In this work, we consider the dynamics of the self-induced collapse of the tachyon wave function in inflationary scenarios. We analyze the modifications on the power spectrum by considering the β-exponential potential, whose parameters have updated constraints by the Planck 2018 baseline data. Moreover, we show that for this kind of potential, just for a narrow range of β-parameter, there is agreement between the theoretical predictions and the current observational data. Considering the proposal for a collapse scheme that leads to the modification of Schr\"odinger evolution of the inflaton wave function from the employment of a Continuous Spontaneous Localization (CSL) approach, we derive the scalar spectral index and tensor-to-scalar ratio. We then obtained the constraints on both collapse and β-parameters that, in turn, yield deviations in the nₛ vs. r plane when compared to the β-exponential potential standard estimate. The CSL scheme applied to tachyonic inflation driven by a β-potential offers an adequate description of the recent data.
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Brito et al. (2024) studied this question.
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