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  • Access by Xinjiang University

Comment on ‘‘Calculating the weak scale in supergravity models’’

M. Drees

  • Physics Department, University of Wisconsin, Madison, Wisconsin 53706

Phys. Rev. D 38, 718 – Published 15 July, 1988

DOI: https://doi.org/10.1103/PhysRevD.38.718

Abstract

Kappen’s ‘‘Λ-space’’ approach to radiative symmetry breaking in supergravity models is discussed. It is shown that this approach does not sum the leading-logarithmic radiative corrections. It is also pointed out that the threshold effects in the conventional renormalization-group (RG) approach are much smaller than apprehended by Kappen. It is finally argued that the threshold effects at the ultrahigh scale cannot be determined in the ‘‘Λ-space’’ approach, and that this definition of scalar masses contains the same ambiguities as the RG approach.

Comments & Replies

Original Article

Calculating the weak scale in supergravity models

H. J. Kappen
Phys. Rev. D 35, 3923 (1987)

References (8)

  1. H. J. Kappen, Phys. Rev. D 35, 3923 (1987).
  2. For reviews see H. P. Nilles, Phys. Rep. 110, 1 (1984); J. Ellis, Reports Nos. CERN-TH 4255, 1985 and CERN-TH 4474, 1986 (unpublished).
  3. For a review of this ``no-scale'' ansatz, see A. B. Lahanas and D. V. Nanopoulos, Phys. Rep. 145, 1 (1987).
  4. See, e.g., L. E. Ibañez, D. Lopez and C. Muñoz, Nucl. Phys. B256, 218 (1985).
  5. H. P. Nilles and M. Nusbaumer, Phys. Lett. 145B, 73 (1984); M. Drees, M. Glück and K. Grassie, ibid. 159B, 118 (1985); P. Majumdar and P. Roy, Phys. Rev. D 33, 2674 (1986); E. Reya, ibid. 33, 773 (1986); M. Drees, ibid. 35, 2910 (1987).
  6. P. Moxhay and K. Yamamoto, Nucl. Phys. B256, 130 (1985).
  7. S. Coleman and E. Weinberg, Phys. Rev. D 7, 1888 (1973).
  8. J. P. Derendinger and C. A. Savoy, Nucl. Phys. B237, 307 (1984).

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