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Journal articles on the topic 'Electrons de recul Compton'

Author: Grafiati

Published: 4 June 2021

Last updated: 12 February 2022

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1

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.

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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 Compton profiles with different maximum and width are superimposed in a measurement.The MethodWe may write the total measured intensity M at a particular energy loss E as a linear combination of coupled Bragg-Compton events. In the case of a systematic row reflection with i excited beams it is always possible to choose n = 2 * (i - 1) angles such that the system of linear equations can be solved with respect to I.

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2

Poutanen, 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.

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3

Zacharias, 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.

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4

Ahuja, 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.

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The Compton profile, projection of electron momentum density distribution along the scattering vector, is very sensitive to the behavior of valence electrons in a variety of materials. In this paper theoretical aspects related to measurement of spin momentum densities of magnetic materials using Compton scattering is reviewed. To highlight the potential of the magnetic Compton scattering, the spin momentum densities in Ni-Mn-Ga Heusler alloys at various temperatures and magnetic fields are presented. The magnetic Compton profiles are mainly analyzed in terms of the contribution from the 3d electrons of Mn. A comparison of the magnetic Compton data with other magnetization studies illustrates its importance in exploring the magnetic effects in ferro- or ferri-magnetic materials.

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5

Kaliman, 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.

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6

Kotkin, 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.

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7

Swanekamp, 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.

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8

Basavaraju, 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.

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9

Zdziarski, 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.

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10

Surić, 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.

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11

White, Timothy R., Alan P. Lightman, and Andrzej A. Zdiziarski. "Compton reflection of gamma rays by cold electrons." Astrophysical Journal 331 (August 1988): 939. http://dx.doi.org/10.1086/166611.

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12

Nagirner, D. I., and V. M. Loskutov. "Compton attenuation coefficient in scattering by maxwellian electrons." Astrophysics 43, no. 3 (July 2000): 343–50. http://dx.doi.org/10.1007/bf02683970.

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13

Krafft, Geoffrey A., and Gerd Priebe. "Compton Sources of Electromagnetic Radiation." Reviews of Accelerator Science and Technology 03, no. 01 (January 2010): 147–63. http://dx.doi.org/10.1142/s1793626810000440.

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When a relativistic electron beam interacts with a high-field laser beam, intense and highly collimated electromagnetic radiation will be generated through Compton scattering. Through relativistic upshifting and the relativistic Doppler effect, highly energetic polarized photons are radiated along the electron beam motion when the electrons interact with the laser light. For example, X-ray radiation can be obtained when optical lasers are scattered from electrons of tens-of-MeV beam energy. Because of the desirable properties of the radiation produced, many groups around the world have been designing, building, and utilizing Compton sources for a wide variety of purposes. In this review article, we discuss the generation and properties of the scattered radiation, the types of Compton source devices that have been constructed to date, and the prospects of radiation sources of this general type. Due to the possibilities of producing hard electromagnetic radiation in a device that is small compared to the alternative storage ring sources, it is foreseen that large numbers of such sources may be constructed in the future.

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14

Schlickeiser, R. "Non-linear synchrotron self-Compton cooling of relativistic electrons." Monthly Notices of the Royal Astronomical Society 398, no. 3 (September 21, 2009): 1483–94. http://dx.doi.org/10.1111/j.1365-2966.2009.15205.x.

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15

Bell, F., J. Felsteiner, and L. P. Pitaevskii. "Cross section for Compton scattering by polarized bound electrons." Physical Review A 53, no. 3 (March 1, 1996): R1213—R1215. http://dx.doi.org/10.1103/physreva.53.r1213.

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16

Booth, Thomas E., and John S. Hendricks. "Monte Carlo Sampling of Compton Scatter Off Moving Electrons." Nuclear Science and Engineering 90, no. 3 (July 1985): 248–55. http://dx.doi.org/10.13182/nse85-a17766.

