Academic literature on the topic 'Electrons de recul Compton'
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Journal articles on the topic "Electrons de recul Compton"
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 (August 12, 1990): 24–25. http://dx.doi.org/10.1017/s0424820100133710.
Full textPoutanen, Juri, and Indrek Vurm. "THEORY OF COMPTON SCATTERING BY ANISOTROPIC ELECTRONS." Astrophysical Journal Supplement Series 189, no. 2 (July 12, 2010): 286–308. http://dx.doi.org/10.1088/0067-0049/189/2/286.
Full textZacharias, Michael, and Reinhard Schlickeiser. "EXTERNAL COMPTON EMISSION IN BLAZARS OF NONLINEAR SYNCHROTRON SELF-COMPTON-COOLED ELECTRONS." Astrophysical Journal 761, no. 2 (December 3, 2012): 110. http://dx.doi.org/10.1088/0004-637x/761/2/110.
Full textAhuja, B. L., Vinit Sharma, and Y. Sakurai. "Magnetic Compton Scattering Study of Shape Memory Alloys." Advanced Materials Research 52 (June 2008): 145–54. http://dx.doi.org/10.4028/www.scientific.net/amr.52.145.
Full textKaliman, Z., N. Orlić, and I. Jelovica. "Polarization effects in Compton scattering from K-electrons." Radiation Physics and Chemistry 71, no. 3-4 (October 2004): 661–63. http://dx.doi.org/10.1016/j.radphyschem.2004.04.044.
Full textKotkin, G. L., S. I. Polityko, and V. G. Serbo. "Polarization of final electrons in the Compton effect." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 405, no. 1 (March 1998): 30–38. http://dx.doi.org/10.1016/s0168-9002(97)01112-1.
Full textSwanekamp, S. B., B. V. Weber, N. R. Pereira, D. D. Hinshelwood, S. J. Stephanakis, and F. C. Young. "Measuring multimegavolt pulsed voltages using Compton-generated electrons." Review of Scientific Instruments 75, no. 1 (January 2004): 166–73. http://dx.doi.org/10.1063/1.1628843.
Full textBasavaraju, G., P. P. Kane, and Suju M. George. "Compton scattering of 279.2-keVγrays byK-shell electrons." Physical Review A 36, no. 2 (July 1, 1987): 655–64. http://dx.doi.org/10.1103/physreva.36.655.
Full textZdziarski, Andrzej A., and Patryk Pjanka. "Compton scattering of blackbody photons by relativistic electrons." Monthly Notices of the Royal Astronomical Society 436, no. 4 (October 24, 2013): 2950–55. http://dx.doi.org/10.1093/mnras/stt1773.
Full textSurić, T., P. M. Bergstrom, K. Pisk, and R. H. Pratt. "Compton scattering of photons by inner-shell electrons." Physical Review Letters 67, no. 2 (July 8, 1991): 189–92. http://dx.doi.org/10.1103/physrevlett.67.189.
Full textDissertations / Theses on the topic "Electrons de recul Compton"
Liu, Shan. "Development of Diamond Sensors for Beam Halo and Compton Spectrum Diagnostics after the Interaction Point of ATF2." Thesis, Paris 11, 2015. http://www.theses.fr/2015PA112112/document.
