Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments

Autor: G. C. Barbarino, Roberta Sparvoli, N. Zampa, L. A. Grishantseva, D. Fedele, M. Bongi, N. De Simone, V. Bonvicini, F. Cafagna, M. Simon, Yu. I. Stozhkov, A. A. Leonov, E. Mocchiutti, M. P. De Pascale, A. M. Galper, S. Yu. Krutkov, G. De Rosa, A. N. Kvashnin, G. V. Vasiliev, V. G. Zverev, Lorenzo Bonechi, O. Adriani, Petter Hofverberg, V. V. Malakhov, V. Malvezzi, E. Taddei, V. M. Boezio, Silvio Orsi, W. Menn, S. V. Koldashov, Yu. T. Yurkin, Marco Ricci, V. V. Mikhailov, P. Spillantini, Giuseppe Osteria, P. Carlson, Marco Casolino, A. Vacchi, A. Bruno, M. A. Bzheumikhova, T. D. Campana, Mark Pearce, S. B. Ricciarini, S. Bottai, P. Papini, E. Vannuccini, T. P. Picozza, V. Di Felice, S. A. Voronov, G. Castellini, L. Marcelli, E. A. Bogomolov, G. Zampa, T. R. Bellotti, G. A. Bazilevskaya

Publikováno v: Bulletin of the Russian Academy of Sciences: Physics. 73:364-366

Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b782c42cbaa3f87e6aa6c2f857b544e9
https://doi.org/10.3103/s1062873809030253

Cosmic ray measurements with Pamela experiment

Autor: P. Spillantini, Roberta Sparvoli, G. I. Vasilyev, V. Bonvicini, E. Mocchiutti, O. Maksumov, Gianluigi Zampa, Y. T. Yurkin, A. M. Galper, Per Carlson, F. Cafagna, G. De Rosa, Petter Hofverberg, L. Marcelli, R. Carbone, S. Bottai, A. Bruno, G. C. Barbarino, N. N. Nikonov, Marco Ricci, Giuseppe Osteria, V. V. Mikhailov, Mark Pearce, S. B. Ricciarini, N. De Simone, Andrea Vacchi, G. Castellini, Yuri Stozhkov, P. Papini, N. Zampa, E. Vannuccini, G. A. Bazilevskaya, S. A. Voronov, Alexey Leonov, V. G. Zverev, E. A. Bogomolov, E. Taddei, O. Adriani, V. Di Felice, W. Menn, D. Campana, L. A. Grishantseva, D. Fedele, Mirko Boezio, M. Bongi, A. N. Kvashnin, Marco Casolino, M. Minori, Sergey Koldashov, Lorenzo Bonechi, P. Picozza, M. Simon, M. P. De Pascale, S. Yu. Krutkov

Publikováno v: Nuclear Physics B - Proceedings Supplements. 190:293-299

PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature hi a wide energy range (protons: 80 MeV-700 GeV, electrons 50 MeV-400 GeV). Main objective is the study of the antimatter

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b14347060e775d4104a352b3d01813d
https://doi.org/10.1016/j.nuclphysbps.2009.03.102

Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment

Autor: S. V. Koldashov, Marco Ricci, Andrea Vacchi, L. A. Grishantseva, M. F. Runtso, S. A. Voronov, S. Y. Krutkov, M. Simon, N. N. Nikonov, G. Zampa, P. Spillantini, D. Campana, A. A. Leonov, P. Picozza, Mark Pearce, S. B. Ricciarini, N. Zampa, Laura Rossetto, M. Bongi, V. G. Zverev, Marco Casolino, P. Papini, E. Vannuccini, G. Castellini, N. De Simone, Y. T. Yurkin, C. Pizzolotto, V. V. Mikhailov, A. V. Karelin, Mirko Boezio, Roberta Sparvoli, V. Di Felice, W. Malvezzi, R. Carbone, I. A. Danilchenko, Lorenzo Bonechi, E. A. Bogomolov, Sergey Koldobskiy, G. C. Barbarino, V. V. Malakhov, O. Adriani, Giovanna Jerse, M. P. De Pascale, E. Mocchiutti, W. Menn, V. Bonvicini, Roberto Bellotti, L. Consiglio, G. Osteria, S. Bottai, A. M. Galper, Per Carlson, A. N. Kvashnin, Ritabrata Sarkar, F. Cafagna, Nicola Mori, Alfonso Monaco, Yuri Stozhkov, C. De Santis, S. V. Borisov, G. I. Vasilyev, William Gillard, L. Marcelli, G. A. Bazilevskaya, Juan Wu, A. Bruno, A. G. Mayorov, F. Palma

Publikováno v: JETP letters (Online) 96 (2013): 621–627. doi:10.1134/S002136401222002X
info:cnr-pdr/source/autori:Adriani O.; Bazilevskaya G.A.; Barbarino G.C.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bonvicini V.; Bongi M.; Bonechi L.; Borisov S.V.; Bottai S.; Bruno A.; Vacchi A.; Vannuccini E.; Vasilyev G.I.; Voronov S.A.; Wu J.; Galper A.M.; Grishantseva L.A.; Danilchenko I.A.; Gillard W.; Jerse G.; Zampa G.; Zampa N.; Zverev V.G.; Casolino M.; Campana D.; Carbone R.; Karelin A.V.; Carlson P.; Castellini G.; Cafagna F.; Kvashnin A.N.; Koldashov S.V.; Koldobskiy S.A.; Krutkov S.Y.; Consiglio L.; Leonov A.A.; Mayorov A.G.; Malakhov V.V.; Malvezzi W.; Marcelli L.; Menn W.; Mikhailov V.V.; Mocchiutti E.; Monaco A.; Mori N.; Nikonov N.N.; Osteria G.; Palma F.; Papini P.; Pizzolotto C.; de Pascale M.P.; Picozza P.; Pearce M.; Ricci M.; Ricciarini S.; Rossetto L.; Runtso M.F.; De Santis C.; Sarkar R.; Simon M.; De Simone N.; Sparvoli R.; Spillantini P.; Stozhkov Y.I.; Di Felice V.; Yurkin Y.T./titolo:Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment/doi:10.1134%2FS002136401222002X/rivista:JETP letters (Online)/anno:2013/pagina_da:621/pagina_a:627/intervallo_pagine:621–627/volume:96

