Relevant bibliographies by topics / Compton electrons and electron-positrons

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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 'Compton electrons and electron-positrons'

Author: Grafiati
Published: 2 June 2025
Last updated: 31 July 2025

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Journal articles on the topic "Compton electrons and electron-positrons"

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Dapor, Maurizio. "Comparison of Electron Compton Scattering with Positron Compton Scattering in Polyethylene." Materials 18, no. 7 (2025): 1609. https://doi.org/10.3390/ma18071609.

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Understanding the interaction of charged particles with polymers is crucial for applications in materials science, radiation physics, and electron spectroscopy. This study investigates the differences in the elastic scattering spectra of electrons and positrons in polyethylene, focusing on the underlying mechanisms that influence the spectral features. The analysis isolates key factors such as recoil energy, Doppler broadening, and the interplay between elastic and inelastic mean free paths. Using Monte Carlo simulations, we analyze the effects of the elastic and inelastic mean free paths on t
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SAKAUE, KAZUYUKI, TAKU SAITO, ISSEI YAMAZAKI, et al. "POLARIZED POSITRON GENERATION BASED ON LASER COMPTON SCHEME AND ITS POLARIZATION MEASUREMENTS." International Journal of Modern Physics B 21, no. 03n04 (2007): 519–26. http://dx.doi.org/10.1142/s021797920704232x.

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We have proposed a new scheme for polarized positron production, consisting of two quantum processes i.e. inverse Compton scatterings of circularly polarized laser light on high-quality electron beams and successive electron-positron pair creations. Using a circularly polarized laser beam of 532 nm scattered off a high-quality electron beam with the energy of 1.28 GeV, we have demonstrated for the first time productions of highly polarized positrons with an intensity of 2×104 e +/ bunch and an average energy of 36 MeV. Hence an average polarization of positrons was determined as 73±15( stat )±
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Jonas, P., P. Schattschneider, and P. Pongratz. "Removal of Bragg-Compton Channel Coupling in Electron Compton Scattering." Proceedings, annual meeting, Electron Microscopy Society of America 48, no. 2 (1990): 24–25. http://dx.doi.org/10.1017/s0424820100133710.

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Electron Compton scattering is inelastic scattering of fast electrons at large angles off core or valence electrons. The energy of the scattered electron is increasingly lowered with scattering angle; the energy distribution can be shown to be an image of the electron momentum density distribution in the ground state.The most dominant problem in ECOSS (Electron Compton Scattering from Solids), is the Bragg-Compton channel coupling. Bragg scattered electrons in the specimen act as new sources for Compton scattering. Since these Compton events correspond to various scattering angles a number of
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Cirelli, Marco, Bradley J. Kavanagh, Nicolao Fornengo, and Elena Pinetti. "Constraining sub-GeV dark matter with the Integral data." Journal of Physics: Conference Series 2156, no. 1 (2021): 012033. http://dx.doi.org/10.1088/1742-6596/2156/1/012033.

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Abstract The goal of this work is to constrain sub-GeV dark matter particles (1 MeV ≤ mDM ≤ 5 GeV) by looking at photons in the keV energy range and by including the inverse Compton scattering contribution to the total flux. In particular, the electrons and positrons produced by dark matter particles can scatter the low-energy photons in the Milky Way up to the X-ray energies. These X rays are probed by the Integral data, which we utilised to constrain the dark matter annihilation cross-section. The relevant annihilation channels are electron, muon and pion. As a result, we derived competitive
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LOTZE, K. H. "SIMULTANEOUS CREATION OF ELECTRON–POSITRON PAIRS AND PHOTONS IN ROBERTSON–WALKER UNIVERSES WITH STATICALLY BOUNDED EXPANSION." International Journal of Modern Physics A 07, no. 12 (1992): 2695–712. http://dx.doi.org/10.1142/s0217751x92001216.