Full textThe investigation of beam halo transverse distributions is an important issue for beam losses and background control in ATF2 and in Future Linear Colliders (FLC). A novel in vacuum diamond sensor (DSv) scanner with four strips has been designed and developed for the investigation of beam halo transverse distributions and also for the diagnostics of Compton recoil electrons after the interaction point (IP) of ATF2, a low energy (1.3 GeV) prototype of the final focus system for ILC and CLIC linear collider projects. This thesis presents the beam halo and Compton recoil electrons studies as well as the characterization, performance studies and tests of the diamond sensors (DS) both at PHIL, a low energy (<10 MeV) photo-injector at LAL, and at ATF2. First beam halo measurement results using wire scanners (WS) and DSv at ATF2 are also presented and compared in this thesis. Simulations using Mad-X and CAIN were done to estimate the rate of the beam halo and Compton recoil electrons. Simulation results have indicated that a large dynamic range of more than 10⁶ is needed for a simultaneous measurement of the beam core, beam halo and Compton recoil electrons. A single crystalline Chemical Vapor-Deposition (sCVD) based DSv was developed for this purpose. Prior to the diamond detector installation, first attempt of beam halo measurements have been performed in 2013 using the currently installed WS. With a limited dynamic range of ~10³ , the beam halo distribution was measured only up to ~±6σ in the extraction (EXT) line. Parametrizations of the measured beam halo distribution showed a consistent distribution with previous measurements done in 2005 at the old ATF beam line. Meanwhile, an asymmetric vertical beam halo distribution was observed for the first time using the post-IP WS, the origin of which is currently under investigation using the DSv.Studies to characterize DS pads with dimensions of 4.5x4.5x0.5 mm³ were carried out using the α and β sources. Charge carrier transport parameters (lifetime, saturation velocity etc.) were obtained using the transient-current technique (TCT). Furthermore, the linearity of the DS response was tested at PHIL with different beam intensities in air: a maximum signal of 108 electrons was measured with a linear response up to 10⁷ electrons. Similar linearity studies were done for the DSv at ATF2, where we have successfully demonstrated and confirmed for the first time a dynamic range of ~10⁶ by a simultaneous beam core (~10⁹ e-) and beam halo (~10³ e-) measurement using the DSv. Present limitations due to signal pick-up and saturation effects, which prevent the DSv from reaching a dynamic range higher than 10⁶ , were also studied.First measurements of the horizontal beam halo distribution using the DSv were performed up to ~±20σx, where the beam halo was proved to be collimated by the apertures. Horizontal beam halo distributions consistent with the 2005 and 2013 parametrizations were confirmed. The possibility of probing the Compton recoil electrons has been investigated and different ways to increase their visibility have been proposed
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.
Full textMossé, Laurent. "Etude de la diffusion Compton virtuelle en régime profondément inélastique pour le dispositif expérimental COMPASS." Paris 11, 2002. http://www.theses.fr/2002PA112027.
Full textRecently, new parton distributions called generalized parton distributions (GPD) appeared in the description of the internal structure of the nucleon. They enrich the pieces of information accessible through the usual parton distributions and connect the latter with the form factors. They are the subject of extensive theoretical as well as experimental studies. The Deeply Virtual Compton Scattering (DVCS) is the simplest process that gives access to these new distributions. It is possible to use the high energy muon beam (1̃00GeV) and the experimental setup of COMPASS at CERN to measure the DVCS process. This PhD thesis is devoted to the studies of GPD and DVCS in general and to its measurement at COMPASS in particular. After a study of the theoretical framework of GPD, the experimental situation in the world is presented, and light is shed on the stake of a DVCS experiment at COMPASS. The feasibility of such an experiment is then validated through a simulation. This experiment takes benefit of the existing apparatus and requires the construction of an hermetic recoil detector, mainly to insure systematically the exclusivity of the measurement. The calculation of the counting rates expected for a 6 months data taking period allows to confirm the interest of the measurements for the study of GPD. Tests of a recoil detector prototype, based on a time of flight measurement and operating in the noisy environment of the COMPASS muon beam, are described and analyzed. A pion of weak impulsion produced in the final state and adding to the DVCS process will be very hard to detect. It is of essential importance to insure that this process will not significantly disrupt the measurement of the DVCS process. A theoretical estimate, based on the derivation of a soft pion theorem is presented
FERRER, JEAN-LUC. "Etude de la dynamique non lineaire du spectre d'un laser a electrons libres dans le regime compton." Paris 11, 1990. http://www.theses.fr/1990PA112285.
Full textLaborie, 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.
Full textGarolfi, Luca. "Accélérateur linéaire d'électrons à fort gradient en bande S pour ThomX." Thesis, Université Paris-Saclay (ComUE), 2018. http://www.theses.fr/2018SACLS007/document.
