Dark 2002 and Beyond

Abstract

Salient aspects of the meeting are summarized, including our knowledge of dark matter at different cosmological and astrophysical distance scales, ranging from large-scale structure to the cores of galaxies, and our speculations on particle candidates for dark matter, including neutrinos, neutralinos, axinos, gravitinos and cryptons. Comments are also made on prospects for detecting dark matter particles and on the dark energy problem.

26 pages, 16 figures, Summary of DARK 2002: 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, 4-9 Feb 2002, Cape Town, South Africa

References in corpus (47)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Evidence for oscillation of atmospheric neutrinos
• The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
• DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum
• Precise Measurement of the Positive Muon Anomalous Magnetic Moment
• A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data
• Neutralino Dark Matter in Focus Point Supersymmetry
• Hadronic light-by-light corrections to the muon g-2: the pion-pole contribution
• Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
• Muon anomalous magnetic dipole moment in supersymmetric theories
• Axinos as Dark Matter
• Gravitino Production After Inflation
• Dark Matter Spikes and Annihilation Radiation from the Galactic Center
• Effect of the galactic halo modeling on the DAMA/NaI annual modulation result: an extended analysis of the data for WIMPs with a purely spin-independent coupling
• Supersymmetric Dark Matter and Yukawa Unification
• Supersymmetry and the Anomalous Anomalous Magnetic Moment of the Muon
• Implications of Muon g-2 for Supersymmetry and for Discovering Superpartners Directly
• Towards a refined cosmic concordance model: joint 11-parameter constraints from CMB and large-scale structure
• Interacting Dark Matter disguised as Warm Dark Matter
• Implications of muon anomalous magnetic moment for supersymmetric dark matter
• Impact of Muon Anomalous Magnetic Moment on Supersymmetric Models
• Upper Limits on Sparticle Masses from g-2 and the Possibility for Discovery of Supersymmetry at Colliders and in Dark Matter Searches
• Detection of B_s->mu mu at the Tevatron Run II and Constraints on the SUSY Parameter Space
• Natural Quintessence and Large Extra Dimensions
• First Results of the EDELWEISS WIMP Search using a 320 g Heat-and-Ionization Ge Detector
• Recent Result from E821 Experiment on Muon g-2 and Unconstrained Minimal Supersymemtric Standard Model
• The Inflaton Field as Self-Interacting Dark Matter in the Braneworld Scenario
• How Finely Tuned is Supersymmetric Dark Matter?
• Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
• Comment on the sign of the pseudoscalar pole contribution to the muon g-2
• On the density of Cold Dark Matter
• On the energy and baseline optimization to study effects related to the $\delta$-phase (CP-/T-violation) in neutrino oscillations at a Neutrino Factory
• Constraints on Neutrino Degeneracy from the Cosmic Microwave Background and Primordial Nucleosynthesis
• Constraints from Accelerator Experiments on the Elastic Scattering of CMSSM Dark Matter
• Cosmic Microwave Background anisotropies beyond the third peak
• Cosmology with a long range repulsive force
• A novel concept for a anti nu_e Neutrino Factory
• CMB and Cosmological Parameters: Current Status and Prospects
• ZEPLIN IV: A One Ton Ultimate WIMP Detector
• Theoretical Status of Muon (g-2)
• Combining Supersymmetric Dark Matter with Recent Accelerator Data
• Unified description of dark matter at the center and in the halo of the Galaxy
• Is Cold Dark Matter Still a Strong Buy? The Lesson from Galaxy Clusters
• Does Dark Matter at the Center and in the Halo of the Galaxy Consist of the Same Particles?
• The Directional Rate and the Modulation Effect for Direct Supersymmetric Dark Matter Detection
• Status of the HDMS experiment, the GENIUS project and the GENIUS-TF