000172619 001__ 172619
000172619 005__ 20180913061021.0
000172619 0247_ $$2doi$$a10.1016/j.physletb.2010.04.025
000172619 02470 $$2ISI$$a000278242600015
000172619 037__ $$aARTICLE
000172619 245__ $$aCDMS stands for Constrained Dark Matter Singlet
000172619 260__ $$c2010
000172619 269__ $$a2010
000172619 336__ $$aJournal Articles
000172619 520__ $$aMotivated by the two candidate Dark Matter events observed by the CDMS experiment, we consider a Constrained Dark Matter Singlet (CDMS) model that, with no free parameters, predicts the DM mass and the DM direct cross section to be in the range weakly favored by CDMS. (c) 2010 Elsevier B.V. All rights reserved.
000172619 6531_ $$aDark Matter
000172619 6531_ $$aCdms
000172619 6531_ $$aWIMP searches
000172619 700__ $$aFarina, Marco$$uScuola Normale Super Pisa, Pisa, Italy
000172619 700__ $$0244446$$aPappadopulo, Duccio$$g190218$$uEcole Polytech Fed Lausanne, ITPP, CH-1015 Lausanne, Switzerland
000172619 700__ $$aStrumia, Alessandro$$uIst Nazl Fis Nucl, Pisa, Italy
000172619 773__ $$j688$$q329-331$$tPhysics Letters B
000172619 909C0 $$0252443$$pITP$$xU10181
000172619 909CO $$ooai:infoscience.tind.io:172619$$particle
000172619 937__ $$aEPFL-ARTICLE-172619
000172619 973__ $$aEPFL$$rREVIEWED$$sPUBLISHED
000172619 980__ $$aARTICLE