Literatura académica sobre el tema "Gamma Ray Burst (GRB)"
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Artículos de revistas sobre el tema "Gamma Ray Burst (GRB)"
ZHANG, BING. "GAMMA-RAY BURST PROMPT EMISSION". International Journal of Modern Physics D 23, n.º 02 (29 de enero de 2014): 1430002. http://dx.doi.org/10.1142/s021827181430002x.
Texto completoBurns, Eric, Dmitry Svinkin, Edward Fenimore, D. Alexander Kann, José Feliciano Agüí Fernández, Dmitry Frederiks, Rachel Hamburg et al. "GRB 221009A: The BOAT". Astrophysical Journal Letters 946, n.º 1 (1 de marzo de 2023): L31. http://dx.doi.org/10.3847/2041-8213/acc39c.
Texto completoIoka, Kunihito, Yudai Suwa, Hiroki Nagakura, Rafael S. de Souza y Naoki Yoshida. "Population III Gamma-Ray Burst". Proceedings of the International Astronomical Union 7, S279 (abril de 2011): 301–4. http://dx.doi.org/10.1017/s1743921312013099.
Texto completoWang, Yun, Lu-Yao Jiang y Jia Ren. "GRB 201104A: A “Repetitive” Short Gamma-Ray Burst?" Astrophysical Journal 935, n.º 2 (1 de agosto de 2022): 179. http://dx.doi.org/10.3847/1538-4357/ac82ec.
Texto completoBisnovatyi-Kogan, G. S. "Physical Restrictions to Cosmological Gamma-Ray Burst Models". International Astronomical Union Colloquium 192 (2005): 491–96. http://dx.doi.org/10.1017/s0252921100009581.
Texto completoŘípa, Jakub y Arman Shafieloo. "Update on testing the isotropy of the properties of gamma-ray bursts". Monthly Notices of the Royal Astronomical Society 486, n.º 3 (26 de abril de 2019): 3027–40. http://dx.doi.org/10.1093/mnras/stz921.
Texto completoKing, Andrew. "Gamma-ray burst models". Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 365, n.º 1854 (9 de febrero de 2007): 1277–80. http://dx.doi.org/10.1098/rsta.2006.1978.
Texto completoHuang, Y. F., T. Lu, Z. G. Dai y K. S. Cheng. "Beaming Effects in Gamma-Ray Burst Afterglows". Symposium - International Astronomical Union 214 (2003): 321–22. http://dx.doi.org/10.1017/s0074180900194653.
Texto completoIvy Wang, Xiangyu, Bin-Bin Zhang y Wei-Hua Lei. "GRB 200826A: A Precursor of a Long Gamma-Ray Burst with Missing Main Emission". Astrophysical Journal Letters 931, n.º 1 (1 de mayo de 2022): L2. http://dx.doi.org/10.3847/2041-8213/ac6c7e.
Texto completoMurase, Kohta, Mainak Mukhopadhyay, Ali Kheirandish, Shigeo S. Kimura y Ke Fang. "Neutrinos from the Brightest Gamma-Ray Burst?" Astrophysical Journal Letters 941, n.º 1 (1 de diciembre de 2022): L10. http://dx.doi.org/10.3847/2041-8213/aca3ae.
Texto completoTesis sobre el tema "Gamma Ray Burst (GRB)"
Laskar, Tanmoy, Kate D. Alexander, Edo Berger, Wen-fai Fong, Raffaella Margutti, Isaac Shivvers, Peter K. G. Williams et al. "A REVERSE SHOCK IN GRB 160509A". IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/624020.
Texto completoNakauchi, Daisuke. "Gamma-Ray Bursts from First Stars and Ultra-Long Gamma-Ray Bursts". 京都大学 (Kyoto University), 2015. http://hdl.handle.net/2433/199100.
Texto completoAlexander, K. D., T. Laskar, E. Berger, C. Guidorzi, S. Dichiara, W. Fong, A. Gomboc et al. "A Reverse Shock and Unusual Radio Properties in GRB 160625B". IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626042.
Texto completoGalante, Douglas. "Efeitos astrofísicos e astrobiológicos de Gamma-Ray Bursts". Universidade de São Paulo, 2009. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-19062009-014454/.
