Sökning: onr:"swepub:oai:DiVA.org:kth-119063" > Measurement of the ...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 04440naa a2201117 4500 | |
001 | oai:DiVA.org:kth-119063 | |
003 | SwePub | |
008 | 130305s2013 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1190632 URI |
024 | 7 | a https://doi.org/10.1134/S002136401222002X2 DOI |
040 | a (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Adriani, O.4 aut |
245 | 1 0 | a Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment |
264 | 1 | c 2013 |
338 | a print2 rdacarrier | |
500 | a QC 20130306 | |
520 | a 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. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a Anti-Protons | |
653 | a Matter | |
700 | 1 | a Bazilevskaya, G. A.4 aut |
700 | 1 | a Barbarino, G. C.4 aut |
700 | 1 | a Bellotti, R.4 aut |
700 | 1 | a Boezio, M.4 aut |
700 | 1 | a Bogomolov, E. A.4 aut |
700 | 1 | a Bonvicini, V.4 aut |
700 | 1 | a Bongi, M.4 aut |
700 | 1 | a Bonechi, L.4 aut |
700 | 1 | a Borisov, S. V.4 aut |
700 | 1 | a Bottai, S.4 aut |
700 | 1 | a Bruno, A.4 aut |
700 | 1 | a Vacchi, A.4 aut |
700 | 1 | a Vannuccini, E.4 aut |
700 | 1 | a Vasilyev, G. I.4 aut |
700 | 1 | a Voronov, S. A.4 aut |
700 | 1 | a Wu, Juanu KTH,Fysik4 aut0 (Swepub:kth)u1y0e14w |
700 | 1 | a Galper, A. M.4 aut |
700 | 1 | a Grishantseva, L. A.4 aut |
700 | 1 | a Danilchenko, I. A.4 aut |
700 | 1 | a Gillard, Williamu KTH,Fysik4 aut0 (Swepub:kth)u171jmfw |
700 | 1 | a Jerse, G.4 aut |
700 | 1 | a Zampa, G.4 aut |
700 | 1 | a Zampa, N.4 aut |
700 | 1 | a Zverev, V. G.4 aut |
700 | 1 | a Casolino, M.4 aut |
700 | 1 | a Campana, D.4 aut |
700 | 1 | a Carbone, R.4 aut |
700 | 1 | a Karelin, A. V.4 aut |
700 | 1 | a Carlson, Peru KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1ua4u32 |
700 | 1 | a Castellini, G.4 aut |
700 | 1 | a Cafagna, F.4 aut |
700 | 1 | a Kvashnin, A. N.4 aut |
700 | 1 | a Koldashov, S. V.4 aut |
700 | 1 | a Koldobskiy, S. A.4 aut |
700 | 1 | a Krutkov, S. Y.4 aut |
700 | 1 | a Consiglio, L.4 aut |
700 | 1 | a Leonov, A. A.4 aut |
700 | 1 | a Mayorov, A. G.4 aut |
700 | 1 | a Malakhov, V. V.4 aut |
700 | 1 | a Malvezzi, W.4 aut |
700 | 1 | a Marcelli, L.4 aut |
700 | 1 | a Menn, W.4 aut |
700 | 1 | a Mikhailov, V. V.4 aut |
700 | 1 | a Mocchiutti, E.4 aut |
700 | 1 | a Monaco, A.4 aut |
700 | 1 | a Mori, N.4 aut |
700 | 1 | a Nikonov, N. N.4 aut |
700 | 1 | a Osteria, G.4 aut |
700 | 1 | a Palma, F.4 aut |
700 | 1 | a Papini, P.4 aut |
700 | 1 | a Pizzolotto, C.4 aut |
700 | 1 | a de Pascale, M. P.4 aut |
700 | 1 | a Picozza, P.4 aut |
700 | 1 | a Pearce, Marku KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u17jptna |
700 | 1 | a Ricci, M.4 aut |
700 | 1 | a Ricciarini, S.4 aut |
700 | 1 | a Rossetto, Laurau KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1tv6cqb |
700 | 1 | a Runtso, M. F.4 aut |
700 | 1 | a De Santis, C.4 aut |
700 | 1 | a Sarkar, R.4 aut |
700 | 1 | a Simon, M.4 aut |
700 | 1 | a De Simone, N.4 aut |
700 | 1 | a Sparvoli, R.4 aut |
700 | 1 | a Spillantini, P.4 aut |
700 | 1 | a Stozhkov, Y. I.4 aut |
700 | 1 | a Di Felice, V.4 aut |
700 | 1 | a Yurkin, Y. T.4 aut |
710 | 2 | a KTHb Fysik4 org |
773 | 0 | t JETP Lettersg 96:10, s. 621-627q 96:10<621-627x 0021-3640x 1090-6487 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-119063 |
856 | 4 8 | u https://doi.org/10.1134/S002136401222002X |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
Kopiera och spara länken för att återkomma till aktuell vy