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edited by, R. Donaldson, M. Gilchriese, World Scientific, Singapore
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Baer, H.1
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44
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84927904623
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As discussed by Haber and Wyler [29], the radiative decays of the neutralino are not very important unless either both neutralinos are Higgsinolike, or (in the case of light neutralinos) one is a light photino and the other a Higgsino.
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45
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84927904622
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ISAJET_, F. Paige and S. Protopopescu, in Supercollider Physics, Proceedings of the Topical Conference, Eugene, Oregon, 1985, edited by D. Soper (World Scientific, Singapore, 1986), p. 41.
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B. Bambah et al., in Z Physics at LEP 1, Proceedings of the Workshop, Geneva, Switzerland, 1989, edited by G. Altarelli, R. Kleiss, and C. Verzegnassi (CERN Yellow Report No. 89-08, Geneva, 1989), Vol. 3, p. 143.
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51
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84927904620
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A 20000 event run of SUSYSM_ on a Vax 3100 M76 takes about 10 h of CPU time.
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56
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84927904619
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Because of a programming error, the E cslT cross sections shown in Fig. 9 of Ref. [19] were too small by a factor of about 3.
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71
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84927904618
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We are grateful to R. Vega for providing us the cross sections for inclusive l+l+ production that we use to obtain the entries in Tables III and IV for backgrounds from W+-W+- production.
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