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相关论文: Interaction Rates in String Gas Cosmology

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We study string gas dynamics in the early universe and seek to realize the Brandenberger - Vafa mechanism - a goal that has eluded earlier works - that singles out three or fewer spatial dimensions as the number which grow large…

高能物理 - 理论 · 物理学 2014-11-20 Brian Greene , Dan Kabat , Stefanos Marnerides

Thermal history of the string universe based on the Brandenberger and Vafa's scenario is examined. The analysis thereby provides a theoretical foundation of the string universe scenario. Especially the picture of the initial oscillating…

高能物理 - 理论 · 物理学 2009-10-22 H. Cateau , K. Sumiyoshi

We investigate some classical aspects of fundamental strings via numerical experiments. In particular, we study the thermodynamics of a string network within a toroidal universe, as a function of string energy density and space…

高能物理 - 理论 · 物理学 2009-10-28 Mairi Sakellariadou

Brandenberger and Vafa have proposed the string cosmological model based on T-duality. In this model, they took the toroidal target space and introduced the new position \tilde{x} conjugate to the winding mode, in addition to the position x…

高能物理 - 理论 · 物理学 2009-10-30 Kenji Hotta , Keiji Kikkawa , Hiroshi Kunitomo

We study string dynamics in the early universe. Our motivation is the proposal of Brandenberger and Vafa, that string winding modes may play a key role in decompactifying three spatial dimensions. We model the universe as a homogeneous but…

高能物理 - 理论 · 物理学 2014-11-18 Richard Easther , Brian R. Greene , Mark G. Jackson , Daniel Kabat

We introduce a very early universe model based on the thermodynamics of a gas of closed strings in a background which is non-perturbative in $\alpha'$. Upon considering the fully $\alpha'$-corrected equations extended to include certain…

高能物理 - 理论 · 物理学 2021-03-04 Heliudson Bernardo , Robert Brandenberger , Guilherme Franzmann

The purpose of this review is to discuss recent developments occurring at the interface of cosmology with string and M-theory. We begin with a short review of 1980s string cosmology and the Brandenberger-Vafa mechanism for explaining…

高能物理 - 理论 · 物理学 2014-11-18 Damien A. Easson

We study the interaction of several types of static straight cosmic strings, including local strings, global strings, and bosonic superconducting strings with and without magnetic currents. First, we evaluate the interaction energy of two…

高能物理 - 唯象学 · 物理学 2023-09-12 Kohei Fujikura , Siyao Li , Masahide Yamaguchi

Motivated in part by string theory, we consider the idea that the standard LambdaCDM cosmological model might be modified by the effect of a long-range scalar dark matter interaction. The variant of this widely-discussed notion considered…

高能物理 - 理论 · 物理学 2009-11-10 Steven S. Gubser , P. J. E. Peebles

We derive the 4D low energy effective field theory for a closed string gas on a time dependent FRW background. We examine the solutions and find that although the Brandenberger-Vafa mechanism at late times no longer leads to radion…

高能物理 - 理论 · 物理学 2009-11-10 Thorsten Battefeld , Scott Watson

We revisit the study of string theory close to the Hagedorn temperature with the aim towards cosmological applications. We consider interactions of open and closed strings in a gas of D$p-$branes, and/or one isolated D$p$-brane, in an…

高能物理 - 理论 · 物理学 2024-03-25 Andrew R. Frey , Ratul Mahanta , Anshuman Maharana , Francesco Muia , Fernando Quevedo , Gonzalo Villa

We derive analytic expressions for the interaction energy between two general $U(1)$ cosmic strings as the function of their relative orientation and the ratio of the coupling constants in the model. The results are relevant to the…

高能物理 - 唯象学 · 物理学 2009-10-28 L. M. A. Bettencourt , R. J. Rivers

String Gas Cosmology is a model of the evolution of the very early universe based on fundamental principles and key new degrees of freedom of string theory which are different from those of point particle field theories. In String Gas…

高能物理 - 理论 · 物理学 2015-05-28 Robert H. Brandenberger

Cosmic strings are topological defects possibly formed in the early Universe, which may be observable due to their gravitational effects on the cosmic microwave background radiation or gravitational wave experiments. To this effect it is…

宇宙学与河外天体物理 · 物理学 2017-03-01 R. P. L. Azevedo , C. J. A. P. Martins

In the Brandenberger-Vafa scenario of string gas cosmology, the Universe starts as a small torus of string length dimension filled with a hot gas of strings. In such extreme conditions, in addition to the departure from Einstein gravity…

高能物理 - 理论 · 物理学 2009-11-11 Monica Borunda , Lotfi Boubekeur

We present a critical review and summary of String Gas Cosmology. We include a pedagogical derivation of the effective action starting from string theory, emphasizing the necessary approximations that must be invoked. Working in the…

高能物理 - 理论 · 物理学 2008-11-26 Thorsten Battefeld , Scott Watson

We investigate scaling and correlations of the energy and momentum in an evolving network of cosmic strings in Minkowski space. These quantities are of great interest, as they must be understood before accurate predictions for the power…

天体物理学 · 物理学 2009-10-28 Graham R. Vincent , Mark Hindmarsh , Mairi Sakellariadou

Over the past decade it has become clear that fundamental strings are not the only fundamental degrees of freedom in string theory. D-branes are also part of the spectrum of fundamental states. In this paper we explore some possible effects…

高能物理 - 理论 · 物理学 2014-11-18 S. Alexander , R. Brandenberger , D. Easson

The implications of string theory for understanding the dimension of uncompactified spacetime are investigated. Using recent ideas in string cosmology, a new model is proposed to explain why three spatial dimensions grew large. Unlike the…

高能物理 - 理论 · 物理学 2010-11-01 Gerald B. Cleaver , Philip J. Rosenthal

Brane gas cosmology is a scenario inspired by string theory which proposes a simple resolution to the initial singularity problem and gives a dynamical explanation for the number of spatial dimensions of our universe. In this work we have…

高能物理 - 理论 · 物理学 2009-11-10 Antonio Campos
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