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Evidence for the presence of extra fields during inflation may be found in the anisotropies of the scalar and tensor spectra across a vast range of scales. Indeed, beyond the single-field slow-roll paradigm, a long tensor mode can modulate…

宇宙学与河外天体物理 · 物理学 2020-02-19 Emanuela Dimastrogiovanni , Matteo Fasiello , Gianmassimo Tasinato

We study the metric perturbations produced during inflation in models with two scalar fields evolving simultaneously. In particular, we emphasize how the large-scale curvature perturbation $\zeta$ on fixed energy density hypersurfaces may…

天体物理学 · 物理学 2016-08-24 Juan Garcia-Bellido , David Wands

We construct a model of hybrid inflation within a controlled five-dimensional effective field theory framework. The inflaton and waterfall fields are realized as naturally light moduli of the 5D compactification. At the quantum level,…

高能物理 - 唯象学 · 物理学 2014-11-20 Raman Sundrum , Christopher M. Wells

We discuss the problem of anisotropy and intermittency in statistical theory of high Reynolds-number turbulence (and turbulent transport). We present a detailed description of the new tools that allow effective data analysis and systematic…

混沌动力学 · 物理学 2009-11-10 Luca Biferale , Itamar Procaccia

Non-adiabatic pressure perturbations naturally occur in models of inflation consisting of more than one scalar field. The amount of non-adiabatic pressure present at the end of inflation can have observational consequences through changes…

宇宙学与河外天体物理 · 物理学 2012-11-30 Ian Huston , Adam J. Christopherson

There are hidden observables for inflation, such as features localized in position space, which do not manifest themselves when only one inflation trajectory is considered. To address this issue, we investigate inflation dynamics in a…

高能物理 - 理论 · 物理学 2012-10-02 Francis Duplessis , Yi Wang , Robert Brandenberger

A new hybrid inflationary scenario in the context of $f(R,{\Box}R)$-gravity is proposed. Demanding the waterfall field to 'support the potential from below' [unlike the original proposal by Stewart in Phys. Lett. B345, 414 (1995)], we…

高能物理 - 理论 · 物理学 2011-03-18 Masao Iihoshi

Generically, the gravitational-wave or tensor-mode contribution to the primordial curvature spectrum of inflation is tiny if the field-range of the inflaton is much smaller than the Planck scale. We show that this pessimistic conclusion is…

高能物理 - 理论 · 物理学 2014-01-15 Arthur Hebecker , Sebastian C. Kraus , Alexander Westphal

The spectrum of curvature perturbation generated during inflation is studied in the case the inflation-driving scalar field (inflaton) $\phi$ crosses over its potential extremum. It is shown that the nondecaying mode of perturbation has a…

高能物理 - 唯象学 · 物理学 2009-11-07 Jun'ichi Yokoyama , Shogo Inoue

Various data analyses of the Cosmic Microwave Background (CMB) provide observational hints of statistical isotropy breaking. Some of these features can be studied within the framework of primordial vector fields in inflationary theories…

宇宙学与河外天体物理 · 物理学 2015-05-28 N. Bartolo , E. Dimastrogiovanni , M. Liguori , S. Matarrese , A. Riotto

We present a scenario where an axion-like field drives inflation until a potential barrier, which keeps a waterfall field at the origin, disappears and a waterfall transition occurs. Such a barrier separates the scale of inflation from that…

高能物理 - 唯象学 · 物理学 2021-08-18 Jinn-Ouk Gong , Kwang Sik Jeong

Several early Universe scenarios predict a direction-dependent spectrum of primordial curvature perturbations. This translates into the violation of the statistical isotropy of cosmic microwave background radiation. Previous searches for…

宇宙学与河外天体物理 · 物理学 2017-03-22 S. Ramazanov , G. Rubtsov , M. Thorsrud , F. R. Urban

We study the primordial bispectrum of curvature perturbation in the uniform- density slicing generated by the interaction between the inflaton and isotropic background gauge fields. We derive the action up to cubic order in perturbation and…

宇宙学与河外天体物理 · 物理学 2013-06-05 Hiroyuki Funakoshi , Kei Yamamoto

The dominant contribution to the primordial curvature perturbation may be generated at the end of inflation. Taking the end of inflation to be sudden, formulas are presented for the spectrum, spectral tilt and non-gaussianity. They are…

天体物理学 · 物理学 2009-11-13 David H. Lyth

We study the emergence of quantum entanglement in multi-field inflation. In this scenario, the perturbations of one field contribute to the observable curvature perturbation, while multi-field dynamics with the other fields affect the…

宇宙学与河外天体物理 · 物理学 2018-09-19 Nadia Bolis , Tomohiro Fujita , Shuntaro Mizuno , Shinji Mukohyama

Correlation anisotropy emerges dynamically in magnetohydrodynamics (MHD), producing stronger gradients across the large-scale mean magnetic field than along it. This occurs both globally and locally, and has significant implications in…

空间物理 · 物理学 2013-12-04 W. H. Matthaeus , S. Servidio , P. Dmitruk , V. Carbone , S. Oughton , M. Wan , K. T. Osman

The statistical properties of the primordial density perturbations has been considered in the past decade as a powerful probe of the physical processes taking place in the early universe. Within the inflationary paradigm, the properties of…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Gabriel Leon , Daniel Sudarsky

We investigate the possibility of embedding the vector curvaton paradigm in D-brane models of inflation in Type IIB string theory in a simple toy model. The vector curvaton is identified with the U(1) gauge field that lives on the world…

高能物理 - 理论 · 物理学 2015-05-30 Konstantinos Dimopoulos , Danielle Wills , Ivonne Zavala

In a model of an Abelian vector boson with a Maxwell kinetic term and non-negative mass-squared it is demonstrated that, under fairly general conditions during inflation, a scale-invariant spectrum of perturbations for the components of a…

高能物理 - 唯象学 · 物理学 2011-02-28 Konstantinos Dimopoulos , Jacques M. Wagstaff

Erickcek, Kamionkowski and Carroll proposed in 2008 that the dipole modulation of the CMB could be due to a very large scale perturbation of the field $\phi$ causing the primordial curvature perturbation. We repeat their calculation using…

宇宙学与河外天体物理 · 物理学 2015-06-15 David H. Lyth