Showing 261 - 270 results of 270 for search '"kinetic energy"', query time: 0.05s Refine Results
  1. 261

    An experimental and numerical study of the ballistic behavior of an epoxy matrix hybrid composite reinforced with aramid fabric and fique fabric by Bernardo Soares Avila de Cêa, Raí Felipe Pereira Junio, Douglas Santos Silva, Fábio da Costa Garcia Filho, Sergio Neves Monteiro, Lucio Fabio Cassiano Nascimento

    Published 2025-03-01
    “…The composites were subjected to ballistics tests to investigate the absorption of kinetic energy. The Weibull probabilistic statistical treatment was used and numerical analyses were compared to the experimental data. …”
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  2. 262
  3. 263

    Synergistic Configuration of Binary Rhodium Single Atoms in Carbon Nanofibers for High‐Performance Alkaline Water Electrolyzer by Natarajan Logeshwaran, Gyuchan Kim, Pandiarajan Thangavel, Sun Seo Jeon, Kaliannan Thiyagarajan, Kampara Roopa Kishore, Hyunjoo Lee, Inseok Seo, Hongseok Yun, Sungho Lee, Byung‐Hyun Kim, Young Jun Lee

    Published 2025-01-01
    “…Abstract Electrochemical alkaline water electrolysis offers significant economic advantages; however, these benefits are hindered by the high kinetic energy barrier of the water dissociation step and the sluggish kinetics of the hydrogen evolution reaction (HER) in alkaline media. …”
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  4. 264

    Photospheric Swirls in a Quiet-Sun Region by Quan Xie, Jiajia Liu, Chris J. Nelson, Robert Erdélyi, Yuming Wang

    Published 2025-01-01
    “…The squared rotation, expansion/contraction and vector speeds, and proxy kinetic energy are all found to follow Gaussian distributions. …”
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  5. 265

    Detection of a New GeV Source in the Outer Region of the Coma Cluster: A Signature of External Accretion Shock? by Xiao-Bin Chen, Kai Wang, Yi-Yun Huang, Hai-Ming Zhang, Shao-Qiang Xi, Ruo-Yu Liu, Xiang-Yu Wang

    Published 2025-01-01
    “…The gamma-ray (0.1−10 ^3 GeV) luminosity of the source, 1.4 × 10 ^42 erg s ^−1 , suggests that a fraction  ~10 ^−3 of the kinetic energy flux through the shock surface is transferred to relativistic CR electrons.…”
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  6. 266

    Implication of Galaxy-scale Negative Feedback by One of the Most Powerful Multiphase Outflows in a Hyperluminous Infrared Galaxy at Intermediate Redshift by Xiaoyang Chen, Masayuki Akiyama, Kohei Ichikawa, Yoshiki Toba, Toshihiro Kawaguchi, Takuma Izumi, Toshiki Saito, Daisuke Iono, Masatoshi Imanishi, Kianhong Lee, Hiroshi Nagai, Hirofumi Noda, Abdurro’uf, Mitsuru Kokubo, Naoki Matsumoto

    Published 2025-01-01
    “…In addition to ejection of kinetic energy, it is also found that the powerful outflow can induce an ionizing shock in the galaxy disk and enhance the excitation and dissociation of molecular gas. …”
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  7. 267

    Constraints on Relativistic Jets from the Fast X-Ray Transient 210423 Using Prompt Radio Follow-up Observations by Dina Ibrahimzade, R. Margutti, J. S. Bright, P. Blanchard, K. Paterson, D. Lin, H. Sears, A. Polzin, I. Andreoni, G. Schroeder, K. D. Alexander, E. Berger, D. L. Coppejans, A. Hajela, J. Irwin, T. Laskar, B. D. Metzger, J. C. Rastinejad, L. Rhodes

    Published 2025-01-01
    “…Considering a wide range of possible redshifts z ≤ 3.5, circumstellar medium density n = 10 ^−6 –10 ^−1 cm ^−3 , and isotropic-equivalent jet kinetic energy E _k _,iso = 10 ^48 –10 ^55 erg, we find that we can rule out wide jets with opening angle θ _j = 15° viewed within 10° off-axis. …”
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  8. 268

    Relativistic and Quantum Revisions of the Multisource Thermal Model in High-Energy Collisions by Fu-Hu Liu, Cai-Xing Tian, Mai-Ying Duan, Bao-Chun Li

    Published 2012-01-01
    “…The distributions of particle momenta, momentum components, transverse momenta, kinetic energies, and velocities in both the classical and relativistic situations are presented to give comparisons.…”
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  9. 269

    A Multimode Approach to Geometrically Nonlinear Free and Forced Vibrations of Multistepped Beams by Issam El Hantati, Ahmed Adri, Hatim Fakhreddine, Said Rifai, Rhali Benamar

    Published 2021-01-01
    “…Discrete expressions of the strain energy and kinetic energies are derived, and Hamilton’s principle is applied to reduce the problem to a solution of a nonlinear algebraic system and then solved by an approximate method. …”
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  10. 270

    Identifying Critical Input Parameters for Improving Drag‐Based CME Arrival Time Predictions by C. Kay, M. L. Mays, C. Verbeke

    Published 2020-01-01
    “…We consider CMEs of different strengths from average to extreme size, speed, and mass (kinetic energies between 9×1029 and 6×1032 erg). For each scale CME, we vary the input parameters to reflect the current observational uncertainty in each and determine how accurately each must be known to achieve predictions that are accurate within 5 hr. …”
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