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We present, based upon quantum electrodynamics in Robertson–Walker flat universes, a thorough analysis of the creation of mutually interacting electron–positron pairs and photons from vacuum. Therefore we discuss at least qualitatively all processes contributing to the number densities of created particles up to the second order in the coupling constant. For two particular expansion laws with Minkowskian in respectively in and out regions, we obtain exact solutions to the Dirac equation and investigate in detail the process of simultaneous creation of electron–positron pairs and photons and th
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Haug, Espen Gaarder. "Relativistic Compton Wavelength." European Journal of Applied Physics 4, no. 4 (2022): 24–27. http://dx.doi.org/10.24018/ejphysics.2022.4.4.190.

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In 1923, Arthur Holly Compton introduced what today is known as the Compton wavelength. Even if the Compton scattering derivation by Compton is relativistic in the sense that it takes into account the momentum of photons traveling at the speed of light, the original Compton derivation indirectly assumes that the electron is stationary at the moment it is scattered by electrons, but not after it has been hit by photons. Here, we extend this to derive Compton scattering for the case when the electron is initially moving at a velocity v.
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Borysova, M. "Studies of high-field QED with the LUXE experiment at the European XFEL." Journal of Instrumentation 16, no. 12 (2021): C12030. http://dx.doi.org/10.1088/1748-0221/16/12/c12030.

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Abstract The LUXE experiment aims at studying high-field QED in electron-laser and photon-laser interactions, with the 16.5 GeV electron beam of the European XFEL and a laser beam with power of up to 350 TW. The experiment will measure the spectra of electrons and photons in non-linear Compton scattering where production rates in excess of 109 are expected per 1 Hz bunch crossing. At the same time positrons from pair creation in either the two-step trident process or the Breit-Wheeler process will be measured, where the expected rates range from 10−3 to 104 per bunch crossing, depending on the
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Schaap, B. H., T. D. C. de Vos, P. W. Smorenburg, and O. J. Luiten. "Photon yield of superradiant inverse Compton scattering from microbunched electrons." New Journal of Physics 24, no. 3 (2022): 033040. http://dx.doi.org/10.1088/1367-2630/ac59eb.

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Abstract Compact x-ray sources offering high-brightness radiation for advanced imaging applications are highly desired. We investigate, analytically and numerically, the photon yield of superradiant inverse Compton scattering from microbunched electrons in the linear Thomson regime, using a classical electrodynamics approach. We show that for low electron beam energy, which is generic to inverse Compton sources, the single electron radiation distribution does not match well to collective amplification pattern induced by a density modulated electron beam. Consequently, for head-on scattering fr
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Wen, Lu, Ke-Yao Wu, Huan Yu, and Jun Fang. "Investigating the energy distribution of the high-energy particles in the Crab nebula." Research in Astronomy and Astrophysics 21, no. 11 (2021): 286. http://dx.doi.org/10.1088/1674-4527/21/11/286.

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Abstract The Crab nebula is a prominent pulsar wind nebula detected in multiband observations ranging from radio to very high-energy γ-rays. Recently, γ-rays with energies above 1 PeV have been detected by the Large High Altitude Air Shower Observatory, and the energy of the most energetic particles in the nebula can be constrained. In this paper, we investigate the broadest spectral energy distribution of the Crab nebula and the energy distribution of the electrons emitting the multiwavelength nonthermal emission based on a one-zone time-dependent model. The nebula is powered by the pulsar, a
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MacKinnon, A. L., and P. C. V. Mallik. "Inverse Compton X-rays from relativistic flare electrons and positrons." Astronomy and Astrophysics 510 (February 2010): A29. http://dx.doi.org/10.1051/0004-6361/200913190.

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Dissertations / Theses on the topic "Compton electrons and electron-positrons"

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AL, SALEH-MAHROUSSEH SALOUA. "Calcul relativiste, en electrodynamique quantique, de la diffusion compton sur un electron lie." Clermont-Ferrand 2, 1988. http://www.theses.fr/1988CLF21098.

