中文
相关论文

相关论文: DILATON-DRIVEN INFLATION IN STRING COSMOLOGY

200 篇论文

String Gas Cosmology is a model of the evolution of the very early universe based on fundamental principles and key new degrees of freedom of string theory which are different from those of point particle field theories. In String Gas…

高能物理 - 理论 · 物理学 2015-05-28 Robert H. Brandenberger

We demonstrate the parametric amplification of the stochastic gravitational wave background during inflationary reheating and during axion/moduli oscillations. This amplification enhances the detectability of the string/inflationary gravity…

天体物理学 · 物理学 2007-05-23 Bruce A. Bassett

We investigate $(n+1)$-dimensional string-dilaton cosmology with effective dilaton potential in presence of perfect-fluid matter.We get exact solutions parametrized by the constant $\gam$ of the state equation $p=(\gam-1)\rho$, the spatial…

广义相对论与量子宇宙学 · 物理学 2008-11-26 S. Capozziello , G. Lambiase , R. Capaldo

In a recent paper, which has been published in Nature, the LIGO Scientific Collaboration (LSC) obtained an upper limit on the stochastic gravitational-wave background of cosmological origin by using the data from a two-year science run of…

广义相对论与量子宇宙学 · 物理学 2015-05-19 Christian Corda

We investigate the cosmological evolution of gravitational waves in Friedman-Robertson-Walker brane world models embedded in a five dimensional anti de-Sitter spacetime. To predict the spectrum of stochastic gravitational background at…

天体物理学 · 物理学 2007-05-23 Kiyotomo Ichiki , Kouji Nakamura

In the pre-reheating era, following cosmic inflation and preceding radiation domination, the energy density may be dominated by an oscillating massive scalar condensate, such as is the case for quadratic chaotic inflation. We have found in…

宇宙学与河外天体物理 · 物理学 2010-05-27 Karsten Jedamzik , Martin Lemoine , Jerome Martin

The cosmon field responsible for dynamical dark energy can induce an inflationary period in early cosmology. Details depend on dilatation symmetry breaking terms in its potential and kinetic term that are relevant only during early stages…

宇宙学与河外天体物理 · 物理学 2015-06-15 C. Wetterich

We develop a cosmological model where primordial inflation is driven by a 'solid', defined as a system of three derivatively coupled scalar fields obeying certain symmetries and spontaneously breaking a certain subgroup of these. The…

高能物理 - 理论 · 物理学 2015-06-11 Solomon Endlich , Alberto Nicolis , Junpu Wang

A synthetic report of the advances in the study of classical and quantum string dynamics in curved backgrounds is provided, namely: the new feature of multistring solutions; the effect of a cosmological constant and of spacial curvature on…

高能物理 - 理论 · 物理学 2011-07-19 Norma G. Sanchez

We study the quantum evolution of the early universe, its semi-classical analogue together with inflationary regime, in view of a generalized modified theory of gravity. The action is built by supplementing the non-minimally coupled…

高能物理 - 理论 · 物理学 2021-01-11 Ranajit Mandal , Dalia Saha , Mohosin Alam , Abhik Kumar Sanyal

We study the cosmological evolution of a type-0 string theory by employing non-criticality, which may be induced by fluctuations of the D3 brane worlds. We check the consistency of the approach to O(alpha ') in the corresponding…

高能物理 - 理论 · 物理学 2009-11-07 G. A. Diamandis , B. C. Georgalas , N. E. Mavromatos , E. Papantonopoulos , I. Pappa

The decay of the string perturbative vacuum into our present cosmological state is associated to the transition from a phase of growing curvature and growing dilaton, to a phase of decreasing curvature and frozen dilaton. The possible…

广义相对论与量子宇宙学 · 物理学 2007-05-23 M. Gasperini

Axion monodromy is a generic phenomenon in string compactifications. We investigate the production of gravitational-wave background from axion monodromy inflation during preheating. By performing lattice simulations using pseudo-spectral…

宇宙学与河外天体物理 · 物理学 2019-09-18 Yu Sang , Qing-Guo Huang

We study the generation of cosmological perturbations during the Hagedorn phase of string gas cosmology. Using tools of string thermodynamics we provide indications that it may be possible to obtain a nearly scale-invariant spectrum of…

高能物理 - 理论 · 物理学 2010-04-06 Ali Nayeri , Robert H. Brandenberger , Cumrun Vafa

Slow-roll inflation generically makes several predictions: a flat Universe, primordial adiabatic density perturbations, and a stochastic gravity-wave background. Each inflation model will further predict specific relations between the…

天体物理学 · 物理学 2007-05-23 Marc Kamionkowski

We explore the homogeneous background dynamics and the evolution of generated perturbations of cosmological inflation that is driven by multiple scalar fields interacting with a perfect fluid.Then we apply the method to warm inflation…

广义相对论与量子宇宙学 · 物理学 2018-04-04 Yang-Yang Wang , Jian-Yang Zhu , Xiao-Min Zhang

In this work, we present the gravitational field generated by a cosmic string carrying a timelike current in the scalar-tensor gravities. The mechanism of formation and evolution of wakes is fully investigated in this framework. We show…

高能物理 - 理论 · 物理学 2009-11-10 A. L. N. Oliveira , M. E. X. Guimaraes

A general family of charge-current carrying cosmic string models is investigated. In the special case of circular configurations in arbitrary axially symmetric gravitational and electromagnetic backgrounds the dynamics is determined by…

高能物理 - 理论 · 物理学 2010-04-06 Arne L. Larsen

It has recently been realized that many theories of physics beyond the Standard Model give rise to cosmological histories exhibiting extended epochs of cosmological stasis. During such epochs, the abundances of different energy components…

宇宙学与河外天体物理 · 物理学 2024-12-17 Keith R. Dienes , Lucien Heurtier , Fei Huang , Tim M. P. Tait , Brooks Thomas

We study inflation and entropy generation in a recently proposed pre-big-bang model universe produced in a collision of gravitational and dilaton waves. It is shown that enough inflation occurs provided the incoming waves are sufficiently…

高能物理 - 理论 · 物理学 2009-10-31 A. Feinstein , K. E. Kunze , M. A. Vazquez-Mozo