Relevant bibliographies by topics / Gamma-rays: burst

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Gamma-rays: burst'

Author: Grafiati
Published: 9 March 2023
Last updated: 31 July 2025

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Journal articles on the topic "Gamma-rays: burst"

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Fishman, Gerald J. "Gamma-Ray Burst Observations with BATSE." Symposium - International Astronomical Union 188 (1998): 159–62. http://dx.doi.org/10.1017/s0074180900114664.

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Gamma-ray bursts (GRBs) will be recorded as one of the outstanding new phenomena discovered in astronomy this century. About once per day, a burst of gamma rays appears from a random direction on the sky. Often, the burst outshines all other sources of gamma-rays in the sky, combined. This paper reviews some of the key observed phenomenon of bursts in the hard x-ray/gamma-ray region, as observed with the BATSE experiment on the Compton Gamma Ray Observatory. The observed time profiles, spectral properties and durations of gamma-ray bursts cover a wide range. Recent breakthroughs in the observa
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Chadwick, Paula M. "Very high-energy gamma rays from gamma-ray bursts." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 365, no. 1854 (2007): 1343–56. http://dx.doi.org/10.1098/rsta.2006.1971.

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Very high-energy (VHE) gamma-ray astronomy has undergone a transformation in the last few years, with telescopes of unprecedented sensitivity having greatly expanded the source catalogue. Such progress makes the detection of a gamma-ray burst at the highest energies much more likely than previously. This paper describes the facilities currently operating and their chances for detecting gamma-ray bursts, and reviews predictions for VHE gamma-ray emission from gamma-ray bursts. Results to date are summarized.
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Epstein, Richard I. "Physical Constraints on Models of Gamma-Ray Bursters." International Astronomical Union Colloquium 89 (1986): 305–21. http://dx.doi.org/10.1017/s0252921100086140.

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AbstractThe power per logarithmic bandwidth in gamma-ray burst spectra generally increases rapidly with energy through the x-ray range and does not cut off sharply above a few MeV. This spectral form indicates that a very small fraction of the energy from a gamma-ray burst source is emitted at low energies or is reprocessed into x-rays and that the high-energy gamma rays are not destroyed by photon-photon interactions. The implications are that the emission mechanism for the gamma-ray bursts is not synchrotron radiation from electrons that lose most of their energy before being re-accelerated
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Aharonian, F., F. Ait Benkhali, J. Aschersleben, et al. "Search for the evaporation of primordial black holes with H.E.S.S." Journal of Cosmology and Astroparticle Physics 2023, no. 04 (2023): 040. http://dx.doi.org/10.1088/1475-7516/2023/04/040.

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Abstract Primordial Black Holes (PBHs) are hypothetical black holes predicted to have been formed from density fluctuations in the early Universe. PBHs with an initial mass around 1014–1015 g are expected to end their evaporation at present times in a burst of particles and very-high-energy (VHE) gamma rays. Those gamma rays may be detectable by the High Energy Stereoscopic System (H.E.S.S.), an array of imaging atmospheric Cherenkov telescopes. This paper reports on the search for evaporation bursts of VHE gamma rays with H.E.S.S., ranging from 10 to 120 seconds, as expected from the final st
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BARSHAY, SAUL, and GEORG KREYERHOFF. "VERY HIGH-ENERGY NEUTRINOS FROM SLOWLY DECAYING, MASSIVE DARK MATTER AS A SOURCE OF EXPLOSIVE ENERGY FOR GAMMA-RAY BURSTS." Modern Physics Letters A 18, no. 07 (2003): 477–89. http://dx.doi.org/10.1142/s0217732303009654.

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We consider a speculative model for gamma-ray bursts (GRB), which predicts that the total kinetic energy in the ejected matter is less than the total energy in the gamma rays. There is also secondary energy in X-rays, which are emitted contemporaneously with the gamma rays. The model suggests that bremsstrahlung and Compton up-scattering by very energetic electrons, are important processes for producing the observed burst radiation. The dynamics naturally allows for the possibility of a moderate degree of beaming of matter and radiation in some gamma-ray bursts. GRB are predicted to have an in
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Harding, Alice K. "Gamma-Ray Burst Theory: Back to the Drawing Board." International Astronomical Union Colloquium 142 (1994): 863–68. http://dx.doi.org/10.1017/s0252921100078222.

