Intrinsic versus super-rough anomalous scaling in spontaneous imbibition

We study spontaneous imbibition using a phase field model in a two dimensional system with a dichotomic quenched noise. By imposing a constant pressure $\mu_{a}<0$ at the origin, we study the case when the interface advances at low velocities, obtaining the scaling exponents $z=3.0\pm 0.1$, $\alpha=1.50\pm 0.02$ and $\alpha_{loc}= 0.95\pm 0.03$ within the intrinsic anomalous scaling scenario. These results are in quite good agreement with experimental data recently published. Likewise, when we increase the interface velocity, the resulting scaling exponents are $z=4.0 \pm 0.1$, $\alpha=1.25\pm 0.02$ and $\alpha_{loc}= 0.95\pm 0.03$. Moreover, we observe that the local properties of the interface change from a super-rough to an intrinsic anomalous description when the contrast between the two values of the dichotomic noise is increased. From a linearized interface equation we can compute analytically the global scaling exponents which are comparable to the numerical results, introducing some properties of the quenched noise.Comment: Accepted for publication in Physical Review

Influence of Disorder Strength on Phase Field Models of Interfacial Growth

We study the influence of disorder strength on the interface roughening process in a phase-field model with locally conserved dynamics. We consider two cases where the mobility coefficient multiplying the locally conserved current is either constant throughout the system (the two-sided model) or becomes zero in the phase into which the interface advances (one-sided model). In the limit of weak disorder, both models are completely equivalent and can reproduce the physical process of a fluid diffusively invading a porous media, where super-rough scaling of the interface fluctuations occurs. On the other hand, increasing disorder causes the scaling properties to change to intrinsic anomalous scaling. In the limit of strong disorder this behavior prevails for the one-sided model, whereas for the two-sided case, nucleation of domains in front of the invading front are observed.Comment: Accepted for publication in PR

Avaliação da composição química das espigas de três híbridos de milho (Zea mays L.) em quatro estádios de maturação.

O objetivo deste experimento foi avaliar a composição química das espigas dos três híbridos de milho BRS 1035, BRS 1031 e BRS 1001 em quatro idades de corte, a partir da determinação dos parâmetros: matéria seca (MS), proteína bruta (PB), fibra detergente neutro (FDN) e fibra detergente ácido (FDA). O delineamento utilizado foi inteiramente casualizado com fatorial3 (híbridos) x 4 (idades de corte), sendo as médias comparadas pelo teste SNK (P<0,05). Todos os híbridos demonstraram um aumento do teor de MS de 87 para 171 dias, com diferença (P<0,05) entre todos os cortes. Não houve diferença (P<0,05) nos valores de PB entre os cortes em todos os híbridos. Aos 94 dias o híbrido BRS 1001 (5,67%) demonstrou um valor de PB superior (P<0,05) ao BRS 1031 (4,66%) e ambos foram semelhantes (P<0,05) ao BRS 1035 (5,11%). Todos os híbridos apresentaram uma queda dos valores de FDN com o avanço da maturidade até 101 dias. A variação dos valores de FDA da espiga foi muito semelhante à variação do FDN já que a correlação dessas características foi 0,97 (P<0,001). Não houve diferença (P<0,05) nos valores de FDA entre os híbridos dentro dos cortes. Os híbridos avaliados neste experimento apresentaram as mesmas tendências de aumento da MS da' espiga com o avançar da maturidade fisiológica com provável acúmulo de amido na espiga, reduzindo os teores de carboidratos estruturais como FDN e FDA nessa fração da planta

Efeito da bracatinga (Mimosa scabrella) na produção de matéria seca de pastagem sob sistema silvipastorial.

Edición de las Memorias de la 22a. Reunión ALPA, 2011, Montevideo. E68 Poster

Mode identification in the high-amplitude {\delta} Scuti star V2367 Cyg

We report on a multi-site photometric campaign on the high-amplitude $\delta$ Scuti star V2367 Cyg in order to determine the pulsation modes. We also used high-dispersion spectroscopy to estimate the stellar parameters and projected rotational velocity. Time series multicolour photometry was obtained during a 98-d interval from five different sites. These data were used together with model atmospheres and non-adiabatic pulsation models to identify the spherical harmonic degree of the three independent frequencies of highest amplitude as well as the first two harmonics of the dominant mode. This was accomplished by matching the observed relative light amplitudes and phases in different wavebands with those computed by the models. In general, our results support the assumed mode identifications in a previous analysis of Kepler data.Comment: 9 pages, 5 figures, 4 tables. Accepted for publication in MNRA

Ultrahigh energy neutrinos and non-linear QCD dynamics

The ultrahigh energy neutrino-nucleon cross sections are computed taking into account different phenomenological implementations of the non-linear QCD dynamic s. Based on the color dipole framework, the results for the saturation model supplemented by DGLAP evolution as well as for the BFKL formalism in the geometric scaling regime are presented. They are contrasted with recent calculations using NLO DGLAP and unified BFKL-DGLAP formalisms.Comment: 5 pages, 2 figures. Version to be published in Physical Review