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Pour expliquer le deplacement et l'elargissement du pic compton,lorsque l'energie du photon est voisine de l'energie de liaison de l'electron, il est necessaire d'introduire non seulement la liaison et le mouvement de l'electron, mais aussi le recul du mnoyau. On donne un calcul relativiste de la valeur quadratique moyenne de l'impulsion de l'electron et une expression generale des fonctions d'onde radiales. Pour le calcul analytique covariant de l'element de matrice ou utilise un propagateur pour un electron lie dans le schema de furry et determine la secton efficace, sans aucune integration
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Laborie, Jean-Marc. "Expérience de diffusion neutrino-électron auprès d'un réacteur nucléaire : étude et développement du détecteur anti-Compton." Université Joseph Fourier (Grenoble), 1998. http://www.theses.fr/1998GRE10036.

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L'experience munu consiste a mesurer la diffusion neutrino-electron aupres d'un reacteur nucleaire du centre de production electrique du bugey. Le detecteur central est une chambre a projection temporelle contenant 1 m#3 de cf#4 gazeux sous 5 bars et le seuil de detection des electrons de recul est place a 500 kev. La chambre est entouree d'un detecteur anti-compton et de blindages passifs. Le detecteur anti-compton est fait de 8 m#3 de scintillateur liquide et de 48 photomultiplicateurs de 20 cm de diametre, avec un seuil en energie de 100 kev. Il permet de detecter la plupart des photons aya
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Mok, Cheuk-wai. "Comparing electron and positron scattering factors for applications in diffraction and holography /." Hong Kong : University of Hong Kong, 1997. http://sunzi.lib.hku.hk/hkuto/record.jsp?B18716337.

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Porter, Troy Anthony. "Signatures of the propagation of primary and secondary cosmic ray electrons and positrons in the galaxy." Title page, table of contents and abstract only, 1999. http://web4.library.adelaide.edu.au/theses/09PH/09php848.pdf.

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Includes bibliographical references (8 p.) Examines some of the consequences of the acceleration and production, and propagation, of high energy electrons and positrons in the Galaxy. In particular, predictions are made of the diffuse photon signals arising from the interactions of electrons and positrons with gas, low energy photons, and the galactic magnetic field during their transport in the Galaxy.
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莫卓威 and Cheuk-wai Mok. "Comparing electron and positron scattering factors for applications indiffraction and holography." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1997. http://hub.hku.hk/bib/B31214459.

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Mikuni, Vinicius Massami. "Measurement of cosmic ray electrons and positrons with the AMS-02 experiment." Universidade de São Paulo, 2017. http://www.teses.usp.br/teses/disponiveis/76/76131/tde-29092017-143310/.

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The Alpha Magnetic Spectrometer (AMS-02) is a high-energy particle physics detector operating on the International Space Station (ISS) since May 2011. Since its launch, the AMS-02 provided a large amount of data whose precision was never before achieved, opening a new path for the study of cosmic rays (CRs). The first published results of AMS-021-3 show tension with the current understanding of the cosmic ray theory, particularly at higher energies. These tensions are directly linked to many fundamental questions like the dark matter nature, the CR origin and their propagation through the gala
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Drebot, Illya. "Electron beam dynamics with and without Compton back scattering." Phd thesis, Université Paris Sud - Paris XI, 2013. http://tel.archives-ouvertes.fr/tel-00920424.

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This thesis introduce my work on transverse and longitudinal non linear dynamics of an electron beam in ThomX, a novel X-ray source based on Compton backscattering. In this work I implemented in simulation code theoretical models to calculate transverse and longitudinal non linear dynamics under Compton back scattering. The processes studied include collective effect such as longitudinal space charge, resistive wall and coherent synchrotron radiation, intra beam scattering. I also implemented a longitudinal feedback algorithm and studied the effect of the feedback's delay in the simulation to
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You, Yan. "Pulsed Laser Injected Enhancement Cavity for Laser-electron Interaction." Phd thesis, Université Paris Sud - Paris XI, 2014. http://tel.archives-ouvertes.fr/tel-01011958.

