... renormalized); E200 MeV/nucleon, essentially flat Silberberg & Tsao 2000 (non-renormalized, renormalized); claim that it works at all energies, ...
Contains c , fortran routines & input files (dat-files, compass gas ... Dermer 1986 method: LE Stecker ?-isobar model (isotropic decay), HE scaling (inv. ...
Intro to the physics that we are working with (?-ray CR connection) ... Pulsar distribution (Lorimer 2004) sun. XCO=N(H2)/WCO: Histo This work, Strong et al.'04 ...
how well can we reconstruct the gas & cosmic-ray distributions in the plane? ... qhiHI =qHI01.HI01 qHI2.HI2 qHI3.HI3 qHI4.HI4 qHI5.HI5 qHI6.HI6 qHI78.HI78 ...
Dark Matter shining by Galactic gamma rays and its possible implications for the LHC Ingredients to this analysis From EGRET excess of diffuse Galactic gamma rays
CONVENTIONAL MODEL: the electron and proton spectra locally measured are ... Looking for pevatrons: the emission from a SNR and from a cloud close to the SNR ...
Service d'Astrophysique, CEA Saclay. sep-04. the local interstellar emission ... NHI from Hartmann & Burton '97 and Dickey & Lockman '90. WCO from Dame et al. '01 ...
EGRET's Excess of Diffuse Gamma Rays. as Dark Matter Tracer. Pearl Sandick ... Whole halo contributes to diffuse ? ray intensity, but only diffusion region (R ...
Spectra 'optimized' to explain EGRET GeV excess without DM (does not work well ... scenarios that were compatible with both the BESS and EGRET measurements! ...
Mandate deliverable from the LAT team (see previous talk) ... Crux. Seven 3EG sources. GLAST LAT Project. LAT Collaboration Meeting, 29 September 2004 8 ...
It's z-component is the only one different from zero and increases linearly with ... with the conventional cosmic ray spectra (Strong et al. 2004) new s model ...
Title: Propagation of Cosmic Rays & Diffuse Galactic Gamma Rays Subject: Propagation of Cosmic Rays in the Galaxy Author: Igor Moskalenko Last modified by
PSR J1629-6902. 3 nearby Fermi-LAT sources. closest 5.1 away. 10. Data on Sample of Pulsars ... point for Hannestad-Raffelt function (n=3) was specified for PSR. ...
... NFW profile from Taylor & Babul, 2004, 2005 ... Milky Way Halo simulated by Taylor & Babul (2005) All-sky map of DM gamma ray emission (Baltz 2006) ...
Service Challenge Workshop. Nov 29 - Dec 1st. Gamma-ray Large Area Space Telescope ... Stefan Funk, Jim Chiang, Max Razzano, Seth Digel, Ping Wang, Alice Harding, ...
H.E.S.S. survey of the Galactic plane revealed a TeV diffuse component (after ... based and a kind of hybrid, fitting linear combinations of templates for gas and ...
Indirect Evidence for Dark Matter from Galactic Gamma Rays DM what is it? We don t know it, because we don t see it! WdB, C. Sander, V. Zhukov, A. Gladyshev, D ...
Residual CR produce unstructured, quasi-isotropic background (after sufficient observation time) ... Improved agreement between simulation and data from ...
The Observational Case For 7-8 GeV Dark Matter: Fermi, CoGeNT and DAMA Dan Hooper Fermilab/University of Chicago University of California Santa Barbara
... underlying theory of this phenomenology, moduli. Comments on LHC ... sometimes new collider phenomenology new light vector bosons with mass 1 GeV, ...
... magnet (BL2= 0.85 Tm2) Silicon Tracker (rigidity, charge) ... AMS on the International Space Station will provide enough statistics to perform a multi ...
discussion on how to combine detection results in different energy bands ... TS ' position for the source characterization step for firmly identified sources ...
During lectures I usually try to read the audience, which will ... A detour cosmic ray diffusion in the Galaxy. Instrumental background. Experimental approaches ...
First glimpse into cosmic ray interaction with ISM ... index = 2.0,2.25,2.5. Scaling law. Scaling law. Isobar. Model (Dermer) Isobar. Model (Dermer) ...
Time evolution of number density is defined by Boltzmann equation: ... Combining this with the fact that the boost factors come all out to be similar ...
This assumes, for no good reason, that there is NO motion normal the average ... Conclusions: Theory is in good shape, but there are too many alternatives. ...
Right now, EGRET data (and more) can be described by scenarios with and without DM ... Explains EGRET data with a photon component from neutralino annihilation ...
Some shocks are very efficient accelerators 50% Magnetic amplification mG- mG ... Most CRs decompress until. expansion sub-Alfvenic. Pulsars, stars more complex! ...
Search for Gamma Rays from. LKP Dark Matter in the. UED framework ... correlative observations of transient events. Orbit. 565 km, circular. periode ~95 mns ...
Measuring Molecular masses in the Milky Way Johann Cohen-Tanugi GLAST Lunch Talk 07/06/06 What are molecular clouds? T~10-50K range, density103cm-3 ~50% of the mass ...
... spectrum of galactic cosmic ray sources: problem for theory ... Diffusion model with reacceleration is bearably compatible with data on cosmic ray anisotropy. ...
Defined to have 2 outbursts, not periodic. Outbursts according to Atoyan & Aharonian (astro-ph ... L49) found this source in outburst for ~2 weeks in EGRET ...
... flare, moon, EGRET Unids ... It is clear that the moon is something that we are going to have ... the details of the impacts of choices made at the ...
For these and other benchmark scenarios, boost factors needed to fit HEAT data ... Center) visible signal in cuspy profile scenarios or other boost factors. ...