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相关论文: Brane inflation and reheating

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We show how the motion through the extra dimensions of a gas of branes and antibranes can, under certain circumstances, produce an era of inflation as seen by observers trapped on a 3-brane, with the inflaton being the inter-brane…

高能物理 - 理论 · 物理学 2010-02-03 C. P. Burgess , M. Majumdar , D. Nolte , F. Quevedo , G. Rajesh , R. -J. Zhang

In this lecture I will review the present status of inflation within string-based brane-world scenarios. The idea is to start from a supersymmetric configuration with two parallel static Dp-branes, and slightly break the supersymmetry…

天体物理学 · 物理学 2007-05-23 Juan Garcia-Bellido

We describe a simple mechanism that can lead to inflation within string-based brane-world scenarios. The idea is to start from a supersymmetric configuration with two parallel static Dp-branes, and slightly break the supersymmetry…

高能物理 - 理论 · 物理学 2014-11-18 J. Garcia-Bellido , R. Rabadan , F. Zamora

We discuss various realizations of the four dimensional braneworld inflation in warped geometries of string theory. In all models the inflaton field is represented by a Dp probe brane scalar specifying its position in the warped throat of…

高能物理 - 理论 · 物理学 2009-11-10 Alex Buchel , Ahmad Ghodsi

We discuss a calculable version of brane inflation, in which a set of parallel D-brane and anti-D-brane worlds, initially displaced in extra dimension, slowly attract each other. In the effective four-dimensional theory this slow motion of…

高能物理 - 理论 · 物理学 2007-05-23 G. Dvali , Q. Shafi , S. Solganik

We study reheating in a recently proposed brane "monodromy inflation" model in which the inflaton is the position of a D4 brane on a "twisted torus". Specifically, we study the repeated collisions between the D4 brane and a D6 brane (on…

高能物理 - 理论 · 物理学 2009-03-27 Robert H. Brandenberger , Anke Knauf , Larissa C. Lorenz

The inflaton potential in four-dimensional theory is rather arbitrary, and fine-tuning is required generically. By contrast, inflation in the brane world scenario has the interesting feature that the inflaton potential is motivated from…

高能物理 - 理论 · 物理学 2011-05-05 Gary Shiu , S. -H. Henry Tye

We consider the interactions between Dp-branes intersecting at an arbitrary number of angles in the context of type II string theory. For cosmology purposes we concentrate in the theory on R^{3,1} x T^6. Interpreting the distance between…

高能物理 - 理论 · 物理学 2009-11-07 M. Gomez-Reino , I. Zavala

We discuss a brane based inflationary scenario in which an initially non-supersymmetric configuration involving a D4 brane is dynamically transformed into a supersymmteric one in a background space-time geometry determined by a stack of D6…

高能物理 - 唯象学 · 物理学 2011-05-12 Bumseok Kyae , Qaisar Shafi

We study inflation arising from the motion of a BPS D3-brane in the background of a stack of k parallel D5-branes. There are two scalar fields in this set up-- (i) the radion field R, a real scalar field, and (ii) a complex tachyonic scalar…

高能物理 - 理论 · 物理学 2008-11-26 Sudhakar Panda , M. Sami , Shinji Tsujikawa , John Ward

In this paper, a inflationary model from the rotation of D4-brane is constructed. We show that for a very wide rage of parameter, this model satisfies the observation and find that regarded as inflaton, the rotation of branes may be more…

高能物理 - 理论 · 物理学 2009-11-10 Yun-Song Piao , Xinmin Zhang , Yuan-Zhong Zhang

As a first step towards inflation in genuinely F-theoretic setups, we propose a scenario where the inflaton is the relative position of two 7-branes on holomorphic 4-cycles. Non-supersymmetric gauge flux induces an attractive inter-brane…

高能物理 - 理论 · 物理学 2013-02-27 Arthur Hebecker , Sebastian C. Kraus , Dieter Lust , Stephan Steinfurt , Timo Weigand

We examine how reheating occurs after brane-antibrane inflation in warped geometries, such as those which have recently been considered for Type IIB string vacua. We adopt the standard picture that the energy released by brane annihilation…

高能物理 - 理论 · 物理学 2008-11-26 N. Barnaby , C. P. Burgess , J. M. Cline

We study inflation and reheating in models for the brane universe, considering hybrid brane inflation without tachyon condensation. We expect that some fields that are localized on different branes interact with O(1) coupling when branes…

高能物理 - 唯象学 · 物理学 2009-11-10 Tomohiro Matsuda

Inflationary models driven by a large number of axion fields are discussed in the context of type IIB compactifications with N=1 supersymmetry. The inflatons arise as the scalar modes of the R-R two-forms evaluated on vanishing two-cycles…

高能物理 - 理论 · 物理学 2008-06-13 Thomas W. Grimm

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

In String theory realizations of inflation, the end point of inflation is often brane-anti brane annihilation. We consider the processes of reheating of the Standard Model universe after brane inflation. We identify the channels of inflaton…

高能物理 - 理论 · 物理学 2014-11-18 Lev Kofman , Piljin Yi

The D3/D7 inflation is studied in the framework of Type 0B string theory. Due to the presence of the closed string tachyon, the constant gauge field flux on the transverse worldvolume of D7-brane is almost arbitrary in having an attractive…

高能物理 - 理论 · 物理学 2007-05-23 Huan-Xiong Yang

The emergence of the cosmological composition (the reheating era) after the inflationary period is analyzed in the framework of the braneworld models, in which our Universe is a three-brane embedded in a five-dimensional bulk, by assuming…

广义相对论与量子宇宙学 · 物理学 2009-11-18 T. Harko , W. F. Choi , K. C. Wong , K. S. Cheng

We construct a model of inflation in string theory after carefully taking into account moduli stabilization. The setting is a warped compactification of Type IIB string theory in the presence of D3 and anti-D3-branes. The inflaton is the…

高能物理 - 理论 · 物理学 2014-11-18 Norihiro Iizuka , Sandip P. Trivedi
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