Time-dependent density-functional theory approach to nonlinear particle-solid interactions in comparison with scattering theory

An explicit expression for the quadratic density-response function of a many-electron system is obtained in the framework of the time-dependent density-functional theory, in terms of the linear and quadratic density-response functions of noninteracting Kohn-Sham electrons and functional derivatives of the time-dependent exchange-correlation potential. This is used to evaluate the quadratic stopping power of a homogeneous electron gas for slow ions, which is demonstrated to be equivalent to that obtained up to second order in the ion charge in the framework of a fully nonlinear scattering approach. Numerical calculations are reported, thereby exploring the range of validity of quadratic-response theory.Comment: 14 pages, 3 figures. To appear in Journal of Physics: Condensed Matte

Lumbosacral column arthtodesis with a system's implant

Lumbosacral column arthrodesis with bone graft and metallic fixation (A-Systems implant) was carried out in 40 patients with spondylolisthesis and lumbosacral instability of the following types: isthmic-lytic in 13, degenerative in 19, traumatic in 2, pathological in 1, and surgical in 5. Preoperative, immediate postoperative, and late postoperative clinical and radiological evaluation was carried out. Clinical follow-up ranged from 10 to 46 months (mean follow-up: 11 months). Patient's and Physician's overall evaluation showed the following results: good results in 36 (39%) patients; improvement as compared to preoperative condition in 3 (7.5%); unchanged condition in 1 (2.5%); normalized labor capability in 29 (72.5%) patients; improvement of 75% in labor capability in 9 (22.5%) patients; and improvement of 50% in 2 (5%) patients. As for the Prolo rate, an increase to 9-10 (excellent) was seen in 21 (52.5%) patients; an increase to 7 and 8 (good) was seen in 14 (35%); an increase to 5 to 6 (moderate) was found in 5 (12.5%) patients. No patient had a Prolo rate of 2, 3, or 4 (poor). Mean time until return to normal activities ranged from 3 to 12 months (mean: 7 months). As compared to similar methods reported in literature, the implant has been shown to be equaally effective, with the following advantages: simplicity, use at different levels; rigidity following assembly.Foram avaliados 40 pacientes com espondilolistese e instabilidade lombossacra: 13 pacientes do tipo ístmica-lítica, 19 do tipo degenerativa, 2 pacientes do tipo traumática, 1 tipo do patológica, e 5 do tipo cirúrgica, nos quais foram realizadas 40 artrodeses da coluna lombossacra com enxerto ósseo e fixação metálica com o implante A-Systems. A avaliação dos pacientes foi realizada clínica e radiograficamente, nos períodos pré-operatório, pós-operatório imediato e pós-operatório tardio. O tempo de acompanhamento clínico máximo foi de 46 meses, o mínimo de 10 meses, obtendo-se um acompanhamento médio de 11 meses. A avaliação global tanto do ponto vista do paciente como da equipe médica mostrou que: 36 (90%) dos pacientes obtiveram bom resultado; três pacientes (7,5%) apresentaram melhora em relação ao pré-operatório e um paciente (2,5%) não obteve melhora. Vinte e nove pacientes (72,5%) tiveram sua capacidade de trabalho normalizada, nove (22,5%) pacientes tiveram sua capacidade melhorada em 75% e dois (5%) pacientes tiveram a capacidade melhorada em 50%. Vinte e um pacientes (52,5%) tiveram o índice de Prolo aumentado entre 9 e 10 (excelente); 14 (35%) tiveram índice de Prolo aumentado para 7 e 8 (bom); em 5 (12,5%) o índice ficou entre 5 e 6 (regular) e nenhum paciente teve índice 2, 3 ou 4 (mau). O tempo médio de retorno para as atividades normais variou de três a doze meses, com uma média de sete meses. Em comparação com métodos similares relatados pela literatura, o implante mostrou-se tão eficiente quanto eles, com as vantagens da simplicidade, da possibilidade de ser usado em vários níveis e da rigidez após montado.Pontíficia Universidade Católica do Rio Grande do Sul Hospital São Lucas Serviço de Ortopedia e TraumatologiaUniversidade de São Paulo Faculdade de MedicinaUniversidade Federal de São Paulo (UNIFESP) Escola Paulista de Medicina Departamento de Ortopedia e TraumatologiaUNIFESP, EPM, Depto. de Ortopedia e TraumatologiaSciEL

First-light LBT nulling interferometric observations: warm exozodiacal dust resolved within a few AU of eta Corvi

