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Primordial non-Gaussianity signatures of extremely heavy particles are re-examined within a simple alternative to the standard inflationary paradigm, in which the primordial fluctuations and the inflationary spacetime expansion are sourced…

高能物理 - 唯象学 · 物理学 2020-06-05 Soubhik Kumar , Raman Sundrum

We investigate the scale-dependence, or the runnings, of linear and second order density perturbations generated in various curvaton scenarios. We argue that the second order perturbations, i.e. non-Gaussianity, can strongly depend on the…

宇宙学与河外天体物理 · 物理学 2012-06-12 Takeshi Kobayashi , Tomo Takahashi

A new model realisation of the vector curvaton paradigm is presented and analysed. The model consists of a single massive Abelian vector field, with a Maxwell type kinetic term. By assuming that the kinetic function and the mass of the…

高能物理 - 唯象学 · 物理学 2010-03-03 Konstantinos Dimopoulos , Mindaugas Karciauskas , Jacques M. Wagstaff

We study a ghost-free model of massive vector curvaton proposed in the literature, where the quick decrease of the vector background expectation value is avoided by a suitable choice of kinetic and mass functions. The curvaton perturbations…

宇宙学与河外天体物理 · 物理学 2013-05-30 Ryo Namba

We perform a combined perturbation and observational investigation of the scenario of non-minimal derivative coupling between a scalar field and curvature. First we extract the necessary condition that ensures the absence of instabilities,…

宇宙学与河外天体物理 · 物理学 2013-12-02 James B. Dent , Sourish Dutta , Emmanuel N. Saridakis , Jun-Qing Xia

A recent proposal for gauge-invariant observables in inflation [R. Brunetti et al., JHEP 1608 (2016) 032] is examined. We give a generalisation of their construction to general background spacetimes. In flat space, we calculate one-loop…

广义相对论与量子宇宙学 · 物理学 2018-02-02 Markus B. Fröb

Cosmological correlation functions of inflaton and graviton perturbations are the fundamental observables of early universe cosmology and remain a primary target for observations. In this work, we ask the following question: are these…

高能物理 - 理论 · 物理学 2026-04-15 David Stefanyszyn , Xi Tong , Yuhang Zhu

We discuss how primordial non-Gaussianity of the curvature perturbation helps to constrain models of the early universe. Observations are consistent with Gaussian initial conditions, compatible with the predictions of the simplest models of…

宇宙学与河外天体物理 · 物理学 2014-11-26 Christian T. Byrnes

In this proceeding, we review modified theories of gravity with a curvature-matter coupling between an arbitrary function of the scalar curvature and the Lagrangian density of matter. This explicit nonminimal coupling induces a…

广义相对论与量子宇宙学 · 物理学 2022-09-20 Francisco S. N. Lobo , Tiberiu Harko

We characterise the primordial perturbations produced due to both inflaton and curvaton fluctuations in models where the curvaton has a quadratic, cosine or hyperbolic potential, and the inflaton potential is characterised by the usual…

宇宙学与河外天体物理 · 物理学 2015-06-04 José Fonseca , David Wands

This paper presents the first derivation of the quadratic action for curvature perturbations, $\zeta$, within the framework of cuscuton gravity. We study the scalar cosmological perturbations sourced by a canonical single scalar field in…

高能物理 - 理论 · 物理学 2017-07-26 Supranta S. Boruah , Hyung J. Kim , Ghazal Geshnizjani

In this work, we review a plethora of modified theories of gravity with generalized curvature-matter couplings. The explicit nonminimal couplings, for instance, between an arbitrary function of the scalar curvature $R$ and the Lagrangian…

广义相对论与量子宇宙学 · 物理学 2014-07-29 Tiberiu Harko , Francisco S. N. Lobo

In curvaton-type models, observable non-gaussianity of the curvature perturbation would come from a contribution of the form $(\delta\sigma)^2$, where $\delta\sigma$ is gaussian. I analyse this situation allowing $\delta\sigma$ to be…

天体物理学 · 物理学 2009-11-11 D. H. Lyth

We calculate the lowest-order non-linear contributions to the power spectrum, two-point correlation function, and smoothed variance of the density field, for Gaussian initial conditions and scale-free initial power spectra, $P(k) \sim k^n$.…

天体物理学 · 物理学 2009-10-28 Roman Scoccimarro , Josh Frieman

We use the delta N -formalism to investigate the non-Gaussianity of the primordial curvature perturbation in the curvaton scenario for the origin of structure. We numerically calculate the full probability distribution function allowing for…

天体物理学 · 物理学 2010-04-06 Misao Sasaki , Jussi Valiviita , David Wands

We study inflationary scenarios driven by a scalar field in the presence of a non-minimal coupling between matter and curvature. We show that the Friedmann equation can be significantly modified when the energy density during inflation…

广义相对论与量子宇宙学 · 物理学 2017-06-28 Cláudio Gomes , João G. Rosa , Orfeu Bertolami

Gravitational waves in the presence of a non-minimal curvature-matter coupling are analysed, both in the Newman-Penrose and perturbation theory formalisms. Considering a cosmological constant as a source, the non-minimally coupled…

广义相对论与量子宇宙学 · 物理学 2018-05-03 Orfeu Bertolami , Cláudio Gomes , Francisco S. N. Lobo

We investigate the phase diagram of quantum gravity with a vertex expansion about constantly-curved backgrounds. The graviton two- and three-point function are evaluated with a spectral sum on a sphere. We obtain, for the first time,…

高能物理 - 理论 · 物理学 2019-11-28 Nicolai Christiansen , Kevin Falls , Jan M. Pawlowski , Manuel Reichert

We study the axion-type curvaton model, with emphasis on the large field regime where analytic results are very difficult to obtain. We evaluate the tensor-scalar ratio $r$ using WMAP normalization and the non-linearity parameters $f_{NL}$…

宇宙学与河外天体物理 · 物理学 2014-11-18 Pravabati Chingangbam , Qing-Guo Huang

Quantum gravity coupled to scalar massive matter fields is investigated within the framework of causal perturbation theory. One-loop calculations include matter loop graviton self-energy and matter self-energy and yield ultraviolet finite…

高能物理 - 理论 · 物理学 2009-10-31 Nicola Grillo