Titlebook: Sources and Detection of Dark Matter and Dark Energy in the Universe; Fourth International David B. Cline Conference proceedings 2001 Sprin

ALLEY

dyspareunia

nuclear-tests

Prospects for MAP & PLANCKth an angular resolution more than 30 times better than COBE. PLANCK, an ESA satellite with even better angular resolution and sensitivity, will follow several years after MAP. These satellites will make precise measurements of the baryon to photon ratio and the dark matter to baryon ratio in the ea

anesthesia

烦人

conjunctivitis

BOON

The Second Peak: The Dark-Energy Density and the Cosmic Microwave Background an aside, we show how the measured height of the first peak probably already points toward a low matter density and places upper limits to the reionization optical depth and gravitational-wave amplitude.

思考

危险

The Cosmological Constant from the Viewpoint of String Theoryvanishing or extreme smallness of the vacuum energy, while on the other hand it is very difficult to modify this framework in a sensible way. In seeking to resolve this problem, one naturally wonders if the real world can somehow be interpreted in terms of a vacuum state with unbroken supersymmetry.

GUILT

Latest Cosmological Constraints on the Densities of Hot and Cold Dark Matterotal (cold+hot) dark matter density is ..Ω. = 0.20.. with at most 38% of it being hot (due to neutrinos). A few assumptions, including negligible neutrinos, tighten this measurement to ..Ω. = 0.13.., .., 2.4 × 10.kg/m. give or take 20%.