We report on the first nulling interferometric observations with the Large Binocular Telescope Interferometer (LBTI), resolving the N' band (9.81 - 12.41 um) emission around the nearby main-sequence star eta Crv (F2V, 1-2 Gyr). The measured source null depth amounts to 4.40% +/- 0.35% over a field-of-view of 140 mas in radius (~2.6\,AU at the distance of eta Corvi) and shows no significant variation over 35{\deg} of sky rotation. This relatively low null is unexpected given the total disk to star flux ratio measured by Spitzer/IRS (~23% across the N' band), suggesting that a significant fraction of the dust lies within the central nulled response of the LBTI (79 mas or 1.4 AU). Modeling of the warm disk shows that it cannot resemble a scaled version of the Solar zodiacal cloud, unless it is almost perpendicular to the outer disk imaged by Herschel. It is more likely that the inner and outer disks are coplanar and the warm dust is located at a distance of 0.5-1.0 AU, significantly closer than previously predicted by models of the IRS spectrum (~3 AU). The predicted disk sizes can be reconciled if the warm disk is not centrosymmetric, or if the dust particles are dominated by very small grains. Both possibilities hint that a recent collision has produced much of the dust. Finally, we discuss the implications for the presence of dust at the distance where the insolation is the same as Earth's (2.3 AU).Comment: 9 pages, 6 figures, accepted for publication in Ap

Testing the Distraction Hypothesis:do extrafloral nectaries reduce ant-pollinator conflict?

1. Ant guards protect plants from herbivores, but can also hinder pollination by damaging reproductive structures and/or repelling pollinators. Natural selection should favour the evolution of plant traits that deter ants from visiting flowers during anthesis, without waiving their defensive services. The Distraction Hypothesis posits that rewarding ants with extrafloral nectar could reduce their visitation of flowers, reducing ant-pollinator conflict while retaining protection of other structures. 2. We characterised the proportion of flowers occupied by ants and the number of ants per flower in a Mexican ant-plant, Turnera velutina. We clogged extrafloral nectaries on field plants and observed the effects on patrolling ants, pollinators and ants inside flowers, and quantified the effects on plant fitness. Based on the Distraction Hypothesis we predicted that preventing extrafloral nectar secretion should result in fewer ants active at extrafloral nectaries, more ants inside flowers and a higher proportion of flowers occupied by ants, leading to ant-pollinator conflict, with reduced pollinator visitation and reduced plant fitness. 3. Overall ant activity inside flowers was low. Preventing extrafloral nectar secretion through clogging reduced the number of ants patrolling extrafloral nectaries, significantly increased the proportion of flowers occupied by ants from 6.1% to 9.7%, and reduced plant reproductive output through a 12% increase in the probability of fruit abortion. No change in the numbers of ants or pollinators inside flowers was observed. This is the first support for the Distraction Hypothesis obtained under field conditions, showing ecological and plant fitness benefits of the distracting function of extrafloral nectar during anthesis. 4. Synthesis: Our study provides the first field experimental support for the Distraction Hypothesis, suggesting that extrafloral nectaries located close to flowers may bribe ants away from reproductive structures during the crucial pollination period, reducing the probability of ant-occupation of flowers, reducing ant-pollinator conflict, and increasing plant reproductive success

The HOSTS Survey for Exozodiacal Dust: Preliminary results and future prospects

[abridged] The presence of large amounts of dust in the habitable zones of nearby stars is a significant obstacle for future exo-Earth imaging missions. We executed an N band nulling interferometric survey to determine the typical amount of such exozodiacal dust around a sample of nearby main sequence stars. The majority of our data have been analyzed and we present here an update of our ongoing work. We find seven new N band excesses in addition to the high confidence confirmation of three that were previously known. We find the first detections around Sun-like stars and around stars without previously known circumstellar dust. Our overall detection rate is 23%. The inferred occurrence rate is comparable for early type and Sun-like stars, but decreases from 71% [+11%/-20%] for stars with previously detected mid- to far-infrared excess to 11% [+9%/-4%] for stars without such excess, confirming earlier results at high confidence. For completed observations on individual stars, our sensitivity is five to ten times better than previous results. Assuming a lognormal luminosity function of the dust, we find upper limits on the median dust level around all stars without previously known mid to far infrared excess of 11.5 zodis at 95% confidence level. The corresponding upper limit for Sun-like stars is 16 zodis. An LBTI vetted target list of Sun-like stars for exo-Earth imaging would have a corresponding limit of 7.5 zodis. We provide important new insights into the occurrence rate and typical levels of habitable zone dust around main sequence stars. Exploiting the full range of capabilities of the LBTI provides a critical opportunity for the detailed characterization of a sample of exozodiacal dust disks to understand the origin, distribution, and properties of the dust.Comment: To appear in SPIE Astronomical Telescopes + Instrumentation 2018 proceedings. Some typos fixed, one reference adde

Primer caso registrado de hernia discal torácica operada en Paraguay. Dificultades y desafíos