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AbstractGamma-ray bursts have always been intriguing sources to study in terms of particle acceleration, but not since their discovery two decades ago has the theory of these objects been in such turmoil. Prior to the launch of Compton Gamma-Ray Observatory and observations by BATSE, there was strong evidence pointing to magnetized Galactic neutron stars as the sources of gamma-ray bursts. However, since BATSE the observational picture has changed dramatically, requiring much more distant and possibly cosmological sources. I review the history of gamma-ray burst theory from the era of growing
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Coelho, Jaziel G., Luana N. Padilha, Rita C. dos Anjos, Cynthia V. Ventura, and Geanderson A. Carvalho. "An updated view and perspectives on high-energy gamma-ray emission from SGR J1935+2154 and its environment." Journal of Cosmology and Astroparticle Physics 2022, no. 10 (2022): 041. http://dx.doi.org/10.1088/1475-7516/2022/10/041.

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Abstract SGR J1935+2154 was discovered in 2016 and is currently one of the most burst-active Soft Gamma-ray Repeaters (SGR), having emitted many X-ray bursts in recent years. In one of our previous articles, we investigated the contribution to high-energy and very high-energy gamma-ray emission (VHE, E > 100 GeV) due to cosmic-ray acceleration of SNR G57.2+0.8 hosting SGR J1935+2154 using the GALPROP propagation code. However, follow-up observations of SGR 1935+2154 were made for 2 hours on April 28, 2020, using the High Energy Stereoscopic System (H.E.S.S.). The observations coincide with
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Huang, Jihong, Yilin Wang, Bingrong Yu, and Shun Zhou. "Invisible neutrino decays as origin of TeV gamma rays from GRB221009A." Journal of Cosmology and Astroparticle Physics 2023, no. 04 (2023): 056. http://dx.doi.org/10.1088/1475-7516/2023/04/056.

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Abstract Recently, the LHAASO collaboration has observed the gamma rays of energies up to ten TeV from the gamma-ray burst GRB221009A, which has stimulated the community of astronomy, particle physics and astrophysics to propose various possible interpretations. In this paper, we put forward a viable scenario that neutrinos are produced together with TeV photons in the gamma-ray burst and gradually decay into the axion-like particles, which are then converted into gamma rays in the galactic magnetic fields. In such a scenario, the tension between previous axion-like particle interpretations an
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Hurley, Kevin. "Observational Features of Cosmic Gamma-Ray Bursts: Evidence for Galactic Versus Extragalactic Origin." International Astronomical Union Colloquium 142 (1994): 857–61. http://dx.doi.org/10.1017/s0252921100078210.

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AbstractThe recent observational data on gamma-ray bursts are reviewed. Burst time histories display features at the millisecond level which suggest a compact object origin. Lines in the energy spectra and spectral evolution point toward a Galactic neutron star origin, even though line features have not yet been confirmed in recent data. The Galactic distribution of burst sources, however, is both isotropic and sampled to its characteristic distance, making it unlikely that the sources are related to populations of Galactic neutrons stars we are familiar with. Counterpart searches, previously
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Vestrand, W. T., J. A. Wren, A. Panaitescu, et al. "The Bright Optical Flash and Afterglow from the Gamma-Ray Burst GRB 130427A." Science 343, no. 6166 (2013): 38–41. http://dx.doi.org/10.1126/science.1242316.

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The optical light generated simultaneously with x-rays and gamma rays during a gamma-ray burst (GRB) provides clues about the nature of the explosions that occur as massive stars collapse. We report on the bright optical flash and fading afterglow from powerful burst GRB 130427A. The optical and >100–megaelectron volt (MeV) gamma-ray flux show a close correlation during the first 7000 seconds, which is best explained by reverse shock emission cogenerated in the relativistic burst ejecta as it collides with surrounding material. At later times, optical observations show the emergence of emis
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Dissertations / Theses on the topic "Gamma-rays: burst"

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NARDINI, MARCO. "Optical versus X–ray afterglows of GRBs: towards understanding the emission processes." Doctoral thesis, Scuola Internazionale Superiore di Studi Avanzati (SISSA), 2009. http://hdl.handle.net/10281/23600.

