Relevant bibliographies by topics / Very high energy electrons

Contents

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

Academic literature on the topic 'Very high energy electrons'

Author: Grafiati
Published: 20 July 2024
Last updated: 31 July 2025

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Journal articles on the topic "Very high energy electrons"

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Clements, Nathan, Nolan Esplen, Magdalena Bazalova-Carter, et al. "271 Grid Therapy with Very-High Energy Electrons." Radiotherapy and Oncology 186 (September 2023): S115—S116. http://dx.doi.org/10.1016/s0167-8140(23)89363-x.

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Fuchs, T., H. Szymanowski, U. Oelfke, et al. "Treatment planning for laser-accelerated very-high energy electrons." Physics in Medicine and Biology 54, no. 11 (2009): 3315–28. http://dx.doi.org/10.1088/0031-9155/54/11/003.

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Osmanov, Zaza N., D. Kuridze, and Swadesh M. Mahajan. "Can the Solar Atmosphere Generate Very-High-Energy Cosmic Rays?" Symmetry 17, no. 3 (2025): 366. https://doi.org/10.3390/sym17030366.

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The origin and acceleration of high-energy particles, constituting cosmic rays, is likely to remain an important topic in modern astrophysics. Among the two categories galactic and solar cosmic rays, the latter are much less investigated. The primary source of solar cosmic ray particles are impulsive explosions of the magnetized plasma, known as solar flares and coronal mass ejections. These particles, however, are characterized by relatively low energies compared to their galactic counterparts. In this work, we explore the resonance wave–wave (RWW) interaction between the polarized electromag
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Papiez, Lech, Colleen DesRosiers, and Vadim Moskvin. "Very High Energy Electrons (50 – 250 MeV) and Radiation Therapy." Technology in Cancer Research & Treatment 1, no. 2 (2002): 105–10. http://dx.doi.org/10.1177/153303460200100202.

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Isravel, Hebzibha, Asaf Pe’er, and Damien Bégué. "Proton Synchrotron Origin of the Very-high-energy Emission of GRB 190114C." Astrophysical Journal 955, no. 1 (2023): 70. http://dx.doi.org/10.3847/1538-4357/acec73.

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Abstract We consider here a proton-synchrotron model to explain the MAGIC observation of GRB 190114C afterglow in the energy band of 0.2–1 TeV, while the X-ray spectra are explained by electron-synchrotron emission. Given the uncertainty of the particle acceleration process, we consider several variations of the model, and show that they all match the data very well. We find that the values of the uncertain model parameters are reasonable: isotropic explosion energy ∼1054.5 erg, ambient density ∼10–100 cm−3, and the fraction of electrons/protons accelerated to a high-energy power law is of a f
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XU, Wangwen, Zhanghu HU, 章虎 胡, Dexuan HUI, and Younian WANG. "High energy electron beam generation during interaction of a laser accelerated proton beam with a gas-discharge plasma." Plasma Science and Technology 24, no. 5 (2022): 055001. http://dx.doi.org/10.1088/2058-6272/ac4d1d.

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Abstract The study of the interaction between ion beam and plasma is very important to the areas of inertial fusion energy and high energy density physics. With detailed one-dimensional electromagnetic particle-in-cell simulations, we investigate here the interaction of a laser-accelerated proton beam assuming an ideal monoenergetic beam with a gas-discharge plasma. After the saturation stage of the two-stream instability excited by the proton beam, significant high energy electrons are observed, with maximum energy approaching 2 MeV, and a new two-stream instability occurs between the high en
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Tibolla, Omar, Sarah Kaufmann, and Paula Chadwick. "Pulsar Wind Nebulae and Unidentified Galactic Very High Energy Sources." J 5, no. 3 (2022): 318–33. http://dx.doi.org/10.3390/j5030022.

