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We present new constraints on the spectral index nT of tensor fluctuations from the recent data obtained by the BICEP2 experiment. We found that the BICEP2 data alone slightly prefer a positive, ``blue,'' spectral index with nT=1.36±0.83 at 68% C.L. However, when a TT prior on the tensor amplitude coming from temperature anisotropy measurements is assumed, we get nT=1.67±0.53 at 68% C.L., ruling out a scale-invariant nT=0 spectrum at more than three standard deviations. These results are at odds with current bounds on the tensor spectral index coming from pulsar timing, big bang nucleosynthesis, and direct measurements from the LIGO experiment. Considering only the possibility of a ``red'' nT<0 spectral index, we obtain the lower limit nT>-0.76 at 68% C.L. (nT>-0.09 when a TT prior is included).
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Gerbino et al. (2014) studied this question.
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