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17

Tvaskis, V., D. Dutta, D. Gaskell, and A. Narayan. "Precise polarization measurements via detection of compton scattered electrons." Physics of Particles and Nuclei 45, no. 1 (January 2014): 285–87. http://dx.doi.org/10.1134/s1063779614011103.

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18

Mosharafa, A. A. "Theoretical compton scattering profile for conduction electrons in lithium." Crystal Research and Technology 24, no. 5 (May 1989): 551–55. http://dx.doi.org/10.1002/crat.2170240512.

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19

Bol'shedvorsky, E., S. Polityko, and A. Misaki. "Spin of Scattered Electrons in the Nonlinear Compton Effect." Progress of Theoretical Physics 104, no. 4 (October 1, 2000): 769–75. http://dx.doi.org/10.1143/ptp.104.769.

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20

Conka-Nurdan, T., K. Nurdan, K. Laihem, A. H. Walenta, C. Fiorini, B. Freisleben, N. Hornel, N. A. Pavel, and L. Struder. "Preliminary results on Compton electrons in silicon drift detector." IEEE Transactions on Nuclear Science 51, no. 5 (October 2004): 2526–32. http://dx.doi.org/10.1109/tns.2004.834817.

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21

Ivanenko, I. P., and V. V. Sizov. "Multiple compton scattering of electrons in a photon field." Astrophysics and Space Science 192, no. 2 (1992): 219–45. http://dx.doi.org/10.1007/bf00684481.

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22

Midhun, C. V., M. M. Musthafa, Shaima Akbar, Swapna Lilly Cyriac, S. Sajeev, Antony Joseph, K. C. Jagadeesan, S. V. Suryanarayana, and S. Ganesan. "Spectroscopy of High-Intensity Bremsstrahlung Using Compton Recoiled Electrons." Nuclear Science and Engineering 194, no. 3 (November 18, 2019): 207–12. http://dx.doi.org/10.1080/00295639.2019.1681210.

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23

Lovesey, Stephen W. "Theories of Compton Scattering by Magnetic Materials." Zeitschrift für Naturforschung A 48, no. 1-2 (February 1, 1993): 261–65. http://dx.doi.org/10.1515/zna-1993-1-249.

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Abstract Theoretical work on the cross-section for Compton scattering by magnetic materials is surveyed. Exact results for scattering by a free polarized electron are contrasted with corresponding results obtained perturbatively for a model of bound electrons with a finite width to the momentum distribution.

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24

Srinivasa, Rao. "Study of Compton broadening due to electron-photon scattering." Serbian Astronomical Journal, no. 180 (2010): 11–18. http://dx.doi.org/10.2298/saj1080011s.

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We have investigated the effects of Compton broadening due to electron-photon scattering in hot stellar atmospheres. A purely electron-photon scattering media is assumed to have plane parallel geometry with an input radia?tion field localized on one side of the slab. The method is based on the discrete space theory of radiative transfer for the intensity of emitted radiation. The solution is developed to study the importance of scattering of radiation by free electrons in high temperature stellar atmospheres which produces a brodening and shift in spectral lines because of the Compton effect and the Doppler effect arising from mass and thermal motions of scattering electrons. It is noticed that the Comptonized spectrum depends on three parameters: the optical depth of the medium, the temperature of the thermal electrons and the viewing angle. We also showed that the Compton effect produces red shift and asymmetry in the line. These two effects increase as the optical depth increases. It is also noticed that the emergent specific intensities become completely asymmetric for higher optical depths.

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25

Baring, Matthew G. "Quiescent Magnetar Emission: Resonant Compton Upscattering." Symposium - International Astronomical Union 218 (2004): 267–70. http://dx.doi.org/10.1017/s0074180900181136.

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A principal candidate for quiescent non-thermal gamma-ray emission from magnetars is resonant inverse Compton scattering in the strong fields of their magnetospheres. This paper outlines expectations for such emission, formed from non-thermal electrons accelerated in a pulsar-like polar cap potential upscattering thermal X-rays from the hot stellar surface. The resultant spectra are found to be strikingly flat, with fluxes and strong pulsation that could be detectable by GLAST.

