Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment

S. A. Koldobskiy; V. Formato; O. Adriani; G. C. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. Boezio; E. A. Bogomolov; L. Bonechi; M. Bongi; V. Bonvicini; S. V. Borisov; S. Bottai; A. Bruno; A. Vacchi; E. Vannuccini; G. Vasilyev; S. A. Voronov; A. M. Galper; I. A. Danilchenko; M. P. De Pascale; C. De Santis; N. De Simone; V. Di Felice; G. Jerse; V. G. Zverev; G. Zampa; N. Zampa; A. V. Karelin; F. Cafagna; D. Campana; R. Carbone; P. Carlson; M. Casolino; G. Castellini; A. N. Kvashnin; S. V. Koldashov; L. Consiglio; S. Y. Krutkov; A. A. Leonov; L. Marcelli; A. G. Mayorov; V. V. Malakhov; W. Menn; V. V. Mikhailov; E. Mocchiutti; A. Monaco; N. Mori; G. Osteria; P. Papini; M. Pearce; P. Picozza; C. Pizzolotto; M. Ricci; S. B. Ricciarini; L. Rossetto; M. F. Runtso; M. M. Simon; R. Sparvoli; P. Spillantini; Y. I. Stozhkov; Y. T. Yurkin

doi:10.3103/s1062873813050274

Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment

S. A. Koldobskiy, V. Formato, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. V. Borisov, S. Bottai, A. Bruno, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, A. M. Galper, I. A. DanilchenkoM. P. De Pascale, C. De Santis, N. De Simone, V. Di Felice, G. Jerse, V. G. Zverev, G. Zampa, N. Zampa, A. V. Karelin, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, A. N. Kvashnin, S. V. Koldashov, L. Consiglio, S. Y. Krutkov, A. A. Leonov, L. Marcelli, A. G. Mayorov, V. V. Malakhov, W. Menn, V. V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, G. Osteria, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, M. F. Runtso, M. M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, Y. T. Yurkin

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Abstract

This work presents the results of measuring the deuteron spectrum of Galactic cosmic rays (GCRs) with the PAMELA experiment. The PAMELA is an international experiment. Its main objectives are to search for antimatter and measure proton, helium nuclei, electron, and positron spectra over a wide range of energies. In addition, the experimental setup allows the detection of deuterons and the reconstruction of their spectra at low energies. Cosmic ray deuteron spectrum and the deuteron-proton ratio measured in the PAMELA experiment in the energy range of 50-650 MeV/nucleon are presented below.

Original language	English
Pages (from-to)	606-608
Number of pages	3
Journal	Bulletin of the Russian Academy of Sciences: Physics
Volume	77
Issue number	5
DOIs	https://doi.org/10.3103/s1062873813050274
State	Published - May 2013
Externally published	Yes

Bibliographical note

Funding Information:
This work was supported by the Russian Founda tion for Basic Research, project no. 10 02 01301a.

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Koldobskiy, S. A., Formato, V., 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., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Galper, A. M., ... Yurkin, Y. T. (2013). Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment. Bulletin of the Russian Academy of Sciences: Physics, 77(5), 606-608. https://doi.org/10.3103/s1062873813050274

@article{473342620a6d4315bbd4ee5054e3eea5,

title = "Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment",

abstract = "This work presents the results of measuring the deuteron spectrum of Galactic cosmic rays (GCRs) with the PAMELA experiment. The PAMELA is an international experiment. Its main objectives are to search for antimatter and measure proton, helium nuclei, electron, and positron spectra over a wide range of energies. In addition, the experimental setup allows the detection of deuterons and the reconstruction of their spectra at low energies. Cosmic ray deuteron spectrum and the deuteron-proton ratio measured in the PAMELA experiment in the energy range of 50-650 MeV/nucleon are presented below.",

author = "Koldobskiy, {S. A.} and V. Formato and O. Adriani and Barbarino, {G. C.} and Bazilevskaya, {G. A.} and R. Bellotti and M. Boezio and Bogomolov, {E. A.} and L. Bonechi and M. Bongi and V. Bonvicini and Borisov, {S. V.} and S. Bottai and A. Bruno and A. Vacchi and E. Vannuccini and G. Vasilyev and Voronov, {S. A.} and Galper, {A. M.} and Danilchenko, {I. A.} and {De Pascale}, {M. P.} and {De Santis}, C. and {De Simone}, N. and {Di Felice}, V. and G. Jerse and Zverev, {V. G.} and G. Zampa and N. Zampa and Karelin, {A. V.} and F. Cafagna and D. Campana and R. Carbone and P. Carlson and M. Casolino and G. Castellini and Kvashnin, {A. N.} and Koldashov, {S. V.} and L. Consiglio and Krutkov, {S. Y.} and Leonov, {A. A.} and L. Marcelli and Mayorov, {A. G.} and Malakhov, {V. V.} and W. Menn and Mikhailov, {V. V.} and E. Mocchiutti and A. Monaco and N. Mori and G. Osteria and P. Papini and M. Pearce and P. Picozza and C. Pizzolotto and M. Ricci and Ricciarini, {S. B.} and L. Rossetto and Runtso, {M. F.} and Simon, {M. M.} and R. Sparvoli and P. Spillantini and Stozhkov, {Y. I.} and Yurkin, {Y. T.}",