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Gamma–Ray Bursts (GRBs) are the most distant objects ever detected after the recombination epoch. They consist of a short intense emission episode of gammarays (10 keV–2 MeV) with typical duration between 10−2 and 103 seconds. This is called the “prompt” emission phase. GRBs are classified, according to their observed duration, into short GRBs (lasting less than 2s) and long GRBs (lasting more than 2 s). During the prompt phase GRBs are the brightest objects in the gamma–ray sky. The gamma–ray prompt emission is accompanied by a long lasting emission, called “afterglow”, covering the w
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Seglar-Arroyo, Monica. "Studying the origin of cosmic-rays : Multi-messenger studies with very-high-energy gamma-ray instruments." Thesis, Université Paris-Saclay (ComUE), 2019. http://www.theses.fr/2019SACLS260.

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Les phénomènes explosifs qui se produisent dans l'Univers à haute énergie sont capables d'accélérer les particules jusqu'aux énergies les plus élevées. Ces processus produisent des particules secondaires de nature différente, c'est-à-dire des photons et des neutrinos. Dans des cas particuliers, ces événements induisent des perturbations sur l'espace-temps, c'est-à-dire des ondes gravitationnelles détectables par des interféromètres sur Terre. La combinaison des informations complémentaires fournies par ces messagers cosmiques peuvent permettre de répondre à des questions ouvertes en astrophysi
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Nakamura, Toshio, Kentarou Nagaya, Fusa Miyake та ін. "炭素14と宇宙線変動 : 奈良時代の異変". 名古屋大学年代測定資料研究センター, 2013. http://hdl.handle.net/2237/20130.

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Vasileiou, Vlasios. "A search for bursts of very high energy gamma rays with milagro." College Park, Md.: University of Maryland, 2008. http://hdl.handle.net/1903/8570.

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Thesis (Ph. D.) -- University of Maryland, College Park, 2008.<br>Thesis research directed by: Dept. of Physics. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.
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DICHIARA, Simone. "A multiwavelength view of the transient sky: gamma-ray bursts and other fast transients from optical to gamma-rays." Doctoral thesis, Università degli studi di Ferrara, 2015. http://hdl.handle.net/11392/2389002.

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Christensen, L., S. D. Vergani, S. Schulze, et al. "Solving the conundrum of intervening strong Mg II absorbers towards gamma-ray bursts and quasars." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/626409.

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Previous studies have shown that the incidence rate of intervening strong Mg II absorbers towards gamma-ray bursts (GRBs) were a factor of 2-4 higher than towards quasars. Exploring the similar sized and uniformly selected legacy data sets XQ-100 and XSGRB, each consisting of 100 quasar and 81 GRB afterglow spectra obtained with a single instrument (VLT/X-shooter), we demonstrate that there is no disagreement in the number density of strong Mg II absorbers with rest-frame equivalent widths W-r(lambda 2796) > 1 angstrom towards GRBs and quasars in the redshift range 0.1 less than or similar to
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Kuehn, Frederick Gabriel. "Finding Gamma Ray Bursts at High Energies and Testing the Constancy of the Speed of Light." The Ohio State University, 2008. http://rave.ohiolink.edu/etdc/view?acc_num=osu1214582047.

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Samuelsson, Filip. "Multi-messenger emission from gamma-ray bursts." Licentiate thesis, KTH, Partikel- och astropartikelfysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-273383.

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Multi-messenger astronomy is a very hot topic in the astrophysical community. A messenger is something that carries information. Different astrophysical messenger types are photons, cosmic rays, neutrinos, and gravitational waves. They all carry unique and complementary information to one another. The idea with multi-messenger astronomy is that the more different types of messengers one can obtain from the same event, the more complete the physical picture becomes. In this thesis I study the multi-messenger emission from gamma-ray bursts (GRBs), the most luminous events known in the Universe.
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Siemens, Xavier. "Gravitational waves and cosmic strings /." Thesis, Connect to Dissertations & Theses @ Tufts University, 2002.

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Thesis (Ph.D.)--Tufts University, 2002.<br>Adviser: Alexander Vilenkin. Submitted to the Dept. of Physics. Includes bibliographical references (leaves 95-98). Access restricted to members of the Tufts University community. Also available via the World Wide Web;
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Di, Piano Ambra. "Detection of short Gamma-Ray Bursts with CTA through real-time analysis." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/19962/.

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With respect to the current IACTs, CTA will cover a larger energy range (~20 GeV - 300 TeV) with one order of magnitude better sensitivity. The facility will be provided with a real-time analysis (RTA) software that will automatically generate science alerts and analyse data from on-going observations in real-time. The RTA will play a key role in the search and follow-up of transients from external alerts (i.e. from on-space gamma-ray missions, observatories operating at other energy bands or targets of opportunity provided by neutrinos and gravitational waves detectors). The scope of this stu
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Books on the topic "Gamma-rays: burst"

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United States. National Aeronautics and Space Administration., ed. An analysis of gamma-ray burst time profiles from the burst and transient source experiment: Final report for grant no. NCC8-82. National Aeronautics and Space Administration, 1996.

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United States. National Aeronautics and Space Administration., ed. An analysis of gamma-ray burst time profiles from the burst and transient source experiment: Final report for grant no. NCC8-82. National Aeronautics and Space Administration, 1996.

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United States. National Aeronautics and Space Administration., ed. An analysis of gamma-ray burst time profiles from the burst and transient source experiment: Final report for grant no. NCC8-82. National Aeronautics and Space Administration, 1996.

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United States. National Aeronautics and Space Administration., ed. An analysis of gamma-ray burst time profiles from the burst and transient source experiment: Final report for grant no. NCC8-82. National Aeronautics and Space Administration, 1996.

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United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., ed. Development of the burst and transient source experiment (BATSE). National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1991.

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Andersen, Michael I. Gamma-rays bursts: Afterglows and host galaxies. University of Oulu, 2002.

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1954-, Ho Cheng, Epstein Richard I, Fenimore Edward E, and Los Alamos Workshop on Gamma-Ray Bursts (1990 : Taos, N.M.), eds. Gamma-ray bursts: Observations, analyses and theories : proceedings of the Los Alamos Workshop on Gamma-Ray Bursts, Taos, New Mexico, July 29-August 3, 1990. Cambridge University Press, 1992.

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United States. National Aeronautics and Space Administration., ed. Observations of gamma-ray bursts. National Aeronautics and Space Administration, 1995.

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United States. National Aeronautics and Space Administration., ed. Observations of gamma-ray bursts. National Aeronautics and Space Administration, 1995.

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United States. National Aeronautics and Space Administration., ed. Observations of gamma-ray bursts. National Aeronautics and Space Administration, 1995.

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Book chapters on the topic "Gamma-rays: burst"

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Oliveira, F. G., Jorge A. Rueda, and R. Ruffini. "X, Gamma-Rays, and Gravitational Waves Emission in a Short Gamma-Ray Burst." In Gravitational Wave Astrophysics. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10488-1_4.

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Varendorff, Martin. "Gamma-Ray Bursts." In The Universe in Gamma Rays. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04593-0_15.

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Hurley, K. "Cosmic Gamma-Ray Bursts." In Cosmic Gamma Rays, Neutrinos, and Related Astrophysics. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0921-2_24.

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Epstein, Richard I. "Gamma-Ray Bursts: A Physical Perspective." In Cosmic Gamma Rays, Neutrinos, and Related Astrophysics. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0921-2_25.

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Wang, X. Y., Z. G. Dai, and T. Lu. "Emission Processes of High-Energy Gamma Rays from Gamma-Ray Bursts." In Astrophysics and Space Science Library. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-0403-8_5.

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Murakami, T., Y. Ueda, R. Fujimoto, et al. "Quick Observations of the Fading X-Rays from Gamma-Ray Bursts with ASCA." In The Hot Universe. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4970-9_40.

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Biermann, Peter L., Sergej Moiseenko, Samvel Ter-Antonyan, and Ana Vasile. "Cosmic Rays from PeV to ZeV, Stellar Evolution, Supernova Physics and Gamma Ray Bursts." In The Early Universe and the Cosmic Microwave Background: Theory and Observations. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-007-1058-0_22.

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Katz, Jonathan I. "Introduction." In The Biggest Bangs. Oxford University PressNew York, NY, 2002. http://dx.doi.org/10.1093/oso/9780195145700.003.0001.

