activity
20012007
most citedDark matter burners

76 citations · 154 across the 8 of their papers we have counts for

collaborators
Showing astro-phShow all

10 papers · 1 filter

astro-ph2007

Novel technique for monitoring the performance of the LAT instrument on board the GLAST satellite

D. Paneque, A. Borgland, A. Bovier +7

The Gamma-ray Large Area Space Telescope (GLAST) is an observatory designed to perform gamma-ray astronomy in the energy range 20 MeV to 300 GeV, with supporting measurements for g…

astro-ph20077 cited

Identifying Dark Matter Burners in the Galactic center

Igor V. Moskalenko, Lawrence L. Wai

If the supermassive black hole (SMBH) at the center of our Galaxy grew adiabatically, then a dense "spike" of dark matter is expected to have formed around it. Assuming that dark m…

astro-ph200776 cited

Dark matter burners

Igor V. Moskalenko, Lawrence L. Wai

We show that a star orbiting close enough to an adiabatically grown supermassive black hole (SMBH) can capture weakly interacting massive particles (WIMPs) at an extremely high rat…

astro-ph20071 cited

The search for Milky Way halo substructure WIMP annihilations using the GLAST LAT

Lawrence Wai, GLAST LAT Collaboration

The GLAST LAT Collaboration is one among several experimental groups, covering a wide range of approaches, pursuing the search for the nature of dark matter. The GLAST LAT has the…

astro-ph20071 cited

Dark Matter Searches with GLAST

Lawrence Wai, GLAST LAT Collaboration

Indirect detection of particle dark matter relies upon pair annihilation of Weakly Interaction Massive Particles (WIMPs), which is complementary to the well known techniques of dir…

astro-ph200667 cited

Can Astrophysical Gamma Ray Sources Mimic Dark Matter Annihilation in Galactic Satellites?

Edward A. Baltz, James E. Taylor, Lawrence L. Wai

The nature of the cosmic dark matter is unknown. The most compelling hypothesis is that dark matter consists of weakly interacting massive particles (WIMPs) in the 100 GeV mass ran…