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X-ray diffraction and scattering, X-ray spectroscopy, and X-ray crystallography are widely used in the life sciences, material science, and medical diagnosis. High-quality and high-brightness X-rays are a strong requirement to improve applications. Inverse Compton scattering (ICS) X-ray source has attracted great interests worldwide lately. To significantly enhance the average X-ray photon flux, a compact electron storage-ring combined with a high finesse optical enhancement cavity (OEC) can be utilized. In such a system, the collision rate between the electron beam and the laser pulse is great
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MUNINI, RICCARDO. "Solar modulation of cosmic ray electrons and positrons measured by the PAMELA experiment during the 23rd solar minimum." Doctoral thesis, Università degli Studi di Trieste, 2016. http://hdl.handle.net/11368/2908077.

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Cosmic rays (CRs) are energetic particles mainly originating outside the Solar System in extremely powerful environments like supernovae remnants (SNRs). The cosmic radiation is composed primarily of high-energy protons, helium and atomic nuclei while only a small fraction are electrons, anti-protons and positrons. During propagation through the Galaxy, CRs interact with the interstellar matter and the Galactic magnetic field. Because of these interactions CRs lose energy and change their spectral features with respect to the injection spectrum. Moreover, before reaching the Earth, CRs trave
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Bowles, Cameron Michael Albert, and cameronbowles@hotmail com. "Pushing the boundaries of condensed matter electron momentum spectroscopy." The Australian National University. Research School of Physical Sciences and Engineering, 2008. http://thesis.anu.edu.au./public/adt-ANU20080409.193948.

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An electron momentum spectrometer at the Australian National University has been used to study various aspects of different solid state systems. EMS is a transmission mode technique and involves the collision of the incident electron with a bound electron, after which both electrons are ejected and measured in coincidence. Through well defined reaction kinematics the complete valence spectral momentum density A(ɛ,q) can be measured. The spectrometer has been used to measure the spectral momentum densities (spectral functions) of single crystal targets, as well as targets in disordered states.
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Books on the topic "Compton electrons and electron-positrons"

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Gupta, Atam D. The electron-positron theory of the nucleus and the constructive role of black holes and of the neutrino and the antineutrino. A.D. Gupta, 1994.

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Simhony, M. The electron-positron lattice space: Cause of relativity and quantum effects. Physics Section 5, Hebrew University, 1988.

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Papanikolaou, N. Handbook of calculated electron momentum distributions, compton profiles, and x-ray form factors of elemental solids. CRC Press, 1991.

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Compton scattering by static and moving media. National Aeronautics and Space Administration, 1997.

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Martin, Colin J. Interaction of ionizing radiations with matter. Oxford University Press, 2015. http://dx.doi.org/10.1093/med/9780199655212.003.0002.

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Interactions of ionizing radiations with matter are fundamental to the practice of radiation protection. They determine the magnitude and distribution of doses in tissues, the performance of detectors and imaging devices, and the attenuating properties of shielding materials. This chapter describes briefly the processes of radioactive decay and the properties of the various particles emitted, and then goes on to consider the interactions of radiation with matter. Electron interactions with metals result in bremsstrahlung and characteristic X-rays that form the basis of X-ray production. The in
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Book chapters on the topic "Compton electrons and electron-positrons"

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Gaskell, Dave. "Electron Polarimetry." In Polarized Beam Dynamics and Instrumentation in Particle Accelerators. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-16715-7_13.

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AbstractElectron polarimetry benefits from the ability to use processes with well-known analyzing powers, hence enabling high precision measurements. Several techniques are employed to measure electron beam polarization, including Mott, Møller, and Compton polarimetry. Each technique has particular advantages and disadvantages, depending on the application. This chapter will focus on the techniques used to measure electron beam polarization, with particular emphasis on the challenges and requirements for achieving high precision. The development of a conceptual design of a Compton polarimeter
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Lee, Jeong Han. "Electron beam line design of A4 Compton backscattering polarimeter." In From Parity Violation to Hadronic Structure and more. Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/3-540-26345-4_32.

