Nonlinear stability of oscillatory wave fronts in chains of coupled oscillators

We present a stability theory for kink propagation in chains of coupled oscillators and a new algorithm for the numerical study of kink dynamics. The numerical solutions are computed using an equivalent integral equation instead of a system of differential equations. This avoids uncertainty about the impact of artificial boundary conditions and discretization in time. Stability results also follow from the integral version. Stable kinks have a monotone leading edge and move with a velocity larger than a critical value which depends on the damping strength.Comment: 11 figure

Molecular line probes of activity in galaxies

The use of specific tracers of the dense molecular gas phase can help to explore the feedback of activity on the interstellar medium (ISM) in galaxies. This information is a key to any quantitative assessment of the efficiency of the star formation process in galaxies. We present the results of a survey devoted to probe the feedback of activity through the study of the excitation and chemistry of the dense molecular gas in a sample of local universe starbursts and active galactic nuclei (AGNs). Our sample includes also 17 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs). From the analysis of the LIRGs/ULIRGs subsample, published in Gracia-Carpio et al.(2007) we find the first clear observational evidence that the star formation efficiency of the dense gas, measured by the L_FIR/L_HCN ratio, is significantly higher in LIRGs and ULIRGs than in normal galaxies. Mounting evidence of overabundant HCN in active environments would even reinforce the reported trend, pointing to a significant turn upward in the Kennicutt-Schmidt law around L_FIR=10^11 L_sun. This result has major implications for the use of HCN as a tracer of the dense gas in local and high-redshift luminous infrared galaxies.Comment: 4 pages, 2 figures, contributed paper to Far-Infrared Workshop 07 (FIR 2007

Succession planning as a business process of talent-management

In this globalized and changing world, companies are looking to be more competitive in order to stay in the market and at the forefront. To generate and maintain a sustainable competitive advantage, companies must not only have adequate organizational elements but also with the human capital best qualified to fulfill its responsibilities. Organizations know they must have the best talent to succeed in the hypercompetitive and increasingly complex global economy. It becomes, then, indispensable to ensure the continuity and permanence of the business over time, by identifying, developing and monitoring its staff with better performance and high potential, so that they are in positions strategic, and thus, value is created through people. For all above, succession plan becomes a strategic process of decision and action for the organization. Contrary to popular belief, succession planning is not a new phenomenon. Companies have been wrestling with ways to identify, develop, and retain their talent for decades. Therefore, why is succession planning suddenly popping up on every company’s radar screen? Today’s organizations are facing higher demands in a global market with the retirement of the Baby Boomers and the widening talent gap. The homegrown and paper-based succession planning that companies relied on in the past is no longer meeting the needs of today’s workforce. Companies need to upgrade and redefine their succession planning initiatives to ensure that their process will benefit both the individual and the overall strategy of the company. Talent management could be also defined as a useful term when it describes an organization's commitment to hire, manage, develop, and retain talented employees. It comprises all of the work processes and systems that are related to retaining and developing a superior workforce

Ripples in a string coupled to Glauber spins

Each oscillator in a linear chain (a string) interacts with a local Ising spin in contact with a thermal bath. These spins evolve according to Glauber dynamics. Below a critical temperature, a rippled state in the string is accompanied by a nonzero spin polarization. The system is shown to form ripples in the string which, for slow spin relaxation, vibrates rapidly about quasi-stationary states described as snapshots of a coarse-grained stroboscopic map. For moderate observation times, ripples are observed irrespective of the final thermodynamically stable state (rippled or not).Comment: 5 pages, 2 figure

Searching for molecular outflows in Hyper-Luminous Infrared Galaxies

We present constraints on the molecular outflows in a sample of five Hyper-Luminous Infrared Galaxies using Herschel observations of the OH doublet at 119 {\mu}m. We have detected the OH doublet in three cases: one purely in emission and two purely in absorption. The observed emission profile has a significant blueshifted wing suggesting the possibility of tracing an outflow. Out of the two absorption profiles, one seems to be consistent with the systemic velocity while the other clearly indicates the presence of a molecular outflow whose maximum velocity is about ~1500 km/s. Our analysis shows that this system is in general agreement with previous results on Ultra-luminous Infrared Galaxies and QSOs, whose outflow velocities do not seem to correlate with stellar masses or starburst luminosities (star formation rates). Instead the galaxy outflow likely arises from an embedded AGN.Comment: Accepted for publication in MNRAS. 13 pages, 11 figures, 4 table

Mechanical properties of double-layer and graded composite coatings of YSZ obtained by atmospheric plasma spraying

