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In this paper, we present two non-perturbative string cosmological solutions without curvature singularities for the bosonic gravi-dilaton system. These solutions are general in the sense that they can straightforwardly match the…

高能物理 - 理论 · 物理学 2024-02-26 Li Song , Deyou Chen

We develop the cosmological perturbations formalism in models with a single non-local scalar field originating from the string field theory description of the rolling tachyon dynamics. We construct the equation for the energy density…

高能物理 - 理论 · 物理学 2012-07-19 Alexey S. Koshelev , Sergey Yu. Vernov

We investigate the cosmological background evolution and perturbations in a general class of spatially covariant theories of gravity, which propagates two tensor modes and one scalar mode. We show that the structure of the theory is…

广义相对论与量子宇宙学 · 物理学 2016-02-09 Tomohiro Fujita , Xian Gao , Jun'ichi Yokoyama

Intrinsic and extrinsic geometric properties of string world sheets in curved space-time background are explored. In our formulation, the only dynamical degrees of freedom of the string are its immersion coordinates. Classical equation of…

高能物理 - 理论 · 物理学 2009-10-30 K. S. Viswanathan , R. Parthasarathy

In the non-relativistic theory of gravity recently proposed by Horava, the Hamiltonian constraint is not satisfied locally at each point in space. The absence of the local Hamiltonian constraint allows the system to have an extra…

宇宙学与河外天体物理 · 物理学 2015-05-13 Tsutomu Kobayashi , Yuko Urakawa , Masahide Yamaguchi

We discuss the evolution of linear perturbations about a Friedmann-Robertson-Walker background metric, using only the local conservation of energy-momentum. We show that on sufficiently large scales the curvature perturbation on spatial…

天体物理学 · 物理学 2009-10-31 David Wands , Karim A. Malik , David H. Lyth , Andrew R. Liddle

We consider the dynamics of a contracting universe ruled by two minimally coupled scalar fields with general exponential potentials. This model describes string-inspired scenarios in the Einstein frame. Both background and perturbations can…

高能物理 - 理论 · 物理学 2009-11-07 Fabio Finelli

We investigate the nature of ordinary cosmic vortices in some scalar-tensor extensions of gravity. We find solutions for which the dilaton field condenses inside the vortex core. These solutions can be interpreted as raising the degeneracy…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Patrick Peter , M. E. X. Guimaraes , V. C. de Andrade

In general relativity, it has been shown that the effective gravitational stress-energy tensor for short-wavelength metric perturbations acts just like that for a radiation fluid, and thus, in particular, cannot provide any effects that…

广义相对论与量子宇宙学 · 物理学 2016-06-21 Keiki Saito , Akihiro Ishibashi

We study density perturbations in several cosmological models motivated by string theory. The evolution and the spectra of curvature perturbations ${\cal R}$ are analyzed in the Ekpyrotic scenario and nonsingular string cosmologies. We find…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Shinji Tsujikawa

In this paper we investigate the cosmological effects of modified gravity with string curvature corrections added to Einstein-Hilbert action in the presence of a dynamically evolving scalar field coupled to Riemann invariants. The scenario…

高能物理 - 理论 · 物理学 2008-11-26 Shin'ichi Nojiri , Sergei D. Odintsov , M. Sami

We show, using purely classical considerations and logical extrapolation of results belonging to point particle theories, that the metric background field in which a string propagates must satisfy an Einstein or an Einstein-like equation.…

高能物理 - 理论 · 物理学 2010-10-27 Sayan Kar

We improve and extend a method introduced in an earlier paper for deriving string field equations. The idea is to impose conformal invariance on a generalized sigma model, using a background field method that ensures covariance under very…

高能物理 - 理论 · 物理学 2009-10-30 Korkut Bardakci

We study the effect of the antisymmetric tensor field $B_{\mu\nu}$ on the large curvature phase of string cosmology. It is well-known that a non-vanishing value of $H=dB$ leads to an anisotropic expansion of the spatial dimensions.…

广义相对论与量子宇宙学 · 物理学 2009-10-30 Stefano Foffa , Michele Maggiore

If more than one curvaton dominate the Universe at different epochs from each other, curvature perturbations can be temporarily enhanced to a value much larger than the observed one 10^{-5}. The traces of the enhancement may be left as…

宇宙学与河外天体物理 · 物理学 2013-05-29 Teruaki Suyama , Jun'ichi Yokoyama

We investigate the cosmological perturbations in generalized gravity, where the Ricci scalar and a scalar field are non-minimally coupled via an arbitrary function. In the Friedmann-Lemaitre-Robertson-Walker background, by studying the…

高能物理 - 理论 · 物理学 2009-07-30 Xiangdong Ji , Tower Wang

We investigate quantum corrections for a cosmological solution of the string effective action. Starting point is a classical solution containing an antisymmetric tensor field, a dilaton and a modulus field which has singularities in the…

高能物理 - 理论 · 物理学 2007-05-23 K. Behrndt

The converging mechanism discussed in [Damour & Nordtvedt, Physical Review Letters,70,15] for scalar-tensor theories has been applied to dilaton-like theories in several subsequent papers. In the present communication, we show that an…

广义相对论与量子宇宙学 · 物理学 2014-06-24 Olivier Minazzoli

A covariant formalism for physical perturbations propagating along a string in an arbitrary curved spacetime is developed. In the case of a stationary string in a static background the propagation of the perturbations is described by a…

高能物理 - 理论 · 物理学 2009-10-22 Arne L. Larsen , Valery P. Frolov

Cosmology in extended theories of gravity is considered assuming the Palatini variational principle, for which the metric and connection are independent variables. The field equations are derived to linear order in perturbations about the…

天体物理学 · 物理学 2015-06-24 Tomi Koivisto , Hannu Kurki-Suonio