Following Chankowski, Ellis and Pokorski we quantify the amount of fine-tuning of input parameters of the Minimal Supersymmetric Standard Model that is needed to respect the lower limits on sparticle and Higgs masses imposed by negative searches so far, direct or indirect. By including the one loop radiative corrections to the effective potential, the amount of fine-tuning is reduced with respect to the results of CEP by a factor of 2 divided by 5, or even larger as tan beta approaches 1. A further reduction factor may come from a more appropriate, less restrictive, definition of the fine-tuning parameter itself. (C) 1998 Elsevier Science B.V. All rights reserved.
About the fine-tuning price of LEP
STRUMIA, ALESSANDRO
1998-01-01
Abstract
Following Chankowski, Ellis and Pokorski we quantify the amount of fine-tuning of input parameters of the Minimal Supersymmetric Standard Model that is needed to respect the lower limits on sparticle and Higgs masses imposed by negative searches so far, direct or indirect. By including the one loop radiative corrections to the effective potential, the amount of fine-tuning is reduced with respect to the results of CEP by a factor of 2 divided by 5, or even larger as tan beta approaches 1. A further reduction factor may come from a more appropriate, less restrictive, definition of the fine-tuning parameter itself. (C) 1998 Elsevier Science B.V. All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
