Approximating the radiatively corrected Higgs mass in the Minimal Supersymmetric Model

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dc.creatorHaber, Howard E.
dc.creatorHempfling, Ralf
dc.creatorHoang, Andre H.
dc.date1996-09-12
dc.date.accessioned2026-07-07T04:00:00Z
dc.date.available2026-07-07T04:00:00Z
dc.descriptionTo obtain the most accurate predictions for the Higgs masses in the minimal supersymmetric model (MSSM), one should compute the full set of one-loop radiative corrections, resum the large logarithms to all orders, and add the dominant two-loop effects. A complete computation following this procedure yields a complex set of formulae which must be analyzed numerically. We discuss a very simple approximation scheme which includes the most important terms from each of the three components mentioned above. We estimate that the Higgs masses computed using our scheme lie within 2 GeV of their theoretically predicted values over a very large fraction of MSSM parameter space.
dc.description31 pages, 10 embedded figures, latex with psfig.sty the complete postscript file of this preprint, including figures, is available via anonymous ftp at ftp://www-ttp.physik.uni-karlsruhe.de/ttp95-09/ttp95-09.ps or via www at http://www-ttp.physik.uni-karlsruhe.de/cgi-bin/preprints/
dc.identifierhttps://arxiv.org/abs/hep-ph/9609331
dc.identifierhttp://arxiv.org/abs/hep-ph/9609331
dc.identifierZ.Phys. C75 (1997) 539-554
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46458
dc.subjectHigh Energy Physics - Phenomenology
dc.titleApproximating the radiatively corrected Higgs mass in the Minimal Supersymmetric Model
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