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The riddle of the origin of Cosmic Rays (CR) has been an open question for over a century. Gamma ray observations above 100 MeV reveal the sites of cosmic ray acceleration to energies where they are unaffected by solar modulation; recent evidence supports the existence of hadronic acceleration in Supernova Remnants (SNR), as expected in the standard model of cosmic ray acceleration. Nevertheless, the results raise new questions, and no final answer has been provided thus far. Among the suggested possible alternative accelerators in the Very High Energy (VHE) gamma ray sky, pulsar wind nebulae
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Kifune, T. "Very High Energy Gamma Rays from Plerions: CANGAROO Results." Symposium - International Astronomical Union 188 (1998): 125–28. http://dx.doi.org/10.1017/s0074180900114597.

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The current status of very high energy gamma ray astronomy (in ~ 1 TeV region) is described by using as example results of CANGAROO (Collaboration of Australia and Nippon for a GAmma Ray Observatory in the Outback). Gamma rays at TeV energies, emitted through inverse Compton effect of electrons or π0 decay from proton interaction, provide direct evidence on “hot” non-thermal processes of the Universe, as well as environmental features, such as the strength of magnetic field in the emission region, for the non-thermal processes.
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Liu, Qingyu, Qinhe Zhang, Min Zhang, and Fazhan Yang. "Study on the Discharge Characteristics of Single-Pulse Discharge in Micro-EDM." Micromachines 11, no. 1 (2020): 55. http://dx.doi.org/10.3390/mi11010055.

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To further study the discharge characteristics and machining mechanism of micro-electrical discharge machining (micro-EDM), the variation trends of the discharge energy and discharge crater size with actual discharge duration are discussed based on single-pulse experiments. The polarity effect of micro-EDM was analyzed according to the motion characteristics of electrons and ions in the discharge plasma channel. The results show that the discharge current and voltage of micro-EDM were independent of the discharge width and open-circuit voltage. The energy utilization rate of the short-pulse di
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Seitz, B. "166 RADIOTHERAPY WITH VERY HIGH ENERGY ELECTRONS GENERATED BY WAKEFIELD ACCELERATORS." Radiotherapy and Oncology 102 (March 2012): S77—S78. http://dx.doi.org/10.1016/s0167-8140(12)70137-8.

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Dissertations / Theses on the topic "Very high energy electrons"

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Ronga, Maria Grazia. "Study and modelling of very high energy electrons (VHEE) radiation therapy." Electronic Thesis or Diss., université Paris-Saclay, 2024. http://www.theses.fr/2024UPAST036.

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Le développement de méthodes innovantes susceptibles de réduire la sensibilité des tissus sains aux radiations, tout en maintenant l'efficacité du traitement sur la tumeur, est un aspect central de l'amélioration de l'efficacité de la radiothérapie pour le traitement du cancer. Parmi les développements et innovations méthodologiques possibles, la combinaison d'une irradiation à ultra-haut débit de dose (FLASH) et d'électrons de très haute énergie (VHEE) pourrait permettre d'exploiter les avantages radiobiologiques de l'effet FLASH pour le traitement des tumeurs profondes. En particulier, les V
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Mallot, Ann Kathrin. "The energy spectrum of cosmic electrons measured with the MAGIC telescopes." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät, 2017. http://dx.doi.org/10.18452/17698.

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Die hier vorgestellte Analyse nutzt die MAGIC Teleskope, zwei abbildende Cherenkov-Teleskope, zum Vermessen des Elektronenflusses. Der Energiebereich dieser Teleskope überschneidet sich großflächig sowohl mit dem der Satellitenmissionen Fermi-LAT und AMS-02 als auch mit den hochenergetischen Messungen der Cherenkov-Teleskope VERITAS und H.E.S.S.. Diese Arbeit hat das Elektronenspektrum im Bereich von 135 GeV bis 4 TeV mittels der MAGIC Teleskope vermesssen. Das Spektrum lässt sich in diesem Bereich mit einem einfachen Potenzgesetz mit dem Index -3.14+-0.05(stat)+-0.5(syst) beschrieben werden.
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Kashiyama, Kazumi. "Origins of High Energy Cosmic-Ray Electrons and Positrons." 京都大学 (Kyoto University), 2012. http://hdl.handle.net/2433/157757.

