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3
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0038161376
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edited by P. Roy and V. Singh (Springer, Heidelberg
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Pran Nath, Richard Arnowitt, and A. H. Chamseddine, in Supersymmetry, Supergravity and Perturbative QCD, edited by P. Roy and V. Singh (Springer, Heidelberg, 1984).
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Nath, P.1
Arnowitt, R.2
Chamseddine, A.H.3
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13
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85035200584
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P. N. Pandita (in preparation)
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P. N. Pandita (in preparation).
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16
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85035194514
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Assuming CP invariance, the neutralino mass matrix is a real symmetric matrix
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Assuming CP invariance, the neutralino mass matrix is a real symmetric matrix.
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19
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0003491424
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edited by G. L. Kane (World Scientific, Singapore
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H. E. Haber, in Perspectives on Higgs Physics, edited by G. L. Kane (World Scientific, Singapore, 1992).
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(1992)
Perspectives on Higgs Physics
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Haber, H.E.1
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21
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85035213759
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We do not consider more exotic Higgs representations which give lower values of the upper bound on the lightest Higgs boson mass in such theories
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We do not consider more exotic Higgs representations which give lower values of the upper bound on the lightest Higgs boson mass in such theories.
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29
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0010796945
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Particles and Fields
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Sao Paulo, Brazil, edited by O. Eboli and V. Rivelles (World Scientific, Singapore, 1994)
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R. Arnowitt and Pran Nath, in Particles and Fields, Proceedings of the 7th Jorge Swieca Summer School, Sao Paulo, Brazil, 1993, edited by O. Eboli and V. Rivelles (World Scientific, Singapore, 1994).
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Proceedings of the 7th Jorge Swieca Summer School
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Arnowitt, R.1
Nath, P.2
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30
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0042912432
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Gauge coupling unification can be achieved even when d, t0, t > 0 by adding colored multiplets or introducing an intermediate scale in the theory
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Gauge coupling unification can be achieved even when d, t0, t > 0 by adding colored multiplets or introducing an intermediate scale in the theory. U. Amaldi, et al., Phys. Lett. B 281, 374 (1992);
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Phys. Lett. B
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Amaldi, U.1
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31
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85035217952
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Grand Unified Theories and Supersymmetry in Particle Physics and Cosmology
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IEKP KA/94 01, (unpublished). We note that the fine tuning involved to maintain gauge coupling unification in such models is much less objectionable as compared to the fine tuning involved in Eq. (14). Since in this case the bounds (16) and (17) depend on the unknown triplet vacuum expectation values y2, they are not calculable in terms of gluino mass only. We, therefore, consider the simplest choice (19) in this paper
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W. de Boer, “Grand Unified Theories and Supersymmetry in Particle Physics and Cosmology, " Institution Report No. IEKP KA/94 01, 1994 (unpublished). We note that the fine tuning involved to maintain gauge coupling unification in such models is much less objectionable as compared to the fine tuning involved in Eq. (14). Since in this case the bounds (16) and (17) depend on the unknown triplet vacuum expectation values y2, they are not calculable in terms of gluino mass only. We, therefore, consider the simplest choice (19) in this paper.
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(1994)
Institution Report No
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De Boer, W.1
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32
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0001306599
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K. Inoue, A. Kakuto, H. Komatsu and S. Takeshita, Prog. Teor. Phys. 68, 927 (1982);
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Inoue, K.1
Kakuto, A.2
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Takeshita, S.4
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33
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0000056673
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K. Inoue, A. Kakuto, H. Komatsu and S. Takeshita, Prog. Teor. Phys. 71, 413 (1984).
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Inoue, K.1
Kakuto, A.2
Komatsu, H.3
Takeshita, S.4
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34
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85035194819
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Two loop corrections to (23) are numerically small, see Refs. Ref. 22 Ref. 23
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Two loop corrections to (23) are numerically small, see Refs. Ref. 22 Ref. 23.
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40
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0003116746
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The grand unified theory (GUT) relation (23) is actually applicable more generally. For one such derivation, see
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The grand unified theory (GUT) relation (23) is actually applicable more generally. For one such derivation, see, Y. Kawamura, H. Murayama and M. Yamaguchi, Phys. Lett. B 324, 52 (1994).
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(1994)
Phys. Lett. B
, vol.324
, pp. 52
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Kawamura, Y.1
Murayama, H.2
Yamaguchi, M.3
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43
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85035229157
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The LEP Collaborations, Phys. Lett. B 270, 247 (1992).
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Phys. Lett. B
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47
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85035215264
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The input gluino mass used here will be radiatively corrected physical mass of the gluino
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The input gluino mass used here will be radiatively corrected physical mass of the gluino.
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