It is shown that a tensor-to-scalar ratio close to r = 0.03 , which can be observed by Planck , is realized in supersymmetric hybrid inflation models with TeV-scale soft supersymmetry breaking terms .
This extends our previous analysis , which also found r \lesssim 0.03 but employed intermediate scale soft terms .
Other cosmological observables such as the scalar spectral index are in good agreement with the WMAP data .