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相关论文: String Driven Cosmology and its Predictions

200 篇论文

Within the context of a super-critical (Liouville) string, we discuss (target-space) two-dimensional string cosmology. A numerical analysis indicates that the identification of time with the Liouville mode results in an expanding universe…

高能物理 - 理论 · 物理学 2009-10-31 G. A. Diamandis , B. C. Georgalas , N. E. Mavromatos , E. Papantonopoulos

The interplay between string theory and early-universe cosmology offers promising avenues to explore high-energy regimes where the standard single-field slow-roll model may no longer provide an accurate description. One intriguing scenario…

高能物理 - 理论 · 物理学 2025-10-28 M. Meo

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

Thermal inflation was proposed as a mechanism to dilute the density of cosmological moduli. Thermal inflation is driven by a complex scalar field possessing a large vacuum expectation value and a very flat potential, called a `flaton'. Such…

宇宙学与河外天体物理 · 物理学 2023-04-13 Robert Brandenberger , Aline Favero

I discuss cosmological models either derived from, or inspired by, string theory or M-theory. In particular I discuss solutions in the low-energy effective theory and the role of the dilaton, moduli and antisymmetric form fields in the…

高能物理 - 理论 · 物理学 2009-11-07 David Wands

We develop a possible cosmology for a Universe with n additional spatial dimensions of variable scale, and an associated scalar field, the radion, which is distinct from the field responsible for inflation, the inflaton. Based on a…

高能物理 - 唯象学 · 物理学 2009-10-31 Eanna E. Flanagan , S. -H. Henry Tye , Ira Wasserman

We study the cosmological evolution of a D3-brane Universe in a type 0 string background. We follow the brane universe along the radial coordinate of the background and we calculate the energy density which is induced on the brane because…

高能物理 - 理论 · 物理学 2007-05-23 I. Pappa

In previous works we have derived a Running Vacuum Model (RVM) for a string Universe, which provides an effective description of the evolution of 4-dimensional string-inspired cosmologies from inflation till the present epoch. In the…

高能物理 - 唯象学 · 物理学 2021-09-20 Nick E. Mavromatos , Joan Sola

Following a suggestion by Gasperini and Veneziano, that String Cosmology can be reconciled with Inflation and, hence, with the Standard Big Bang, we display an analytical solution which possesses four interesting properties: (1) it is…

天体物理学 · 物理学 2011-04-20 Carlo Angelantonj , Luca Amendola , Marco Litterio , Franco Occhionero

We obtain cosmological constraints on models of inflation which exhibit rapid roll solutions. Rapid roll attractors exist for potentials with large mass terms and are thus of interest for inflationary model building within string theory. We…

宇宙学与河外天体物理 · 物理学 2010-04-15 Takeshi Kobayashi , Shinji Mukohyama , Brian A. Powell

String theory abounds with light scalar fields (the dilaton and various moduli) which create a host of observational problems, and notably some serious cosmological difficulties similar to the ones associated with the Polonyi field in the…

高能物理 - 理论 · 物理学 2009-10-28 Thibault Damour , Alexander Vilenkin

String cosmology aims at providing a reliable description of the very early Universe in the regime where standard-model physics is no longer appropriate, and where we can safely apply the basic ingredients of superstring models such as…

广义相对论与量子宇宙学 · 物理学 2014-04-24 M. Gasperini

A four-dimensional universe, arising from a flux compactification of Type IIB string theory, contains scalar fields with a potential determined by topological and geometric parameters of the internal -hidden- dimensions. We show that…

天体物理学 · 物理学 2007-05-23 Joan Simon , Raul Jimenez , Licia Verde , Per Berglund , Vijay Balasubramanian

The string $\alpha^\prime$-correction to the usual Einstein action comprises a Gauss-Bonnet integrand multiplied by non-trivial functions of the modulus field $\chi$ and/or the dilaton field $\phi$. We discuss how the presence of such terms…

高能物理 - 理论 · 物理学 2007-05-23 Ishwaree P Neupane

In this paper we examine the classical evolution of a cosmological model derived from the low-energy tree-level limit of a generic string theory. The action contains the metric, dilaton, central charge and an antisymmetric tensor field. We…

高能物理 - 理论 · 物理学 2009-10-28 Richard Easther , Kei-ichi Maeda , David Wands

We study the cosmological evolution of a D3-brane Universe in a type 0 string background. We follow the brane-universe along the radial coordinate of the background and we calculate the energy density which is induced on the brane because…

高能物理 - 理论 · 物理学 2009-10-31 E. Papantonopoulos , I. Pappa

Inflation is now a basic ingredient of the modern cosmology. After reviewing the basic characteristics of inflation, we briefly discuss inflation in string and brane theories, focusing on the problem of the exit from inflation in these…

高能物理 - 理论 · 物理学 2016-01-28 E. Papantonopoulos

We present a wholly self-consistent, complete cyclic bouncing cosmology based on components drawn from string theory and constructed in a way that is under perturbative control throughout (e.g., with temperature much less than the string…

广义相对论与量子宇宙学 · 物理学 2025-08-14 Nissan Itzhaki , Uri Peleg , Paul J. Steinhardt

After 25 years of its existence, inflationary theory gradually becomes the standard cosmological paradigm. However, we still do not know which of the many versions of inflationary cosmology will be favored by the future observational data.…

高能物理 - 理论 · 物理学 2011-05-24 Andrei Linde

Cosmic inflation is the cornerstone of modern cosmology. In particular, following the Planck mission reports presented in 2015 regarding cosmic microwave background (CMB), there is an increasing interest in searching for inflaton candidates…

高能物理 - 理论 · 物理学 2018-08-14 K. Sravan Kumar