Double-layer and graded composite coatings of yttria-stabilized zirconia were sprayed on metallic substrates by atmospheric plasma spray. The coating architecture was built up by combining two different feedstocks: one micro- and one nanostructured. Microstructural features and mechanical properties (hardness and elastic modulus) of the coatings were determined by FE-SEM microscopy and nanoindentation technique, respectively. Additional adherence and scratch tests were carried out in order to assess the failure mechanisms occurring between the layers comprising the composites. Microstructural inspection of the coatings confirms the two-zone microstructure. This bimodal microstructure which is exclusive of the layer obtained from the nanostructured feedstock negatively affects the mechanical properties of the whole composite. Nanoindentation tests suitably reproduce the evolution of mechanical properties through coatings thickness on the basis of the position and/or amount of nanostructured feedstock used in the depositing layer. Adhesion and scratch tests show the negative effect on the coating adhesion of layer obtained from the nanostructured feedstock when this layer is deposited on the bond coat. Thus, the poor integrity of this layer results in lower normal stresses required to delaminate the coating in the adhesion test as well as minor critical load registered by using the scratch test.This work has been supported by the Spanish Ministry of Science and Innovation (Project MAT2012-38364-C03) and co-funded by ERDF (European Regional Development Funds).Carpio-Cobo, P.; Rayón Encinas, E.; Salvador Moya, MD.; Lusvarghi, L.; Sanchez, E. (2016). Mechanical properties of double-layer and graded composite coatings of YSZ obtained by atmospheric plasma spraying. Journal of Thermal Spray Technology. 25(4):778-787. https://doi.org/10.1007/s11666-016-0390-zS778787254Y.S. Tian, C.Z. Chen, D.Y. Wang, and J.I. Quianmao, Recent Developments in Zirconia Thermal Barrier Coatings, Surf. Rev. Lett., 2005, 12, p 369-378S. Sampath, U. Schulz, M.O. Jarligo, and S. Kuroda, Processing Science of Advanced Thermal-Barrier Systems, MRS Bull., 2012, 37(10), p 903-910D.R. Clarke, M. Oeschsner, and N.P. Padture, Thermal-Barrier Coatings for More Efficient Gas-Turbine Engines, MRS Bull., 2012, 37(10), p 891-898A. Feuersein, J. Knapp, T. Taylor, A. Ashary, A. Bolcavage, and N. Hitchman, Technical and Economical Aspects of Current Thermal Barrier Coating Systems for Gas Turbine Engines by Thermal Spray and EBPVD: A Review, J. Therm. Spray Technol., 2008, 17(2), p 199-213R.S. Lima and B.R. Marple, Thermal Spray Coatings Engineered from Nanostructured Ceramic Agglomerated Powders for Structural, Thermal Barrier and Biomedical Applications: A Review, J. Therm. Spray Technol., 2007, 16(1), p 40-63P. Fauchais, G. Montavon, R.S. Lima, and B.R. Marple, Engineering a New Class of Thermal Spray Nano-based Microstructures from Agglomerated Nanostructured Particles, Suspensions and Solutions: An Invited Review, J. Phys. D Appl. Phys., 2011, 44(9), p 093001P. Carpio, Q. Blochet, B. Pateyron, L. Pawlowski, M.D. Salvador, A. Borrell, and E. Sánchez, Correlation of Thermal Conductivity of Suspension Plasma Sprayed Yttira Stabilized Zirconia Coatings with some Microstructural Effects, Mater. Lett., 2013, 107, p 370-373R. Vassen, A. Stuke, and D. Stöver, Recent Developments in the Field of Thermal Barrier Coatings, J. Therm. Spray Technol., 2009, 18(2), p 181-186H. Dai, X. Zhong, J. Li, Y. Zhang, J. Meng, and X. Cao, Thermal Stability of Double-Ceramic-Layer Thermal Barrier Coatings with Various Coating Thickness, Mater. Sci. Eng. A—Struct., 2006, 433(1), p 1–7V. Viswanathan, G. Dwivedi, and S. Sampath, Multimaterial Thermal Barrier Coating Systems: Design, Synthesis, and Performance Assessment, J. Am. Ceram. Soc., 2015, 98(6), p 1769-1777M. Saremi and Z. Valefi, Thermal and Mechanical Properties of Nano-YSZ-Alumina Functionally Graded Coatings Deposited by Nano-agglomerated Powder Plasma Spraying, Ceram. Int., 2014, 40(8), p 13453-13459A. Portinham, V. Teixeira, J. Carneiro, J. Martins, M.F. Costa, R. Vassen, and D. Stoever, Characterization of Thermal Barrier Coatings with a Gradient Porosity, Surf. Coat. Technol., 2005, 195(2), p 245-251P. Carpio, E. Bannier, M.D. Salvador, R. Benavente, and E. Sánchez, Multilayer and Particle Size-Graded YSZ Coatings Obtained by Plasma Spraying of Micro- and Nanostructured Feedstocks, J. Therm. Spray Technol., 2014, 23(8), p 1362-1372S. Nath, I. Manna, and J.D. Majumdar, Nanomechanical Behavior of Yttria Stabilized Zirconia (YSZ) Based Thermal Barrier Coating, Ceram. Int., 2015, 41(4), p 5247-5256P. Carpio, E. Rayón, L. Pawlowski, A. Cattini, R. Benavente, E. Bannier, M.D. Salvador, and E. Sánchez, Microstructure and Indentation Mechanical Properties of YSZ Nanostructured Coatings Obtained by Suspension Plasma Spraying, Surf. Coat. Technol., 2013, 220, p 237-243H.B. Guo, H. Murakami, and S. Kuroda, Effect of Hollow Spherical Powder Size Distribution on Porosity and Segmentation Cracks in Thermal Barrier Coatings, J. Am. Ceram. Soc., 2006, 89(12), p 3797-3804R.S. Lima, A. Kucuk, and C.C. Berndt, Integrity of Nanostructured Partially Stabilized Zirconia After Plasma Spray Processing, Mater. Sci. Eng. A, 2001, 313(1), p 75-82E. Rayón, V. Bonache, M.D. Salvador, and E. Sánchez, Hardness and Young’s Modulus Distributions in Atmospheric Plasma Sprayed WC-Co Coatings Using Nanoindentation, Surf. Coat. Technol., 2011, 205(17), p 4192-4197J.A. Wollmershauser, B.N. Feigelson, E.P. Gorzkowski, C.T. Ellis, R. Goswami, S.B. Qadri, J.G. Tischler, F.J. Kub, and R.K. Everett, An Extend Hardness Limit in Bulk Nanoceramics, Acta Mater., 2014, 69, p 9-16L. Wang, Y. Wang, X.G. Sun, J.Q. He, Z.Y. Pan, and C.H. Wang, Microstructure and Indentation Mechanical Properties of Plasma Sprayed Nano-Bimodal and Conventional ZrO2-8 wt% Y2O3 Thermal Barrier Coatings, Vacuum, 2012, 86(8), p 1174-1185G.S. Barroso, W. Krenkel, and G. Motz, Low Thermal Conductivity Coating System for Application up to 1000 °C by Simple PDC Processing with Active and Passive Fillers, J. Eur. Ceram. Soc., 2015, 35(12), p 3339-3348R. Ghasemi, R. Shoja-Razavi, R. Mozafarinia, H. Jamali, M. Hajizadh-Oghaz, and R. Ahmadi-Pidani, The Influence of Laser Treatment on Hot Corrosion Behavior of Plasma-Sprayed Nanostructured Yttria Stabilized Zirconia Thermal Barrier Coatings, J. Eur. Ceram. Soc., 2014, 34(8), p 2013-2021E. Rayón, V. Bonache, M.D. Salvador, E. Bannier, E. Sánchez, A. Denoirjean, and H. Ageorges, Nanoindentation Study of the Mechanical and Damage Behaviour of Suspension Plasma Sprayed TiO2 Coatings, Surf. Coat. Technol., 2012, 206(10), p 2655-2660J.J. Roa, E. Jiménez-Piqué, R. Martínez, G. Ramírez, J.M. Tarragó, R. Rodríguez, and L. Llanes, Contact Damage and Fracture Micromechanisms of Multilayered TiN/CrN Coatings at Micro- and Nano-length Scales, Thin Solid Films, 2014, 571(2), p 308-31