La hernia discal de la columna torácica sintomática con indicación quirúrgica es poco frecuente. La dificultad para el diagnóstico temprano radica en encontrar signos y síntomas que orienten a solicitar la Resonancia Magnética Nuclear de la columna a nivel torácica para obtener una rápida identificación del fenómeno compresivo sobre la médula espinal. El objetivo de este trabajo es realizar la presentación de la primera hernia discal de la columna torácica tratada quirúrgicamente en forma exitosa en Paraguay, discutir la historia natural y determinar las dificultades del diagnóstico clínico y manejo quirúrgico. El caso presentado es el de un paciente de sexo masculino, de 61 años, con historia de dolor lumbar y posterior debilidad progresiva rápida del miembro inferior izquierdo hasta la paraplejia. Los datos de la rutina laboratorial de sangre y líquido cefalorraquídeo, ni estudios electromiográficos mostraron un patrón típico. El estudio por imágenes determinó con precisión el diagnostico. El tratamiento quirúrgico constituyó un abordaje anterior transtorácico, intrapleural y disectomía parcial de una de una hernia fibrosa dura, sin necesidad de adicionar algún sistema de artrodesis. La evolución fue excelente con recuperación total de la movilidad y sensibilidad de los miembros inferiores

Mitochondrial Cumulative Damage Induced by Mitoxantrone: Late Onset Cardiac Energetic Impairment

Mitoxantrone (MTX) is a chemotherapeutic agent, which presents late irreversible cardiotoxicity. This work aims to highlight the mechanisms involved in the MTX-induced cardiotoxicity, namely the effects toward mitochondria using in vivo and in vitro studies. Male Wistar rats were treated with 3 cycles of 2.5 mg/kg MTX at day 0, 10, and 20. One treated group was euthanized on day 22 (MTX22) to evaluate the early MTX cardiac toxic effects, while the other was euthanized on day 48 (MTX48), to allow the evaluation of MTX late cardiac effects. Cardiac mitochondria isolated from 4 adult untreated rats were also used to evaluate in vitro the MTX (10 nM, 100 nM, and 1 lM) direct effects upon mitochondria functionality. Two rats of MTX48 died on day 35, and MTX treatment caused a reduction in relative body weight gain in both treated groups with no significant changes in water and food intake. Decreased levels of plasma total creatine kinase and CK-MB were detected in the MTX22 group, and increased plasma levels of lactate were seen in MTX48. Increased cardiac relative mass and microscopic changes were evident in both treated groups. Considering mitochondrial effects, for the first time, it was evidenced that MTX induced an increase in the complex IV and complex V activities in MTX22 group, while a decrease in the complex V activity was accompanied by the reduction in ATP content in the MTX48 rats. No alterations in mitochondria transmembrane potential were found in isolated mitochondria from MTX48 rats or in isolated mitochondria directly incubated with MTX. This study highlights the relevance of the cumulative MTX-induced in vivo mitochondriopathy to the MTX cardiotoxicity.This work was supported by the Fundação para a Ciência e Tecnologia (FCT)—project (EXPL/DTP-FTO/0290/ 2012)—QREN initiative with EU/FEDER financing through COMPETE— Operational Programme for Competitiveness Factors. LGR, VMC, and RJD-O thank FCT for their PhD Grant (SFRH/BD/63473/ 2009) and Post-doc Grants (SFRH/BPD/63746/2009) and (SFRH/ BPD/36865/2007), respectively. The authors are grateful to Fundação para a Ciência e Tecnologia for grant no. Pest C/EQB/LA0006/2011

Vacuum decay in quantum field theory

We study the contribution to vacuum decay in field theory due to the interaction between the long and short-wavelength modes of the field. The field model considered consists of a scalar field of mass $M$ with a cubic term in the potential. The dynamics of the long-wavelength modes becomes diffusive in this interaction. The diffusive behaviour is described by the reduced Wigner function that characterizes the state of the long-wavelength modes. This function is obtained from the whole Wigner function by integration of the degrees of freedom of the short-wavelength modes. The dynamical equation for the reduced Wigner function becomes a kind of Fokker-Planck equation which is solved with suitable boundary conditions enforcing an initial metastable vacuum state trapped in the potential well. As a result a finite activation rate is found, even at zero temperature, for the formation of true vacuum bubbles of size $M^{-1}$. This effect makes a substantial contribution to the total decay rate.Comment: 27 pages, RevTeX, 1 figure (uses epsf.sty

Vacuum decay in quantum field theory

We study the contribution to vacuum decay in field theory due to the interaction between the long and short-wavelength modes of the field. The field model considered consists of a scalar field of mass $M$ with a cubic term in the potential. The dynamics of the long-wavelength modes becomes diffusive in this interaction. The diffusive behaviour is described by the reduced Wigner function that characterizes the state of the long-wavelength modes. This function is obtained from the whole Wigner function by integration of the degrees of freedom of the short-wavelength modes. The dynamical equation for the reduced Wigner function becomes a kind of Fokker-Planck equation which is solved with suitable boundary conditions enforcing an initial metastable vacuum state trapped in the potential well. As a result a finite activation rate is found, even at zero temperature, for the formation of true vacuum bubbles of size $M^{-1}$. This effect makes a substantial contribution to the total decay rate.Comment: 27 pages, RevTeX, 1 figure (uses epsf.sty