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1041“…Abstract: We analyse the high-energy behavior of tree-level graviton Compton amplitudes for particles of mass m and arbitrary spin, concentrating on a combination of forward amplitudes that will be unaffected by eventual cross- couplings to other, higher spins. …”
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1042por Totani, T“…Three radiation processes can be considered for very high energy gamma-ray production: inverse- Compton, photo-pion production, and proton synchrotron, all of which could be an efficient energy loss process of GRBs. …”
Publicado 2001
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1043por YAZAKI, Yuji“…In 1928, Klein and Nishina investigated Compton scattering based on the Dirac equation just proposed in the same year, and derived the Klein–Nishina formula for the scattering cross section of a photon. …”
Publicado 2017
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1044por Auffray, Etiennette, Ben Mimoun Bel Hadj, Faraah, Cortinovis, Daniele, Doroud, Katayoun, Garutti, Erika, Lecoq, Paul, Liu, Zheng, Martinez, Rosana, Paganoni, Marco, Pizzichemi, Marco, Silenzi, Alessandro, Xu, Chen, Zvolský, Milan“…Finally, the average energy resolution at 511 keV is about 13 %, enough for effective Compton rejection.…”
Publicado 2015
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1045por Jones, L“…The material Cadmium Zinc Telluride (CZT) is now available which operates at room temperature and can be used to measure the energy of gamma radiation. In a compton camera configuration the direction of the radiation can also be determined. …”
Publicado 2008
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1046por Guskov, Alexey“…The electromagnetic structure of pions is probed in $\pi^{−} + (A,Z)\rightarrow\pi^{−} + (A,Z) +\gamma$ Compton scattering in inverse kinematics (Primakoff reaction) and described by the electric $(\bar{\alpha_{\pi}})$ and the magnetic $(\bar{\beta_{\pi}})$ polarizabilities that depend on the rigidity of pion’s internal structure as a composite particle. …”
Publicado 2008
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1047por Ghosh, Oindrila“…--HTML-->TeV blazars dominate the extragalactic gamma-ray sky and highly energetic pair beams arising from such blazar jets underproduce gamma rays in the GeV band while inverse-Compton scattering off the cosmic microwave background. …”
Publicado 2023
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1048por Wijers, R A M J“…Recently,the discoveries made with BATSE and other instruments on board NASA's Compton GAMMAY-Ray Observatory,have accelerated research in the field. …”
Publicado 1995
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1049por Billy, J C, Bonon, J P, Henrist, Bernard, Hilleret, Noël, Jiménez, J M, Laugier, I, Strubin, Pierre M“…At this high photon energy, the energy dissipation of the photons in aluminium is done predominantly via the Compton process. This absorption mechanism leads to a larger enhancement of the gas desorption with the photon energy compared to the photoelectric effect. …”
Publicado 2001
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1050“…We calculate various moments of the distributions, including the form factors that appear in the handbag approximation to wide-angle Compton scattering. This allows us to estimate the minimal momentum transfer required for reliable predictions in that approach to be around |t|~3 GeV^2. …”
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1051por Bielert, E, Bremer, J, Doshita, N, Geyer, R, Hashimoto, R, Horikawa, N, Ishimoto, S, Iwata, T, Kondo, K, Mallot, G K, Matsuda, H, Matsuda, T, Miyachi, Y, Nukazuka, G, Pirotte, O, Suzuki, H, Suzuki, S, Vullierme, B“…A 2.5 m long liquid hydrogen target has been developed for the COMPASS experiment at CERN to investigate the nucleon spin structure via the Deeply Virtual Compton Scattering (DVCS) process. To recognize exclusive DVCS events, produced photons and slow protons need to be detected. …”
Publicado 2014
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1052por Apostolakis, J, Asai, M, Bagulya, A, Brown, J M C, Burkhardt, H, Chikuma, N, Cortes-Giraldo, M A, Elles, S, Grichine, V, Guatelli, S, Incerti, S, Ivanchenko, V N, Jacquemier, J, Kadri, O, Maire, M, Pandola, L, Sawkey, D, Toshito, T, Urban, L, Yamashita, T“…Improvements have been made in models of the photoelectric effect, Compton scattering, gamma conversion to electron and muon pairs, fluctuations of energy loss, multiple scattering, synchrotron radiation, and high energy positron annihilation. …”
