PAMELA and electrons

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

doi:10.1016/j.nima.2010.06.021

PAMELA and electrons

E. Mocchiutti, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, L. ConsiglioM. P. De Pascale, C. De Santis, V. Di Felice, A. M. Galper, L. Grishantseva, W. Gillard, P. Hofverberg, G. Jerse, S. V. Koldashov, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, O. Maksumov, V. Malakhov, V. Malvezzi, L. Marcelli, W. Menn, V. V. Mikhailov, N. Mori, N. Nikonov, G. Osteria, P. Papini, M. Pearce, P. Picozza, M. Ricci, S. B. Ricciarini, L. Rossetto, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, J. Wu, Y. T. Yurkin, G. Zampa, N. Zampa, V. G. Zverev

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Abstract

The 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicontungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV100's GeV) with high statistics. The measurement of the positron to electron fraction and of the electron energy spectrum in order to search for exotic sources, such as dark matter particle annihilations, are within the PAMELA primary scientific goal.

Original language	English
Pages (from-to)	28-35
Number of pages	8
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	630
Issue number	1
DOIs	https://doi.org/10.1016/j.nima.2010.06.021
State	Published - 21 Feb 2011
Externally published	Yes

Keywords

Dark matter
Electrons
PAMELA
Positron fraction

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Mocchiutti, E., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., ... Zverev, V. G. (2011). PAMELA and electrons. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 630(1), 28-35. https://doi.org/10.1016/j.nima.2010.06.021

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abstract = "The 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicontungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV100's GeV) with high statistics. The measurement of the positron to electron fraction and of the electron energy spectrum in order to search for exotic sources, such as dark matter particle annihilations, are within the PAMELA primary scientific goal.",

keywords = "Dark matter, Electrons, PAMELA, Positron fraction",

author = "E. Mocchiutti 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 S. Borisov and S. Bottai and A. Bruno and F. Cafagna and D. Campana and R. Carbone and P. Carlson and M. Casolino and G. Castellini and L. Consiglio and {De Pascale}, {M. P.} and {De Santis}, C. and {Di Felice}, V. and Galper, {A. M.} and L. Grishantseva and W. Gillard and P. Hofverberg and G. Jerse and Koldashov, {S. V.} and Krutkov, {S. Y.} and Kvashnin, {A. N.} and A. Leonov and O. Maksumov and V. Malakhov and V. Malvezzi and L. Marcelli and W. Menn and Mikhailov, {V. V.} and N. Mori and N. Nikonov and G. Osteria and P. Papini and M. Pearce and P. Picozza and M. Ricci and Ricciarini, {S. B.} and L. Rossetto and M. Simon and R. Sparvoli and P. Spillantini and Stozhkov, {Y. I.} and A. Vacchi and E. Vannuccini and G. Vasilyev and Voronov, {S. A.} and J. Wu and Yurkin, {Y. T.} and G. Zampa and N. Zampa and Zverev, {V. G.}",

year = "2011",

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doi = "10.1016/j.nima.2010.06.021",

language = "אנגלית",

volume = "630",

pages = "28--35",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier B.V.",

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Mocchiutti, E, Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Consiglio, L, De Pascale, MP, De Santis, C, Di Felice, V, Galper, AM, Grishantseva, L, Gillard, W, Hofverberg, P, Jerse, G, Koldashov, SV, Krutkov, SY, Kvashnin, AN, Leonov, A, Maksumov, O, Malakhov, V, Malvezzi, V, Marcelli, L, Menn, W, Mikhailov, VV, Mori, N, Nikonov, N, Osteria, G, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, SB, Rossetto, L, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, YI, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, SA, Wu, J, Yurkin, YT, Zampa, G, Zampa, N & Zverev, VG 2011, 'PAMELA and electrons', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 630, no. 1, pp. 28-35. https://doi.org/10.1016/j.nima.2010.06.021

TY - JOUR

T1 - PAMELA and electrons

AU - Mocchiutti, E.

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.

AU - Bottai, S.

AU - Bruno, A.

AU - Cafagna, F.

AU - Campana, D.

AU - Carbone, R.

AU - Carlson, P.

AU - Casolino, M.

AU - Castellini, G.

AU - Consiglio, L.

AU - De Pascale, M. P.

AU - De Santis, C.

AU - Di Felice, V.

AU - Galper, A. M.

AU - Grishantseva, L.

AU - Gillard, W.

AU - Hofverberg, P.

AU - Jerse, G.

AU - Koldashov, S. V.

AU - Krutkov, S. Y.

AU - Kvashnin, A. N.

AU - Leonov, A.

AU - Maksumov, O.

AU - Malakhov, V.

AU - Malvezzi, V.

AU - Marcelli, L.

AU - Menn, W.

AU - Mikhailov, V. V.

AU - Mori, N.

AU - Nikonov, N.

AU - Osteria, G.

AU - Papini, P.

AU - Pearce, M.

AU - Picozza, P.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Rossetto, L.

AU - Simon, M.

AU - Sparvoli, R.

AU - Spillantini, P.

AU - Stozhkov, Y. I.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasilyev, G.

AU - Voronov, S. A.

AU - Wu, J.

AU - Yurkin, Y. T.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

PY - 2011/2/21

Y1 - 2011/2/21

N2 - The 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicontungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV100's GeV) with high statistics. The measurement of the positron to electron fraction and of the electron energy spectrum in order to search for exotic sources, such as dark matter particle annihilations, are within the PAMELA primary scientific goal.

AB - The 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicontungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV100's GeV) with high statistics. The measurement of the positron to electron fraction and of the electron energy spectrum in order to search for exotic sources, such as dark matter particle annihilations, are within the PAMELA primary scientific goal.

KW - Dark matter

KW - Electrons

KW - PAMELA

KW - Positron fraction

UR - http://www.scopus.com/inward/record.url?scp=79951726997&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2010.06.021

DO - 10.1016/j.nima.2010.06.021

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:79951726997

SN - 0168-9002

VL - 630

SP - 28

EP - 35

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

IS - 1

ER -

PAMELA and electrons

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Keywords

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