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Bonolis, Luisa. "Bruno Touschek (1921–1978). The Path to Electron-Positron Collisions." In Springer Proceedings in Physics. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-23042-4_2.

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AbstractThe 100th anniversary of Bruno Touschek’s birth also marks 60 years since the first beams of electrons and positrons circulated in AdA, the first ever matter-antimatter collider, built in Frascati National Laboratories following Touschek’s visionary proposal of February 1960. Touschek’s path to such idea is briefly outlined, beginning with his early years as a student—first in Vienna and later in Germany—through his first experiences with Rolf Widerøe’s betatron and the electron synchrotron accelerator in Glasgow after the war, along with his relationships with the fathers of modern ph
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Oomi, Gendo, Fuminori Honda, Tomoko Kagayama, et al. "Effect of pressure on the Compton scattering of metallic Li." In Electron, Spin and Momentum Densities and Chemical Reactivity. Springer Netherlands, 2000. http://dx.doi.org/10.1007/0-306-46943-x_25.

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Brancewicz, Marek, Henryk Reniewicz, Andrzej Andrejczuk, Ludwik Dobrzyński, Eugeniusz Żukowski, and Stanisław Kaprzyk. "Electron Momentum Density of Hexagonal Magnesium Studied by Compton Scattering." In Solid State Phenomena. Trans Tech Publications Ltd., 2006. http://dx.doi.org/10.4028/3-908451-19-1.123.

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Derishev, E. V., V. V. Kocharovsky, Vl V. Kocharovsky, and P. Mészáros. "GRB Synchrotron-Self-Compton Emission Generated by Self-Consistent Electron Distribution." In Gamma-Ray Bursts in the Afterglow Era. Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/10853853_87.

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Orszag, M. "Quantum and Many-Body Effects in a Compton Regime Free-Electron Laser." In Springer Proceedings in Physics. Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71407-8_24.

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Bonifacio, R., and F. Casagrande. "Cooperative Effects and Superradiance in Compton Scattering and Their Relevance to Free Electron Lasers." In Complex Systems — Operational Approaches in Neurobiology, Physics, and Computers. Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/978-3-642-70795-7_27.

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Maruani, Jean. "The Dirac Electron: Spin, Zitterbewegung, the Compton Wavelength, and the Kinetic Foundation of Rest Mass." In Quantum Systems in Chemistry and Physics. Springer Netherlands, 2012. http://dx.doi.org/10.1007/978-94-007-5297-9_2.

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Pickrell, Mark. "Matter/Anti-Matter Propulsion." In Propulsion Systems - Recent Advances, New Perspectives and Applications [Working Title]. IntechOpen, 2023. http://dx.doi.org/10.5772/intechopen.110310.

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One of the key potential technologies for generating high speeds in space is matter/anti-matter annihilation. With the Compton effect, if positrons and electrons can be annihilated in a controlled way, and in sufficient quantities, then humans are able to achieve relativistic speeds in space. This chapter describes a technology, matter/anti-matter propulsion, which is likely to enable the generation of relativistic speeds in space. To explain this technology, background information and prior efforts to promote matter/anti-matter annihilation as a propulsion source are introduced. Further, base
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Conference papers on the topic "Compton electrons and electron-positrons"

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Balanov, Amnon, Ron Ruimy, and Ido Kaminer. "Toward high-gain laser-driven electron undulation." In CLEO: Fundamental Science. Optica Publishing Group, 2024. http://dx.doi.org/10.1364/cleo_fs.2024.fw3c.2.

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We find an unexplored regime of inverse Compton scattering, achieving high-gain undulation as in FELs. We show the potential for soft-X-ray and extreme ultraviolet radiation sources based on next-generation electron sources and state-of-the-art laser sources.
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Tilton, Sean E., Elena L. Ros, Kevin E. Schmidt, et al. "Laser-Based Undulator Design for Soft X-ray Free Electron Laser." In CLEO: Fundamental Science. Optica Publishing Group, 2024. http://dx.doi.org/10.1364/cleo_fs.2024.fw3c.1.