Full textThe ThomX source should provide quasi-monochromatic high-quality X-rays (range 45-90 keV). The framework of the thesis is the electron beam linac energy upgrade from 50 MeV to 70 MeV necessary to achieve X-rays of 90 keV. For this purpose, the development of a compact high-gradient S-band electron accelerating structure is needed. It implies a research and development (R&D) activity at LAL in partnership with a French company (PMB-Alcen) in the High-Gradient (HG) technology of accelerating structures. The LAL-PMB-Alcen collaboration aims at the fabrication of a normal-conducting HG S-band structure by tackling the technological aspects that limit the achievement of high-gradient acceleration mostly due to vacuum RF breakdown and pulsed heating fatigue. Basically, the electromagnetic and thermal design of the HG S-band accelerating section has been performed at LAL. Meanwhile, PMB-Alcen was in charge to perform the fabrication, tuning and low power tests of prototypes and the final accelerating section. In this work, a fully coupled electromagnetic-thermal-structural finite element analysis on the THOMX RF gun has been performed with Ansys workbench. The HG accelerating section final regular cell dimensions and the power coupler design have been optimized. In particular, the electromagnetic simulation techniques and outcomes have been applied to constant impedance (CI) TW prototypes and also to a constant gradient (CG) final accelerating section. This allowed to verify the geometry choice, validate the fabrication procedure and check the fulfilment of the normal operating conditions. Moreover, a coupled thermo-mechanical study on a CI copper prototype has been performed. The water cooling system has been simulated to validate the capability to extract the heat generated by the dissipated power on the walls of the structure and guarantee a uniform temperature distribution along the section. Also, vacuum simulations have been performed on a 16-cells CI copper prototype and also on the final CG accelerating section. In addition, the main steps for the fabrication of the RF gun at LAL and a 7-cells aluminium prototype at PMB-Alcen have been presented. RF low power tests on the prototype have been performed in order to validate the 3D geometry design and the machining process. Taking into account the experimental results, mechanical problems and technological constraints have been tackled and some solutions have been proposed for the future copper prototype fabrication. Finally, beam dynamics simulations of the ThomX linac has been carried out by ASTRA code. The aim is to reduce as much as possible the energy spread and the transverse emittance to preserve the spectral purity of the produced X-rays, at the electron-photon interaction point. A model as close as possible to the characteristics of the real components, such as RF gun, TW section and solenoids has been considered. Important results came out from these simulations regarding laser parameters (spot size and duration), the maximum magnetic field of solenoids for high space charge effect compensation, dephasing between the RF and laser in the gun and effect of the travelling wave electromagnetic field on the particle dynamics. Different options for the parameter settings of machine operation and a new configuration of the solenoids position have been proposed. An optimization of the beam dynamics properties has been obtained by using a genetic algorithm and the ultimate performances of the electron beam have been highlighted
Giesen, Gaelle. "Dark Matter Indirect Detection with charged cosmic rays." Thesis, Paris 11, 2015. http://www.theses.fr/2015PA112160/document.
Full textOverwhelming evidence for the existence of Dark Matter (DM), in the form of an unknownparticle filling the galactic halos, originates from many observations in astrophysics and cosmology: its gravitational effects are apparent on galactic rotations, in galaxy clusters and in shaping the large scale structure of the Universe. On the other hand, a non-gravitational manifestation of its presence is yet to be unveiled. One of the most promising techniques is the one of indirect detection, aimed at identifying excesses in cosmic ray fluxes which could possibly be produced by DM annihilations or decays in the Milky Way halo. The current experimental efforts mainly focus in the GeV to TeV energy range, which is also where signals from WIMPs (Weakly Interacting Massive Particles) are expected. Focussing on charged cosmic rays, in particular antiprotons, electrons and positrons, as well as their secondary emissions, an analysis of current and forseen cosmic ray measurements and improvements on astrophysical models are presented. Antiproton data from PAMELA imposes contraints on annihilating and decaying DM which are similar to (or even slightly stronger than) the most stringent bounds from gamma ray experiments, even when kinetic energies below 10 GeV are discarded. However, choosing different sets of astrophysical parameters, in the form of propagation models and halo profiles, allows the