Dark matter and background light

@article{Overduin2004DarkMA,
  title={Dark matter and background light},
  author={James Overduin and Paul S. Wesson},
  journal={Physics Reports},
  year={2004},
  volume={402},
  pages={267-406}
}
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We study the prospects for detecting gamma-rays from decaying dark matter (DM), focusing in particular on gravitino DM in R-parity breaking vacua. Given the substantially different angular
Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: II. Numerical results
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Gravitational, lensing and stability properties of Bose-Einstein condensate dark matter halos
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References

SHOWING 1-10 OF 840 REFERENCES
Background Radiation Constraints on Supersymmetric Weakly Interacting Particles
Dark matter particles that annihilate each other or decay with long lifetimes can be constrained by data in various wavebands. Here we apply this method to supersymmetric weakly interacting massive
Detection of Leptonic Dark Matter
Weakly interacting massive particles (WIMPs) are among the favored candidates for cold dark matter in the universe. The phenomenology of supersymmetric WIMPs has been quite developed during recent
New Light on Dark Matter
TLDR
How studies of the density, demography, history, and environment of smaller-scale structures may distinguish among these possibilities and shed new light on the nature of dark matter is discussed.
Cosmic microwave background constraints on a baryonic dark matter-dominated universe
In recent years, upper limits on the cosmic microwave background (CMB) anisotropies, combined with predictions made by theories of galaxy formation, have been extremely powerful in ruling out purely
Detectability of γ-rays from clumps of dark matter
IF the dark matter in our Galaxy is made up of weakly interacting massive particles (WIMPs) with masses of the order of several GeV (for example, photinos or Higgsinos), γ-rays produced by their
Constraints on decaying neutrinos from the far-ultraviolet extragalactic background light
We consider light neutrinos as dark matter candidates, concentrating on those proposed by Sciama, with rest energies near 30 eV and decay lifetimes of (2 +/- 1) x 10 exp 23 s. Using equations
Dark matter annihilation in the halo of the Milky Way
If the dark matter in the Universe is made of weakly self-interacting particles, they may self-annihilate and emit γ-rays. We use high-resolution numerical simulations to estimate directly the
Problems of modern cosmology: how dominant is the vacuum?
TLDR
The review of evidence for and against the mysterious dark matter consists of as many as four separate ingredients: baryons, massive neutrinos, new "exotic" dark matter particles, and vacuum energy concludes by exploring the possibility that the energy density of the vacuum is in fact so dominant as to leave little room for significant amounts of exotic dark matter.
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