution by stimulating recombination and genetic flow. Despite their ubiquity, it is unclear how ISs interact with the host. Here, we report a survey of the orientation patterns of ISs in bacterial chromosomes with the objective of gaining insight into the interplay between ISs and host chromosomal functions. We find that a significant fraction of IS families present a consistent and family-specific orientation bias with respect to chromosomal DNA replication, especially in Firmicutes. Additionally, we find that the transposases of up to nine different IS families with different transposition pathways interact with the β sliding clamp, an essential replication factor, suggesting that this is a widespread mechanism of interaction with the host. Although we find evidence that the interaction with the β sliding clamp is common to all bacterial phyla, it also could explain the observed strong orientation bias found in Firmicutes, because in this group β is asymmetrically distributed during synthesis of the leading or lagging strands. Besides the interaction with the β sliding clamp, other asymmetries also play a role in the biased orientation of some IS families. The utilization of the highly conserved replication sliding clamps suggests a mechanism for host regulation of IS proliferation and also a universal platform for IS dispersal and transmission within bacterial populations and among phylogenetically distant species.
    Electronic ISSN: 1759-6653
    Topics: Biology
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  • 8
    Publication Date: 2014-12-13
    Description: Grapevine leafroll disease threatens the economic sustainability of the grape and wine industry in the United States and around the world. This viral disease reduces yield, delays fruit ripening, and affects wine quality. Although there is new information on the disease spatial-dynamic diffusion, little is known about profit-maximizing control strategies. Using cellular automata, we model the disease spatial-dynamic diffusion for individual plants in a vineyard, evaluate nonspatial and spatial control strategies, and rank them based on vineyard expected net present values. Nonspatial strategies consist of roguing and replacing symptomatic grapevines. In spatial strategies, symptomatic vines are rogued and replaced, and their nonsymptomatic neighbors are virus-tested, then rogued and replaced if the test is positive. Both nonspatial and spatial classes of strategies are formulated and examined with and without considering vine age. We find that spatial strategies targeting immediate neighbors of symptomatic vines dominate nonspatial strategies, increasing the vineyard expected net present value by 18% to 19% relative to the strategy of no disease control. We also find that age-structured disease control is preferred to non-age-structured control but only for nonspatial strategies. Sensitivity analyses show that disease eradication is possible if either the disease transmission rate or the virus undetectability period is substantially reduced.
    Keywords: C15 - Simulation Methods, C63 - Computational Techniques, D24 - Production ; Cost ; Capital and Total Factor Productivity ; Capacity
    Print ISSN: 0002-9092
    Electronic ISSN: 1467-8276
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition , Economics
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  • 9
    Publication Date: 2014-12-14
    Description: In this first paper, we simulate the population of disc red clump stars to be observed by Gaia . We generate a set of test particles and we evolve it in a 3D barred Milky Way like galactic potential. We assign physical properties of the red clump trace population and a realistic 3D interstellar extinction model. We add Gaia observational constraints and an error model according to the pre-commissioning scientific performance assessments. We present and analyse two mock catalogues, offered to the community, that are an excellent test bed for testing tools being developed for the future scientific exploitation of Gaia data. The first catalogue contains stars up to Gaia G ~20, while the second is the subset containing Gaia radial velocity data with a maximum error of $\sigma _{V_{\rm r}}=10$ km s –1 . Here, we present first attempts to characterize the density structure of the Galactic bar in the Gaia space of observables. The Gaia large errors in parallax and the high interstellar extinction in the inner parts of the Galactic disc prevent us to model the bar overdensity. This result suggests the need to combine Gaia and IR data to undertake such studies. We find that IR photometric distances for this Gaia sample allow us to recover the Galactic bar orientation angle with an accuracy of ~5°.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 10
    Publication Date: 2014-04-11
    Description: We map the kinematics of stars in simulated galaxy discs with spiral arms using the velocity ellipsoid vertex deviation ($l_{\rm v}$). We use test particle simulations, and for the first time, fully self-consistent high-resolution N -body models. We compare our maps with the tight winding approximation model analytical predictions. We see that for all barred models, spiral arms rotate closely to a rigid body manner and the vertex deviation values correlate with the density peak's position bounded by overdense and underdense regions. In such cases, vertex deviation sign changes from negative to positive when crossing the spiral arms in the direction of disc rotation, in regions where the spiral arms are in between corotation radius (CR) and the Outer Lindblad Resonance (OLR). By contrast, when the arm sections are inside the CR and outside the OLR, $l_{\rm v}$ changes from negative to positive. We propose that measurements of the vertex deviation's pattern can be used to trace the position of the main resonances of the spiral arms. We propose that this technique might exploit future data from Gaia and APO Galactic Evolution Experiment (APOGEE) surveys. For unbarred N -body simulations with spiral arms corotating with disc material at all radii, our analysis suggests that no clear correlation exists between $l_{\rm v}$ and density structures.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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