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Kazuki Abe

Publications and source records attributed to Kazuki Abe.

4 recordsLinked to original sources

Quasi-DNS with chemical kinetics for near blow-out dynamics of a single multi-injection burner element for future gas turbine applications

Gas turbine combustors increasingly operate close to lean blow-out (LBO) limits, where small changes in fuel-air mixing or flow structure can destabilize the flame and alter near-blow-out dynamics. Conventional design practice relies mainly on Reynolds-averaged Navier-Stokes (RANS) simulations, which often overpredict turbulent mixing and cannot resolve unsteady flame anchoring and local extinction near burner hardware. We develop a Quasi-DNS workflow with detailed methane-air chemistry for a single element of a multiple-injection burner, modeled as a coaxial burner with a mixing tube and downstream combustion chamber, as a methodological basis for near-blow-out analysis. The workflow is implemented in OpenFOAM and comprises: (i) a simplified three-dimensional sector geometry with a 30-degree domain to capture circumferential vortices at the mixing tube outlet, (ii) boundary conditions and inlet profiles reproducing coaxial jet and preheated air conditions, (iii) a reduced Yang-Pope mechanism validated against GRI 3.0 using Cantera laminar flame speed, ignition delay, and counterflow diffusion flame calculations, (iv) grid generation and convergence checks based on flame structure and scalar dissipation rate, and (v) diagnostics including methane- and CO-based flame indices to classify local combustion modes. We demonstrate the workflow for a partially premixed methane flame at an overall equivalence ratio of phi = 0.45 and a perfectly premixed reference at the same phi. The Quasi-DNS results show limited mixing inside the mixing tube and strong vortical mixing at the outlet, leading to extended and structured heat-release regions that differ markedly from the smoother, more compact flames predicted by RANS. The methodology provides a reusable framework for analyzing flame structure, stabilization, and LBO-relevant dynamics in coaxial burners with mixing tubes.

physics.flu-dyn

Passive Luminescent Bellows Mechanism

The use of robots in disaster sites has rapidly expanded, with soft robots attracting particular interest due to their flexibility and adaptability. They can navigate through narrow spaces and debris, facilitating efficient and safe operations. However, low visibility in such environments remains a challenge. This study aims to enhance the visibility of soft robots by developing and evaluating a passive luminescent exible actuator activated by a black light. Using Ecoex mixed with phosphorescent powder, we fabricated an actuator and confirmed its fluorescence phosphorescence and deformation ability. Furthermore the effects of the mixing ratio on optical and mechanical properties were assessed.

cs.RO

Reflexive Input-Output Causality Mechanisms

This paper explores the concept of reflexive actuation, examining how robots may leverage both internal and external stimuli to trigger changes in the motion, performance, or physical characteristics of the robot, such as its size, shape, or configuration, and so on. These changes themselves may in turn be sequentially re-used as input to drive further adaptations. Drawing inspiration from biological systems, where reflexes are an essential component of the response to environmental changes, reflexive actuation is critical to enable robots to adapt to diverse situations and perform complex tasks. The underlying principles of reflexive actuation are analyzed, with examples provided from existing implementations such as contact-sensitive reflexive arms, physical counters, and their applications. The paper also outlines future directions and challenges for advancing this research area, emphasizing its significance in the development of adaptive, responsive robotic systems.

cs.RO

Chasing Gravitational Waves with the Cherenkov Telescope Array

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts of this gravitational wave event, ushered in a new era of multimessenger astronomy, providing the first direct evidence that BNS mergers are progenitors of short gamma-ray bursts (GRBs). Such events may also produce very-high-energy (VHE, > 100GeV) photons which have yet to be detected in coincidence with a gravitational wave signal. The Cherenkov Telescope Array (CTA) is a next-generation VHE observatory which aims to be indispensable in this search, with an unparalleled sensitivity and ability to slew anywhere on the sky within a few tens of seconds. New observing modes and follow-up strategies are being developed for CTA to rapidly cover localization areas of gravitational wave events that are typically larger than the CTA field of view. This work will evaluate and provide estimations on the expected number of of gravitational wave events that will be observable with CTA, considering both on- and off-axis emission. In addition, we will present and discuss the prospects of potential follow-up strategies with CTA.

astro-ph.HE