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We discuss the possible existence of features in both the primordial power spectrum and bispectrum generated during a stage of single field cosmic inflation. We argue that there are two main classes of features: those produced by a sudden…

高能物理 - 理论 · 物理学 2015-06-23 Gonzalo A. Palma

If time-dependent disruptions from slow-roll occur during inflation, the correlation functions of the primordial curvature perturbation should have scale-dependent features, a case which is marginally supported from the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2018-06-04 Jinn-Ouk Gong , Gonzalo A. Palma , Spyros Sypsas

We describe models of single-field inflation with small and sharp step features in the potential (and sound speed) of the inflaton field, in the context of the Effective Field Theory of Inflation. This approach allows us to study the…

宇宙学与河外天体物理 · 物理学 2015-06-16 Nicola Bartolo , Dario Cannone , Sabino Matarrese

We investigate the generation of features at large scales in the primordial power spectrum (PPS) when inflation is driven by two scalar fields. In canonical single field models of inflation, these features are often generated due to…

宇宙学与河外天体物理 · 物理学 2020-08-19 Matteo Braglia , Dhiraj Kumar Hazra , L. Sriramkumar , Fabio Finelli

We discuss new consistency relations for single field models of inflation capable of generating primordial black holes (PBH), and their observational implications for CMB $\mu$-space distortions. These inflationary models include a short…

宇宙学与河外天体物理 · 物理学 2022-02-09 Ogan Özsoy , Gianmassimo Tasinato

Heavy fields coupled to the inflaton reduce the speed of sound in the effective theory of the adiabatic mode each time the background inflationary trajectory deviates from a geodesic. This can result in features in the primordial spectra.…

宇宙学与河外天体物理 · 物理学 2013-06-12 Ana Achúcarro , Jinn-Ouk Gong , Gonzalo A. Palma , Subodh P. Patil

If cosmic inflation suffered tiny time-dependent deviations from the slow-roll regime, these would induce the existence of small scale-dependent features imprinted in the primordial spectra, with their shapes and sizes revealing information…

宇宙学与河外天体物理 · 物理学 2016-09-21 Sander Mooij , Gonzalo A. Palma , Grigoris Panotopoulos , Alex Soto

We study single-field inflationary models with steep step-like features in the potential that lead to the temporary violation of the slow-roll conditions during the evolution of the inflaton. These features enhance the power spectrum of the…

宇宙学与河外天体物理 · 物理学 2022-02-18 I. Dalianis , G. P. Kodaxis , I. D. Stamou , N. Tetradis , A. Tsigkas-Kouvelis

We employ the formalism of the effective field theory of inflation to study the effects of a sudden change in the speed of sound of the inflationary perturbations. Such an event generates a feature with high frequency oscillations both in…

宇宙学与河外天体物理 · 物理学 2013-05-30 Minjoon Park , Lorenzo Sorbo

We study the effects of a general type of features of the inflaton potential on the spectrum and bispectrum of primordial curvature perturbations. These features correspond to a discontinuity in the $n$-th order derivative of the potential…

宇宙学与河外天体物理 · 物理学 2015-08-25 Alexander Gallego Cadavid

We investigate the features generated by a sharp turn along the inflationary trajectory in a two-field model of Dirac-Born-Infeld inflation, where one of the fields is heavy. Distinct features are generated by two different effects: the…

高能物理 - 理论 · 物理学 2015-06-19 Shuntaro Mizuno , Ryo Saito , David Langlois

We extend our previous work on the enhancement of the curvature spectrum during inflation to the two-field case. We identify the slow-roll parameter $\eta$ as the quantity that can trigger the rapid growth of perturbations. Its two…

宇宙学与河外天体物理 · 物理学 2022-09-07 K. Boutivas , I. Dalianis , G. P. Kodaxis , N. Tetradis

We study the degeneracy of the primordial spectrum and bispectrum of the curvature perturbation in single field inflationary models with a class of features in the inflaton potential. The feature we consider is a discontinuous change in the…

宇宙学与河外天体物理 · 物理学 2018-06-07 Alexander Gallego Cadavid , Antonio Enea Romano , Misao Sasaki

We explore the correlations between correlation functions of the primordial curvature perturbation produced during inflation. We find that for general single field inflation, other than the source terms which depend on the model details,…

宇宙学与河外天体物理 · 物理学 2014-04-02 Jinn-Ouk Gong , Koenraad Schalm , Gary Shiu

Cosmological perturbations, originating in the quantum fluctuations of the fields that drive inflation, are observed to be nearly scale invariant at the largest scales. At smaller scales, however, perturbations are not severely constrained…

宇宙学与河外天体物理 · 物理学 2024-07-09 Ioannis Dalianis

Sudden violations of the slow-roll regime during inflation, a natural prediction of many UV-complete inflationary models, give rise to sharp features in the primordial power spectrum. At large scales, these features provide a unique window…

宇宙学与河外天体物理 · 物理学 2025-02-05 Clément Stahl , Denis Werth , Vivian Poulin

We numerically investigate density perturbations generated in the smooth hybrid new inflation model, a kind of double inflation model that is designed to reproduce the running spectral index suggested by the WMAP results. We confirm that…

高能物理 - 唯象学 · 物理学 2008-11-26 Masahiro Kawasaki , Tsutomu Takayama , Masahide Yamaguchi , Jun'ichi Yokoyama

We prove an exact relation between the tensor and the scalar primordial power spectra generated during inflation. Such a mapping considerably simplifies the derivation of any power spectra as they can be obtained from the study of the…

宇宙学与河外天体物理 · 物理学 2013-09-04 Jose Beltran Jimenez , Marcello Musso , Christophe Ringeval

We derive a direct correlation between the power spectrum and bispectrum of the primordial curvature perturbation in terms of the Goldstone mode based on the effective field theory approach to inflation. We show examples of correlated…

宇宙学与河外天体物理 · 物理学 2017-04-19 Jinn-Ouk Gong , Masahide Yamaguchi

The possibility that primordial black holes constitute a fraction of dark matter motivates a detailed study of possible mechanisms for their production. Black holes can form by the collapse of primordial curvature fluctuations, if the…

宇宙学与河外天体物理 · 物理学 2020-05-06 Ogan Özsoy , Gianmassimo Tasinato
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