Sub-arcsecond CO(1-0) and CO(2-1) observations of the ultraluminous infrared galaxy IRAS 10190+1322

We present the results of high resolution mapping of the CO(1-0) and CO(2-1) emission of the ultraluminous infrared galaxy (ULIRG) IRAS 10190+1322, with the IRAM interferometer, down to an angular resolution of ~0.3 arcsec. This object is composed of two interacting galaxies with a projected nuclear separation of 6 kpc, and was selected to analyze the physical and dynamical properties of the molecular gas in each galaxy in order to study the conditions that lead a galaxy pair to become ultraluminous in the infrared. With the exception of Arp 220, the closest ULIRG, this is the first time that the CO emission is morphologically and kinematically resolved in the two interacting galaxies of a ULIRG system. In one of the galaxies the molecular gas is highly concentrated, distributed in a circumnuclear disk of 1.7 kpc in size. The molecular gas in the presumably less infrared luminous galaxy is distributed in a more extended disk of 7.4 kpc. The molecular gas mass accounts for ~10% of the dynamical mass in each galaxy. Both objects are rich enough in molecular gas, Mgas ~ 4 10^9 Msun, as to experience an infrared ultraluminous phase.Comment: 4 pages, 3 figures. Accepted for publication in A&A Letters Special Issue for the new extended configuration of the Plateau de Bure Interferomete

