Phenomenological Introduction to Direct Dark Matter Detection
P. Gondolo. (1996)cite arxiv:hep-ph/9605290Comment: 9 pages. uses epsf, rotate. 4 embedded postscript figures. Invited talk at the XXXI Rencontres de Moriond, "Dark Matter in Cosmology, Quantum Measurements, Experimental Gravitation," Les Arcs, France, January 1996.
Abstract
The dark matter of our galactic halo may be constituted by elementary
particles that interact weakly with ordinary matter (WIMPs). In spite of the
very low counting rates expected for these dark matter particles to scatter off
nuclei in a laboratory detector, such direct WIMP searches are possible and are
experimentally carried out at present. An introduction to the theoretical
ingredients entering the counting rates predictions, together with a short
discussion of the major theoretical uncertainties, is here presented.
Description
Phenomenological Introduction to Direct Dark Matter Detection
cite arxiv:hep-ph/9605290Comment: 9 pages. uses epsf, rotate. 4 embedded postscript figures. Invited talk at the XXXI Rencontres de Moriond, "Dark Matter in Cosmology, Quantum Measurements, Experimental Gravitation," Les Arcs, France, January 1996
%0 Generic
%1 gondolo1996phenomenological
%A Gondolo, Paolo
%D 1996
%K dark direct matter phenomenological
%T Phenomenological Introduction to Direct Dark Matter Detection
%U http://arxiv.org/abs/hep-ph/9605290
%X The dark matter of our galactic halo may be constituted by elementary
particles that interact weakly with ordinary matter (WIMPs). In spite of the
very low counting rates expected for these dark matter particles to scatter off
nuclei in a laboratory detector, such direct WIMP searches are possible and are
experimentally carried out at present. An introduction to the theoretical
ingredients entering the counting rates predictions, together with a short
discussion of the major theoretical uncertainties, is here presented.
@misc{gondolo1996phenomenological,
abstract = {The dark matter of our galactic halo may be constituted by elementary
particles that interact weakly with ordinary matter (WIMPs). In spite of the
very low counting rates expected for these dark matter particles to scatter off
nuclei in a laboratory detector, such direct WIMP searches are possible and are
experimentally carried out at present. An introduction to the theoretical
ingredients entering the counting rates predictions, together with a short
discussion of the major theoretical uncertainties, is here presented.},
added-at = {2012-11-21T14:29:12.000+0100},
author = {Gondolo, Paolo},
biburl = {https://www.bibsonomy.org/bibtex/214cf8743018a4272ab15d596c34ca34a/crokoking},
description = {Phenomenological Introduction to Direct Dark Matter Detection},
interhash = {d41fe1f522d4fa013050c28b2c8636cb},
intrahash = {14cf8743018a4272ab15d596c34ca34a},
keywords = {dark direct matter phenomenological},
note = {cite arxiv:hep-ph/9605290Comment: 9 pages. uses epsf, rotate. 4 embedded postscript figures. Invited talk at the XXXI Rencontres de Moriond, "Dark Matter in Cosmology, Quantum Measurements, Experimental Gravitation," Les Arcs, France, January 1996},
timestamp = {2012-11-21T14:29:12.000+0100},
title = {Phenomenological Introduction to Direct Dark Matter Detection},
url = {http://arxiv.org/abs/hep-ph/9605290},
year = 1996
}