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J. C. do Nascimento

Publications and source records attributed to J. C. do Nascimento.

2 recordsLinked to original sources

All-optical 3-input OR and 2-input AND/NIMPLY logic gates in a linear planar three-core optical fiber coupler

Most all-optical logic processing devices reported in the literature rely on nonlinear effects to achieve logical discrimination, which typically results in increased implementation complexity, higher optical power requirements, and limited scalability over larger optical circuits. Here, we present the numerical modeling and analysis of two all-optical logic gates based on a fully linear, dispersion-free planar symmetric three-core optical fiber coupler. The proposed devices operate with low-powered amplitude-modulated pulses and require no nonlinear materials, material doping, or optoelectronic components. By exploiting only the fiber geometry and coupled-mode theory, we demonstrate two logic processing functionalities: a 3-input OR gate and a configurable gate that performs either the AND or the NIMPLY operation based on a control signal. Logical discrimination is measured using a contrast-based performance metric, showing clear separation between logic levels for all input combinations. The simplicity of the proposed linear structure, combined with its scalability and compatibility with different fiber technologies, favor compact implementation and integration into larger photonic signal processing and optical computing systems.

physics.optics↗

Ionised Gas Kinematics in MaNGA AGN. Extents of the Narrow Line and Kinematically Disturbed regions

We analyse the kinematics of 170 AGN host galaxies as compared to those of a matched control sample of non-active galaxies from the MaNGA survey in order to characterise and estimate the extents of the Narrow Line Region (NLR) and of the kinematically disturbed region (KDR) by the AGN. We define the observed NLR radius as the farthest distance from the nucleus within which both [Oiii]/Hβand [Nii]/Hαratios fall in the AGN region of the BPT diagram and the Hαequivalent width is required to be larger than 3.0Å. The extent of the KDR is defined as the distance from the nucleus within which the AGN hosts galaxies shows a more disturbed gas kinematics than the control galaxies. The kinematics derived from the [Oiii] line profiles reveal that, on average, the most luminous AGN (L[Oiii] > 3.8 * 10^40 erg s^-1) possess higher residual difference between the gaseous and stellar velocities and velocities dispersion than their control galaxies. Spatially resolved NLR's and KDR's were found in 55 and 46 AGN host galaxies, with corrected radii 0.2 < r_KDR,c < 2.3 kpc and 0.4 < r_NLR,c < 10.1 kpc, with a relation between the two given by log r_KDR,c = (0.53\pm0.12) log r_NLR,c + (1.07\pm0.22), respectively. The extension of the KDR corresponds to about 30 per cent of that of the NLR. Assuming that the KDR is due to an AGN outflow, we have estimated ionised gas mass outflow rates that range between 10^-5 and \approx 1 Myr^-1, and kinetic powers that range from 10^34 to 10^40 erg s^-1. Comparing the power of the AGN ionised outflows with the AGN luminosities, they are always below the 0.05 L_AGN model threshold for having an important feedback effect on their respective host galaxies. The mass outflow rates (and power) of our AGN sample correlate with their luminosities, populating the lowest AGN luminosity range of the correlations previously found for more powerful sources.

astro-ph.GA↗