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26

JUNG, YOUNG-DAE. "Inelastic Compton scattering of photons by bound atomic electrons in weakly coupled plasmas." Journal of Plasma Physics 64, no. 1 (July 2000): 89–95. http://dx.doi.org/10.1017/s0022377800008473.

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Plasma screening effects on inelastic Compton scattering of photons by bound atomic electrons of hydrogenic target ions in weakly coupled plasmas are investigated. The particle interaction potential in weakly coupled plasmas is obtained using the Debye–Hückel model. The screened wave functions and energy eigenvalues for the ground and excited states of the target ion are obtained using the Ritz variational method. The expression for the lowest-order transition matrix element is obtained from a two-photon process associated with terms quadratic in the vector potential A. The inelastic Compton scattering cross-section from the 1s ground state to the 2p excited state is obtained as a function of the incident photon energy, including plasma screening effects. It is found that plasma screening effects significantly reduce the inelastic Compton scattering cross-section.

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27

Ehlotzky, F. "Laser-induced Compton scattering from a bound electron." Canadian Journal of Physics 70, no. 1 (January 1, 1992): 72–77. http://dx.doi.org/10.1139/p92-007.

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We investigate nonrelativistically Compton scattering by an electron bound in hydrogen in a powerful laser field. The corresponding nonlinear rates and cross sections are evaluated in a Keldysh-type of approximation and compared with the rates and cross sections of multiphoton ionization and harmonic generation. We find that multiphoton ionization overshadows Compton scattering by many orders of magnitude, however, Compton scattering may well compete with harmonic generation above the ionization threshold, since, in particular, both processes have the same angular distribution and only odd harmonics can be created by bound electrons, while in bound-free Compton scattering all harmonics will be generated.

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28

SAKAI, Nobuhiko. "Observation of magnetic compton scattering. Momentum distribution of magnetic electrons." Nihon Kessho Gakkaishi 33, no. 1 (1991): 13–20. http://dx.doi.org/10.5940/jcrsj.33.13.

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29

Stepanek, J. "Parametric study of laser Compton-backscattering from free relativistic electrons." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 412, no. 1 (June 1998): 174–82. http://dx.doi.org/10.1016/s0168-9002(98)00099-0.

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30

Chang, Zhe, Yunguo Jiang, and Hai-Nan Lin. "GAMMA-RAY POLARIZATION INDUCED BY COLD ELECTRONS VIA COMPTON PROCESSES." Astrophysical Journal 769, no. 1 (May 6, 2013): 70. http://dx.doi.org/10.1088/0004-637x/769/1/70.

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31

Chatzidimitriou-Dreismann, C. Aris. "Attosecond Neutron Compton Scattering from Protons Entangled with Adjacent Electrons." Acta Physica Hungarica A) Heavy Ion Physics 26, no. 1-2 (November 1, 2006): 203–12. http://dx.doi.org/10.1556/aph.26.2006.1-2.24.

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32

Swiderski, 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 LaBr$_{3}$:Ce Scintillator." IEEE Transactions on Nuclear Science 57, no. 3 (June 2010): 1697–701. http://dx.doi.org/10.1109/tns.2010.2045899.

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33

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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34

Singh, B. "Study of Compton scattering of gamma rays from atomic electrons." Indian Journal of Physics 85, no. 12 (December 2011): 1687–94. http://dx.doi.org/10.1007/s12648-011-0200-x.

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35

Kirk, J. G., Lewis Ball, and O. Skjæraasen. "Predictions of inverse Compton radiation from PSR B1259–63." International Astronomical Union Colloquium 177 (2000): 531–32. http://dx.doi.org/10.1017/s0252921100060528.

