Causality Bounds on the Primordial Power Spectrum
Mariana Carrillo Gonz\'alez, Sebasti\'an C\'espedes

TL;DR
This paper investigates how causality constraints in the effective field theory of inflation limit the possible enhancements of the primordial power spectrum, impacting models of primordial black holes and gravitational waves.
Contribution
It derives bounds on the primordial power spectrum from causality and EFT principles, constraining scenarios with varying sound speeds and large spectrum growth.
Findings
Causality enforces luminal sound speeds to imply free theories.
Significant spectrum growth is incompatible with causal EFT constraints.
Constraints limit the parameter space for models producing primordial black holes.
Abstract
Effective field theories (EFTs) parametrize our ignorance of the underlying UV theory through their Wilson coefficients. However, not all values of these coefficients are consistent with fundamental physical principles. In this paper, we explore the consequences of imposing causal propagation on the comoving curvature perturbation in the EFT of inflation, particularly its impact on the primordial power spectrum and the effective sound speed . We investigate scenarios where undergoes a transition, remaining consistent with CMB constraints at early times but later experiencing a drastic change, becoming highly subluminal. Such scenarios allow the primordial power spectrum to grow at small scales, potentially leading to the formation of primordial black holes or the generation of scalar-induced gravitational waves. We find the generic feature that in a…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