note = "Funding Information: This work was supported by the Russian Founda tion for Basic Research, project no. 10 02 01301a.",

year = "2013",

month = may,

doi = "10.3103/s1062873813050274",

language = "אנגלית",

volume = "77",

pages = "606--608",

journal = "Bulletin of the Russian Academy of Sciences: Physics",

issn = "1062-8738",

publisher = "Pleiades Publishing",

number = "5",

}

Koldobskiy, SA, Formato, V, Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, SV, Bottai, S, Bruno, A, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, SA, Galper, AM, Danilchenko, IA, De Pascale, MP, De Santis, C, De Simone, N, Di Felice, V, Jerse, G, Zverev, VG, Zampa, G, Zampa, N, Karelin, AV, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Kvashnin, AN, Koldashov, SV, Consiglio, L, Krutkov, SY, Leonov, AA, Marcelli, L, Mayorov, AG, Malakhov, VV, Menn, W, Mikhailov, VV, Mocchiutti, E, Monaco, A, Mori, N, Osteria, G, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, SB, Rossetto, L, Runtso, MF, Simon, MM, Sparvoli, R, Spillantini, P, Stozhkov, YI & Yurkin, YT 2013, 'Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment', Bulletin of the Russian Academy of Sciences: Physics, vol. 77, no. 5, pp. 606-608. https://doi.org/10.3103/s1062873813050274

TY - JOUR

T1 - Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment

AU - Koldobskiy, S. A.

AU - Formato, V.

AU - Adriani, O.

AU - Barbarino, G. C.

AU - Bazilevskaya, G. A.

AU - Bellotti, R.

AU - Boezio, M.

AU - Bogomolov, E. A.

AU - Bonechi, L.

AU - Bongi, M.

AU - Bonvicini, V.

AU - Borisov, S. V.

AU - Bottai, S.

AU - Bruno, A.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasilyev, G.

AU - Voronov, S. A.

AU - Galper, A. M.

AU - Danilchenko, I. A.

AU - De Pascale, M. P.

AU - De Santis, C.

AU - De Simone, N.

AU - Di Felice, V.

AU - Jerse, G.

AU - Zverev, V. G.

AU - Zampa, G.

AU - Zampa, N.

AU - Karelin, A. V.

AU - Cafagna, F.

AU - Campana, D.

AU - Carbone, R.

AU - Carlson, P.

AU - Casolino, M.

AU - Castellini, G.

AU - Kvashnin, A. N.

AU - Koldashov, S. V.

AU - Consiglio, L.

AU - Krutkov, S. Y.

AU - Leonov, A. A.

AU - Marcelli, L.

AU - Mayorov, A. G.

AU - Malakhov, V. V.

AU - Menn, W.

AU - Mikhailov, V. V.

AU - Mocchiutti, E.

AU - Monaco, A.

AU - Mori, N.

AU - Osteria, G.

AU - Papini, P.

AU - Pearce, M.

AU - Picozza, P.

AU - Pizzolotto, C.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Rossetto, L.

AU - Runtso, M. F.

AU - Simon, M. M.

AU - Sparvoli, R.

AU - Spillantini, P.

AU - Stozhkov, Y. I.

AU - Yurkin, Y. T.

N1 - Funding Information: This work was supported by the Russian Founda tion for Basic Research, project no. 10 02 01301a.

PY - 2013/5

Y1 - 2013/5

N2 - This work presents the results of measuring the deuteron spectrum of Galactic cosmic rays (GCRs) with the PAMELA experiment. The PAMELA is an international experiment. Its main objectives are to search for antimatter and measure proton, helium nuclei, electron, and positron spectra over a wide range of energies. In addition, the experimental setup allows the detection of deuterons and the reconstruction of their spectra at low energies. Cosmic ray deuteron spectrum and the deuteron-proton ratio measured in the PAMELA experiment in the energy range of 50-650 MeV/nucleon are presented below.

AB - This work presents the results of measuring the deuteron spectrum of Galactic cosmic rays (GCRs) with the PAMELA experiment. The PAMELA is an international experiment. Its main objectives are to search for antimatter and measure proton, helium nuclei, electron, and positron spectra over a wide range of energies. In addition, the experimental setup allows the detection of deuterons and the reconstruction of their spectra at low energies. Cosmic ray deuteron spectrum and the deuteron-proton ratio measured in the PAMELA experiment in the energy range of 50-650 MeV/nucleon are presented below.

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U2 - 10.3103/s1062873813050274

DO - 10.3103/s1062873813050274

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AN - SCOPUS:84879103297

SN - 1062-8738

VL - 77

SP - 606

EP - 608

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

IS - 5

ER -

Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment

Abstract

Bibliographical note

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