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Unpulsed high energy (TeV) emission has been detected from several isolated pulsars (Aharonian 1999) and presumably results from relativistic electrons accelerated at the termination shock of an MHD wind driven by the pulsar itself. These electrons inverse Compton scatter target photons from either the cosmic microwave background, or from their own synchrotron radiation.The rotation-powered binary pulsar PSR B1259–63 (Johnston et al. 1996) is also thought to drive an MHD wind, and the synchrotron radiation of electrons accelerated at its termination shock is probably the source of the unpulsed X-rays seen from this object by ROSAT, OSSE and ASCA (Tavani & Arons 1997). Compared to the isolated pulsars, however, the the pulsar’s Be-star companion provides an energy density of target photons available for inverse Compton scattering which is some 11 orders of magnitude larger. Using delta-function approximations to the emissivities and a monochromatic approximation to the spectrum of the target photons, we modelled the observed X-ray synchrotron emission and predicted the TeV emission in a recent paper (Kirk et al. 1999). In this contribution we improve these calculations in two respects – by treating the target spectrum more precisely, as described in the companion paper (Ball & Kirk 1999), and by relaxing the approximations made in the emissivities.

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36

SCHOPPER, RÜDIGER, HARTMUT RUHL, THOMAS A. KUNZL, and HARALD LESCH. "Kinetic simulation of the coherent radio emission from pulsars." Laser and Particle Beams 21, no. 1 (January 2003): 109–13. http://dx.doi.org/10.1017/s0263034603211204.

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On hand of 3D PIC simulations we show that in a strongly magnetized plasma a relativistic electron beam can be forced to emit highly coherent radio emission by self-induced nonlinear density fluctuations. Such slowly moving nonlinear structures oscillate with the local plasma frequency at which the relativistic electrons are scattered. Beam electrons dissipate a significant amount of their kinetic energy by inverse Compton radiation at a frequency of about γ2ωpe. Since the beam is sliced into pancake structures which experience the same electric field the inverse Compton scattering is coherent. Such a process is a very promising candidate for the coherent radio emission of pulsars.

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37

Supper, Rodrigo. "ICS as a Limiting Factor for Electron Energies in Pulsar Magnetospheres." International Astronomical Union Colloquium 177 (2000): 469–72. http://dx.doi.org/10.1017/s0252921100060334.

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AbstractBased on the polar cap model, we investigated in the energy loss of accelerated electrons in a neutron star magnetosphere by inverse Compton scattering of thermal photospheric radiation. An analytical treatment is presented, which turns out ranges in the magnetic field strength and thermal temperature where ultrarelativistic electrons can not survive.

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38

Mohanmurthy, Prajwal, Amrendra Narayan, and Dipangkar Dutta. "A test of local Lorentz invariance with Compton scattering asymmetry." Modern Physics Letters A 31, no. 38 (November 25, 2016): 1650220. http://dx.doi.org/10.1142/s0217732316502205.

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We report on a measurement of the constancy and anisotropy of the speed of light relative to the electrons in photon–electron scattering. We used the Compton scattering asymmetry measured by the new Compton polarimeter in Hall C at Jefferson Lab (JLab) to test for deviations from unity of the vacuum refractive index (n). For photon energies in the range of 9–46 MeV, we obtain a new limit of 1 − n < 1.4 × 10[Formula: see text]. In addition, the absence of sidereal variation over the six-month period of the measurement constrains any anisotropies in the speed of light. These constitute the first study of Lorentz invariance (LI) using Compton asymmetry. Within the minimal Standard Model extension (MSME) framework, our result yield limits on the photon and electron coefficients [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text]. Although these limits are several orders of magnitude larger than the current best limits, they demonstrate the feasibility of using Compton asymmetry for tests of LI. Future parity-violating electron-scattering experiments at JLab will use higher energy electrons enabling better constraints.

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39

Oomi, G., F. Honda, T. Kagayama, F. Itoh, H. Sakurai, H. Kawata, and O. Shimomura. "High-pressure system for Compton scattering experiments." Journal of Synchrotron Radiation 5, no. 3 (May 1, 1998): 932–34. http://dx.doi.org/10.1107/s0909049598000429.

