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Volumn 45, Issue 1, 1992, Pages 142-160

Multilepton signals from supersymmetry at hadron supercolliders

Author keywords

[No Author keywords available]

Indexed keywords


EID: 4243491066     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.45.142     Document Type: Article
Times cited : (98)

References (86)
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    • R. M. Barnett and A. White, in Research Directions for the Decade [19].
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    • V. Fonseca, S. Kahn, M. Murtaugh, and F. Paige, in Research Directions for the Decade [19].
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    • C. Albajar et ~al., in Proceedings of the ECFA Large Hadron Collider Workshop, Aachen, Germany, 1990, edited by G. Jarlskog and D. Rein (CERN Report No. 90-10, Geneva, Switzerland, 1990), Vol. II, p. 621.
  • 44
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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.
  • 45
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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.
  • 51
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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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    • 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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    • 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.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.