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Searching for dark matter signatures in the glast lat electron flux
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Moiseev, Alexander Profumo, Stefano |
| Copyright Year | 2008 |
| Description | We explored several viable scenarios of how LAT might observe DM, when the spectral feature is predicted to be observed in the HE electron flux It has been demonstrated elsewhere that LAT will be capable to detect HE electrons flux in energy range from 20 GeV to - 1 TeV with 520% energy resolution and good statistics If there is a DM-caused feature in the HE electron flux (in the range 20 GeV - 1 TeV), LAT will be the best current instrument to observe it! |
| File Size | 346740 |
| Page Count | 13 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20080031736 |
| Archival Resource Key | ark:/13960/t4tj3gs5h |
| Language | English |
| Publisher Date | 2008-02-20 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Sensitivity Dark Matter Energy Spectra Sensory Feedback Spectra Flux Rate High Energy Electrons Signatures Cosmic Rays Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |