The cosmic-ray positron energy spectrum measured by PAMELA

Autor: PAMELA Collaboration, Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bianco, A., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge', M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, L., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stochaj, S. J., Stockton, J. C., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G.

Publikováno v: Phys. Rev. Lett. 111 (2013) 081102

Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make

Externí odkaz: http://arxiv.org/abs/1308.0133

Cosmic-Ray Positron Energy Spectrum Measured by PAMELA

Autor: PAMELA Collaboration, Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bianco, A., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge', M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, L., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stochaj, S. J., Stockton, J. C., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G.

Publikováno v: Physical review letters (CD-ROM) 111 (2013). doi:10.1103/PhysRevLett.111.081102
info:cnr-pdr/source/autori:Adriani, O., Barbarino, G.C., Bazilevskaya, G.A., Bellotti, R., Bianco, Castellini, G.,Ricciarini, S.B., et al./titolo:Cosmic-ray positron energy spectrum measured by PAMELA/doi:10.1103%2FPhysRevLett.111.081102/rivista:Physical review letters (CD-ROM)/anno:2013/pagina_da:/pagina_a:/intervallo_pagine:/volume:111

Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e55a6306687fc719f6f46e9e4b16169
http://hdl.handle.net/11390/1125110

Radiative Correction to e+e-->e+e- in the Electroweak Theory. II: Corrected Elastic Cross Section and Positron Energy Spectrum

Autor: Yoshimitsu Shimizu, Keijiro Tobimatsu

Publikováno v: Progress of Theoretical Physics. 75:905-913

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::dc7e36a2039f8c8702f572bba0e5c534
https://doi.org/10.1143/ptp.75.905

Cosmic–ray positron energy spectrum measured by PAMELA

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

Publikováno v: Scopus-Elsevier

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::14829bd879029e96c482008447856efc
http://www.scopus.com/inward/record.url?eid=2-s2.0-85052290420&partnerID=MN8TOARS

The Relation of the Positron Energy Spectrum to the Decay Constant and to the Energy of the Bombarding Protons

Autor: Carl D. Anderson, Seth H. Neddermeyer

Publikováno v: Physical Review. 45:653-654

We have reported(1) approximate energy distributions of the positrons emitted by various substances activated by proton or deuton bombardment. A typical photograph is reproduced in Fig. 1. To find whether a relation exists between the maximum energy

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af49f225b94fe89b94e7662369447c2e
https://doi.org/10.1103/physrev.45.653