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1by Glushkov, A. V.“... longitude of about 137 degres. On a global scale, the lowest temperature of the cosmic microwave background...”
Published 2012
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2“... longitude of about 137 degres. On a global scale, the lowest temperature of the cosmic microwave background...”
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3“... due to interactions of cosmic rays with the cosmic microwave background, the Greisen-Zatsepin-Kuzmin...”
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4“... due to interactions of cosmic rays with the cosmic microwave background, the Greisen-Zatsepin-Kuzmin...”
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5“... 10^{19} eV due to interactions of cosmic rays with the cosmic microwave background, the Greisen...”
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6“... due to interactions of cosmic rays with the cosmic microwave background, the Greisen–Zatsepin–Kuzmin...”
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7“... 10^{19} eV due to interactions of cosmic rays with the cosmic microwave background, the Greisen...”
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8“...-positron pair production on the cosmic microwave background (CMB) radiation. For a power-law generation...”
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9“... acquire when they propagate through the cosmic microwave background (CMB) radiation in presence of TMFs...”
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10by Aloisio, R., Berezinsky, V., Blasi, P., Gazizov, A., Grigorieva, S., Hnatyk, B.“...-positron pair production on the cosmic microwave background (CMB) radiation. For a power-law generation...”
Published in Astroparticle Physics (2006)
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11by Veniamin Berezinsky, S. Grigorieva, Bohdan Hnatyk, A. Gazizov, Pasquale Blasi, Roberto Aloisio“...-positron pair production on the cosmic microwave background (CMB) radiation. For a power-law generation...”
Published in Astroparticle Physics (2007)
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12“...-positron pair production on the cosmic microwave background (CMB) radiation. For a power-law generation...”
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