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  1. 1

    The Multimessenger Contribution of Ultra-High-Energy Cosmic Rays from Gamma-Ray Bursts by Zhenjiang Li, Fangsheng Min, Yi Jin, Yiqing Guo

    Published 2025-01-01
    “…It has long been debated whether gamma-ray bursts (GRBs) could serve as potential sources of ultra-high-energy cosmic rays (UHECRs). …”
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    Study of Long-term Spectral Evolution and X-Ray and γ-Ray Correlation of Blazars Seen by HAWC by R. Alfaro, C. Alvarez, A. Andrés, J.C. Arteaga-Velázquez, D. Avila Rojas, H.A. Ayala Solares, R. Babu, E. Belmont-Moreno, A. Bernal, K.S. Caballero-Mora, T. Capistrán, A. Carramiñana, F. Carreón, S. Casanova, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, D. Depaoli, N. Di Lalla, R. Diaz Hernandez, B.L. Dingus, M.A. DuVernois, M. Durocher, J.C. Díaz-Vélez, K. Engel, C. Espinoza, K.L. Fan, N. Fraija, S. Fraija, J.A. García-González, F. Garfias, A. Gonzalez Muñoz, M.M. González, J.A. Goodman, S. Groetsch, J.P. Harding, S. Hernández-Cadena, I. Herzog, D. Huang, F. Hueyotl-Zahuantitla, A. Iriarte, V. Joshi, S. Kaufmann, D. Kieda, A. Lara, W.H. Lee, J. Lee, H. León Vargas, J.T. Linnemann, A.L. Longinotti, G. Luis-Raya, K. Malone, O. Martinez, I. Martinez-Castellanos, J. Martínez-Castro, J.A. Matthews, P. Miranda-Romagnoli, J.A. Montes, E. Moreno, M. Mostafá, A. Nayerhoda, L. Nellen, M.U. Nisa, R. Noriega-Papaqui, N. Omodei, M. Osorio, Y. Pérez Araujo, E.G. Pérez-Pérez, C.D. Rho, D. Rosa-González, E. Ruiz-Velasco, H. Salazar, D. Salazar-Gallegos, A. Sandoval, M. Schneider, J. Serna-Franco, A.J. Smith, Y. Son, R.W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, E. Varela, L. Villaseñor, X. Wang, I.J. Watson, K. Whitaker, E. Willox, S. Yun-Cárcamo, H. Zhou, C. de León, HAWC collaboration, Abraham D. Falcone, Fredric Hancock

    Published 2025-01-01
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    Thirty-Year Periodicity of Cosmic Rays by Jorge Pérez-Peraza, Víctor Velasco, Igor Ya. Libin, K. F. Yudakhin

    Published 2012-01-01
    “…Cosmogenic isotopes have frequently been employed as proxies of ancient cosmic ray fluxes. On the basis of periodicities of the 10Be time series (using data from both the South and North Poles) and the 14C time series (with data from Intercal-98), we offer evidence of the existence of cosmic ray fluctuations with a periodicity of around 30 years. …”
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    Clustering of X-Ray-Selected AGN by N. Cappelluti, V. Allevato, A. Finoguenov

    Published 2012-01-01
    “…The study of the angular and spatial structure of the X-ray sky has been under investigation since the times of the Einstein X-ray Observatory. …”
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    Pore structure characterization of porous building material by X-ray computed tomography (XCT) and X-ray microscopy (XRM) by Chengnan Shi, Jeroen Soete, Hans Janssen

    Published 2025-02-01
    “…To address the conflict between the field of view and resolution, an image chain with eight three-dimensional greyscale image sets is acquired through X-ray computed tomography (XCT) and X-ray microscopy (XRM), with their voxel sizes progressively spanning from nanometers to micrometers. …”
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    Cosmic Rays Report from the Structure of Space by A. Annila

    Published 2015-01-01
    “…Spectrum of cosmic rays follows a broken power law over twelve orders of magnitude. …”
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    Gamma-Ray Bursts as Multienergy Neutrino Sources by Katsuaki Asano, Kohta Murase

    Published 2015-01-01
    “…We review theoretical models for nonelectromagnetic emission, mainly neutrinos and cosmic rays, from gamma-ray bursts (GRBs). In various stages of the relativistic jet propagation, cosmic-ray ion acceleration and subsequent neutrino emission are expected. …”
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    Development and Motion Testing of a Robotic Ray by Jianhui He, Yonghua Zhang

    Published 2015-01-01
    “…The fin undulating motion patterns, fin ray angle, and fin shape to be investigated are briefly introduced. …”
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    Ray Tracing RF Field Prediction: An Unforgiving Validation by E. M. Vitucci, V. Degli-Esposti, F. Fuschini, J. S. Lu, M. Barbiroli, J. N. Wu, M. Zoli, J. J. Zhu, H. L. Bertoni

    Published 2015-01-01
    “…In the present work, however, we show that a great deal of work is still needed to make ray tracing really unleash its potential in practical use. …”
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    The Observer’s Guide to the Gamma-Ray Burst Supernova Connection by Zach Cano, Shan-Qin Wang, Zi-Gao Dai, Xue-Feng Wu

    Published 2017-01-01
    “…We present a detailed report of the connection between long-duration gamma-ray bursts (GRBs) and their accompanying supernovae (SNe). …”
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    Reverse Shock Emission in Gamma-Ray Bursts Revisited by He Gao, Peter Mészáros

    Published 2015-01-01
    “…A generic synchrotron external shock model is the widely preferred paradigm used to interpret the broadband afterglow data of gamma-ray bursts (GRBs), including predicted observable signatures from a reverse shock which have been confirmed by observations. …”
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    Long-Term Cosmic Ray Variability and the CME-Index by Helen Mavromichalaki, Evangelos Paouris

    Published 2012-01-01
    “…The cosmic ray modulation in relation to solar activity indices and heliospheric parameters during the period January 1996–October 2011, covering the solar cycle 23 and the ascending phase of solar cycle 24, is studied. …”
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    Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets by Odysseas Kosmas, Theodoros Smponias

    Published 2018-01-01
    “…In this work, we simulate γ-rays created in the hadronic jets of the compact object in binary stellar systems known as microquasars. …”
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    Resolution of (heavy) primaries in ultra high energy cosmic rays by Blaž Bortolato, Jernej F. Kamenik, Michele Tammaro

    Published 2024-12-01
    “…Abstract Measurements of ultra-high energy cosmic rays (UHECR) suggest a complex composition with significant contributions from heavy nuclei at the highest energies. …”
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    X-Ray Performance of SiC NPN Radiation Detector by Jing Wang, Leidang Zhou, Liang Chen, Silong Zhang, Fangbao Wang, Tingting Fan, Zhuo Chen, Song Bai, Xiaoping Ouyang

    Published 2024-12-01
    “…The response properties of the fabricated SiC npn radiation detector were characterized by high-energy X-ray illumination with a maximum X-ray photon energy of 30 keV. …”
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