Texto completoThe present work has the main goal of understanding the possible effects of the hard gamma radiation produced during a Gamma-Ray Burst (GRB) event both on the interstellar medium surrounding the source of the burst and on planets possibly illuminated. Gamma-Ray Bursts were first detected on the 60s and quickly have attracted the attention of the astrophysical community, since the energies emitted just in could reach 1054erg, the rest mass of the Sun. No mechanism was known to be so efficient in extracting gravitational energy to produce such emission. Later on, the possibility of the emission being collimated has lowered the energy of the to 5x1051erg, but the central engine has not yet been completely understood, and there is still ample room for exotic alternatives. We have studied the effects of GRB on the ISM, in an attempt to distinguish the candidates of GRB remnants from those generated by multiple supernovae. We have used both energetic arguments and the possibility of chemical alterations due to photonuclear reactions. We have also worked on the biological implications of the illumination of planets by a GRB, concluding that the effects of such event could seriously harm the biosphere of a planet even at distances of ~10kpc.
Fong, W., R. Margutti, R. Chornock, E. Berger, B. J. Shappee, A. J. Levan, N. R. Tanvir et al. "THE AFTERGLOW AND EARLY-TYPE HOST GALAXY OF THE SHORT GRB 150101B AT z = 0.1343". IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622673.
Texto completoHarris, Pauline Lisa. "A search for gamma ray burst neutrinos using the Radio Ice Cherenkov Experiment". Thesis, University of Canterbury. Physics and Astronomy, 2008. http://hdl.handle.net/10092/2166.
Texto completoChapman, Robert. "Gamma-ray bursts in the local universe". Thesis, University of Hertfordshire, 2009. http://hdl.handle.net/2299/2809.
Texto completoMARTONE, RENATO. "A perspective on the high-energy transient sky: from gamma-ray bursts to the search for fast radio burst counterparts". Doctoral thesis, Università degli studi di Ferrara, 2020. http://hdl.handle.net/11392/2488025.
Texto completoHarstad, Emelie. "A Targeted LIGO-Virgo Search for Gravitational Waves Associated with Gamma-Ray Bursts Using Low-Threshold Swift GRB Triggers". Thesis, University of Oregon, 2013. http://hdl.handle.net/1794/13003.
Texto completoRAVASIO, MARIA EDVIGE. "New insights into the physics of Gamma-Ray Burst prompt emission". Doctoral thesis, Università degli Studi di Milano-Bicocca, 2022. http://hdl.handle.net/10281/350073.
Texto completoThe nature of the GRB prompt emission is still uncertain, preventing us from constraining the sources' physical properties, which are strictly connected to fundamental open issues such as jet composition and energy dissipation. The typical observed prompt emission spectrum consists of two power-laws with slopes α and β smoothly connected at a peak energy Epeak. Synchrotron from fast cooling electrons is the most natural radiative process, given the non-thermal shape of the observed spectrum and the strong magnetic fields expected in the emitting region. However, the observed spectra of thousands of GRBs being harder than synchrotron predictions represented a major issue for decades. Oganesyan et al. 2017 recently discovered in the soft X-rays the presence of an additional spectral break, which has been identified as the synchrotron cooling frequency. Motivated by this result, I searched for the presence of a break at higher energies, using Fermi/GBM data. The time-resolved analysis of the 10 long brightest GRBs has revealed in the ~70% of the spectra the presence of a break energy Ebreak, located between ~20 and 500 keV. The slopes of the power-laws below and above the break are remarkably consistent with the predicted values for synchrotron emission in fast cooling regime (-2/3 and -3/2, respectively). Spectral simulations suggest that the separation of Ebreak from Epeak and the photon statistics of the spectrum can hamper the identification of the break, which might explain why this fundamental feature has not been identified before. The consistency with synchrotron emission has been tested also fitting a physical synchrotron model to the spectrum of the long GRB 180720B, confirming the results obtained with the empirical function. In addition, I investigated, for the first time, the presence of the break in 10 short GRBs: contrary to long ones, short GRBs do not show the break, but the low-energy photon index is consistent with -2/3. The results presented in this thesis imply a set of physical parameters that challenges the GRB standard model. The relative small ratio of the synchrotron frequencies (closer to unity for short GRBs) implies that the emitting particles do not cool completely. In turn this requires a low magnetic field (B’≲10 G) implying a distant emission region (R~1016cm), at odds with the typical ~ms variability timescale of GRBs. A possible solution may come from the proton-synchrotron scenario: thanks to the longer cooling timescale of the protons, this scenario can explain the observed spectral shape assuming standard values both for the magnetic field (B’~106 G) and for the radius of the emitting region (R~1013cm). Moreover, I expanded my study of the prompt emission spectrum by including its characterization at higher energies. The addition of LAT data in the spectral analysis revealed in 10 out of 22 bursts the presence of a spectral cutoff at high energies (~100 MeV): interpreted as due to pair-production opacity, they provide estimates of the bulk Lorentz factor Γof the jet in the range 100-400. The extension at high energies allowed me also to study the high-energy power-law slope β, which is a key parameter to constrain the corresponding slopes p of the underlying energy distribution of non-thermal accelerated particles. Assuming the emission as due to synchrotron, I found a broad distribution of p, centered around p=2.86 (with a tail up to p~5-7). Given the theoretical uncertainties on the energy distribution of accelerated particles in mildly-relativistic shocks, these results provide useful observational benchmarks for the development of the theory of particle acceleration applied to the prompt emission case. My PhD project also included the study of the emission at lower frequencies of the first 3 GRBs detected at ~TeV energies (GRB 180720B, GRB 190114C, GRB 190829A), which allowed me to find interesting constraints on the macro- and micro-physical parameters of GRBs.