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High-pressure apparatus for Compton scattering experiments has been developed to study the momentum distribution of conduction electrons in metals and alloys at high pressure. This apparatus was applied to observe the Compton profile of metallic Li under pressure. It was found that the Compton profile at high pressure could be obtained within several hours by using this apparatus and synchrotron radiation. The result on the pressure dependence of the Fermi momentum of Li obtained here is in good agreement with that predicted from the free-electron model.

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40

Ahuja, B. L., M. Sharma, and S. Mathur. "Electronic Structure of Liquid Mercury Using Compton Scattering Technique." Zeitschrift für Naturforschung A 59, no. 9 (September 1, 2004): 543–49. http://dx.doi.org/10.1515/zna-2004-0903.

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The isotropic Compton profile of mercury has been measured, using 661.65 keV gamma-rays from a 20 Ci 137Cs source. To extract the true experimental Compton line shape, besides the usual systematic corrections we have incorporated for the first time the background correction due to bremsstrahlung radiation generated by photo and Compton electrons. Theoretical computations have been carried out, using the renormalised-free-atom (RFA) for the electron configuration 4f145d106s2 and free electron models. It is found that the present experimental data with bremsstrahlung background correction are in better agreement with the RFA calculations. This work suggests the incorporation of the bremsstrahlung background correction in Compton scattering experiments of heavy materials using high-energy gamma-ray sources.

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41

Khera, Shabha, Narayan Lal Heda, Sonal Mathur, and Babu Lal Ahuja. "Electronic Structure of Gadolinium and Dysprosium Using Compton Scattering Technique." Zeitschrift für Naturforschung A 61, no. 5-6 (June 1, 2006): 299–305. http://dx.doi.org/10.1515/zna-2006-5-615.

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In this paper we present the first ever measured Compton profiles of polycrystalline gadolinium and dysprosium using 661.65 keV gamma-rays. The Compton data are compared with renormalized-freeatom (RFA) and free-electron model profiles. In both cases the RFA model (with e− - e− correlation) gives a better agreement with the experiment. The hybridization effects of s-, p-, d-, and f-electrons are discussed, using the first derivatives of the Compton profiles. We also report the cohesive energy of both samples, computed from the RFA calculations. - PACS numbers: 13.60.F, 71.15.Nc, 78.70. -g, 78.70.Ck

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42

Krajewska, K., and J. Z. Kamiński. "Spin effects in nonlinear Compton scattering in ultrashort linearly-polarized laser pulses." Laser and Particle Beams 31, no. 3 (July 11, 2013): 503–13. http://dx.doi.org/10.1017/s0263034613000165.

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AbstractThe nonlinear Compton scattering by a linearly polarized laser pulse of finite duration is analyzed, with a focus on the spin effects of target electrons. We show that, although the Compton scattering accompanied by the electron no-spin flip is dominant, for some energy regions of Compton photons their emission is dominated by the process leading to the electron spin flip. This feature is observed for different pulse durations, and can be treated as a signature of quantum behavior. Similar conclusions are reached when analyzing the scattered electron energy spectra. This time, the sensitivity of spin effects to the carrier-envelope phase of the driving pulse is demonstrated. The possibility of electron acceleration by means of Compton scattering is also discussed.

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43

Qiao, Chen-Kai, Jian-Wei Wei, and Lin Chen. "An Overview of the Compton Scattering Calculation." Crystals 11, no. 5 (May 10, 2021): 525. http://dx.doi.org/10.3390/cryst11050525.

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The Compton scattering process plays significant roles in atomic and molecular physics, condensed matter physics, nuclear physics and material science. It could provide useful information on the electromagnetic interaction between light and matter. Several aspects of many-body physics, such us electronic structures, electron momentum distributions, many-body interactions of bound electrons, etc., can be revealed by Compton scattering experiments. In this work, we give a review of ab initio calculation of Compton scattering process. Several approaches, including the free electron approximation (FEA), impulse approximation (IA), incoherent scattering function/incoherent scattering factor (ISF) and scattering matrix (SM) are focused on in this work. The main features and available ranges for these approaches are discussed. Furthermore, we also briefly introduce the databases and applications for Compton scattering.

