%0 Journal Article %1 Adriani2013 %A Adriani, O. %A Bazilevskaya, G. A. %A Barbarino, G. C. %A Bellotti, R. %A Boezio, M. %A Bogomolov, E. A. %A Bonvicini, V. %A Bongi, M. %A Bonechi, L. %A Borisov, S. V. %A Bottai, S. %A Bruno, A. %A Vacchi, A. %A Vannuccini, E. %A Vasilyev, G. I. %A Voronov, S. A. %A Wu, J. %A Galper, A. M. %A Grishantseva, L. A. %A Danilchenko, I. A. %A Gillard, W. %A Jerse, G. %A Zampa, G. %A Zampa, N. %A Zverev, V. G. %A Casolino, M. %A Campana, D. %A Carbone, R. %A Karelin, A. V. %A Carlson, P. %A Castellini, G. %A Cafagna, F. %A Kvashnin, A. N. %A Koldashov, S. V. %A Koldobskiy, S. A. %A Krutkov, S. Y. %A Consiglio, L. %A Leonov, A. A. %A Mayorov, A. G. %A Malakhov, V. V. %A Malvezzi, W. %A Marcelli, L. %A Menn, W. %A Mikhailov, V. V. %A Mocchiutti, E. %A Monaco, A. %A Mori, N. %A Nikonov, N. N. %A Osteria, G. %A Palma, F. %A Papini, P. %A Pizzolotto, C. %A de Pascale, M. P. %A Picozza, P. %A Pearce, M. %A Ricci, M. %A Ricciarini, S. %A Rossetto, L. %A Runtso, M. F. %A De Santis, C. %A Sarkar, R. %A Simon, M. %A De Simone, N. %A Sparvoli, R. %A Spillantini, P. %A Stozhkov, Y. I. %A Di Felice, V. %A Yurkin, Y. T. %D 2013 %J JETP Letters %K pamela_exp %N 10 %P 621--627 %R 10.1134/S002136401222002X %T Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment %U https://doi.org/10.1134/S002136401222002X %V 96 %X It is interesting to measure the antiproton galactic component in cosmic rays in order to study the mechanisms by which particles and antiparticles are generated and propagate in the Galaxy and to search for new sources of, e.g., annihilation or decay of dark matter hypothetical particles. The antiproton spectrum and the ratio of the fluxes of primary cosmic ray antiprotons to protons with energies of 60 MeV to 350 GeV found from the data obtained from June 2006 to January 2010 in the PAMELA experiment are presented. The usage of the advanced data processing method based on the data classification mathematical model made it possible to increase statistics and analyze the region of higher energies than in the earlier works.

@article{Adriani2013, abstract = {It is interesting to measure the antiproton galactic component in cosmic rays in order to study the mechanisms by which particles and antiparticles are generated and propagate in the Galaxy and to search for new sources of, e.g., annihilation or decay of dark matter hypothetical particles. The antiproton spectrum and the ratio of the fluxes of primary cosmic ray antiprotons to protons with energies of 60 MeV to 350 GeV found from the data obtained from June 2006 to January 2010 in the PAMELA experiment are presented. The usage of the advanced data processing method based on the data classification mathematical model made it possible to increase statistics and analyze the region of higher energies than in the earlier works.}, added-at = {2019-03-12T12:33:20.000+0100}, author = {Adriani, O. and Bazilevskaya, G. A. and Barbarino, G. C. and Bellotti, R. and Boezio, M. and Bogomolov, E. A. and Bonvicini, V. and Bongi, M. and Bonechi, L. and Borisov, S. V. and Bottai, S. and Bruno, A. and Vacchi, A. and Vannuccini, E. and Vasilyev, G. I. and Voronov, S. A. and Wu, J. and Galper, A. M. and Grishantseva, L. A. and Danilchenko, I. A. and Gillard, W. and Jerse, G. and Zampa, G. and Zampa, N. and Zverev, V. G. and Casolino, M. and Campana, D. and Carbone, R. and Karelin, A. V. and Carlson, P. and Castellini, G. and Cafagna, F. and Kvashnin, A. N. and Koldashov, S. V. and Koldobskiy, S. A. and Krutkov, S. Y. and Consiglio, L. and Leonov, A. A. and Mayorov, A. G. and Malakhov, V. V. and Malvezzi, W. and Marcelli, L. and Menn, W. and Mikhailov, V. V. and Mocchiutti, E. and Monaco, A. and Mori, N. and Nikonov, N. N. and Osteria, G. and Palma, F. and Papini, P. and Pizzolotto, C. and de Pascale, M. P. and Picozza, P. and Pearce, M. and Ricci, M. and Ricciarini, S. and Rossetto, L. and Runtso, M. F. and De Santis, C. and Sarkar, R. and Simon, M. and De Simone, N. and Sparvoli, R. and Spillantini, P. and Stozhkov, Y. I. and Di Felice, V. and Yurkin, Y. T.}, biburl = {https://www.bibsonomy.org/bibtex/2bd2e2c4e7c8aceb5e0c94e2808c9aef1/pamela_exp}, day = 01, doi = {10.1134/S002136401222002X}, interhash = {a3ea9af8b361abfd7010be3697fcdc9d}, intrahash = {bd2e2c4e7c8aceb5e0c94e2808c9aef1}, issn = {1090-6487}, journal = {JETP Letters}, keywords = {pamela_exp}, month = jan, number = 10, pages = {621--627}, timestamp = {2019-03-12T12:33:20.000+0100}, title = {Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment}, url = {https://doi.org/10.1134/S002136401222002X}, volume = 96, year = 2013 }