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 dec

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b8fc6c7aaff8641240a3c3fb62f2ef5c
http://hdl.handle.net/11390/1126696

High-energy cosmic ray proton spectrum

Autor: S. V. Borisov, Marco Ricci, Mark Pearce, S. B. Ricciarini, S. Bottai, Lorenzo Bonechi, P. Spilantini, P. Papini, E. Vannuccini, D. Campana, G. A. Bazilevskaya, L. Marcelli, S. A. Koldobsky, A. Vacchi, Yu. T. Yurkin, Marco Casolino, G. Zampa, A. Bruno, Mirko Boezio, S. V. Koldashev, A. M. Galper, N. Zampa, G. C. Barbarino, N. De Simone, R. Belotti, Yu. I. Stozhkov, P. Picozza, V. V. Malakhov, A. N. Kvashnin, G. V. Vasil’ev, V. G. Zverev, M. P. De Pascale, M. F. Runtso, A. V. Karelin, S. A. Voronov, E. Mocchiutti, V. V. Mikhailov, P. Carlson, E. A. Bogomolov, V. Di Feliche, Roberta Sparvoli, L. A. Grishantseva, I. A. Danilchenko, G. Osteria, A. G. Mayorov, F. Cafagna, M. Simon, A. A. Leonov, V. Bonvicini, V. Malvezzi, D. Fedele, M. Bongi, O. Adriani, W. Menn

The method is describes and the results of measurements of the high-energy cosmic ray proton spectrum in the PAMELA experiment are presented. This experiment is performed onboard an artificial satellite and is directed to study cosmic ray particle sp

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11efc9ff5216191f4a3b9c31a2b79347
http://hdl.handle.net/11588/492769

The search for antihelium in cosmic rays using data from the PAMELA experiment

Autor: N. V. Nikonov, L. A. Grishantseva, V. V. Mikhailov, P. Carlson, G. Jerse, Roberta Sparvoli, S. A. Koldobsky, William Gillard, Mirko Boezio, Yu. T. Yurkin, P. Pizzolotto, Y. Wu, M. F. Runtso, A. Bruno, S. A. Voronov, F. Cafagna, Yu. I. Stozhkov, V. G. Zverev, P. Picozza, Roberto Bellotti, P. Spillantini, I. A. Danilchenko, E. A. Bogomolov, Nicola Mori, Andrea Vacchi, Lorenzo Bonechi, G. I. Vasiliev, S. Bottai, A. M. Galper, M. P. De Pascale, N. De Simone, S. V. Borisov, D. Campana, G. Castellini, S. Yu. Krutkov, A. N. Kvashnin, R. Carbone, Marco Casolino, V. V. Malakhov, A. V. Karelin, G. C. Barbarino, Gianluigi Zampa, L. Marcelli, M. Pearce, Giuseppe Osteria, N. Zampa, G. A. Bazilevskaya, O. Adriani, W. Menn, M. Bongi, V. Bonvicini, S. B. Ricciarini, P. Papini, E. Vannuccini, E. Mocchiutti, V. Di Felice, S. V. Koldashov, M. Simon, Marco Ricci, V. Malvezzi, A. A. Leonov, A. G. Mayorov

Publikováno v: Bulletin of the Russian Academy of Sciences. Physics 75 (2011): 331–333. doi:10.3103/S1062873811030282
info:cnr-pdr/source/autori:Mayorov A.G.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bonechi L.; Bongi M.; Bonvicini V.; Borisov S.V.; Bottai S.; Bruno A.; Cafagna F.; Campana D.; Carbone R.; Carlson P.; Casolino M.; Castellini G.; Danilchenko I.A.; De Pascale M.P.; Di Felice V.; Galper A.M.; Gillard W.; Grishantseva L.A.; Jerse G.; Karelin A.V.; Koldashov S.V.; Koldobsky S.A.; Krutkov S.Yu.; Kvashnin A.N.; Leonov A.A.; Malakhov V.V.; Malvezzi V.; Marcelli L.; Menn W.; Mikhailov V.V.; Mocchiutti E.; Mori N.; Nikonov N.V.; Osteria G.; Papini P.; Pearce M.; Picozza P.; Pizzolotto P.; Ricci M.; Ricciarini S.B.; Runtso M.F.; Simon M.; De Simone N.; Sparvoli R.; Spillantini P.; Stozhkov Yu.I.; Vacchi A.; Vannuccini E.; Vasiliev G.I.; Voronov S.A.; Wu Y.; Yurkin Yu.T.; Zampa G.; Zampa N.; Zverev V.G./titolo:The search for antihelium in cosmic rays using data from the PAMELA experiment/doi:10.3103%2FS1062873811030282/rivista:Bulletin of the Russian Academy of Sciences. Physics/anno:2011/pagina_da:331/pagina_a:333/intervallo_pagine:331–333/volume:75

The generally accepted theory explaining the observed cosmological baryon asymmetry involves mechanisms of baryosynthesis that generate asymmetry in an initially baryon symmetric Universe. Due to the possible inhomogeneous spatial nature of such mech

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d25592c8b25ff0d1eb8312016b52d8f9
https://doi.org/10.3103/s1062873811030282