Post-vaccination Symptoms with Second Dose of AstraZeneca in a Sample of Immunized Population of Ecuadorian Public Servants

Since AstraZeneca is a new vaccine against SARSCOV2, it should be monitored worldwide. This study presents the adverse reactions caused by the second dose of the AstraZeneca vaccine. Thequantitative, descriptive, cross-sectional research used a validated survey conducted on 428 public staff who were vaccinated with the second dose of the ChAdOx1-S vaccine at the Escuela Superior Politécnica de Chimborazo, the results were processed in Jamovi. 289 respondents reported having symptoms after inoculation, women (13.15%) presented more symptoms than men (7.27%). Most of the symptoms, both local and systemic, were mild and subsided with the administration of oral analgesics and lasted up to three days in 50% of the cases. AstraZeneca’s vaccine proves to be a safe biologic vaccine to generate antibodies against SARSCOV” in the adult population, and its use is therefore recommended. Keywords: drug-related side effects and adverse reactions, coronavirus infections, pharmacovigilance Resumen Introducción: Dado que se trata de una nueva vacuna contra el SARSCOV2, debe ser monitoreada a nivel mundial, el presente estudio presenta las reacciones adversas presentadas con la segunda dosis de la vacuna AstraZeneca. Materiales y Métodos: La presente investigación cuantitativa, descriptiva, transversal, utilizó una encuesta validada aplicada a 428 funcionarios públicos que fueron vacunados con la segunda dosis de la vacuna ChAdOx1- S en la Escuela Superior Politécnica de Chimborazo, los resultados fueron procesados en Jamovi . Resultados: 289 encuestados informaron tener síntomas después de la inoculación, las mujeres (13,15%) presentaron más síntomas que los hombres (7,27%). La mayoría de los síntomas, tanto locales como sistémicos, fueron leves y cedieron con la administración de analgésicos orales y duraron hasta tres días en el 50% de los casos. Conclusiones: La vacuna de AstraZeneca demuestra ser una vacuna biológica segura para generar anticuerpos frente al SARSCOV” en la población adulta, por lo que se recomienda su uso. Palabras Clave: kwd2

Chemically Distinct Nuclei and Outflowing Shocked Molecular Gas in Arp 220

We present the results of interferometric spectral line observations of Arp 220 at 3.5mm and 1.2mm from the Plateau de Bure Interferometer (PdBI), imaging the two nuclear disks in H$^{13}$CN$(1 - 0)$ and $(3 - 2)$, H$^{13}$CO$^+(1 - 0)$ and $(3 - 2)$, and HN$^{13}$C$(3 - 2)$ as well as SiO$(2 - 1)$ and $(6 - 5)$, HC$^{15}$N$(3 - 2)$, and SO$(6_6 - 5_5)$. The gas traced by SiO$(6 - 5)$ has a complex and extended kinematic signature including a prominent P Cygni profile, almost identical to previous observations of HCO$^+(3 - 2)$. Spatial offsets $0.1''$ north and south of the continuum centre in the emission and absorption of the SiO$(6 - 5)$ P Cygni profile in the western nucleus (WN) imply a bipolar outflow, delineating the northern and southern edges of its disk and suggesting a disk radius of $\sim40$ pc, consistent with that found by ALMA observations of Arp 220. We address the blending of SiO$(6 - 5)$ and H$^{13}$CO$^+(3 - 2)$ by considering two limiting cases with regards to the H$^{13}$CO$^+$ emission throughout our analysis. Large velocity gradient (LVG) modelling is used to constrain the physical conditions of the gas and to infer abundance ratios in the two nuclei. Our most conservative lower limit on the [H$^{13}$CN]/[H$^{13}$CO$^+$] abundance ratio is 11 in the WN, cf. 0.10 in the eastern nucleus (EN). Comparing these ratios to the literature we argue on chemical grounds for an energetically significant AGN in the WN driving either X-ray or shock chemistry, and a dominant starburst in the EN.Comment: 28 pages, 17 figures, accepted to Ap