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We derive semi-analytic formulae for the local bispectrum and trispectrum in general two-field inflation and provide a simple geometric recipe for building observationally allowed models with observable non-Gaussianity. We use the \delta N…

宇宙学与河外天体物理 · 物理学 2015-03-17 Courtney M. Peterson , Max Tegmark

High-energy modifications to general relativity introduce changes to the perturbations generated during inflation, and the latest high-precision cosmological data can be used to place constraints on such modified inflation models. Recently…

天体物理学 · 物理学 2009-11-10 Shinji Tsujikawa , M. Sami , Roy Maartens

An inflation model with inverse symmetry breaking of two scalar fields is proposed. Constraints on the parameters for a successful inflation are obtained. In general the inequality $\lambda_1\ll g <\lambda_2$ should be satisfied, where…

高能物理 - 唯象学 · 物理学 2014-11-17 Jae-weon Lee , In-guy Koh

We investigate the clustering of halos in cosmological models starting with general local-type non-Gaussian primordial fluctuations. We employ multiple Gaussian fields and add local-type non-Gaussian corrections at arbitrary order to cover…

宇宙学与河外天体物理 · 物理学 2015-06-04 Takahiro Nishimichi

Classic inflation, the theory described in textbooks, is based on the idea that, beginning from typical initial conditions and assuming a simple inflaton potential with a minimum of fine-tuning, inflation can create exponentially large…

宇宙学与河外天体物理 · 物理学 2014-08-18 Anna Ijjas , Paul J. Steinhardt , Abraham Loeb

We investigate an inflation model with the inflaton being identified with a Higgs boson responsible for the breaking of U(1)B-L symmetry. We show that supersymmetry must remain a good symmetry at scales one order of magnitude below the…

高能物理 - 唯象学 · 物理学 2012-03-13 Kazunori Nakayama , Fuminobu Takahashi

We propose a method that provides an observational signature of the quantum origin of primordial fluctuations generated during inflation. The method gives a prescription for testing a Bell inequality constructed exclusively from the…

宇宙学与河外天体物理 · 物理学 2026-03-30 Pablo Tejerina-Pérez , Leonid Sarieddine , Daniele Bertacca , Raul Jimenez

In our previous work the nonlinearity parameter f_NL, which characterizes nongaussianity in the cosmic microwave background, was estimated for a class of inflationary models based on nonlocal field theory. These models include p-adic…

高能物理 - 理论 · 物理学 2009-08-25 Neil Barnaby , James M. Cline

For any unitary conformal field theory in two dimensions with the central charge $c$, we prove that, if there is a nontrivial primary operator whose conformal dimension $\Delta$ vanishes in some limit on the conformal manifold, the…

高能物理 - 理论 · 物理学 2024-07-12 Hirosi Ooguri , Yifan Wang

We investigate consistency relations for non-Gaussianity. We provide a model-independent dynamical proof for the consistency relation of 3-point correlation functions from the Hamiltonian and field redefinition. This relation can be applied…

高能物理 - 理论 · 物理学 2009-02-09 Miao Li , Yi Wang

We calculate the three-point correlation function evaluated at horizon crossing for a set of interacting scalar fields coupled to gravity during inflation. This provides the initial condition for the three-point function of the curvature…

天体物理学 · 物理学 2008-11-26 David Seery , James E. Lidsey

The natural inflation model with a periodic cosine potential is ruled out by recent Planck 2018 data for the decay constant $f \lesssim 5.5~M_{\rm Pl}$. If the Planck data is combined with the BICEP Keck array and BAO data, the model is…

宇宙学与河外天体物理 · 物理学 2024-12-24 Khursid Alam , Koushik Dutta , Nur Jaman

We consider small-field models which invoke the usual framework for the effective field theory, and large-field models which go beyond that. Present and future possibilities for discriminating between the models are assessed, on the…

天体物理学 · 物理学 2015-06-24 Laila Alabidi , David Lyth

In the early Universe matter can be described as a conformal invariant ultra-relativistic perfect fluid, which does not contribute, on classical level, to the evolution of the isotropic and homogeneous metric. If we suppose that there is…

高能物理 - 理论 · 物理学 2009-10-31 J. C. Fabris , A. M. Pelinson , I. L. Shapiro

A novel inflection-point inflation model is analysed. The model considers a massless scalar field, whose self-coupling's running is stabilised by a non-renormalisable operator. The running is controlled by a fermion loop. We find that…

高能物理 - 唯象学 · 物理学 2018-07-05 Konstantinos Dimopoulos , Charlotte Owen , Antonio Racioppi

In hybrid inflationary models, inflation ends by a sudden instability associated with a steep ridge in the potential. Here we argue that this feature can generate a large contribution to the curvature perturbation on observable scales. This…

宇宙学与河外天体物理 · 物理学 2010-02-21 David Mulryne , David Seery , Daniel Wesley

We explain why the concept of a spontaneously broken superconformal symmetry is useful to describe inflationary models favored by the Planck. Non-minimal coupling of complex scalars to curvature, N(X, X*) R, is compulsory for superconformal…

高能物理 - 理论 · 物理学 2014-02-05 Renata Kallosh

We find constraints on inflationary dynamics that yield a large local bispectrum and/or trispectrum during two-field slow-roll inflation. This leads to simple relations between the non-Gaussianity parameters, simplifying the…

宇宙学与河外天体物理 · 物理学 2013-02-21 Joseph Elliston

We examine a class of gauge theories obtained by projecting out certain fields from an N=4 supersymmetric SU(N) gauge theory. These theories are non-supersymmetric and in the large N limit are known to be conformal. Recently it was proposed…

高能物理 - 理论 · 物理学 2009-09-17 Csaba Csaki , Witold Skiba , John Terning

We consider the ghost-free higher order corrections to the Starobinsky model in the old minimal supergravity. In general, higher order corrections cannot be forbidden by symmetries, which likely violate the flatness of the scalaron…

高能物理 - 理论 · 物理学 2015-01-26 Kohei Kamada , Jun'ichi Yokoyama
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