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Carlton, Ashley Kelly. "Characterizing high-energy electrons in space using science imagers." Thesis, Massachusetts Institute of Technology, 2018. http://hdl.handle.net/1721.1/120413.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Aeronautics and Astronautics, 2018.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 129-140).<br>Harsh radiation in the form of ionized, highly energetic particles is part of the space environment and can affect the operation, performance, and lifetime of spacecraft and their instruments. Jupiter has the largest and strongest magnetosphere of all of the planets in the solar system and it is dominated by high-energy electrons. Measuring and characterizing megaelectron volt (MeV) particles
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Aizatsky, N. I., N. P. Dikiy, A. N. Dovbnya, et al. "Properties of Zirconia Nanoceramics under High-Energy Electrons Irradiation." Thesis, Sumy State University, 2013. http://essuir.sumdu.edu.ua/handle/123456789/35622.

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Formation of radioactive isotopes is investigated under irradiation by relativistic electrons with energy up to 100 MeV. Radioactive isotopes 87,88Y, 88,89,95Zr, 95Nb, 175Hf are registered after irradiation by relativistic electrons with energy 47.2 MeV. The present data are necessary for the choice of a material for a dielectric wakefield accelerator. The greatest danger at operation of accelerators represents 88Y. Formation of radiation defects in nanoceramics is investigated. The various types of radiation defects are found out at an irradiation by relativistic electrons with energy 47
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Dickinson, Hugh John. "Very high energy gamma-rays from binary systems." Thesis, Durham University, 2010. http://etheses.dur.ac.uk/290/.

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This thesis presents a study of the very high energy (VHE) gamma-ray emission from X-ray binary systems using the H.E.S.S. imaging atmospheric Cherenkov array. The historical background and basic principles of ground-based gamma-ray astronomy are briefly reviewed and an overview of the design and capabilities of the H.E.S.S. telescope system is presented. The broadband observational properties of X-ray binary systems and their relevance in a broader astrophysical context is also discussed. A review of the radiative emission mechanisms which relate to VHE gamma-ray emission in X-ray binaries is
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Guillaud, Mathilde. "Neutrino oscillations at very high energy/matter density." Thesis, KTH, Fysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-292510.

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Neutrino oscillations in matter can be studied in different regimes, depending on the energy of the incoming neutrinos and the matter density of the medium. In this thesis we investigate neutrino oscillations in dense matter at very high energy (TeV-PeV range), taking into account the absorption that the neutrinos may undergo in such dense media. This absorption phenomenon is relevant for neutrino telescope measurements of astrophysical neutrinos. We begin with a brief reminder on neutrino oscillations in vacuum and the construction of the PMNS matrix. Then, we proceed with calculations for de
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Sritragool, Kunlapaporn. "Modification of Rubber Particle filled Thermoplastic with High Energy Electrons." Doctoral thesis, Universitätsbibliothek Chemnitz, 2010. http://nbn-resolving.de/urn:nbn:de:bsz:ch1-201000954.

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In present study, high energy electrons were used to modify blends based on RP and PP under two conditions: stationary and in-stationary conditions. Modification of blend under stationary condition is a process which is established in industrial application and where required absorbed dose is applied to form parts (after molding) at room temperature and in solid state. On the contrary, the modification of blend with high energy electrons under in-stationary condition is a new process (electron induced reactive processing) where required absorbed dose is applied to a molten state during melt mi
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Williams, Andrew James. "A water calorimeter for high energy x-rays and electrons." Thesis, University College London (University of London), 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.394541.

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Lemieux, François 1979. "Are inflationary predictions sensitive to very high energy physics?" Thesis, McGill University, 2003. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=80316.