Libros sobre el tema "Gamma Ray Burst (GRB)"
Katz, Jonathan I. Radio optical emission, spectral shapes and breaks in GRB. [Washington, DC: National Aeronautics and Space Administration, 1994.
Buscar texto completoKatz, Jonathan I. Radio and optical emission, spectral shapes and breaks in GRB. [Washington, DC: National Aeronautics and Space Administration, 1994.
Buscar texto completoMcEnery, J. E. (Julie E.), Racusin, J. L. (Judy L.) y Gehrels Neil, eds. Gamma ray bursts 2010: GRB 2010 : Annapolis, MD, USA, 1-4 November 2010. Melville, N.Y: American Institute of Physics, 2011.
Buscar texto completoMagnus, Axelsson y Ryde Felix, eds. Gamma-ray bursts: Prospects for GLAST : Stockholm symposium on GRBs, Stockholm, Sweden, 1 September 2006. Melville, N.Y: American Institute of Physics, 2007.
Buscar texto completoA, Meegan C. y United States. National Aeronautics and Space Administration., eds. Do gamma-ray burst sources repeat? [Washington, D.C: National Aeronautics and Space Administration, 1994.
Buscar texto completoA, Meegan C. y United States. National Aeronautics and Space Administration., eds. Do gamma-ray burst sources repeat? [Washington, D.C: National Aeronautics and Space Administration, 1994.
Buscar texto completoA, Meegan C. y United States. National Aeronautics and Space Administration., eds. Do gamma-ray burst sources repeat? [Washington, D.C: National Aeronautics and Space Administration, 1995.
Buscar texto completoA, Meegan C. y United States. National Aeronautics and Space Administration., eds. Do gamma-ray burst sources repeat? [Washington, D.C: National Aeronautics and Space Administration, 1994.
Buscar texto completoA, Meegan C. y United States. National Aeronautics and Space Administration., eds. Do gamma-ray burst sources repeat? [Washington, D.C: National Aeronautics and Space Administration, 1995.
Buscar texto completoA, Meegan C. y United States. National Aeronautics and Space Administration., eds. Do gamma-ray burst sources repeat? [Washington, D.C: National Aeronautics and Space Administration, 1994.
Buscar texto completoCapítulos de libros sobre el tema "Gamma Ray Burst (GRB)"
Zhang, Bing, Hou-Jun Lü y En-Wei Liang. "GRB Observational Properties". En Gamma-Ray Bursts, 5–34. Dordrecht: Springer Netherlands, 2016. http://dx.doi.org/10.1007/978-94-024-1279-6_2.
Texto completoMesler, Robert Allan. "Calorimetry of GRB 030329". En Searching for the Long-Duration Gamma-Ray Burst Progenitor, 87–98. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-06626-4_5.
Texto completoMesler, Robert Allan. "VLBI and Archival VLA and WSRT Observations of GRB 030329". En Searching for the Long-Duration Gamma-Ray Burst Progenitor, 73–86. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-06626-4_4.
Texto completoBjörnsson, G., J. Hjorth, P. Jakobsson, L. Christensen, E. J. Lindfors y S. Holland. "The Jet and the Supernova in GRB 990712". En Gamma-Ray Bursts in the Afterglow Era, 157–59. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/10853853_41.
Texto completoSpeziali, R., F. D’Alessio, L. A. Antonelli, A. Di Paola, L. Burderi, F. Fiore, G. Israel et al. "IR and Optical Observations of GRB from Campo Imperatore". En Gamma-Ray Bursts in the Afterglow Era, 424–26. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/10853853_117.
Texto completoAtteia, J. L. "Statistics of the Gamma-Ray Burst Population". En The Gamma Ray Sky with Compton GRO and SIGMA, 369–80. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0067-0_27.
