Related Experiment Video
Updated: Jun 22, 2026

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector
R Abbasi1, Y Abdou, M Ackermann
1Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA.
Abstract:
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the weakly interacting massive particle (WIMP) proton cross sections for WIMP masses in the range 250-5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.
Related Concept Videos
Fermi Level Dynamics
Electron affinity in semiconductors refers to the energy gap between the minimum of its conduction band and the vacuum level and it is a critical parameter in determining how easily a semiconductor can accept additional electrons.
The work...
Thomson's e/m Experiment
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The magnetic...
Fermi Level
At absolute zero temperature, electrons fill all energy states up to the Fermi level, leaving upper states empty. As the temperature rises,...
Nuclear Transmutation
Magnetostatic Boundary Conditions
Subatomic Particles
