Bounds on Very Weakly Interacting Sub-eV Particles (WISPs) from Cosmology and Astrophysics
arXiv:0810.3200
Abstract
Many weakly interacting sub-electronVolt particles (WISPs) are easily accommodated in extensions of the standard model. Generally the strongest bounds on their existence come from stellar evolution and cosmology, where to the best of our knowledge observations seem to agree with the standard budget of particles. In this talk I review the most demanding constraints for axions and axion-like-particles, hidden photons and mini-charged particles.
6 pages, 4 figures. To appear in the proceedings of 4th Patras Workshop on Axions, WIMPs and WISPs - Training Workshop, Hamburg, Germany, 18-21 Jun 2008
References in corpus (6)
- Helioscope Bounds on Hidden Sector Photons
- Probing Hidden Sector Photons through the Higgs Window
- Probing the Effective Number of Neutrino Species with Cosmic Microwave Background
- Can the PVLAS particle be compatible with the astrophysical bounds?
- The Physics Case for Axions, WIMPs, WISPs and Other Weird Stuff
- WISP hunting - some new experimental ideas