Publicado 2015
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1053“…These fits suggest that at least a third of the observed electron cosmic rays from DM annihilation could come from subhalos, opening up the possibility of a relaxation of recent stringent constraints from inverse Compton gamma rays originating from the high-energy leptons.…”
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1054por Briceño, Raúl A., Davoudi, Zohreh, Hansen, Maxwell T., Schindler, Matthias R., Baroni, Alessandro“…Applications include Compton scattering of the pion $(πγ^*→[ππ,K\overline{K}]→πγ^*)$, kaon $(Kγ^*→[πK,ηK]→Kγ^*)$, and nucleon $(Nγ^*→Nπ→Nγ^*)$, as well as double-$β$ decays, and radiative corrections to the single-$β$ decay, of QCD-stable hadrons. …”
Publicado 2019
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1055“…We assess the potential of future electron-positron linear colliders operating in the $e^\pm\gamma$ mode in detecting charged Higgs bosons with mass around and larger than the top quark mass, using Compton back-scattered photons from laser light. We compare the pair production mode, $e^-\gamma\to e^- H^+H^-$, to a variety of channels involving only one charged Higgs scalar in the final state, such as the tree-level processes $e^-\gamma\to \nu_e H^- \Phi^0 $ ($\Phi^0=h^0,H^0$ and $A^0$) and $e^-\gamma\to \nu_e f\bar f H^-$ ($f=b,\tau$ and $\nu_\tau$) as well as the loop-induced channel $e^-\gamma\to \nu_e H^-$. …”
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1056por Jentschel, M, Blanc, A, de France, G, Köster, U, Leoni, S, Mutti, P, Simpson, G, Soldner, T, Ur, C, Urban, W, Ahmed, S, Astier, A, Augey, L, Back, T, Ba̧czyk, P, Bajoga, A, Balabanski, D, Belgya, T, Benzoni, G, Bernards, C, Biswas, D C, Bocchi, G, Bottoni, S, Britton, R, Bruyneel, B, Burnett, J, Cakirli, R B, Carroll, R, Catford, W, Cederwall, B, Celikovic, I, Cieplicka-Oryńczak, N, Clement, E, Cooper, N, Crespi, F, Csatlos, M, Curien, D, Czerwiński, M, Danu, L S, Davies, A, Didierjean, F, Drouet, F, Duchêne, G, Ducoin, C, Eberhardt, K, Erturk, S, Fraile, L M, Gottardo, A, Grente, L, Grocutt, L, Guerrero, C, Guinet, D, Hartig, A L, Henrich, C, Ignatov, A, Ilieva, S, Ivanova, D, John, B V, John, R, Jolie, J, Kisyov, S, Krticka, M, Konstantinopoulos, T, Korgul, A, Krasznahorkay, A, Kröll, T, Kurpeta, J, Kuti, I, Lalkovski, S, Larijani, C, Leguillon, R, Lica, R, Litaize, O, Lozeva, R, Magron, C, Mancuso, C, Martinez, E Ruiz, Massarczyk, R, Mazzocchi, C, Melon, B, Mengoni, D, Michelagnoli, C, Million, B, Mokry, C, Mukhopadhyay, S, Mulholland, K, Nannini, A, Napoli, D R, Olaizola, B, Orlandi, R, Patel, Z, Paziy, V, Petrache, C, Pfeiffer, M, Pietralla, N, Podolyak, Z, Ramdhane, M, Redon, N, Regan, P, Regis, J M, Regnier, D, Oliver, R J, Rudigier, M, Runke, J, Rza̧ca-Urban, T, Saed-Samii, N, Salsac, M D, Scheck, M, Schwengner, R, Sengele, L, Singh, P, Smith, J, Stezowski, O, Szpak, B, Thomas, T, Thürauf, M, Timar, J, Tom, A, Tomandl, I, Tornyi, T, Townsley, C, Tuerler, A, Valenta, S, Vancraeyenest, A, Vandone, V, Vanhoy, J, Vedia, V, Warr, N, Werner, V, Wilmsen, D, Wilson, E, Zerrouki, T, Zielinska, M“…The target was surrounded by an array of eight to ten anti-Compton shielded EXOGAM Clover detectors, four to six anti-Compton shielded large coaxial GASP detectors and two standard Clover detectors. …”
Publicado 2017
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1057por Schill, C.“…GPDs can be probed experimentally in hard exclusive meson production or deeply virtual Compton scattering (DVCS). The COMPASS experiment at CERN is a unique place to study these reactions. …”
Publicado 2008
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1058“…The following chapters then apply these insights to various atomic processes, such as photoionization as a many-body problem, dominant mechanisms for the production of ions at higher energies, Compton scattering and ionization accompanied by creation of e-e+ pairs, and the photoionization of endohedral atoms (e.g. fullerene). …”
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1059por CERN. Geneva. Track Chambers Division (TC)“…Those are due primarily to electrons captured by the magnetic field across the chamber, and produdsd by Compton effect to electron pairs produced by gamma rays associated with the beam.…”
Publicado 2022
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1060“…In the second section, we investigate photon production via Laser Compton scattering (LCS).…”
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