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Secondary production Moskalenko & Strong 98Pulsar ComponentAtoyan et al. 95Pulsar ComponentZhang & Cheng 01Pulsar ComponentYksel et al. 08KKDM (mass 300 GeV)Hooper & Profumo 07 . . .

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Model-independent implications of the e+, e-, anti-proton cosmic ray spectra on properties of Dark MatterMarco Cirelli, Mario Kadastik, Martti Raidal, Alessandro Strumia

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positronsantiprotonsYes!Yes! . . .

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Arxiv.org 0811.0176 . . .

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nx for M1 TeV . . .

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Kaluza-Klein DM in UEDKaluza-Klein DM in RS AxionAxinoGravitinoPhotinoSM NeutrinoSterile NeutrinoSneutrinoLight DMLittle Higgs DMWimpzillasQ-ballsMirror MatterChamps (charged DM)D-matterCryptonsSelf-interactingSuperweakly interactingBraneworld DMHeavy neutrinoNEUTRALINOMessenger States in GMSBBranonsChaplygin GasSplit SUSYPrimordial Black Holes . . .

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(a) The predicted positron fraction from AH decay via the kinetic mixing with U(1)BL(blue line) and U(1)5 (magenta line), compared with the experimental data, including the recent PAMELA results; (b) For U(1)BL case only, using different sets of parameters in solving.Arxiv.org 0811.3357 : . . .

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.. , - , http://www.roscosmos.ru/main.php?id=133P. Picozza , A.M. Galper, G. Castellini, et al., Astroparticle Physics, v.27, pp.296-315, 2007.O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, An anomalous positron abundance in cosmic rays with energies 1.5100 GeV. Nature, 2009, v. 458, pp. 607-609.O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, New measurement of the Antiproton-to-Proton Flux Ratio up to 100 GeV in the Cosmic Radiation. Phys. Rev. Lett. 2009, v. 102, pp. 051101-1 - 051101-5.. , .. , .. . . http://cr2010.sinp.msu.ru/cr2010/pcr/pcr_30.pdf. . -, . . . 2000.Dan Hooper and Joseph Silk. Searching for Dark Matter with Future Cosmic positron Experiment. arxiv 0409104v1.W. de Boer et all. EGRET Excess of Diffuse Galactic Gamma-Rays Interpreted as a signal of Dark Matter Annihiletion. Phys. Rev. Lett. 95, 209001 (2005). . . . . . 2007.. . , . . . . , , 2007 .V. Zacek. Dark Matter. arxiv: 0707.0472v1.. . , . . , . . . . . 178 11, 1129-1164, 2008.Marko Cirelli, Roberto Franceschini, Allessandro Strumia Minimal Dark Matter predictions for galactic positrons, antiprotons, photons. IFUP TH/2008-05. SaCLAY-T08/034.Stephen L. Addler. Planet-bound Dark Matter and the internal heat of Uranus, Neptune and hot-Jupiter exoplanets. arxiv: 0808.2823v4.J. Chang, J. H. Adams, H. S. Ahn, An excess of cosmic ray electrons at energies of 300-800 GeV, Nature 456, 362-365.Graciela B. Gelmini. Search for Dark Matter. arxiv: 0810.3733v1.Wim de Boer. Indirect Dark Matter Signals. arxiv: 0810.1472v3.Malcolm Fairbairn and Jure Zupen. Two component Dark Matter. arxiv: 0810.4147v1.Peng-fei Yin et all. Pamela data and leptonically decaying Dark Matter. arxiv: 0811.0176v2.Stefano Profumo. arxiv: 0812.4457.Martin Pohl Cosmic-ray electron signatures of Dark Matter. arxiv: 0812.1174v1.Jonafhan L. Feng at all. Searches for Supersymmetry at High-Energy Colliders. arxiv: 0903.0046v2. Guido DAmico, Marc Kamionkowski and Kris Sigurdson Dark mater Astrophysics. arxiv: 0907.1912v1.Xiao-Gong He. A Brief Review on Dark Matter Annihilation Explanation for electron-positron Excesses in Cosmic Ray. arxiv: 0908.2908v1.