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We present an optical undulator design of a soft X-ray compact free electron laser with a laser-based undulator feasible with commercially available laser systems. We simulate the Inverse Compton Scattering process and investigate engineering constraints.
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Takada, Atsushi, Tomonori Ikeda, Mitsuru Abe, et al. "Celestial MeV gamma-ray observation using electron-tracking Compton camera loaded on long duration balloons (SMILE-3)." In Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, edited by Jan-Willem A. den Herder, Kazuhiro Nakazawa, and Shouleh Nikzad. SPIE, 2024. http://dx.doi.org/10.1117/12.3016872.

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McDonald, Kirk. "Laser Electron Studies of Nonlinear QED." In High-Energy Density Physics with Subpicosecond Laser Pulses. Optica Publishing Group, 1989. http://dx.doi.org/10.1364/hpslp.1989.m6.

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An experimental program is underway to use collisions of intense laser pulses with free electrons to study nonlinear QED processes such as nonlinear Compton scattering, pair creation by light, light-by-light scattering, and vacuum Cerenkov radiation.
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Swiderski, L., R. Marcinkowski, M. Szawlowski, et al. "Non-proportionality of electron response and energy resolution of Compton electrons in scintillators." In 2010 IEEE Nuclear Science Symposium and Medical Imaging Conference (2010 NSS/MIC). IEEE, 2010. http://dx.doi.org/10.1109/nssmic.2010.5873766.

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Schumacher, D. W., P. H. Bucksbaum, and M. Bashkansky. "Stimulated Compton Backscattering and the High Intensity Kapitza-Dirac Effect*." In Short Wavelength Coherent Radiation: Generation and Applications. Optica Publishing Group, 1988. http://dx.doi.org/10.1364/swcr.1988.hilim236.

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We report the scattering of low energy free electrons from an optical standing wave at intensities of 1013 to 1014W/cm2.1 This interaction is the high intensity limit of the Kapitza-Dirac effect,2 wherein electrons Bragg scatter from the standing wave "lattice". In this regime, the momentum exchanged exceeds the reciprocal lattice vector by a factor of 500 or more, and the scattering rate is compar able to the optical frequency. The electron motion is most easily analyzed by classical mechanics.
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Mohideen, U., H. W. K. Tom, R. R. Freeman, J. Bokor, and P. H. Bucksbaum. "Nonlinear Compton Scattering in a Pulsed Focused Laser Beam." In Short Wavelength Coherent Radiation: Generation and Applications. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/swcr.1991.tub2.

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We have calculated the radiation emitted from free electrons in an ultrashort pulsed laser focus. For low electron densities, where space charge is negligible, we find that ponderomotive forces limit the effective volume where the radiation is emitted to a region much smaller than the waist at the focus. For typical focal parameters, the emitting region is significantly smaller than the fundamental wavelength. Nonetheless, constructive inteference plays a significant role in the collective radiation spectrum. Phase mismatch becomes important only for the higher harmonics. These studies are int
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Belenov, E. M., S. V. Grigoriev, A. V. Nazarkin, and I. V. Smetanin. "Optical Wiggler Free-Electron X-Ray Laser as a Two-Level Quantum, Generator with Fully Inverted Medium." In Short Wavelength Coherent Radiation: Generation and Applications. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/swcr.1991.wa2.

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Recently the possibility was widely discussed of creation of an X-ray free-electron laser (FEL) using a high-power laser pulse as the undulator (optical wiggler FEL) [1]. Optical wiggler FEL is characterized by relatively small energy of the used electrons (ε ~ 1÷10 MeV). In order to achieve high values of the gain for X-rays it is necessary to use rather monoenergetic electron beams (Δγ/γ ~ 10–4) and the wigglers with a large number of periodic elements (N ≥ 104). In such FEL the energy of X-ray quantum can exceed the induced emission Cabsorption) linewidth: ωX > max {εΔγ/γ, ε(4N–1)}. We h
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Belenov, E. M., S. V. Grigoriev, A. V. Nazarkin, and I. V. Smetanin. "Optical Wiggler Free-Electron X-Ray Laser as a Two-Level Quantum Generator with Fully Inverted Medium." In Soft X-Ray Projection Lithography. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/sxray.1991.wa2.

