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1081por Pawelec, Graham“…The problems associated with the ageing immune system and vaccination were discussed recently at an international workshop at the Jenner Institute for Vaccine Research, Compton, UK, 6–7 October, 2005. This is a commentary on that session. …”
Publicado 2005
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1082“…Theoretical X-ray spectra produced from two KAERI X-ray generators were estimated using a modified Kramers' theory with target attenuation and backscatter correction and their spectral distributions experimentally measured by a high-purity germanium semiconductor detector through proper corrections for measured pulse height distributions with photopeak efficiency, Compton fraction, and K-escape fraction. The average energies and conversion coefficients obtained from the computation and experimental methods, when compared with ANSI N13.11 and the recently published National Institute of Standards and Technology X-ray beams, appeared to be in good agreement--(+/-)3% between corresponding values--and thus, could be satisfactorily applied in the performance test of personal dosimeters.…”
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1083por Bode, Peter, Bueno, Maria Izabel Maretti Silveira, Bortoleto, Gisele G., Hoffmann, Gaby, van den Ingh, Ted S. G. A. M., Rothuizen, Jan“…However, hair and nail samples were also analyzed by X-ray tube excitation, taking advantage of the X-ray Compton, Rayleigh, and Raman scattering which reflects the organic components such as the type of melanin. …”
Publicado 2008
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1084“…These theoretical results allow the reconstruction of two-dimensional images from Compton scattered radiation collected on a one-dimensional collimated camera. …”
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1085“…It was also demonstrated that a spectral measurement of the FEL-based Compton scattering X-ray beam was effective for directly observing the switching of the harmonic order. …”
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1086“…The prompt $\gamma$-ray emission --the GRB-- is explained extremely well by inverse Compton scattering of light in the near environment of the SN by the electrons in the CBs' plasma. …”
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1087“…We show that their prompt gamma-ray emission can be explained by inverse Compton scattering (ICS) of the progenitor's glory light, and their extended soft emission component by ICS of high density light or synchrotron radiation (SR) in a high density interstellar medium within the cluster. …”
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1088“…We consider the diffuse gamma ray data from FERMI first year observations and compare them to the gamma ray fluxes predicted by Dark Matter annihilation or decay (both from prompt emission and from Inverse Compton Scattering), for different observation regions of the sky and a range of Dark Matter masses, annihilation/decay channels and Dark Matter galactic profiles. …”
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1089“…Besides the prompt gamma-ray flux, we also take into account the contribution from the electrons/positrons produced in dark matter annihilations to the gamma-ray signal via inverse Compton scattering off the interstellar photon background, which turns out to be crucial in the case of dark matter annihilations into mu+mu- and e+e- pairs. …”
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1090“…This explanation requires the existence of a new spin-2 field of a planetary Compton wave-length that is coupled to neutrinos and the rest of the matter asymmetrically, both in the magnitude and in the sign. …”
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1091por Laycock, Paul“…These include the inclusive electron-proton scattering cross section and the related structure functions $F_2$ and $F_L$, as well as exclusive processes such as deeply-virtual Compton scattering and quasi-elastic heavy vector meson production and diffractive virtual photon dissociation. …”
Publicado 2012
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1092por Vergados, J D“…The Feynman diagrams are introduced and applied, in a way undertandable by first year graduate students, for evaluating the decay widths of the gauge bosons and some cross sections for interesting processes such as Rutherford scattering, electron to proton scattering (elementary proton or described by a form factor, and inelastic scattering) and Compton scattering. After that the classic topics like the role of C, P, CP symmetries and the experimental methods needed to verify their conservation or violation are discussed in some detail. …”
Publicado 2017
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1093por Vaccarezza, C., Alesini, D., Bacci, A., Cianchi, A., Chiadroni, E., Croia, M., Diomede, M., Ferrario, M., Gallo, A., Giribono, A., Latina, A., Marocchino, A., Petrillo, V., Pompili, R., Romeo, S., Rossetti Conti, M., Rossi, A.R., Serafini, L., Spataro, B.“…A 500-TW Laser system is also foreseen for electron and ion production experiments and a Compton backscattering Interaction is planned together with extraction beamlines at intermediate electron beam energy for neutron beams and THz radiation production. …”
Publicado 2018
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1094por Kurcewicz, W, Grant, I S, Gulda, K, Aas, A J, Billowes, J, García-Borge, M J, Burke, D G, Butler, P A, Cocks, J F C, Fogelberg, B, Freeman, S J, Jones, G D, Hagebø, E, Hoff, P, Hønsi, J, Lindroth, A, Løvhøiden, G, Mach, H, Martínez, T, Naumann, R A, Nybø, K, Nyman, G H, Ravn, H L, Rubio, B, Simpson, J, Smith, A G, Smith, J F, Steffensen, K, Taín, J L, Tengblad, O, Thorsteinsen, T F“…The $\gamma$-rays following the $\beta^{-}$-decay of $^{227}$Rn have been investigated by means of $\gamma$-ray singles and $\gamma\gamma$-coincidence measurements using an array of 12 Compton-suppressed Ge detectors. The fast timing $\beta\gamma\gamma$(t) method has been used to measure six level lifetimes. …”
Publicado 1997
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1095por Totani, T“…Gamma-ray bursts (GRBs) and following afterglows are considered to be produced by dissipation of kinetic energy of a relativistic fireball and radiation process is widely believed as synchrotron radiation or inverse Compton scattering of electrons. We argue that the transfer of kinetic energy of ejecta into electrons may be inefficient process and hence the total energy released by a GRB event is much larger than that emitted in soft gamma-rays, by a factor of \sim (m_p/m_e). …”
Publicado 1998
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1096por Harding, A K“…Outer gap models predict more gradual high-energy turnovers at around 10 GeV, but also predict an inverse Compton component extending to TeV energies. Detection of pulsed TeV emission, which would not survive attenuation at the polar caps, is thus an important test of outer gap models. …”
Publicado 2000
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1097“…It is based on the model of lepton nucleon interactions via three single-photon-exchange processes: photon-gluon fusion (PGF), QCD Compton (QCDC) and leading process (LP). A method of simultaneous extraction of the Sivers asymmetries of the three processes with the use of Monte Carlo (MC) and neural networks (NN) approach is presented. …”
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1098por Bradamante, Franco“…Preliminary results from a test run on deeply virtual compton scattering of 160 GeV muons on a liquid hydrogen target are also given, as well as plans for a two-year long run in 2016 and 2017 with a suitably modified spectrometer.…”
Publicado 2016
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1099“…Imaging processes built on the Compton scattering effect have been under continuing investigation since it was first suggested in the 50s. …”
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1100por Fornaro, Juergen, Leschka, Sebastian, Hibbeln, Dennis, Butler, Anthony, Anderson, Nigel, Pache, Gregor, Scheffel, Hans, Wildermuth, Simon, Alkadhi, Hatem, Stolzmann, Paul“…Dual-energy CT uses two X-ray spectra enabling material differentiation by analysing material-dependent photo-electric and Compton effects. Elemental concentrations can thereby be determined using three-material decomposition algorithms. …”
Publicado 2011
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