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It was recently proposed that modifications to physics at trans-Planckian energies could lead to a non-adiabatic evolution of the scalar fluctuations responsible for the temperature anisotropy of the cosmological microwave background. If such a possibility was to be confirmed, it would provide us the first possibility to ever get experimental measurements of the physics near the Planck scale. This work investigates the physicality of such non-adiabatic evolutions, by avoiding the introduction of any exotic physics, by working well below the Planck scale. Simple 'hybrid-like' models of i
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Books on the topic "Very high energy electrons"

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Turver, K. E., ed. Very High Energy Gamma Ray Astronomy. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3831-1.

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E, Turver K., and North Atlantic Treaty Organization. Scientific Affairs Division., eds. Very high energy gamma ray astronomy. D. Reidel Pub. Co., 1987.

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Wolfe, Gregory John. Effects of large doses of high energy electrons on a TB CU 06+ high temperature superconductor. Naval Postgraduate School, 1989.

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Brill, Aryeh Louis. Advancing Blazar Science with Very-High-Energy Gamma-Ray Telescopes. [publisher not identified], 2021.

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Burkel, Eberhard. Inelastic scattering of x-rays with very high energy resolution. Springer-Verlag, 1991.

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Akerlof, Carl W. Correlative studies of astrophysical sources of very high and ultra high energy gamma-rays. National Aeronautics and Space Administration, 1993.

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Akerlof, Carl W. Correlative studies of astrophysical sources of very high and ultra high energy gamma-rays. National Aeronautics and Space Administration, 1993.

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E, Singler Robert, and United States. National Aeronautics and Space Administration., eds. Joining carbon-carbon composites and high-temperature materials with high energy electron: Progress report ... July 1, 1997 to November 30, 1997. National Aeronautics and Space Administration, 1998.

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E, Singler Robert, and United States. National Aeronautics and Space Administration., eds. Joining carbon-carbon composites and high-temperature materials with high energy electron: Progress report ... July 1, 1997 to November 30, 1997. National Aeronautics and Space Administration, 1998.

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Ribeiro, Deivid. Observations of Transient Events with Very-High-Energy Gamma-Ray Telescopes. [publisher not identified], 2022.

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Book chapters on the topic "Very high energy electrons"

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Fan, Danlei, Yi Yuan, Jian Wang, Kuanjun Fan, and Jian Lei. "A Proposed Beamline Optics for Focused Very High Energy Electron Radiotherapy." In Lecture Notes in Electrical Engineering. Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-97-0869-7_42.

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Gul, Osman Vefa. "Flash Radiation Therapy: Current Insights and Future Prospects." In The Latest Innovative Approaches in Radiation Therapy. Nobel Tip Kitabevleri, 2024. http://dx.doi.org/10.69860/nobel.9786053359425.5.

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FLASH radiotherapy (RT) is an innovative approach used in cancer treatment. The FLASH effect is observed at ultra-high dose rates (UHDR) of approximately 40 Gy/s or higher. This treatment method has the potential to effectively destroy tumor cells while causing less damage to healthy tissues. It has been shown that FLASH irradiation reduces the severity of toxicity in normal tissues compared to conventional dose rate (CONV) irradiation that is currently being utilized in clinical settings. The shortened treatment durations characteristic of FLASH-RT, typically falling below 0.1 seconds, offer
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Khaneja, Navin. "Relativity, Electrons, and Photons." In High Energy Physics. Springer Nature Switzerland, 2024. https://doi.org/10.1007/978-3-031-75645-0_2.

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Morawiec, Adam. "Diffraction of High Energy Electrons." In Indexing of Crystal Diffraction Patterns. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-11077-1_3.

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Drukarev, Evgeny G., and Aleksandr I. Mikhailov. "Annihilation of Positrons with Atomic Electrons." In High-Energy Atomic Physics. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-32736-5_11.

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Grieder, Peter K. F. "Electrons and Photons." In Exentsive Air Showers and High Energy Phenomena. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76941-5_15.

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Andresen, H. G., K. Aulenbacher, M. Ertel, E. Reichert, and K. H. Steffens. "Source of Polarized Electrons for MAMI B." In High Energy Spin Physics. Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-76661-9_3.

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Gerbi, Bruce J., Youlia M. Kirova, and Roberto Orecchia. "Clinical Applications of High-Energy Electrons." In Medical Radiology. Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/174_2011_321.