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Abstract Gamma-ray bursts are the most violent events since the birth of the universe. They are perhaps ten times as energetic as the most energetic supernovas, the explosions that destroy massive stars and make neutron stars and black holes. More remarkable, the energy in a gamma-ray burst is concentrated into a small amount of mass moving at 99.999% of the speed of light. It has even been suggested that the most energetic cosmic rays—single elementary particles, each with enough energy to lift a 150-pound man an inch off the floor—are produced in gamma-ray bursts.
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Katz, Jonathan I. "A Supernova Connection?" In The Biggest Bangs. Oxford University PressNew York, NY, 2002. http://dx.doi.org/10.1093/oso/9780195145700.003.0016.

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Abstract By the spring of 1998 most of the pieces of the gamma-ray-burst puzzle seemed to be in place: Bursts are produced when dense matter, a neutronic doughnut, is accreted by a black hole. This doughnut makes a series of pair fireballs that accelerate thin shells (or portions of shells) of matter to high energy, with speeds closely approaching the speed of light. This matter is probably directed into jets, but only roughly, like water from a fire hose rather than light from a laser. The gamma rays themselves are made when these shells collide with each other, the faster overtaking the slow
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Meli, A. "COSMIC-RAYS AND GAMMA RAY BURSTS." In Gamma-ray Bursts: 15 Years of GRB Afterglows. EDP Sciences, 2020. http://dx.doi.org/10.1051/978-2-7598-1002-4-106.

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Conference papers on the topic "Gamma-rays: burst"

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Mason, Paul, and Peter L. Biermann. "Cosmic Rays, Supernovae, Gamma-Ray Bursts, and Life." In The Golden Age of Cataclysmic Variables and Related Objects - VI. Sissa Medialab, 2024. http://dx.doi.org/10.22323/1.460.0046.

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Atoyan, Armen. "Neutrinos and Gamma Rays from Photomeson Processes in Gamma Ray Bursts." In GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810825.

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Mészáros, P. "Ultra-high Energy Gamma-rays, Neutrinos, and Gravitational Waves from GRBs." In GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810815.

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Wick, S. D. "High-Energy Cosmic Rays from Galactic and Extragalactic Gamma-Ray Bursts." In GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP, 2004. http://dx.doi.org/10.1063/1.1810818.

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Dingus, Brenda L. "Observations of the Highest Energy Gamma Rays from Gamma-Ray Bursts." In GAMMA-RAY BURST AND AFTERGLOW ASTRONOMY 2001: A Workshop Celebrating the First Year of the HETE Mission. AIP, 2003. http://dx.doi.org/10.1063/1.1579348.

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Waxman, Eli. "High Energy Cosmic-Rays and Neutrinos from Cosmological Gamma-Ray Burst Fireballs." In Proceedings of Nobel Symposium 109. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812810434_0013.

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Shibata, Sanshiro, Nozomu Tominaga, Hiroyuki Sagawa, et al. "Origin of Ultra-High Energy Cosmic Rays: Nuclear Composition of Gamma-ray Burst Jets." In INTERNATIONAL SYMPOSIUM ON THE RECENT PROGRESS OF ULTRA-HIGH ENERGY COSMIC RAY OBSERVATION. AIP, 2011. http://dx.doi.org/10.1063/1.3628755.

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Liang, Edison P. "X-rays from gamma ray bursts." In Gamma-ray bursts: Second workshop. AIP, 1994. http://dx.doi.org/10.1063/1.45921.

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Rachen, Jörg P., and P. Mészáros. "Cosmic rays and neutrinos from gamma-ray bursts." In GAMMA-RAY BURSTS. ASCE, 1998. http://dx.doi.org/10.1063/1.55402.

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Hudec, R., L. Pina, L. Sveda, et al. "The feasibility of independent observations∕detections of GRBs in X-rays." In GAMMA-RAY BURST: Sixth Huntsville Symposium. AIP, 2009. http://dx.doi.org/10.1063/1.3155882.

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Reports on the topic "Gamma-rays: burst"

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Murase, Kohta, Kunihito Ioka, Shigehiro Nagataki, and Takashi Nakamura. High Energy Neutrinos and Cosmic-Rays From Low-Luminosity Gamma-Ray Bursts? Office of Scientific and Technical Information (OSTI), 2006. http://dx.doi.org/10.2172/886791.

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Tajima, T., and Y. Takahashi. Laboratory laser acceleration and high energy astrophysics: {gamma}-ray bursts and cosmic rays. Office of Scientific and Technical Information (OSTI), 1998. http://dx.doi.org/10.2172/674811.

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