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Grand unified inflation confronts WMAP
Author(s) -
Bumseok Kyae,
Qaisar Shafi
Publication year - 2003
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2003/11/036
Subject(s) - cmb cold spot , physics , inflaton , leptogenesis , baryon asymmetry , particle physics , cosmic microwave background , grand unified theory , spectral index , scalar (mathematics) , inflation (cosmology) , higgs boson , minimal supersymmetric standard model , anisotropy , theoretical physics , supersymmetry , quantum mechanics , lepton , spectral line , geometry , mathematics , electron
In a class of realistic four and five dimensional supersymmetric grandunified models, the scalar spectral index is found to be $n_s=0.98 (\pm 0.01)$,in excellent agreement with the values determined by several previousexperiments and most recently by the Wilkinson Microwave Anisotropy Probe(WMAP). The models predict $dn_s/d{\rm ln}k\sim 10^{-3}$ and a negligibletensor-to-scalar ratio $r\sim 10^{-8}$. A new five dimensional supersymmetricSO(10) model along these is presented in which inflation is associated with thebreaking of SO(10) to SU(5) at scale $M$, with $\delta T/T\propto (M/M_{\rmPlanck})^2$, so that $M\simeq 10^{16}$ GeV. The inflaton decay leads to theobserved baryon asymmetry via leptogenesis. We also discuss how the monopoleproblem is solved without the use of non-renormalizable terms.Comment: A new resolution of the monopole problem proposed. 1+9 page

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