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相关论文: Old Inflation in String Theory

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Braneworld inflation on the resolved warped deformed conifold is represented by the dynamics of a D3-brane probe with the world volume of a brane spanning the large dimensions of the observable Universe. This model was recently proposed as…

高能物理 - 理论 · 物理学 2008-11-26 Alex Buchel

We construct a string-inspired nonsingular cosmological scenario in which an inflaton field is driven up the potential before the graceful exit by employing a low-energy string effective action with an orbifold compactification. This sets…

高能物理 - 理论 · 物理学 2015-06-26 Yun-Song Piao , Shinji Tsujikawa , Xinmin Zhang

We consider a cosmological scenario within the KKLT framework for moduli stabilization in string theory. The universal open string tachyon of decaying non-BPS D-brane configurations is proposed to drive eternal topological inflation.…

高能物理 - 理论 · 物理学 2009-11-11 Daniel Cremades , Fernando Quevedo , Aninda Sinha

In this paper, we investigate the noncommutative KKLMMT D3/anti-D3 brane inflation scenario in detail. Incorporation of the brane inflation scenario and the noncommutative inflation scenario can nicely explain the large negative running of…

高能物理 - 理论 · 物理学 2009-11-11 Xin Zhang

The curvaton and the inhomogeneous reheating scenarios for the generation of the cosmological curvature perturbation on large scales represent an alternative to the standard slow-roll scenario where the observed density perturbations are…

天体物理学 · 物理学 2009-11-10 L. Pilo , A. Riotto , A. Zaffaroni

An inflationary stage dominated by a $D$-term avoids the slow-roll problem of inflation in supergravity and may emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. The most intriguing and commonly invoked possibility…

高能物理 - 唯象学 · 物理学 2009-10-31 J. R. Espinosa , A. Riotto , G. G. Ross

Usual inflation is realized with a slow rolling scalar field minimally coupled to gravity. In contrast, we consider dynamics of a scalar with a flat effective potential, conformally coupled to gravity. Surprisingly, it contains an attractor…

高能物理 - 理论 · 物理学 2008-11-26 Lev Kofman , Shinji Mukohyama

We calculate the three-point correlation function of the comoving curvature perturbation generated during an inflationary epoch driven by false vacuum energy. We get a novel false vacuum shape bispectrum, which peaks in the equilateral…

宇宙学与河外天体物理 · 物理学 2014-11-20 Jinn-Ouk Gong , Chunshan Lin , Yi Wang

Inflationary models whose vacuum energy arises from a D-term are believed not to suffer from the supergravity eta problem of F-term inflation. That is, D-term models have the desirable property that the inflaton mass can naturally remain…

高能物理 - 理论 · 物理学 2009-11-11 Liam McAllister

We compare the simplest realistic brane inflationary model to recent cosmological data, including WMAP 3-year cosmic microwave background (CMB) results, Sloan Digital Sky Survey luminous red galaxies (SDSS LRG) power spectrum data and…

高能物理 - 理论 · 物理学 2010-10-27 Rachel Bean , Sarah E. Shandera , S. H. Henry Tye , Jiajun Xu

The slow-roll inflation is a beautiful paradigm, yet the inflaton potential can hardly be sufficiently flat when unknown gravitational effects are taken into account. However, the hybrid inflation models constructed in D = 4 N = 1…

高能物理 - 理论 · 物理学 2014-11-18 Fumikazu Koyama , Yuji Tachikawa , Taizan Watari

This thesis is dedicated to the study of inflationary scenarios based on string theory. Inflation is a brief period of accelerated expansion in the very early Universe which gives natural explanations for problems of the Standard Big Bang…

宇宙学与河外天体物理 · 物理学 2010-02-15 Larissa C. Lorenz

We investigate whether explicit models of warped D-brane inflation are possible in string compactifications. To this end, we study the potential for D3-brane motion in a warped conifold that includes holomorphically-embedded D7-branes…

高能物理 - 理论 · 物理学 2008-11-26 Daniel Baumann , Anatoly Dymarsky , Igor R. Klebanov , Liam McAllister , Paul J. Steinhardt

We demonstrate an inflationary solution to the cosmological horizon problem during the Hagedorn regime in the early universe. Here the observable universe is confined to three spatial dimensions (a three-brane) embedded in higher…

高能物理 - 理论 · 物理学 2007-05-23 Steven Abel , Katherine Freese , Ian Kogan

We demonstrate an inflationary solution to the cosmological horizon problem during the Hagedorn regime in the early universe. Here the observable universe is confined to three spatial dimensions (a three-brane) embedded in higher…

高能物理 - 理论 · 物理学 2014-11-18 Steven Abel , Katherine Freese , Ian Kogan

The pre-big-bang cosmology inspired by superstring theories has been suggested as an alternative to slow-roll inflation. We analyze, in both the Jordan and Einstein frames, the effect of spatial curvature on this scenario and show that too…

高能物理 - 理论 · 物理学 2016-08-25 Michael S. Turner , Erick J. Weinberg

We present a curvaton model from type IIB string theory compactified on a warped throat with approximate isometries. Considering an (anti-)D3-brane sitting at the throat tip as a prototype standard model brane, we show that the brane's…

高能物理 - 理论 · 物理学 2009-07-21 Takeshi Kobayashi , Shinji Mukohyama

We argue that brane anti-brane inflation in string theory de-Sitter vacua of Kachru-Kallosh-Linde-Trivedi (KKLT) is captured by the dynamics of a D3-brane probe in the local KKLT model constructed in hep-th/0203041. This provides a…

高能物理 - 理论 · 物理学 2010-04-05 Alex Buchel , Radu Roiban

We analyse the cosmological implications of brane-antibrane systems in string-theoretic orbifold and orientifold models. In a class of realistic models, consistency conditions require branes and antibranes to be stuck at different fixed…

高能物理 - 理论 · 物理学 2014-11-18 C. P. Burgess , P. Martineau , F. Quevedo , G. Rajesh , R. -J. Zhang

String theory gives rise to various mechanisms to generate primordial inflation, of which ``brane inflation'' is one of the most widely considered. In this scenario, inflation takes place while two branes are approaching each other, and the…

高能物理 - 理论 · 物理学 2009-11-10 R. Brandenberger , G. Geshnizjani , S. Watson