Introduction to Non-Baryonic Dark Matter
arXiv:astro-ph/0403064
Abstract
These lectures on non-baryonic dark matter matter are divided into two parts. In the first part, I discuss the need for non-baryonic dark matter in light of recent results in cosmology, and I present some of the most popular candidates for non-baryonic dark matter. These include neutrinos, axions, neutralinos, WIMPZILLAs, etc. In the second part, I overview several observational techniques that can be employed to search for WIMPs (weakly interacting massive particles) as non-baryonic dark matter. Among these techniques, I discuss the direct detection of WIMP dark matter, and its indirect detection through high-energy neutrinos, gamma-rays, positrons, etc.
Lectures delivered at the NATO Advanced Study Institute "Frontiers of the Universe", 8-20 Sept 2003, Cargese, France; 50 pages, 28 figures
References in corpus (48)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Observational evidence for self-interacting cold dark matter
- A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: I. Morphology of the Sagittarius Core and Tidal Arms
- Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56
- Non-Baryonic Dark Matter - Observational Evidence and Detection Methods
- Stellar Orbits Around the Galactic Center Black Hole
- Dark matter annihilation at the galactic center
- High Proper Motion Stars in the Vicinity of Sgr A*: Evidence for a Supermassive Black Hole at the Center of Our Galaxy
- Neutralino Relic Density including Coannihilations
- Near-infrared flares from accreting gas around the supermassive black hole at the Galactic Centre
- Rapid X-ray flaring from the direction of the supermassive black hole at the Galactic Centre
- The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
- Kaluza-Klein Dark Matter
- The Stellar Cusp Around the Supermassive Black Hole in the Galactic Center
- Neutrinos in cosmology
- Sterile Neutrino Hot, Warm, and Cold Dark Matter
- Superheavy dark matter
- Neutralino Dark Matter in Focus Point Supersymmetry
- The Kinematics, Orbit, and Survival of the Sagittarius Dwarf Spheroidal Galaxy
- Cosmological dark matter annihilations into gamma-rays - a closer look
- Nonthermal Supermassive Dark Matter
- Weakly Self-Interacting Dark Matter and the Structure of Dark Halos
- An Improved RF Cavity Search for Halo Axions
- Improved Exclusion Limits from the EDELWEISS WIMP Search
- A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing
- Dark Matter Spikes and Annihilation Radiation from the Galactic Center
- Sagittarius Tidal Debris 90 kpc from the Galactic Center
- Spectral Gamma-ray Signatures of Cosmological Dark Matter Annihilation
- Sneutrino Cold Dark Matter With Lepton-Number Violation
- Ultra-High Energy Cosmic Rays, Superheavy Long-Living Particles, and Matter Creation after Inflation
- Brane-world dark matter
- The cosmic ray positron excess and neutralino dark matter
- The Effects of the Sagittarius Dwarf Tidal Stream on Dark Matter Detectors
- Detectability of Weakly Interacting Massive Particles in the Sagittarius Dwarf Tidal Stream
- Implications of muon anomalous magnetic moment for supersymmetric dark matter
- Indirect Detection of Dark Matter in km-size Neutrino Telescopes
- Limits on Collisional Dark Matter from Elliptical Galaxies in Clusters
- Recoil momentum spectrum in directional dark matter detectors
- Low Pressure Negative Ion Drift Chamber for Dark Matter Search
- Supersymmetry and the positron excess in cosmic rays
- Signatures of Hierarchical Clustering in Dark Matter Detection Experiments
- Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
- Minimal Theoretical Uncertainties in Inflationary Predictions
- Improved constraints on supersymmetric dark matter from muon g-2
- Indirect detection of a subdominant density component of cold dark matter
- Gamma-Ray Summary Report
- Neutrinos and Dark Matter
- Neutrinos from the Big Bang
Cited by in corpus (4)
- The first WIMPy halos
- Phenomenological constraints on accretion of non-annihilating dark matter on the PSR B1257+12 pulsar from orbital dynamics of its planets
- Is Dark Matter Heavy Because of Electroweak Symmetry Breaking? Revisiting Heavy Neutrinos
- Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales