منابع مشابه
WIMP direct detection overview ∗
This review on weakly interacting massive particle (WIMP) dark matter direct detection focuses on experimental approaches and the corresponding physics basics. The presentation is intended to provide a quick and concise introduction for non-specialists to this fast evolving topic of astroparticle physics.
متن کاملWIMP Dark Matter Direct Detection
D. Bauer, A. Borgland, B. Cabrera, F. Calaprice, J. Cooley, P. Cushman, T. Empl, R. Essig, E. Figueroa-Feliciano, R. Gaitskell, C. Galbiati, S. Golwala, J. Hall, R. Hill, A. Hime, E. Hoppe, L. Hsu, E. Hungerford, R. Jacobsen, M. Kelsey, R. F. Lang, W. H. Lippincott, B. Loer, S. Luitz, V. Mandic, J. Mardon, J. Maricic, R. Maruyama, D. N. McKinsey, R. Mahapatra, H. Nelson, J. Orrell, K. Palladino...
متن کاملWIMP direct detection and halo structure
Weakly Interacting Massive Particle (WIMP) direct detection experiments are just reaching the sensitivity required to detect Galactic dark matter in the form of neutralinos (or indeed any stable weakly interacting particle). Detection strategies and data analyses are often based on the simplifying assumption of a standard spherical, isothermal halo model, but observations and numerical simulati...
متن کاملInterpreting data from WIMP direct detection experiments
Weakly Interacting Massive Particle (WIMP) direct detection experiments are closing in on the region of parameter space where relic neutralinos may constitute the galactic halo dark matter. We discuss two issues in the interpretation of data, in particular the calculation of exclusion limits, from these experiments. Firstly we show that the technique that has been used for calculating exclusion...
متن کاملExperimental Searches for Non - Baryonic Dark Matter : WIMP Direct Detection
Experimental observations and robust theoretical arguments have established that our universe is essentially non-visible, the luminous matter scarcely accounting for one per cent of the energy density of a flat universe. The distribution of a flat universe (Ω = ΩM + ΩΛ = 1) attributes to the dark energy about ΩΛ ∼ 70%, whereas the matter density takes the remaining ΩM ∼ 30%, consisting of, both...
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ژورنال
عنوان ژورنال: Nuclear Physics B - Proceedings Supplements
سال: 2003
ISSN: 0920-5632
DOI: 10.1016/s0920-5632(03)01327-6