id	author	title	date	pages	extension	mime	words	sentences	flesch	summary	cache	txt
work_o3qyijc6jnarxa5gd6i57be3qa	Kingman Cheung	Collider phenomenology of light strange-beauty squarks	2004	23	.pdf	application/pdf	7818	1363	90	study direct strange-beauty squark-pair production, as well as the feed down from gluinopair production and the associated production of s̃b1 with a gluino. However, for squark mass above 300 GeV, the feed down from gluino-pair We have set the generic SUSY scale at TeV, except for the gluino and the light strangebeauty squark s̃b1, which could be as light as 500 and 200 GeV, respectively. We employ a tree-level calculation for gluino-pair production, though including the nextto-leading order (NLO) corrections [9] the cross section may increase by more than 50%. Gluino-pair production cross sections at the Tevatron are given in Fig. 3(b). gluino mass of 500 GeV the cross section is only a few fb, and thus this contribution becomes TABLE I: Cross sections for direct strange-beauty squark pair production at the Tevatron, with However, as the squark mass is above 300 GeV, the feed down from gluino-pair production	./cache/work_o3qyijc6jnarxa5gd6i57be3qa.pdf	./txt/work_o3qyijc6jnarxa5gd6i57be3qa.txt