contraints to span over one or two orders of magnitude. In order to exploit fully the power of antiprotons to constrain or discover DM, effects which were previously perceived as subleading turn out to be relevant especially for the analysis of the newly released AMS-02 data. In fact, including energy losses, diffusive reaccelleration and solar modulation can somewhat modify the current bounds, even at large DM masses. A wrong interpretation of the data may arise if they are not taken into account. Finally, using the updated proton and helium fluxes just released by the AMS-02 experiment, the astrophysical antiproton to proton ratio and its uncertainties are reevaluated and compared to the preliminarly reported AMS-02 measurements. No unambiguous evidence for a significant excess with respect to expectations is found. Yet, some preference for thicker halos and a flatter energy dependence of the diffusion coefficient starts to emerge. New stringed constraints on DM annihilation and decay are derived. Secondary emissions from electrons and positrons can also be used to constrain DM annihilation or decay in the galactic halo. The radio signal due to synchrotron radiation of electrons and positrons on the galactic magnetic field, gamma rays from bremsstrahlung processes on the galactic gas densities and from Inverse Compton scattering processes on the interstellar radiation field are considered. With several magnetic field configurations, propagation scenarios and improved gas density maps and interstellar radiation field, state-of-art tools allowing the computaion of synchrotron and bremssttrahlung radiation for any WIMP DM model are provided. All numerical results for DM are incorporated in the release of the Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID). Finally, the possible GeV gamma-ray excess identified in the Fermi-LAT data from the Galactic Center in terms of DM annihilation, either in hadronic or leptonic channels is studied. In order to test this tantalizing interprestation, a multi-messenger approach is used: first, the computation of secondary emisison from DM with respect to previous works confirms it to be relevant for determining the DM spectrum in leptonic channels. Second, limits from antiprotons severely constrain the DM interpretation of the excess in the hadronic channel, for standard assumptions on the Galactic propagation parameters and solar modulation. However, they considerably relax if more conservative choices are adopted
Books on the topic "Electrons de recul Compton"
L, Imhof William, and United States. National Aeronautics and Space Administration., eds. Compton Gamma Ray Observatory/BATSE observations of energetic electrons scattered by cyclotron resonance with waves from powerful VLF transmitters. [Washington, DC: National Aeronautics and Space Administration, 1994.
Find full textL, Imhof William, and United States. National Aeronautics and Space Administration., eds. Compton Gamma Ray Observatory/BATSE observations of energetic electrons scattered by cyclotron resonance with waves from powerful VLF transmitters. [Washington, DC: National Aeronautics and Space Administration, 1994.
Find full text1954-, Zdziarski Andrzej A., Svensson R, and United States. National Aeronautics and Space Administration., eds. Can the cosmic X-ray and gamma-ray background be due to reflection of a steep power law spectrum and Compton scattering by relativistic electrons? [Washington, DC: National Aeronautics and Space Administration, 1991.
Find full text1954-, Zdziarski Andrzej A., Svensson Roland, and United States. National Aeronautics and Space Administration., eds. Can the cosmic X-ray and gamma-ray background be due to reflection of a steep power law spectrum and Compton scattering by relativistic electrons? [Washington, DC: National Aeronautics and Space Administration, 1991.
Find full text1954-, Zdziarski Andrzej A., Svensson Roland, and United States. National Aeronautics and Space Administration., eds. Can the cosmic X-ray and gamma-ray background be due to reflection of a steep power law spectrum and Compton scattering by relativistic electrons? [Washington, DC: National Aeronautics and Space Administration, 1991.
Find full textBook chapters on the topic "Electrons de recul Compton"
"COMPTON SCATTERING OF LASER LIGHT." In Novel Radiation Sources Using Relativistic Electrons, 89–98. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789812817129_0004.
Full text"MULTIPHOTON COMPTON SCATTERING AND PONDEROMOTIVE FORCES IN AN INHOMOGENEOUS LIGHT FIELD." In Atomic and Free Electrons in a Strong Light Field, 131–82. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789812817204_0003.
Full textZubairy, M. Suhail. "De Broglie Waves: Are Electrons Waves or Particles?" In Quantum Mechanics for Beginners, 100–120. Oxford University Press, 2020. http://dx.doi.org/10.1093/oso/9780198854227.003.0007.
Full textKrishnan, Kannan M. "X-Ray Diffraction." In Principles of Materials Characterization and Metrology, 408–80. Oxford University Press, 2021. http://dx.doi.org/10.1093/oso/9780198830252.003.0007.