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44

Wadiasingh, Zorawar, Matthew G. Baring, Peter L. Gonthier, and Alice K. Harding. "Hard Spectral Tails in Magnetars." Proceedings of the International Astronomical Union 13, S337 (September 2017): 108–11. http://dx.doi.org/10.1017/s1743921317009073.

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AbstractPulsed non-thermal quiescent emission between 10 keV and around 150 keV has been observed in ~10 magnetars. For inner magnetospheric models of such hard X-ray signals, resonant Compton upscattering of soft thermal photons from the neutron star surface is the most efficient radiative process. We present angle-dependent hard X-ray upscattering model spectra for uncooled monoenergetic relativistic electrons. The spectral cut-off energies are critically dependent on the observer viewing angles and electron Lorentz factor. We find that electrons with energies less than around 15 MeV will emit most of their radiation below 250 keV, consistent with the observed turnovers in magnetar hard X-ray tails. Moreover, electrons of higher energy still emit most of the radiation below around 1 MeV, except for quasi-equatorial emission locales for select pulses phases. Our spectral computations use new state-of-the-art, spin-dependent formalism for the QED Compton scattering cross section in strong magnetic fields.

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45

Van Oss, R. F., G. H. J. Van Den Oord, and M. Kuperus. "Accretion Disk Flares in Energetic Radiation Fields." Symposium - International Astronomical Union 157 (1993): 217–18. http://dx.doi.org/10.1017/s0074180900174157.

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We consider the physics of magnetic flares in the energetic radiation field of an accretion disk corona (ADC). The X-ray emission from these flares is thought to be responsable for the observed hard powerlaw component in the X-ray spectra of galactic black hole candidates in their ‘high’ spectral state. During the flare event (inverse Compton) scattering of soft photons from the underlying disk into hard photons occurs on accelerated electrons in current sheets. The electrons are decelerated by the radiation drag force that results from the up-scattering. This friction-like effect of the intense background radiation field on the motion of the electrons in the sheet can be considered as a form of resistivity in the magnetohydrodynamical picture of the current sheet: Compton resistivity. A spectrum is derived for the up-scattered radiation from current sheets in the ADC and it is found that this spectrum mimics a powerlaw above a critical photon energy.

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46

Thanomngam, P., and P. N. Johnston. "Compton scattering from the K-shell electrons of Ta and Pb." Radiation Physics and Chemistry 71, no. 3-4 (October 2004): 681–82. http://dx.doi.org/10.1016/j.radphyschem.2004.04.056.

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47

Pašić, S., and K. Ilakovac. "Measurement of Compton scattering on bound electrons by the coincidence method." Radiation Physics and Chemistry 75, no. 11 (November 2006): 1683–87. http://dx.doi.org/10.1016/j.radphyschem.2005.07.026.

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48

Beloborodov, Andrei M., and Andrei F. Illarionov. "Compton Heating and Superthermal Electrons in Gamma-loud Active Galactic Nuclei." Astrophysical Journal 450 (September 1995): 64. http://dx.doi.org/10.1086/176119.

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Zhang, Bo, and Zi-Gao Dai. "Synchro-curvature self-Compton radiation of electrons in curved magnetic fields." Monthly Notices of the Royal Astronomical Society 414, no. 4 (June 9, 2011): 2785–92. http://dx.doi.org/10.1111/j.1365-2966.2010.18187.x.

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Friberg, Stephen R., and Raymond J. Hawkins. "Compton scattering of electrons from optical pulses for quantum nondemolition measurements." Journal of the Optical Society of America B 12, no. 1 (January 1, 1995): 166. http://dx.doi.org/10.1364/josab.12.000166.

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