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Impact of Postshock Transcutaneous Pacing on Chest Compression Quality during Resuscitation: A Simulation-Based Pilot Study
Published 2021-01-01“…Potential utility of external, transcutaneous postshock pacing in patients with SCA in shockable rhythms has not been determined. …”
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The Effects of Selective Muscle Weakness on Muscle Coordination in the Human Arm
Published 2018-01-01“…Subsequently, muscle weakness was induced by a motor point block of brachialis muscle. Postblock subjects repeated the force generation tasks. …”
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Composite Strain Hardening Properties of High Performance Hybrid Fibre Reinforced Concrete
Published 2014-01-01“…In addition, the relative performance levels of different hybrid fibres in improving the matrix strain hardening, postcrack toughness, and residual strength capacity of slag based concretes were evaluated systematically.…”
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Implementation of Surface Radiation and Fluid-Structure Thermal Coupling in Atmospheric Reentry
Published 2012-01-01“…In this paper, we investigate how the thermal radiation coming from the postshock region interacts with the spacecraft structure. …”
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Flexural Properties of ECC-Concrete Composite Beam
Published 2018-01-01“…But the unbonded composite beam showed better postcrack energy absorption capacity with higher midspan deflection. …”
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New Occurrence of Seifertite and Stishovite in Chang’E‐5 Regolith
Published 2022-06-01“…Both seifertite and stishovite formed via solid‐state transformation mechanism, in which seifertite formed by transition from α‐cristobalite upon pressure loading whereas stishovite may form from seifertite when postshock temperature was significant during pressure release. …”
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Nonthermal Signatures of Radiative Supernova Remnants. II. The Impact of Cosmic Rays and Magnetic Fields
Published 2025-01-01“…Near the ends of their lives, supernova remnants (SNRs) enter a “radiative phase,” when efficient cooling of the postshock gas slows expansion. Understanding SNR evolution at this stage is crucial for estimating feedback in galaxies, as SNRs are expected to release energy and momentum into the interstellar medium near the ends of their lives. …”
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Damage Identification by Using a Self-Synchronizing Multipoint Laser Doppler Vibrometer
Published 2015-01-01“…Experiments are conducted to measure the natural frequencies and mode shapes of pre- and postcrack cantilever beams. Mode shape curvature is calculated by numerical interpolation and windowed Fourier analysis. …”
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Ultrasound-guided deep versus superficial continuous serratus anterior plane block for pain management in patients with multiple rib fractures: A prospective randomized double-blin...
Published 2025-01-01“…A significant increase in the median IS-V in group D compared to group S at 90 minutes (P = 0.02) and 12h postblock (P = 0.004) LUSS was significantly lower in D group at 90 min, 12 h, and 24 h (P = 0.04, 0.001, 0.031). …”
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Behaviour of Textile-Reinforced Concrete Beams versus Steel-Reinforced Concrete Beams
Published 2021-01-01“…The flexural behaviour of TRC beams shows no similarity to that of SRC beams at postcracking formation. Besides, the moment capacity and tension stiffening of TRC beams were found 56% and 7 times higher than those of SRC beams, respectively. …”
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A Novel Method to Evaluate the Effect of Slope Blasting under Impact Loading
Published 2020-01-01“…The entire evaluation process selects eleven indicators to form an evaluation set, including the boulder yield, root rate, flying distance of flyrock, explosive consumption, postcracking distance, detonator unit consumption, vibration velocity, loose coefficient, cast distance, throw rate, and blasted volume per meter of hole. …”
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HCG 57: Evidence for Shock-heated Intergalactic Gas from X-Rays and Optical Emission Line Spectroscopy
Published 2025-01-01“…These different shock velocities can be reconciled by considering the contributions of rotation to collision velocity in different parts of the disks, and the clumpy nature of the preshock medium in the galaxies, which likely lead to different shock velocities in different components of the turbulent postshocked gas. We examine the diffuse X-ray emission in the group members and their associated point sources, identifying X-ray active galactic nuclei in HCG 57A, B, and D. …”
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