Full text"into account. Therefore, every time a new batch of food is to be irradiated, the operator must establish the dose and dose distribution by strategically placing dose meters into and between the food packages and evaluating the dose meter reading. Once the process is running smoothly, it is usually not necessary to carry out dosimetry on all the product. Monitoring the process parameters and making occasional dosimetric checks is now sufficient (23). In most countries government regulations require that food irradiation proces sors maintain records that describe for each food lot the radiation source, source calibration, dosimetry, dose distribution in the product, and certain other process parameters (see Chapter 11). A short introduction to the interaction of ionizing radiation with matter is appro priate at this point, although the effects of ionizing radiation on food components will be described in more detail in Chapter 3. When high-energy electrons are absorbed by a medium they lose their kinetic energy by interacting with electrons of the medium. (At very high energy, far above that allowed for food irradiation, accelerated electrons can also interact with nuclei of the medium.) The interaction with orbital electrons of the atoms of the medium (the absorber) causes ionizations and excitations. Ionization means that orbital electrons are ejected from atoms of the medium; excitation means that orbital electrons move to an orbit of higher energy. Ejected electrons (secondary electrons), carrying a large portion of the energy of the incident electron, also lose energy through interaction with orbital electrons of the absorber. Electrons at low velocities (subexcitation energy level) can cause molecular vibrations on their way to becoming thermalized. As a result of the collisions with atoms of the absorber material the incident electrons can change direction. Repeated collisions cause multiple changes of direction. The result is a scattering of electrons in all directions. This is shown schematically in Figure 12a. When gamma or x-ray photons interact with the absorber, three types of interaction can occur: The photoelectric effect The Compton effect, and Pair production (i.e., formation of pairs of electrons and positrons) Photoelectric absorption occurs largely with photons of energies below 0.1 MeV and pair production primarily with photons of energies above 10 MeV. Both are of minor importance in food irradiation, where the Compton effect predominates. As portrayed in Figure 13, in the Compton effect an incident photon interacts with an absorber atom in such a way that an orbital electron is ejected. The incident photon continues after the collision in a changed direction and with less." In Safety of Irradiated Foods, 47–48. CRC Press, 1995. http://dx.doi.org/10.1201/9781482273168-37.
Full text"than its original energy. The ejected electron (Compton electron) has enough kinetic energy to cause excitations and ionizations in the absorber atoms. It thus interacts with the absorber in the same way as the ejected secondary electrons produced by an electron accelerator beam (Fig. 12b). Because Compton electrons are produced when gamma or x-ray photons interact with a medium, and because the Compton electrons cause ionizations and excitations in the same way as secondary electrons produced by accelerator beam electrons, the radiation-induced chemical changes in the irradiated medium are largely the same, regardless of the type of radiation used. The purpose of dose meters is to measure the amount of radiation energy absorbed by the irradiated product. The instrument that gives a reading of absorbed dose directly is the calorimeter. It measures the total energy dissipated or the rate of energy dissipation in a material in terms of the thermal properties of the absorbing body. This instrument, therefore, is considered to be an absolute dose meter that can be used for calibrating other dose meters. The principle of radiation calorime try is implicit in the definition of the radiation dose unit 1 Gy (gray) = 1 J (joule)/ kg. Ideally the temperature elevation should be measured in the irradiated food product itself— but in practice this is usually not done because the thermal properties of foodstuffs vary widely. A substance with known, reproducible thermal properties is taken instead, which serves as a heat-sensing calorimetric body, included in an adiabatic system (adiabatic = without transmission of heat). Water, graphite, aluminum, or a water-equivalent plastic is usually chosen, and the thermal change is determined by small calibrated thermocouples or thermis tors embedded in the calorimetric body. The practice of using radiation calorimetry is not simple, and ways to use it in a routine fashion have been developed only recently (24,25). Because the process of temperature elevation should run under adiabatic or quasi-adiabatic conditions, the dose has to be applied in a very short time. Calorimetry is therefore mostly used for measuring electron accelerator beam doses. The absorbed dose in the calorimetric body can be converted to that of the material of interest (foodstuff) by taking into consideration the different density and the different energy absorp tion coefficients of the two materials. The temperature elevation depends on radiation dose and on the specific heat of the material irradiated. A dose of 10 kGy causes a temperature elevation as follows: 2.3K in water (specific heat 4.2 kJ/kg • K) 6.2K in dry protein (specific heat 1.6 kJ/kg • K) 7.1K in dry carbohydrate (specific heat 1.4 kJ/kg • K) 12.5 K in glass (specific heat 0.8 kJ/kg • K)." In Safety of Irradiated Foods, 49. CRC Press, 1995. http://dx.doi.org/10.1201/9781482273168-38.