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Moffeit, K. C. "Spin Physics with Polarized Electrons at the SLC." In High Energy Spin Physics. Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-86995-2_13.

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Gougar, Hans D. "The Very High Temperature Reactor." In Nuclear Energy Encyclopedia. John Wiley & Sons, Inc., 2011. http://dx.doi.org/10.1002/9781118043493.ch26.

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Conference papers on the topic "Very high energy electrons"

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Cayley, J., M. Lerch, A. Rosenfeld, and Y. E. Tan. "MOSkin dosimetryfor very high-energy electron FLASHat Australian Synchrotron PEER." In 2024 IEEE Nuclear Science Symposium (NSS), Medical Imaging Conference (MIC) and Room Temperature Semiconductor Detector Conference (RTSD). IEEE, 2024. http://dx.doi.org/10.1109/nss/mic/rtsd57108.2024.10656176.

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Fu, Wenjie, Yingchao Li, Dake Xu, and Tingyue Gu. "Comparison of Two Different Types of Anaerobic Copper Biocorrosion Mechanisms by a Sulfate Reducing Bacterium and a Nitrate Reducing Bacterium." In CORROSION 2014. NACE International, 2014. https://doi.org/10.5006/c2014-3878.

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Abstract Biocorrosion, also known as Microbiologically Influenced Corrosion or MIC, is caused by biofilms. Anaerobic MIC has at least two distinct types. Type I MIC involves utilization of extracellular electrons released by the oxidation of an energetic metal such as elemental iron (Fe0). These electrons are transported by sessile cells on or very close to the metal surface across their cell walls to the cytoplasm where the electrons are used for reduction of an exogenous electron acceptor (oxidant) such as sulfate and nitrate under biocatalysis. The biofilm benefits from the energy released
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Kaifas, Theodoros N. F. "State of the Art and Innovations needed for Direct Radiating Arrays to place Very High Throughput Satellite Communications into Technology Reach." In 2024 5th International Conference on Communications, Information, Electronic and Energy Systems (CIEES). IEEE, 2024. https://doi.org/10.1109/ciees62939.2024.10811417.

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Kokurewicz, K., G. H. Welsh, E. Brunetti, et al. "Laser-plasma generated very high energy electrons (VHEEs) in radiotherapy." In SPIE Optics + Optoelectronics, edited by Kenneth W. D. Ledingham. SPIE, 2017. http://dx.doi.org/10.1117/12.2271183.

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Terrier, R. "A study of very high energy gamma-rays and electrons with GLAST." In GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP, 2001. http://dx.doi.org/10.1063/1.1419448.

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DesRosiers, Colleen, Vadim Moskvin, Minsong Cao, Chandrashekhar J. Joshi, and Mark Langer. "Laser-plasma generated very high energy electrons in radiation therapy of the prostate." In Lasers and Applications in Science and Engineering, edited by Joseph Neev, Stefan Nolte, Alexander Heisterkamp, and Christopher B. Schaffer. SPIE, 2008. http://dx.doi.org/10.1117/12.761663.

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Nishihara, K., and H. Yasui. "3d Particle Simulation on Interaction of Ultrashort Laser Pulse with Solid Density Hydrogen Plasma." In High-Energy Density Physics with Subpicosecond Laser Pulses. Optica Publishing Group, 1989. http://dx.doi.org/10.1364/hpslp.1989.pdp6.

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The interaction of very short laser pulses with matter has become an important field.1,2)If a pulse duration of a laser light is so short that no significant hydrodynamic expansion of a matter takes place, the electric field of a laser interacts directly with a solid density matter. The mean ion distance, a~ (3/4πni)1/3is of the order of one angstrom at a solid density. The quivering distance of electrons oscillating at a laser frequency, δx=eE 0 / mω 0 2 , exceeds the mean ion distance at a high intensity. In addition to that, the ion coupling coefficient, Γ=eϕ/kt=z2e2/akt, is of the order of
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Labate, Luca, Daniele Palla, Daniele Panetta, et al. "Perspectives for effective applications of laser-driven Very High Energy Electrons in medicine and biology." In Applying Laser-driven Particle Acceleration II, Medical and Nonmedical Uses of Distinctive Energetic Particle and Photon Sources: SPIE Optics + Optoelectronics Industry Event, edited by Paul R. Bolton. SPIE, 2021. http://dx.doi.org/10.1117/12.2596504.

