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We calculate the spectral index and tensor-to-scalar ratio for patch inflation arisen from the Gauss-Bonnet braneworld scenario. The patch cosmological models consist of Gauss-Bonnet (GB), Randall-Sundrum (RS), and 4D general relativistic…

天体物理学 · 物理学 2010-04-05 Hungsoo Kim , Kyong Hee Kim , Hyung Won Lee , Yun Soo Myung

Single field inflationary models that seek to greatly enhance small scale power in order to form primordial black holes predict both a squeezed bispectrum that is enhanced by this small scale power and a potentially detectable enhancement…

宇宙学与河外天体物理 · 物理学 2022-06-08 David Zegeye , Keisuke Inomata , Wayne Hu

Enormous information about interactions is contained in the non-Gaussianities of the primordial curvature perturbations, which are essential to break the degeneracy of inflationary models. We study the primordial bispectra for G-inflation…

宇宙学与河外天体物理 · 物理学 2021-04-21 Fengge Zhang , Yungui Gong , Jiong Lin , Yizhou Lu , Zhu Yi

We provide a detailed quantitative description of singular inflation. Its close analogy with finite-time future singularity which is associated to dark energy era is described. Calling and classifying the singularities of such inflation as…

广义相对论与量子宇宙学 · 物理学 2015-05-27 S. Nojiri , S. D. Odintsov , V. K. Oikonomou

In this work we shall calculate in detail the effect of an GW170817-compatible Einstein-Gauss-Bonnet theory on the energy spectrum of the primordial gravitational waves. The spectrum is affected by two characteristics, the overall…

广义相对论与量子宇宙学 · 物理学 2022-04-27 V. K. Oikonomou

In single-field inflation, violation of the slow-roll approximation can lead to growth of curvature perturbation outside the horizon. This violation is characterized by a period with a large negative value of the second slow-roll parameter.…

宇宙学与河外天体物理 · 物理学 2024-10-11 Jason Kristiano , Jun'ichi Yokoyama

Power spectra play an important role in the theory of inflation, and their ability to reproduce current observational data to high accuracy is often considered a triumph of inflation, largely because of a lack of credible alternatives. In…

宇宙学与河外天体物理 · 物理学 2020-05-21 Herbert W. Hamber , Lu Heng Sunny Yu , Hasitha E. Pituwala Kankanamge

The primordial spectrum of fluctuations may present a large peak as a result of enhancing features during inflation. This may include, but is not limited to, bumps in the inflaton's potential, phases of ultra-slow-roll or turns in…

宇宙学与河外天体物理 · 物理学 2022-09-30 Shyam Balaji , Guillem Domenech , Joseph Silk

In this work, we examine cosmological constraints on models of composite inflation based on the slow-roll approximation by using the recent Planck measurement. We compare the spectral index of curvature perturbation (and its running) and…

高能物理 - 唯象学 · 物理学 2016-06-30 Phongpichit Channuie

Motivated by the idea that inflation occurs at the GUT symmetry breaking scale, in this paper we construct a new class of large field inflaton potentials where the inflaton starts with a power law potential; after initial period of relative…

宇宙学与河外天体物理 · 物理学 2014-09-24 Dhiraj Kumar Hazra , Arman Shafieloo , George F. Smoot , Alexei A. Starobinsky

We investigate the cosmological inflation for the Einstein-Hilbert action plus the Higgs potential function and the Gauss-Bonnet term coupled with the Higgs scalar field through a dilaton-like coupling. Then, using the…

广义相对论与量子宇宙学 · 物理学 2026-05-29 Zahra Ahghari , Mehrdad Farhoudi

The leading candidate for the very early universe is described by a period of rapid expansion known as inflation. While the standard paradigm invokes a single slow-rolling field, many different models may be constructed which fit the…

宇宙学与河外天体物理 · 物理学 2011-12-30 D. M. Regan

Calculating the primordial bispectrum predicted by a model of inflation and comparing it to what we see in the sky is very computationally intensive, necessitating layers of approximations and limiting the models which can be constrained.…

宇宙学与河外天体物理 · 物理学 2021-08-11 Philip Clarke , E. P. S. Shellard

We study multifield contributions to the scalar power spectrum in an ensemble of six-field inflationary models obtained in string theory. We identify examples in which inflation occurs by chance, near an approximate inflection point, and we…

宇宙学与河外天体物理 · 物理学 2015-06-05 Liam McAllister , Sébastien Renaux-Petel , Gang Xu

We derive general analytic formulae for the power spectrum and spectral index of the curvature perturbation produced during inflation driven by a multi-component inflaton field, up to the second order in the slow-roll approximation. We do…

天体物理学 · 物理学 2009-10-28 Takahiro T. Nakamura , Ewan D. Stewart

In single-field inflationary models with a low sound speed, the orthogonal shape of the primordial bispectrum arises due to partial cancellations between equilateral-type shapes. This fact allows for a speed of sound c_s as low as about…

宇宙学与河外天体物理 · 物理学 2015-06-15 Sebastien Renaux-Petel

We have explicitly demonstrated that scalar coupled Gauss-Bonnet gravity in four dimension can have non-trivial effects on the early inflationary stage of our universe. In particular, we have shown that the scalar coupled Gauss-Bonnet term…

广义相对论与量子宇宙学 · 物理学 2018-11-13 Sumanta Chakraborty , Tanmoy Paul , Soumitra SenGupta

We extend the work of Contaldi et al. and derive analytical approximations for primordial power spectra arising from models of inflation which include primordial spatial curvature. These analytical templates are independent of any specific…

宇宙学与河外天体物理 · 物理学 2022-05-25 Ayngaran Thavanesan , Denis Werth , Will Handley

In low-energy effective string theory and modified gravity theories, the propagating speed $c_T$ of primordial gravitational waves may deviate from unity. We find that the step-like variation of $c_T$ during slow-roll inflation may result…

宇宙学与河外天体物理 · 物理学 2015-05-20 Yong Cai , Yu-Tong Wang , Yun-Song Piao

In light of the recent Planck 2015 results for the measurement of the CMB anisotropy, we study simple inflationary models in the context of the Gauss-Bonnet brane-world cosmology. The brane-world cosmological effect modifies the power…

高能物理 - 唯象学 · 物理学 2017-03-15 Nobuchika Okada , Satomi Okada
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