Search Results - "Sigalotti, L. Di G."

Flow Modeling of a Non-Newtonian Viscous Fluid in Elastic-Wall Microchannels by Rubio Martínez, A., Chávez Castellanos, A. E., Noguez Méndez, N. A., Aragón Rivera, F., Pliego Díaz, M., Sigalotti, L. Di G., Vargas, C. A.

“…The use of polymer microspheres is becoming increasingly widespread. Along with their most common applications, they are beginning to be used in the synthesis…”
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The impact of the initial core temperature on protostellar disc fragmentation by Sigalotti, L Di G, Cruz, F, Hareter, M, Gabbasov, R, Klapp, J, Fierro-Santillán, C R, Ramírez-Velásquez, J M, Zsargó, J

“…ABSTRACT Ground-based and satellite observations have revealed dust temperatures as low as ∼5−7 K in the centre of low-mass, pre-stellar cloud cores, where…”
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impetus: consistent SPH calculations of 3D spherical Bondi accretion on to a black hole by Ramírez-Velasquez, J M, Sigalotti, L Di G, Gabbasov, R, Cruz, F, Klapp, J

“…Abstract We present three-dimensional calculations of spherically symmetric Bondi accretion on to a stationary supermassive black hole of mass 108 M⊙ within a…”
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Dissipation of Standing Slow Magnetoacoustic Waves in Hot Coronal Loops by Sigalotti, L. Di G., Mendoza-Briceño, C. A., Luna-Cardozo, M.

“…Issue Title: MHD Waves and Oscillations in Solar Magnetic Structures / Guest Editor: R. Erdélyi The damping of standing slow waves in hot (T>6 MK) coronal…”
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Relativistic dynamics of the deuteron: An estimate of the nuclear force parameters by Sigalotti, L. Di G., Mejias, A.

“…A relativistic dynamical model of the deuteron nucleus is presented. The neutron and proton are assumed to interact via a short-range Yukawa interaction of…”
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Propagation and Damping of a Localized Impulsive Longitudinal Perturbation in Coronal Loops by Sigalotti, L. Di G., Guerra, J. A., Mendoza-Briceño, C. A.

“…We use linear analysis to simulate the evolution of a coronal loop in response to a localized impulsive event. The disturbance is modeled by injecting a narrow…”
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SPH simulations of turbulent flow in curved pipes with different geometries. A comparison with experiments by Alvarado-Rodriguez, C. E, Sigalotti, L. Di G, Klapp, J, Fierro-Santillan, C. R, Aragon, F, Uribe-Ramirez, A. R

“…J. Fluids Eng, Volume 143, Issue 9 September 2021 The swirling secondary flow in curved pipes is studied in three-space dimensions using a weakly compressible…”
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Creating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra by Zsargo, J, Fierro-Santillan, C. R, Klapp, J, Arrieta, A, Arias, L, Valencia, J. M, Sigalotti, L. Di G, Hareter, M, Puebla, R. E

“…$Aims.$ We present a database of 43,340 atmospheric models ($\sim$80,000 models at the conclusion of the project) for stars with stellar masses between 9 and…”
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Radiative non-isothermal Bondi accretion onto a massive black hole by Ramirez-Velasquez, J. M, Sigalotti, L. Di G, Gabbasov, R, Cruz, F, Klapp, J, Contreras, Ernesto

“…A&A 631, A13 (2019) In this paper, we present the classical Bondi accretion theory for the case of non-isothermal accretion processes onto a supermassive black…”
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Autonomous choices among deterministic evolution-laws as source of uncertainty by Trujillo, L, Meyroneinc, A, Campos, K, Rendon, O, Sigalotti, L. Di G

“…Communications in Nonlinear Science and Numerical Simulation 56C (2018) pp. 405-418 We provide evidence of an extreme form of sensitivity to initial conditions…”
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Impetus: Consistent SPH calculations of 3D spherical Bondi accretion onto a black hole by Ramirez-Velasquez, J. M, Sigalotti, L. Di G, Gabbasov, R, Cruz, F, Klapp, J

“…We present three-dimensional calculations of spherically symmetric Bondi accretion onto a stationary supermassive black hole (SMBH) of mass $10^{8}$…”
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Numerical Study of the Mixing Process of Unconfined Diffusion Flame in a Laminar to Transition-to-Turbulent Regime in a Four-Port Array Burner by De la Cruz-Ávila, M, De León-Ruiz, J. E, Martínez-Espinosa, E, Carvajal-Mariscal, I, Sigalotti, L. Di G

“…The mixing process of multiple jets of liquefied petroleum gas and air in a diffusion flame is numerically analysed. The case study considers a four-port array…”
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Image Convolution-Based Method and Statistical Modelling for Experimental Height Estimations of Laminar to Transition-to-Turbulent Regime Diffusion Flames by De La Cruz-Ávila, M, De León-Ruiz, J. E, Carvajal-Mariscal, I, Peña-Polo, F, Sigalotti, L. Di G

“…This paper presents an experimental methodology to measure the height of the flame using convolution image processing and statistical analysis. The…”
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Luminous Flame Height Correlation Based on Fuel Mass Flow for a Laminar to Transition-to-Turbulent Regime Diffusion Flame by De la Cruz-Ávila, M, De León-Ruiz, J. E, Carvajal-Mariscal, I, Polupan, G, Sigalotti, L. Di G

“…This paper presents a flame-height correlation for laminar to transition-to-turbulent regime diffusion flames. Flame-height measurements are obtained by means…”
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Modelling free surface flows with smoothed particle hydrodynamics by L.Di G.Sigalotti, J.Daza, A.Donoso

“…In this paper the method of Smoothed Particle Hydrodynamics (SPH) is extended to include an adaptive density kernel estimation (ADKE) procedure. It is shown…”
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SPH modeling of natural convection around a heated horizontal cylinder: A comparison with experiments by Aragón, F, Guzmán, J. E. V, Sigalotti, L. Di G, Klapp, J, Alvarado-Rodríguez, C. E, Carvajal-Mariscal, I, Uribe-Ramírez, A. R

“…An experimental and numerical smoothed particle hydrodynamics (SPH) analysis was performed for the convective flow arising from a horizontal, thin cylindrical…”
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Gravitational collapse of gas clouds with spherical, cylindrical or plane symmetry in the linear wave flow approximation by IBAÑEZ, M. H, SIGALOTTI, L. DI G

“…The equations of gas dynamics are solved, quasi-analytically by applying McVittie's method for spherical, cylindrical and plane configurations. The hypothesis…”
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Multiple fragmentation models of centrally condensed molecular cloud cores by Di G. Sigalotti, Leonardo, Klapp, Jaime

“…The protostellar collapse of centrally condensed, rapidly rotating (β≈0.17) cores, along with implicitly assumed m = 2 density variations — as appropriate for…”
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Gravitational collapse of rotating protostellar gas clouds not constrained by the condition of equatorial symmetry by SIGALOTTI, L. DI G

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Numerical models of tidally interacting protostellar binary systems by Sigalotti, Leonardo Di G., Klapp, Jaime

“…The tidally induced deformation of a rotating, collapsing adiabatic ( γ = 7/5) protostar, due to a similar companion of comparable mass moving past in an…”
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