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相关论文: De Sitter Bounces

200 篇论文

We revisit the classical theory of ten-dimensional two-derivative gravity coupled to fluxes, scalar fields, D-branes, anti D-branes and Orientifold-planes. We show that such set-ups do not give rise to a four-dimensional positive curvature…

高能物理 - 理论 · 物理学 2015-06-18 Keshav Dasgupta , Rhiannon Gwyn , Evan McDonough , Mohammed Mia , Radu Tatar

Viable models of modified gravity which satisfy both local as well as cosmological tests are investigated. It is demonstrated that some versions of such highly non-linear models exhibit multiply de Sitter universe solutions, which often…

广义相对论与量子宇宙学 · 物理学 2009-02-20 G. Cognola , E. Elizalde , S. D. Odintsov , P. Tretyakov , S. Zerbini

We construct a class of Einstein-vector theories where the vector field couples bilinearly to the curvature polynomials of arbitrary order in such a way that only Riemann tensor rather than its derivative enters the equations of motion. The…

高能物理 - 理论 · 物理学 2016-02-17 Wei-Jian Geng , H. Lu

Conditions for the existence and stability of de Sitter space in modified gravity are derived by considering inhomogeneous perturbations in a gauge-invariant formalism. The stability condition coincides with the corresponding condition for…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Valerio Faraoni , Shahn Nadeau

We obtain a general class of time-dependent, asymptotically de Sitter backgrounds which solve the first order bosonic equations that extremize the action for supergravity with gauged non-compact $R$-symmetry. These backgrounds correspond…

高能物理 - 理论 · 物理学 2009-09-17 Klaus Behrndt , Mirjam Cvetic

Explicit time-dependent solutions of the 10D vacuum Einstein equations are found for which spacetime is compactified on six-dimensional warped spaces. We explicitly work out an example where the internal manifold is a six-dimensional…

高能物理 - 理论 · 物理学 2014-11-18 Ishwaree P. Neupane

We consider $d$-dimensional static spacetimes in Einstein gravity with a cosmological constant in the presence of a minimally coupled massless scalar field. The spacetimes have a $(d-2)$-dimensional base manifold given by an Einstein space…

高能物理 - 理论 · 物理学 2012-06-08 Sebastian Garcia Saenz , Cristian Martinez

A quantum mechanical formulation of de Sitter cosmological spacetimes still eludes string theory. In this paper we conjecture a potentially rigorous framework in which the status of de Sitter space is the same as that of a resonance in a…

高能物理 - 理论 · 物理学 2017-03-15 Jonathan Maltz , Leonard Susskind

The two-particle models in de Sitter space-time with time-asymmetric retarded-advanced interactions are constructed. Particular cases of the field-type electromagnetic and scalar interactions are considered. The manifestly covariant…

广义相对论与量子宇宙学 · 物理学 2026-02-18 Askold Duviryak

We review two ways in which smooth cosmological evolution between two de Sitter phases can be obtained from M/string-theory. Firstly, we perform a hyperbolic reduction of massive IIA* theory to D=6 N=(1,1) SU(2)xU(1) gauged de Sitter…

高能物理 - 理论 · 物理学 2017-08-23 H. Lu , J. F. Vazquez-Poritz

We present spinning Q-balls and boson stars in four dimensional anti-de Sitter spacetime. These are smooth, horizonless solutions for gravity coupled to a massive complex scalar field with a harmonic dependence on time and the azimuthal…

广义相对论与量子宇宙学 · 物理学 2015-06-05 Eugen Radu , Bintoro Subagyo

Two ways in which de Sitter space can arise in supergravity theories are discussed. In the first, it arises as a solution of a conventional supergravity, in which case it necessarily has no Killing spinors. For example, de Sitter space can…

高能物理 - 理论 · 物理学 2010-02-03 C. M. Hull

We investigate the cosmology of a recently proposed deformation of Einstein gravity, emerging from quantum gravity heuristics. The theory is constructed to have de Sitter space as a vacuum solution, and thus to be relevant to the…

天体物理学 · 物理学 2009-11-11 Damien A. Easson , Frederic P. Schuller , Mark Trodden , Mattias N. R. Wohlfarth

It is believed that gravity will be explained in the framework of the existing quantum theory when one succeeds in eliminating divergencies at large momenta or small distances (although the phenomenon of gravity has been observed only at…

广义相对论与量子宇宙学 · 物理学 2008-07-28 Felix Lev

Exact and explicit string solutions in de Sitter spacetime are found. (Here, the string equations reduce to a sinh-Gordon model). A new feature without flat spacetime analogy appears: starting with a single world-sheet, several (here two)…

高能物理 - 理论 · 物理学 2009-10-22 H. J. de Vega , A. V. Mikhailov , N. Sanchez

We use the superspace formulation of (massive) IIA supergravity to obtain the explicit form of the dilatino terms, and we find that the quartic-dilatino term is positive. The theory admits a ten-dimensional de Sitter solution, obtained by…

高能物理 - 理论 · 物理学 2018-02-21 Bertrand Souères , Dimitrios Tsimpis

A spatially flat Robertson-Walker spacetime driven by a cosmological constant is non-conformally coupled to a massless scalar field. The equations of semiclassical gravity are explicitly solved for this case, and a self-consistent de Sitter…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Guillem Perez-Nadal , Albert Roura , Enric Verdaguer

The dynamical generation of a four-dimensional classical universe from nothing but fundamental quantum excitations at the Planck scale is a long-standing challenge to theoretical physicists. A candidate theory of quantum gravity which…

高能物理 - 理论 · 物理学 2009-01-08 J. Ambjorn , A. Goerlich , J. Jurkiewicz , R. Loll

Einstein-Gauss-Bonnet gravity in five-dimensional spacetime provides an excellent example of a theory that, while including higher-order curvature corrections to General Relativity, still shares many of its features, such as second-order…

高能物理 - 理论 · 物理学 2015-06-05 Fernando Izaurieta , Eduardo Rodríguez

Scalar-tensor gravity is one of the most competitive gravity theory to Einstein's relativity. We reconstruct the exact de Sitter solution in scalar-tensor gravity, in which the non-minimal coupling scalar is rolling along the potential.…

广义相对论与量子宇宙学 · 物理学 2011-07-04 Hongsheng Zhang , Xin-Zhou Li