The Contribution Of Inverse Compton Scattering To The Diffuse Extragalactic Gamma-Ray Background From Annihilating Dark Matter
arXiv:0906.2251 · doi:10.1103/PhysRevD.81.043505
Abstract
In addition to gamma-rays, dark matter annihilation products can include energetic electrons which inverse Compton scatter with the cosmic microwave background to produce a diffuse extragalactic background of gamma-rays and X-rays. In models in which the dark matter particles annihilate primarily to electrons or muons, the measurements of EGRET and COMPTEL can provide significant constraints on the annihilation cross section. The Fermi Gamma-Ray Space Telescope will likely provide an even more stringent test of such scenarios.
7 pages, 3 figures
References in corpus (18)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- A Theory of Dark Matter
- Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
- A new measurement of the antiproton-to-proton flux ratio up to 100 GeV in the cosmic radiation
- Multi-Component Dark Matter
- Dark matter interpretation of recent electron and positron data
- Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
- Dark matter annihilation or unresolved astrophysical sources? Anisotropy probe of the origin of cosmic gamma-ray background
- Statistics of Cosmological Black Hole Jet Sources: Blazar Predictions for GLAST
- Extragalactic Inverse Compton Light from Dark Matter Annihilation and the Pamela Positron Excess
- How Dark Matter Reionized The Universe
- Angular Signatures of Annihilating Dark Matter in the Cosmic Gamma-Ray Background
- Extended MSSM Neutralinos as the Source of the PAMELA Positron Excess
- Angular Signatures of Dark Matter in the Diffuse Gamma Ray Background
- Dark matter annihilation from intermediate-mass black holes: Contribution to the extragalactic gamma-ray background
- Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
- Cosmic Ray Positrons from Annihilations into a New, Heavy Lepton
- Protohalo Constraints to the Resonant Annihilation of Dark Matter
Cited by in corpus (37)
- Exploring Portals to a Hidden Sector Through Fixed Targets
- A review of indirect searches for particle dark matter
- The Fermi Haze: A Gamma-Ray Counterpart to the Microwave Haze
- Diffuse gamma ray constraints on annihilating or decaying Dark Matter after Fermi
- Constraints on Cosmological Dark Matter Annihilation from the Fermi-LAT Isotropic Diffuse Gamma-Ray Measurement
- Implications of High-Resolution Simulations on Indirect Dark Matter Searches
- Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
- The nature of the Diffuse Gamma-Ray Background
- Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays
- Nonabelian dark matter: models and constraints
- Constraints on Decaying Dark Matter from the Isotropic Gamma-Ray Background
- Consistent Scenarios for Cosmic-Ray Excesses from Sommerfeld-Enhanced Dark Matter Annihilation
- Effects of Dark Matter Annihilation on the Cosmic Microwave Background
- Circum-Galactic Gas and the Isotropic Gamma Ray Background
- Cosmological constraints on dark matter models with velocity-dependent annihilation cross section
- CLUMPY v3: -ray and signals from dark matter at all scales
- Extragalactic gamma-ray background radiation from dark matter annihilation
- Enhancement of the annihilation of dark matter in a radiative seesaw model
- Can multistate dark matter annihilation explain the high-energy cosmic ray lepton anomalies?
- Impact of Primordial Ultracompact Minihaloes on the Intergalactic Medium and First Structure Formation
- Annihilation vs. Decay: Constraining dark matter properties from a gamma-ray detection
- The cosmic X-ray and gamma-ray background from dark matter annihilation
- The Isotropic Radio Background and Annihilating Dark Matter
- Decaying into the Hidden Sector
- Gamma-ray Constraints on Hadronic and Leptonic Activities of Decaying Dark Matter
- Discriminating the source of high-energy positrons with AMS-02
- The Morphology of the Galactic Dark Matter Synchrotron Emission with Self-Consistent Cosmic Ray Diffusion Models
- Gamma-ray signatures of annihilation to charged leptons in dark matter substructure
- Diffuse Gamma Ray Background from Annihilating Dark Matter in Density Spikes around Supermassive Black Holes
- Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
- Positrons in Cosmic Rays from Dark Matter Annihilations for Uplifted Higgs Regions in MSSM
- MiXDM: Cosmic Ray Signals from Multiple States of Dark Matter
- Galactic Positron Excess from Selectively Enhanced Dark Matter Annihilation
- Dependence of accessible dark matter annihilation cross-sections on the density profiles of dwarf spheroidal galaxies with the Cherenkov Telescope Array
- Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
- A New Method to Study the Origin of the EGB and the First Application on AT20G
- A New Approach to Searching for Dark Matter Signals in Fermi-LAT Gamma Rays