Full textConference papers on the topic "Electrons de recul Compton"
Poutanen, Juri. "Compton scattering matrix for relativistic Maxwellian electrons." In COMPTON GAMMA-RAY OBSERVATORY. AIP, 1993. http://dx.doi.org/10.1063/1.44318.
Full textSwiderski, L., M. Moszynski, W. Czarnacki, A. Syntfeld-Kazuch, T. Szczesniak, R. Marcinkowski, G. Pausch, C. Plettner, and K. Roemer. "Energy resolution of Compton electrons in scintillators." In 2009 IEEE Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC 2009). IEEE, 2009. http://dx.doi.org/10.1109/nssmic.2009.5402321.
Full textConka-Nurdan, T., K. Nurdan, K. Laihem, A. H. Walenta, C. Fiorini, N. Hornel, L. Struder, and C. Venanzi. "Compton electrons in Silicon Drift Detector: first results." In 2003 IEEE Nuclear Science Symposium. Conference Record (IEEE Cat. No.03CH37515). IEEE, 2003. http://dx.doi.org/10.1109/nssmic.2003.1352290.
Full textWhite, Timothy R., Alan P. Lightman, and Andrzej A. Zdziarski. "Compton reflection of gamma-rays by cold electrons." In AIP Conference Proceedings Volume 170. AIP, 1988. http://dx.doi.org/10.1063/1.37229.
Full textHollerman, W. A. "Measurement of Compton scattered electrons using monochromatic X-rays." In The CAARI 2000: Sixteenth international conference on the application of accelerators in research and industry. AIP, 2001. http://dx.doi.org/10.1063/1.1395283.
Full textSzawlowski, M., M. Kapusta, L. Swiderski, R. Marcinkowski, M. Moszynski, T. Szczesniak, M. Grodzicka, D. Wolski, and A. Celler. "Linearity and energy resolution of compton electrons in CZT measured using the wide angle compton coincidence technique." In 2010 IEEE Nuclear Science Symposium and Medical Imaging Conference (2010 NSS/MIC). IEEE, 2010. http://dx.doi.org/10.1109/nssmic.2010.5874540.
Full textBayerlein, Reimund, Ivor Fleck, Todd E. Peterson, and Hedia Bcker. "Gamma-Ray Imaging Using Cherenkov Cone Detection from Energetic Compton Electrons." In 2019 IEEE Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC). IEEE, 2019. http://dx.doi.org/10.1109/nss/mic42101.2019.9059810.
Full textFilipescu, D., H. Utsunomiya, I. Gheorghe, T. Glodariu, O. Tesileanu, T. Shima, K. Takahisa, and S. Miyamoto. "Geant4 simulations on Compton scattering of laser photons on relativistic electrons." In EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS: Carpathian Summer School of Physics 2014. AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4909594.
Full textCastoldi, Andrea, Antonio Galimberti, Chiara Guazzoni, Robert Hartmann, and Lothar Struder. "Compton electrons' tracking within a single silicon layer with controlled-drift detectors." In 2006 IEEE Nuclear Science Symposium Conference Record. IEEE, 2006. http://dx.doi.org/10.1109/nssmic.2006.353835.
Full textREBREYEND, D., J. P. Bocquet, D. Moricciani, V. Bellini, M. Beretta, L. Casano, A. DAngelo, et al. "SEARCH FOR LIGHT-SPEED ANISOTROPIES USING COMPTON SCATTERING OF HIGH-ENERGY ELECTRONS." In Proceedings of the Fifth Meeting. WORLD SCIENTIFIC, 2010. http://dx.doi.org/10.1142/9789814327688_0008.
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