Results 31 to 40 of about 271,848 (328)
Light Element Evolution and Cosmic Ray Energetics [PDF]
, 1999 Using cosmic-ray energetics as a discriminator, we investigate evolutionary
models of LiBeB. We employ a Monte Carlo code which incorporates the delayed
mixing into the ISM both of the synthesized Fe, due to its incorporation into
high velocity dust ...Benzion Kozlovsky, Bloemen H., Bykov A., Bykov A. M., Engelmann J. J., Epstein R. I., Ginzburg V. L., Higdon H. C., Kozasa T., Lijowski M., Lingenfelter R. E., Mihara K., Nissen P. E., Pagel B. E. J., Parizot E. M. G., Ramaty R., Ramaty R., Ramaty R., Reuven Ramaty, Richard E. Lingenfelter, Sean T. Scully, Shapiro M. M., Tsujimoto T., van den Bergh S., Yorke H. +24 morecore +2 more sourcesDark cosmic rays
Physics Letters B, 2017 If dark matter particles have an electric charge, as in models of millicharged dark matter, such particles should be accelerated in the same astrophysical accelerators that produce ordinary cosmic rays, and their spectra should have a predictable rigidity dependence. Depending on the charge, the resulting "dark cosmic rays" can be detected as muon-like Hu, Ping-Kai, Kusenko, Alexander, Takhistov, Volodymyr +2 moreopenaire +3 more sourcesCOSMIC RAY ANTIPROTONS [PDF]
Particles, Strings and Cosmology (PASCOS 99), 2000 Cosmic ray antiprotons have been detected for over 20 years and are now measured reliably. Standard particle and astrophysics predict a conventional spectrum and abundance of secondary antiprotons consistent with all current measurements. These measurements place limits on exotic Galactic antiproton sources and non-standard antiproton properties ...openaire +2 more sourcesRadiation Exposure in the Lower Atmosphere during Different Periods of Solar Activity
Atmosphere, 2022 In recent years, there has been a huge increase in air travel, both for business and leisure. For this reason, entities such as the European Commission and the International Committee on Radiological Protection have provided several recommendations for ...Anastasia Tezari, Pavlos Paschalis, Argyris Stassinakis, Helen Mavromichalaki, Pantelis Karaiskos, Maria Gerontidou, Dimitris Alexandridis, Anastasios Kanellakopoulos, Norma Crosby, Mark Dierckxsens +9 moredoaj +1 more sourceUnparticle effects on cosmic ray photon and $e^\pm$ [PDF]
, 2009 We study the effects of unparticle physics on the cosmic ray photon and
$e^\pm$, including on the pair production (PP) and elastic scattering (ES) of
cosmic ray photon off various background radiations, and on the inverse Compton
scattering of cosmic ray H.E.S.S. collaboration, HEAT collaboration, I.V. Moskalenko, O. Cakir, PPB-BETS collaboration, Rong Hu, Shao-Xia Chen +6 morecore +1 more sourceThe Density Spike in Cosmic-Ray-Modified Shocks: Formation, Evolution,
and Instability [PDF]
, 1996 We examine the formation and evolution of the density enhancement (density
spike) that appears downstream of strong, cosmic-ray-modified shocks. This
feature results from temporary overcompression of the flow by the combined
cosmic-ray shock precursor ...Axford W. I., Bandiera R., Bell A. R., Byung‐Il Jun, Dorfi E. A., Drury L., Drury L., Frank A., Jones F. C., Krymsky G. F., T. W. Jones, Webb G. M., Webb G. M. +12 morecore +3 more sourcesDetection of the temporal variation of the sun's cosmic ray shadow with the IceCube detector [PDF]
, 2018 We report on the observation of a deficit in the cosmic ray flux from the directions of the Moon and Sun with five years of data taken by the IceCube Neutrino Observatory.Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, Jan, Axani, S., Backes, P., Bagherpour, H., Bai, X., Barbano, A., Barron, J. P., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Becker Tjus, J., Becker, K.-H., BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Bos, F., Botner, O., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bretz, H.-P., Bron, S., Brostean-Kaiser, J., Burgman, A., Busse, R. S., Börner, M., Böser, S., Carver, T., Chen, C., Cheung, E., Chirkin, D., Clark, K., Classen, L., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., Day, M., de André, J. P. A. M., De Clercq, C., De Ridder, S., de Vries, K. D., de Wasseige, G., de With, M., DeLaunay, J. J., Dembinski, H., Deoskar, K., Desiati, P., DeYoung, T., Dujmovic, H., Dunkman, M., Dvorak, E., Díaz-Vélez, J. C., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eller, P., Evenson, P. A., Fahey, S., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, Erik, Garrappa, S., Gerhardt, L., Ghorbani, K., Giang, W., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Griffith, Z., Haack, Christian, Hallgren, A., Halve, Lasse Yannik, Halzen, F., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Hultqvist, K., Hussain, R., Hünnefeld, M., IceCube Collaboration, In, S., Iovine, N., Ishihara, A., Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Kalaczynski, P., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Kolanoski, H., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Kroll, M., Krückl, G., Kunwar, S., Kurahashi, N., Kyriacou, A., Köpke, L., Labare, M., Lanfranchi, J. L., Larson, M. J., Lauber, F., Leonard, K., Leuermann, Martin, Liu, Q. R., Lohfink, E., Lozano Mariscal, C. J., Lu, L., Luszczak, W., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Makino, Y., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., Maunu, R., Meagher, K., Medici, M., Meier, M., Menne, T., Merino, G., Meures, T., Miarecki, S., Micallef, J., Momenté, G., Montaruli, T., Moore, R. W., Moulai, M., Nagai, R., Nahnhauer, R., Nakarmi, P., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., O'Murchadha, A., O'Sullivan, E., Obertacke Pollmann, A., Olivas, A., Palczewski, T., Pandya, H., Pankova, D. V., Peiffer, P., Pepper, J. A., Pieloth, D., Pinat, E., Pizzuto, A., Plum, M., Price, P. B., Przybylski, G. T., Pérez de los Heros, C., Raab, C., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Reimann, René, Relethford, B., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, Martin, Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Sanchez Herrera, S. E., Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Sarkar, S., Satalecka, K., Schaufel, Merlin, Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schumacher, Lisa Johanna, Schöneberg, S., Sclafani, S., Seckel, D., Seunarine, S., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stasik, A., Stein, R., Stettner, Jöran Benjamin, Steuer, A., Stezelberger, T., Stokstad, R. G., Strotjohann, N. L., Stuttard, T., Stößl, A., Sullivan, G. W., Sutherland, M., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, Roxanne, Turley, C. F., Ty, B., Tönnis, C., Unger, E., Unland Elorrieta, M. A., Usner, M., Van Driessche, Ward, van Eijk, D., van Eijndhoven, N., van Santen, J., Vandenbroucke, J., Vanheule, S., Vraeghe, M., Walck, C., Wallace, A., Wallraff, Marius, Wandkowsky, N., Wandler, F. D., Watson, T. B., Weaver, C., Weiss, M. J., Wendt, C., Werthebach, J., Westerhoff, S., Whelan, B. J., Whitehorn, N., Wiebe, K., Wiebusch, Christopher, Wille, L., Williams, D. R., Wills, L., Wolf, M., Wood, J., Wood, T. R., Woolsey, E., Woschnagg, K., Wrede, G., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T. +329 morecore +5 more sources