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Recently the possibility was widely discussed of creation of an X-ray free-electron laser (FEL) using a high-power laser pulse as the undulator (optical wiggler FEL) [1]. Optical wiggler FEL is characterized by relatively small energy of the used electrons (ε~1÷l0 MeV). In order to achieve high values of the gain for X-rays it is necessary to use rather monoenergetic electron beams (Δγ/γ~10−4) and the wigglers with a large number of periodic elements (N ≥ 104). In such FEL the energy of X-ray quantum can exceed the induced emission (absorption) linewidth:ωX> max {ℇΔγ/γ,ε(4N−1)}. We have sho
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Kryukov, P. G. "Possibility of Experimental Studies of Nonlinear Quantum Electrodynamics Effects Using High Power Ultrashort Laser Pulses." In International Conference on Ultrafast Phenomena. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/up.1992.tua3.

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Investigation of interaction of electrons and γ-quanta with very strong electromagnetic fields having the strength about Fo = m2c3 /eħ = 1.32×1016V/cm (characteristic QED field strength) is of principal interest for fundamental physics. Such a field performs the work equal to the electron rest energy (mc2) at its Compton wavelength (ħ/mc). Therefore one may think that intrinsic properties of an electron would be manifested due to action the field ~FO on parts of an elementary charge. If such a field is produced with a laser then frequency and wavelength must have values ω ~mc2/ħ and λ h/mc in
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Reports on the topic "Compton electrons and electron-positrons"

1

Pogorelsky, I. V., I. Ben-Zvi, and T. Hirose. Laser-electron Compton interaction in plasma channels. Office of Scientific and Technical Information (OSTI), 1998. http://dx.doi.org/10.2172/291126.

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2

POGORELSKY, I. V. LASER-ELECTRON COMPTON INTERACTION IN PLASMA CHANNELS. Office of Scientific and Technical Information (OSTI), 1998. http://dx.doi.org/10.2172/10392.

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3

Espy, Michelle A., and Amanda E. Gehring. Measuring x-ray spectra with a Compton electron spectrometer. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1115546.

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4

Malyzhenkov, Alexander, and Nikolai Yampolsky. Optimization of Compton Source Performance through Electron Beam Shaping. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1329533.

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5

Hahm, T. S. Flow shear induced Compton scattering of electron drift instability. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/5746326.

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6

Hahm, T. S. Flow shear induced Compton scattering of electron drift instability. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/10125128.

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7

Ohgaki, T. Analysis and simulation for laser-Compton cooling of electron beams. Office of Scientific and Technical Information (OSTI), 1999. http://dx.doi.org/10.2172/764352.

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8

Malyzhenkov, Alexander. PHASE-SPACE MANIPULATIONS OF ELECTRON BEAMS FOR X-RAY FREE-ELECTRON LASERS AND INVERSE COMPTON SCATTERING SOURCES. Office of Scientific and Technical Information (OSTI), 2018. http://dx.doi.org/10.2172/1489921.

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9

Mackinnon, A., B. Copsey, and J. Celeste. The Effectiveness of the Compton Radiography Snout Electron Deflection Yoke and its Application as an Electron Spectrometer. Office of Scientific and Technical Information (OSTI), 2009. http://dx.doi.org/10.2172/1057222.

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10

Melissinos, A., N. Bigelow, M. Fitch, et al. Compton scattering x-ray experiments at the Fermilab electron source facility. Office of Scientific and Technical Information (OSTI), 1997. http://dx.doi.org/10.2172/1847745.

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