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(20 Jan 2013) Key: citeulike:11934765
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In this work we determine the power spectrum of the gravitational potential of the primordial fluctuations for an inflationary model whose inflaton is a non-canonical scalar field of the tachyon-type. The respective background field equations for an inverse-square potential produce a power-law inflation, and it is explicitly shown that for such a potential the power spectrum tends to be scale-independent for highly accelerated regimes in the inflationary expansion.
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