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Jets in a Gamma-Ray Burst during Its Prompt Emission: Evolution of the Lorentz Factor
The Astrophysical Journal, 2023 Knowledge about the Lorentz factor and its evolution of relativistic jets in gamma-ray bursts (GRBs) is crucial to understand their physics. An exact value of the bulk Lorentz factor can be estimated based on a high-energy spectral cutoff, which may ...Jing Li, Da-Bin Lin, Rui-Jing Lu, Yun Wang, Lu-Yao Jiang, Shen-Shi Du, Wen-Qiang Liang, Xiang-Gao Wang, En-Wei Liang +8 moredoaj +1 more sourceThe Physics of Gamma-Ray Bursts
, 2018 Gamma-ray bursts (GRBs) are the most luminous explosions in the universe, which within seconds release energy comparable to what the Sun releases in its entire lifetime. The field of GRBs has developed rapidly and matured over the past decades.Bing Zhangsemanticscholar +1 more sourceA long-duration gamma-ray burst with a peculiar origin [PDF]
Nature, 2022 It is generally believed that long-duration gamma-ray bursts (GRBs) are associated with massive star core collapse1, whereas short-duration GRBs are associated with mergers of compact star binaries2.J. Yang, Shunke Ai, Bin-Bin Zhang, Bing Zhang, Zibo Liu, X. Wang, Yu-Han Yang, Yi-Han Yin, Ye Li, Hou-Jun Lu +9 moresemanticscholar +1 more sourceAre there MeV gamma-ray bursts? [PDF]
AIP Conference Proceedings, 1996 It is often stated that gamma-ray bursts (GRBs) have typical energies of several hundred keV. Is this a real feature of GRBs or is it due to an observational bias? We consider the possibility that bursts of a given bolometric luminosity occur with a hardness distribution $p(H)d \log H \propto H^ d \log H$. We model the detection efficiency of BATSE as Tsvi Piran, Ramesh Narayanopenaire +4 more sourcesOptical and Near-infrared Observations of the Distant but Bright “New Year’s Burst” GRB 220101A
The Astrophysical Journal, 2023 High-redshift gamma-ray bursts (GRBs) are useful to probe the early Universe, but only a few candidates have been detected so far. Here, we report the optical and near-infrared observations of the afterglow of a relatively high-redshift event GRB 220101A,Zi-Pei Zhu, Wei-Hua Lei, Daniele B. Malesani, Shao-Yu Fu, Dong-Jie Liu, Dong Xu, Paolo D’Avanzo, José Feliciano Agüí Fernández, Johan P. U. Fynbo, Xing Gao, Ana Nicuesa Guelbenzu, Shuai-Qing Jiang, David Alexander Kann, Sylvio Klose, Jin-Zhong Liu, Xing Liu, Massimiliano De Pasquale, Antonio de Ugarte Postigo, Bringfried Stecklum, Christina Thöne, Joonas Kari Markku Viuho, Yi-Nan Zhu, Jin-Da Li, He Gao, Tian-Hua Lu, Shuo Xiao, Yuan-Chuan Zou, Li-Ping Xin, Jian-Yan Wei +28 moredoaj +1 more sourceBurst Image Restoration and Enhancement [PDF]
arXiv, 2021 Modern handheld devices can acquire burst image sequence in a quick
succession. However, the individual acquired frames suffer from multiple
degradations and are misaligned due to camera shake and object motions. The
goal of Burst Image Restoration is to effectively combine complimentary cues
across multiple burst frames to generate high-quality ...arxiv AN ALL-SKY SEARCH FOR THREE FLAVORS OF NEUTRINOS FROM GAMMA-RAY BURSTS WITH THE ICECUBE NEUTRINO OBSERVATORY [PDF]
, 2016 We present the results and methodology of a search for neutrinos produced in the decay of charged pions created in interactions between protons and gamma-rays during the prompt emission of 807 gamma-ray bursts (GRBs) over the entire sky.I. C. M. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, T. Arlen, J. Auffenberg, X. Bai, S. Barwick, V. Baum, R. Bay, J. Beatty, J. Tjus, K. Becker, E. Beiser, S. Benzvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. Boersma, C. Bohm, M. Borner, F. Bos, D. Bose, S. Boser, O. Botner, J. Braun, L. Brayeur, H. Bretz, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. Collin, J. Conrad, D. Cowen, A. H. C. Silva, J. Daughhetee, J. Davis, M. Day, J. Andr'e, C. Clercq, E. del Pino Rosendo, H. Dembinski, S. Ridder, P. Desiati, K. D. Vries, G. Wasseige, M. With, T. DeYoung, J. C. D'iaz-V'elez, V. Lorenzo, H. Dujmovic, J. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, S. Euler, P. Evenson, S. Fahey, A. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C.-C. Fosig, T. Fuchs, T. Gaisser, R. Gaior, J. Gallagher, L. Gerhardt, K. Ghorbani, D. Gier, L. Gladstone, M. Glagla, T. Glusenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. G'ora, D. Grant, Z. Griffith, C. Ha, C. Haack, A. H. Ismail, A. Hallgren, F. Halzen, E. Hansen, B. Hansmann, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. Hill, K. Hoffman, R. Hoffmann, K. Holzapfel, A. Homeier, K. Hoshina, F. Huang, M. Huber, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. Japaridze, M. Jeong, K. Jero, B. Jones, M. Jurkovič, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. Kelley, J. Kemp, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, S. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Kopke, C. Kopper, S. Kopper, D. Koskinen, M. Kowalski, K. Krings, G. Kroll, M. Kroll, G. Kruckl, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. Lanfranchi, M. Larson, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, J. Leuner, L. Lu, J. Lunemann, J. Madsen, G. Maggi, K. Mahn, M. Mandelartz, R. Maruyama, K. Mase, H. Matis, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, E. Middell, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. Nowicki, D. Nygren, A. Pollmann, A. Olivas, A. Omairat, A. O'Murchadha, T. Palczewski, H. Pandya, D. Pankova, L. Paul, J. Pepper, C. Heros, C. Pfendner, D. Pieloth, E. Pinat, J. Posselt, P. Price, G. Przybylski, M. Quinnan, C. Raab, L. Radel, M. Rameez, K. Rawlins, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, S. Richter, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, L. Sabbatini, H. Sander, A. Sandrock, J. Sandroos, S. Sarkar, K. Schatto, M. Schimp, P. Schlunder, T. Schmidt, S. Schoenen, S. Schoneberg, A. Schonwald, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. Spiczak, C. Spiering, M. Stahlberg, M. Stamatikos, T. Stanev, Alexander Stasik, A. Steuer, T. Stezelberger, R. Stokstad, A. Stossl, R. Strom, N. Strotjohann, G. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, S. Ter-Antonyan, A. Terliuk, G. Tevsi'c, S. Tilav, P. Toale, M. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, S. Vallecorsa, J. Vandenbroucke, N. Eijndhoven, S. Vanheule, J. Santen, J. Veenkamp, M. Vehring, M. Voge, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, C. Weaver, C. Wendt, S. Westerhoff, B. Whelan, K. Wiebe, C. Wiebusch, L. Wille, D. Williams, L. Wills, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, D. Xu, X. Xu, Y. Xu, J. Yáñez, G. Yodh, S. Yoshida, M. Zoll +315 moresemanticscholar +1 more source