D. A. Diver at al. On the surface extraction of electrons in pulsar. arxiv: 0909.3581v1.Wilfried Buchmuller. Gravitino Dark Matter. arxiv: 0910.1870v1.Christoph Wenigcr. Dark Matter Decay and Cosmic Rays. arxiv: 0910.5625v1.Laura Covi, Michael Grefe, Alejandro Ibarra, David Trann. Neutrino Signals from Dark Matter Decay. arxiv: 0912.3521.Ranven Essig et all. An Electron Fixed Target Experiment to Search for a New Vector Boson ADecaying to e+ e -. arxiv: 1001.2557.C. Pallis. Tracking Quintessence, WIMP Relic Density, PAMELA and Fermi LAT. arxiv: 1001.2870.Xin Gao, Zhaofeng Kang, Tianjin Li. The Supersymmetric Standard Model With Decay and Stable Dark Matter. arxiv: 1001.3278.A. A. Ablo et all. Fermi LAT Search for Photon Lines from 30-200 GeV and Dark Matter Implicatins. arxiv: 1001.4836Qiang Yuan et all. Gamma-Rays neutrinos from Dark Matter annihilation in Galaxy Clasters. arxiv: 1002.0197.Borut Bajc et all. MSSM in view of PAMELA and Fermi/LAT. arxiv: 1002.3631.. A. Abdo et all. Constraints of Cosmological Dark Matter Annihilation from the Fermi-LAT Isotropic Diffuse Gamma-Ray Measuremant. arxiv: 1002.4415.C. B. Jackson et all. Higgs in Space. arxiv: 0912.0004.Jonathan L. Feng. Dark Matter Candidates from Particle Physics and Methods of Detection. arxiv: 1003.0904.Daniel Feldman et all. Multicomponent Dark Matter in Supersymmetric Hidden Sector Extensions. arxiv: 1004.0649.Paolo Gondolo et all. Dark Matter that come from Dark Stars. arxiv: 1004.1258.Gert Hutsi Andi Hektor et all. Implications of the Fermi-LAT diffuse gamma-ray measurements on annihilating or decaying Dark Matter. arxiv: 1004.2036.Mattheev R. Buckley and Dan Hooper. Dark Matter Subhalos In the Fermi First Sources Catalog. arxiv: 1004.1644.Chiara Arina et all. Tight Connection between Direct and Indirect Detection of Dark Matter through Higgs Portal Couplings to a Hidden Sector. arxiv: 1004.3953.Sergio Colafrancesco. Dark Matter in Modern Cosmology. arxiv: 1004.3869.G. B, C. Grojean, G. D. Krils, C. Shepherd-Themistocleous. New Physics at LHC: a Les Houd Report. arxiv: 1005.1229.Feng Huang et all. Dark Matter annihilasim and non-thermal Sungaev-Zeldovich effect: II. Dwarf Spheroidal Galaxy. J. M. Cline. Excited Dark Matter versus PAMELA/Fermi. arxiv: 1005.5001.Marco Cirell, James M. Cline. Can multistate Dark Matter annihilation explain the high-energy cosmic-ray lepton anomalies?. arxiv: 1005.1779.Manuel Oress, Ju Min Kim, Eun-Kyung Park. Direct and Indirect Detection of Neutralino Dark Matter and Collider Signatures in an SO(10) Model with Intermediate Scales. arxiv: 1006.2100.Marco Cirell, James M. Cline. Can multistate Dark Matter annihilation explain the high-energy cosmic-ray lepton anomalies?. arxiv: 1005.1779.

*****What PAMELA aims to study*******************How data are collected and sent to ground.

Collected data are stored in a 2GB memory.

About every # hours a download macrocommand is sent: the MM is readout and data are transferred to the satellite memory.

When the satellite is visible from the ground station data are transferred to ground. About ## downlink sessions per day, for a total of ##GB of transmitted data.

Data kept ## hours in the satellite memory, in case retransmission is required due to high error rate. ************