학술논문

Inferred cosmic-ray spectrum from ${\it Fermi}$-LAT $\gamma$-ray observations of the Earth's limb
Document Type
Working Paper
Author
Collaboration, Fermi-LATAckermann, M.Ajello, M.Albert, A.Allafort, A.Baldini, L.Barbiellini, G.Bastieri, D.Bechtol, K.Bellazzini, R.Blandford, R. D.Bloom, E. D.Bonamente, E.Bottacini, E.Bouvier, A.Brandt, T. J.Brigida, M.Bruel, P.Buehler, R.Buson, S.Caliandro, G. A.Cameron, R. A.Caraveo, P. A.Cecchi, C.Charles, E.Chaves, R. C. G.Chekhtman, A.Chiang, J.Chiaro, G.Ciprini, S.Claus, R.Cohen-Tanugi, J.Conrad, J.Cutini, S.Dalton, M.D'Ammando, F.de Angelis, A.de Palma, F.Dermer, C. D.Digel, S. W.Di Venere, L.Silva, E. do Couto eDrell, P. S.Drlica-Wagner, A.Favuzzi, C.Fegan, S. J.Ferrara, E. C.Focke, W. B.Franckowiak, A.Fukazawa, Y.Funk, S.Fusco, P.Gargano, F.Gasparrini, D.Germani, S.Giglietto, N.Giordano, F.Giroletti, M.Glanzman, T.Godfrey, G.Gomez-Vargas, G. A.Grenier, I. A.Grove, J. E.Guiriec, S.Gustafsson, M.Hadasch, D.Hanabata, Y.Harding, A. K.Hayashida, M.Hayashi, K.Hewitt, J. W.Horan, D.Hou, X.Hughes, R. E.Inoue, Y.Jackson, M. S.Jogler, T.Jóhannesson, G.Johnson, A. S.Kamae, T.Kawano, T.Knödlseder, J.Kuss, M.Lande, J.Larsson, S.Latronico, L.Longo, F.Loparco, F.Lovellette, M. N.Lubrano, P.Mayer, M.Mazziotta, M. N.McEnery, J. E.Mehault, J.Michelson, P. F.Mitthumsiri, W.Mizuno, T.Moiseev, A. A.Monte, C.Monzani, M. E.Morselli, A.Moskalenko, I. V.Murgia, S.Nemmen, R.Nuss, E.Ohsugi, T.Okumura, A.Orienti, M.Orlando, E.Ormes, J. F.Paneque, D.Panetta, J. H.Perkins, J. S.Pesce-Rollins, M.Piron, F.Pivato, G.Porter, T. A.Rainò, S.Rando, R.Razzano, M.Razzaque, S.Reimer, A.Reimer, O.Ritz, S.Roth, M.Schaal, M.Schulz, A.Sgrò, C.Siskind, E. J.Spandre, G.Spinelli, P.Strong, A. W.Takahashi, H.Takeuchi, Y.Thayer, J. G.Thayer, J. B.Thompson, D. J.Tibaldo, L.Tinivella, M.Torres, D. F.Tosti, G.Troja, E.Tronconi, V.Usher, T. L.Vandenbroucke, J.Vasileiou, V.Vianello, G.Vitale, V.Werner, M.Winer, B. L.Wood, K. S.Wood, M.Yang, Z.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
Recent accurate measurements of cosmic-ray (CR) species by ATIC-2, CREAM, and PAMELA reveal an unexpected hardening in the proton and He spectra above a few hundred GeV, a gradual softening of the spectra just below a few hundred GeV, and a harder spectrum of He compared to that of protons. These newly-discovered features may offer a clue to the origin of high-energy CRs. We use the ${\it Fermi}$ Large Area Telescope observations of the $\gamma$-ray emission from the Earth's limb for an indirect measurement of the local spectrum of CR protons in the energy range $\sim 90~$GeV-$6~$TeV (derived from a photon energy range $15~$GeV-$1~$TeV). Our analysis shows that single power law and broken power law spectra fit the data equally well and yield a proton spectrum with index $2.68 \pm 0.04$ and $2.61 \pm 0.08$ above $\sim 200~$GeV, respectively.
Comment: Accepted by PRL for publication; Contact authors: Stefan Funk, Warit Mitthumsiri, Igor Moskalenko; 2 figures