'Electron spectrum' presentation slideshows

Dark matter searches by charged cosmic rays detection in space

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PAMELA Collaboration

The PAMELA space experiment: results after s even y ears in orbit Mirko Boezio INFN Trieste, Italy On behalf of the PAMELA collaboration INFN-Space/3, Frascati September 18 th 2013. Italy:. CNR, Florence. Bari. Florence. Frascati. Naples. Rome. Trieste. Russia:. Moscow

546 views • 54 slides

The Neutron Alphabet Exploring the properties of fundamental interactions with cold neutrons

The Neutron Alphabet Exploring the properties of fundamental interactions with cold neutrons. Hartmut Abele. The Neutron Alphabet and Symmetries. A: P-odd B: P-odd C: P-odd D: T-odd a N R: T-odd. A. Neutron Spin. ?. Electron. B. Neutrino. C. Proton.

623 views • 50 slides

Dark Matter Particle Search by High Energy Electron and Gamma-ray Observation

Dark Matter Particle Search by High Energy Electron and Gamma-ray Observation. J. Chang Purple Mountain Observatory,CAS, China. Outline. Astrophysical Significance ATIC Results Chinese missions for high energy electron Summary. Astrophysical Significance Dark Matter Signatures

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The Cosmic Ray Electron Excess

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GeV-TeV Gamma-ray Astronomy

International Workshop on Extremely High Energy Cosmic Rays, March 22-23, 2001, Kashiwa. GeV-TeV Gamma-ray Astronomy. Masaki Mori ICRR, Univ. Tokyo. http://icrhp9.icrr.u-tokyo.ac.jp. Gamma-ray astronomy: short history. Prediction of nuclear gamma-rays Hayakawa 1952; Morrison 1958

553 views • 39 slides

WG7: Particle acceleration and transport

WG7: Particle acceleration and transport. Regular Participants. Our Goal. Topic I : Signatures of particle acceleration before (pre-event), during (impulsive phase) and long after the flare.

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Over view of charm production at RHIC

All nice talks on data are Over I am offering my own view. Over view of charm production at RHIC. Presentions: Xiaorong Wang, PHENIX (Forward muon) Yifei Zhang, STAR (mid-rapidity, muon, electron) Haibin Zhang, STAR (STAR overview)

333 views • 27 slides

Alexander Moiseev NASA Goddard Space Flight Center and University of Maryland

New results on high energy cosmic ray electrons observed with Fermi LAT and their implications on the existence of nearby cosmic ray sources. Alexander Moiseev NASA Goddard Space Flight Center and University of Maryland for the Fermi LAT Collaboration.

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Ordered States of Adatoms in Graphene

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GALILEO MEETING Nobeyama 10/11 July, 2002 UK BCS PRESENTATION

GALILEO MEETING Nobeyama 10/11 July, 2002 UK BCS PRESENTATION. Len Culhane Mullard Space Science Laboratory University College London. SUMMARY. Brief history of BCS concept Summary of instrument properties Some scientific highlights People involved in Galileo project

292 views • 22 slides

Electron Observation : Past, Present and Future

Electron Observation : Past, Present and Future. S.Torii : Waseda University (Japan). Rome PAMELA Workshop 11.05.2009. Model Dependence of Nearby Source Effect. Kobayashi et al. ApJ 2003. Ec=? ? ?T=0 yr, Do=2x10 29 cm 2 /s at 1 TeV. Do=5 x 10 29 cm 2 /s. Ec= 20 TeV.

220 views • 14 slides

Regularized Mean and Accelerated Electron Flux Spectra in Solar Flares

Regularized Mean and Accelerated Electron Flux Spectra in Solar Flares. Eduard P. Kontar University of Glasgow Michele Piana , Anna Maria Massone ( INFM, UdR di Genova ), A. Gordon Emslie ( The University of Alabama in Huntsville ), and John C. Brown ( University of Glasgow ).

240 views • 13 slides

NuMI Beam Study

NuMI Beam Study. ? e component the LE beam configuration. Benjamin Brown University of Pittsburgh. NuMI LE Configuration. Contains ? ? , ? e ? ? absolute flux ~ 8.6 * 10 16 / m 2 year (@ 2.5 * 10 20 PoT/year) ? e contamination absolute flux about %1. Predicted CC Events.

208 views • 10 slides