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Kunz, R. R., T. E. Allen, and T. M. Mayer. "Thin Film Growth and Deposition by Low Energy Electron Stimulated Surface Chemistry." In Microphysics of Surfaces, Beams, and Adsorbates. Optica Publishing Group, 1987. http://dx.doi.org/10.1364/msba.1987.tua2.

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Direct materials processing by focused particle beams has received considerable attention in recent years. The electron beam, traditionally used for resist exposure in electron beam lithography applications, is among the candidates for direct materials modification. High energy electrons (&gt;1keV) are not very chemically active due to small cross sections for inelastic scattering processes such as bond dissociation and attachment. Low energy electrons are expected to be much more efficient at stimulating chemical processes. In particular, secondary electrons produced by particle or photon bom
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de Naurois, Mathieu. "The Very-High-Energy electron spectrum observed with H.E.S.S." In 38th International Cosmic Ray Conference. Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.444.0261.

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Reports on the topic "Very high energy electrons"

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Cimino, Roberto. Can Low Energy Electrons Affect High Energy Physics Accelerators? Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/826848.

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Lamb, R. C., and D. A. Lewis. Very high energy gamma ray astrophysics. Office of Scientific and Technical Information (OSTI), 1990. http://dx.doi.org/10.2172/5076918.

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Lamb, R. C., and D. A. Lewis. Very high energy gamma ray astrophysics. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/5693223.

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Maximon, Leonard C., and Alfred Lepretre. Angular distribution of high energy electrons following radiation. National Bureau of Standards, 1985. http://dx.doi.org/10.6028/nbs.ir.84-2854.

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Teitsma and Shuttleworth. PR-004-03127-R01 Gas Coupled Ultrasonic Pipeline Inspection. Pipeline Research Council International, Inc. (PRCI), 2008. http://dx.doi.org/10.55274/r0010897.

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The gas coupled ultrasonics (GCUS) project aims to develop a method for inspecting gas pipelines using a modification of the standard ultrasonic method that does not require a liquid couplant. Ultrasonic inspection is the highest accuracy inspection method readily available for measuring remaining wall thickness and measures it directly rather than inferring it from measurements of metal loss as occurs with other methods, for example MFL. Traditional ultrasonic methods require a liquid couplant between the transducer and the wall that, although it has been done, requires the unwanted introduct
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Laffan, Clair. Trigger Rate of High Energy Electrons in the Mu2e Experiment [Poster]. Office of Scientific and Technical Information (OSTI), 2019. http://dx.doi.org/10.2172/1579219.

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Kaganovich, I. D., R. C. Davidson, M. A. Dorf, et al. Physics of Neutralization of Intense High-Energy Ion Beam Pulses by Electrons. Office of Scientific and Technical Information (OSTI), 2010. http://dx.doi.org/10.2172/981704.

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Gurevich, Aleksander V. Nonlinear Structuring and High-energy Electrons: Role in Ionosphere and in Thunderstorm Atmosphere Processes. Defense Technical Information Center, 2010. http://dx.doi.org/10.21236/ada535278.

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Rich, J. W., Walter R. Lempert, and Igor V. Adamovich. Energy Transfer Processes Among Electrons and Vibrationally Excited Air Species in High Enthalpy Flows. Defense Technical Information Center, 2007. http://dx.doi.org/10.21236/ada478735.

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Horton-Smith, G. A. A study of high field quantum electrodynamics in the collision of high energy electrons with a terawatt laser. Office of Scientific and Technical Information (OSTI), 1998. http://dx.doi.org/10.2172/663331.

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