Dark Matter as Dense Color Superconductor
arXiv:astro-ph/0204218 · doi:10.1016/S0920-5632(03)02087-5
Abstract
We discuss a novel cold dark matter candidate which is formed from the ordinary quarks during the QCD phase transition when the axion domain wall undergoes an unchecked collapse due to the tension in the wall. If a large number of quarks is trapped inside the bulk of a closed axion domain wall, the collapse stops due to the internal Fermi pressure. In this case the system in the bulk, may reach the critical density when it undergoes a phase transition to a color superconducting phase with the ground state being the quark condensate, similar to BCS theory. If this happens, the new state of matter representing the diquark condensate with a large baryon number B > 10^{20} becomes a stable soliton-like configuration. Consequently, it may serve as a novel cold dark matter candidate.
To appear in the Proceedings "Dark Matter 2002"
References in corpus (2)
Cited by in corpus (11)
- Macro Dark Matter
- Lepton asymmetry and the cosmic QCD transition
- Baryon Asymmetry, Dark Matter and Quantum Chromodynamics
- Cold Dark Matter as Compact Composite Objects
- 511 KeV Photons From Color Superconducting Dark Matter
- Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
- Resonant bar detector constraints on macro dark matter
- Difficulties for Compact Composite Object Dark Matter
- CMB Spectral Distortions from Cooling Macroscopic Dark Matter
- Updated cosmological constraints on Macroscopic Dark Matter
- Primordial constraints on inelastic macro dark matter revisited