Texto completoMasetti, Nicola. "The GRB Followup Euro-US Consortium: Results from the ESO Telescopes". En Gamma-Ray Bursts in the Afterglow Era, 127–29. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/10853853_32.
Texto completoDerishev, E. V., V. V. Kocharovsky, Vl V. Kocharovsky y P. Mészáros. "GRB Synchrotron-Self-Compton Emission Generated by Self-Consistent Electron Distribution". En Gamma-Ray Bursts in the Afterglow Era, 327–29. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/10853853_87.
Texto completoDainotti, Maria. "GRB models". En Gamma-ray Burst Correlations. IOP Publishing, 2019. http://dx.doi.org/10.1088/2053-2563/aae15cch2.
Texto completoDainotti, Maria. "GRB models". En Gamma-ray Burst Correlations, 2–1. IOP Publishing, 2019. http://dx.doi.org/10.1088/978-0-7503-1575-3ch2.
Texto completoActas de conferencias sobre el tema "Gamma Ray Burst (GRB)"
Fynbo, J. P. U. "The GRB-SN Connection: GRB 030329 and XRF 030723". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810852.
Texto completoDella Valle, M. "SN 2002lt and GRB 021211: a SN/GRB Connection at z = 1". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810874.
Texto completoDaigne, Frédéric. "The Low-Luminosity Tail of the GRB Distribution: the Case of GRB 980425". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810858.
Texto completoYamazaki, Ryo. "GRB 980425 in the Off-Axis Jet Model of the Standard GRBs". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810877.
Texto completoDoty, John. "Scaling and GRB Mission Optimization". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810941.
Texto completoTopinka, Martin. "Further Analysis of GRB 030501". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810833.
Texto completoBeloborodov, A. M. "Early Stages of the GRB Explosion". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810828.
Texto completoTaylor, Greg. "High Resolution Observations of GRB 030329". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810857.
Texto completoLindsay, K. "GRB 030329 with SARA and TLS". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810859.
Texto completoCorsi, A. "GRB 970228 Within the EMBH Model". En GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810880.
Texto completoInformes sobre el tema "Gamma Ray Burst (GRB)"
Hurley, K. Analysis of gamma-ray burst energy spectra. Office of Scientific and Technical Information (OSTI), enero de 1990. http://dx.doi.org/10.2172/6062431.
Texto completoTerrell, J., R. W. Klebesadel, P. Lee y J. W. Griffee. Gamma-ray burst data from DMSP satellites. Office of Scientific and Technical Information (OSTI), diciembre de 1991. http://dx.doi.org/10.2172/10114304.
Texto completoPeng, F. Two-Component Jet Models of Gamma-Ray Burst Sources. Office of Scientific and Technical Information (OSTI), enero de 2005. http://dx.doi.org/10.2172/839640.
Texto completoFenimore, Edward E. Gamma Ray Burst, one reason why "astronomical is an adjective". Office of Scientific and Technical Information (OSTI), octubre de 2013. http://dx.doi.org/10.2172/1095855.
Texto completoEichler, David y Jonathan Granot. The Case for Anisotropic Afterglow Efficiency Within Gamma-Ray Burst Jets. Office of Scientific and Technical Information (OSTI), octubre de 2005. http://dx.doi.org/10.2172/878093.
Texto completoLee, A. Properties of gamma-ray burst time profiles using pulse decomposition analysis. Office of Scientific and Technical Information (OSTI), febrero de 2000. http://dx.doi.org/10.2172/753294.
Texto completoLee, A. Intrinsic and cosmological signatures in gamma-ray burst time profiles: Time dilation. Office of Scientific and Technical Information (OSTI), febrero de 2000. http://dx.doi.org/10.2172/753295.
Texto completoKocevski, Daniel y Vahe Petrosian. On The Lack of Time Dilation Signatures in Gamma-ray Burst Light Curves. Office of Scientific and Technical Information (OSTI), febrero de 2013. http://dx.doi.org/10.2172/1074191.
Texto completoSako, M. A Search for Discrete X-Ray Spectral Features in a Sample of Bright Gamma-Ray Burst Afterglows. Office of Scientific and Technical Information (OSTI), septiembre de 2004. http://dx.doi.org/10.2172/833044.
Texto completoWilliams, G. Early-time observations of gamma-ray burst error boxes with the Livermore optical transient imaging system. Office of Scientific and Technical Information (OSTI), agosto de 2000. http://dx.doi.org/10.2172/15007544.
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