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We investigate the possibility to induce double peaks of gravitational wave(GW) spectrum from primordial scalar perturbations in inflationary models with three inflection points.Where the inflection points can be generated from a polynomial…

宇宙学与河外天体物理 · 物理学 2021-06-30 Tie-Jun Gao , Xiu-Yi Yang

The gravitational wave (GW) signal offers a promising window into the dynamics of the early universe. The recent results from the pulsar timing arrays (PTAs) could be the first glimpse of such new physics. In particular, they could point to…

宇宙学与河外天体物理 · 物理学 2025-11-13 Haipeng An , Boye Su , Hanwen Tai , Lian-Tao Wang , Chen Yang

We show how observations of the density perturbation (scalar) spectrum and the gravitational wave (tensor) spectrum allow a reconstruction of the potential responsible for cosmological inflation. A complete functional reconstruction or a…

高能物理 - 唯象学 · 物理学 2009-10-22 Edmund J. Copeland , Edward W. Kolb , Andrew R. Liddle , James E. Lidsey

We investigate the spectrum of gravitational waves arising from primordial inflation in the presence of a string-theoretical higher curvature correction, specifically, the Gauss-Bonnet coupling term for the inflaton (modulus) field. We show…

宇宙学与河外天体物理 · 物理学 2023-11-22 Shinsuke Kawai , Jinsu Kim

We review inflationary cosmology in modified gravity such as $R^2$ gravity with its extensions in order to generalize the Starobinsky inflation model. In particular, we explore inflation realized by three kinds of effects: modification of…

高能物理 - 理论 · 物理学 2015-03-11 Kazuharu Bamba , Sergei D. Odintsov

In the context of Quantum Cosmology and the Wheeler-DeWitt equation we investigate the possible effects of a non semiclassical wave-function of the universe on the evolution of the inflationary perturbations. These are associated with the…

广义相对论与量子宇宙学 · 物理学 2018-06-20 A. Y. Kamenshchik , A. Tronconi , T. Vardanyan , G. Venturi

We investigate the gravitational-wave background predicted by a two-scalar-field cosmological model that aims to unify primordial inflation with the dark sector, namely late-time dark energy and dark matter, in a single and self-consistent…

广义相对论与量子宇宙学 · 物理学 2026-02-05 Orlando Luongo , Tommaso Mengoni , Paulo M. Sá

The 2015 Planck data release tightened the region of the allowed inflationary models. Inflationary models with convex potentials have now been ruled out since they produce a large tensor to scalar ratio. Meanwhile the same data offers…

宇宙学与河外天体物理 · 物理学 2017-03-22 Eleonora Di Valentino , Laura Mersini-Houghton

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

We review the status of bouncing cosmologies as alternatives to cosmological inflation for providing a description of the very early universe, and a source for the cosmological perturbations which are observed today. We focus on the…

高能物理 - 理论 · 物理学 2017-03-08 Robert Brandenberger , Patrick Peter

Inflationary cosmology is developed in the second Randall-Sundrum braneworld scenario, where the accelerated expansion arises through potentials that are too steep to drive inflation in conventional cosmology. A relationship between the…

天体物理学 · 物理学 2009-11-06 Greg Huey , James E. Lidsey

We study an inflationary scenario with a vector impurity. We show that the universe undergoes anisotropic inflationary expansion due to a preferred direction determined by the vector. Using the slow-roll approximation, we find a formula to…

高能物理 - 唯象学 · 物理学 2008-11-26 Sugumi Kanno , Masashi Kimura , Jiro Soda , Shuichiro Yokoyama

Inflationary cosmology is the leading explanation of the very early universe. Many different models of inflation have been constructed which fit current observational data. In this work theoretical and numerical methods for constraining the…

宇宙学与河外天体物理 · 物理学 2010-06-29 Ian Huston

We consider an inflationary scenario where the energy scale of inflation stems from gauge theory dynamics. We point out its generic implications on vacuum selection of our universe, in particular, on determination of spacetime symmetries…

高能物理 - 唯象学 · 物理学 2009-10-31 K. -I. Izawa , T. Yanagida

Recent Planck data show the anomalies of CMB fluctuations on large angular scales, which confirms the early observations by WMAP. We continue studying an inflationary model, in which before the slow roll inflation the universe is in a…

宇宙学与河外天体物理 · 物理学 2013-10-15 Zhi-Guo Liu , Zong-Kuan Guo , Yun-Song Piao

We develop a possibility of generating tensor non-Gaussianity in a kind of anisotropic inflation, where a $U(1)$ gauge field is kinetically coupled to a spectator scalar field. Owing to this coupling, the coherent mode of the electric field…

宇宙学与河外天体物理 · 物理学 2021-03-31 Takashi Hiramatsu , Kai Murai , Ippei Obata , Shuichiro Yokoyama

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

We investigate the pre-inflationary dynamics of inflation with the Starobinsky potential, favored by recent data from the Planck mission, using techniques developed to study cosmological perturbations on quantum spacetimes in the framework…

广义相对论与量子宇宙学 · 物理学 2016-03-23 Béatrice Bonga , Brajesh Gupt

We study the noncommutative inflation with a time-dependent noncommutativity between space and time. From the numerical analysis of power law inflation, there are clues that the CMB spectrum indicates a nonconstant noncommutative inflation.…

高能物理 - 理论 · 物理学 2008-11-26 Wei Xue , Bin Chen , Yi Wang

Recent tentative findings of non-Gaussian structure in the COBE-DMR dataset have triggered renewed attention to candidate models from which such intrinsic signature could arise. In the framework of slow roll inflation with built-in non…

天体物理学 · 物理学 2009-10-31 Alejandro Gangui , Jerome Martin
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