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Related papers: Puzzles with Tachyon in SSFT and Cosmological Appl…

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We study cosmological perturbations in models with a single non-local scalar field originating from the string field theory description of the rolling tachyon dynamics. We construct the equation for the energy density perturbations of the…

High Energy Physics - Theory · Physics 2012-11-06 Alexey S. Koshelev , Sergey Yu. Vernov

Nonlocal cosmological models derived from String Field Theory are considered. A new method for constructing rolling tachyon solutions in the FRW metric in two field configuration is proposed and solutions of the Friedman equations with…

High Energy Physics - Theory · Physics 2008-11-26 L. Joukovskaya

Cosmological scenarios built upon the generalized non-local String Field Theory and $p$-adic tachyons are examined. A general kinetic operator involving an infinite number of derivatives is studied as well as arbitrary parameter $p$. The…

High Energy Physics - Theory · Physics 2010-10-27 Alexey S. Koshelev

In this note cosmological models coming out of the String Field Theory (SFT) in application to the Dark Energy are reviewed. A way of constructing solutions in the case of linear models is outlined, cosmological perturbations and…

High Energy Physics - Theory · Physics 2014-11-20 Alexey S. Koshelev

There are many different phenomenological models describing the cosmological dark energy and accelerating Universe by choosing adjustable functions. In this paper we consider a specific model of scalar tachyon field which is derived from…

Astrophysics · Physics 2007-05-23 I. Ya. Aref'eva

A string field theory(SFT) nonlocal model of the cosmological dark energy providing w<-1 is briefly surveyed. We summarize recent developments and open problems, as well as point out some theoretical issues related with others applications…

High Energy Physics - Theory · Physics 2008-11-26 Irina Ya. Aref'eva

A general class of cosmological models driven by a non-local scalar field inspired by string field theories is studied. In particular cases the scalar field is a string dilaton or a string tachyon. A distinguished feature of these models is…

High Energy Physics - Theory · Physics 2008-11-26 I. Ya. Aref'eva , L. V. Joukovskaya , S. Yu. Vernov

In this paper we study the tachyon cosmology in non-interacting and interacting cases in non-flat FRW universe. Then we reconstruct the potential and the dynamics of the tachyon field which describe tachyon cosmology.

General Relativity and Quantum Cosmology · Physics 2010-03-12 M R Setare , J Sadeghi , A R Amani

Tachyon condensation in quantum field theory (QFT) plays a central role in models of fundamental interactions and cosmology. Inspired by tower truncation in string field theory, ultraviolet completions were proposed with infinite-derivative…

High Energy Physics - Theory · Physics 2024-04-03 Florian Nortier

We study the role that tachyon fields may play in cosmology as compared to the well-established use of minimally coupled scalar fields. We first elaborate on a kind of correspondence existing between tachyons and minimally coupled scalar…

High Energy Physics - Theory · Physics 2009-11-10 V. Gorini , A. Yu. Kamenshchik , U. Moschella , V. Pasquier

Cosmological implication of rolling tachyons is reported in the context of effective field theory. With a brief review of rolling tachyons in both flat and curved spacetimes, we study the string cosmological model with both tachyon and…

High Energy Physics - Theory · Physics 2007-05-23 Chanju Kim , Hang Bae Kim , Yoonbai Kim , O-Kab Kwon , Chong Oh Lee

A general class of nonlocal cosmological models is considered. A new method for solving nonlocal Friedmann equations is proposed, and solutions of the Friedmann equations with nonlocal operator are presented. The cosmological properties of…

High Energy Physics - Theory · Physics 2008-11-26 Liudmila Joukovskaya

We develop the cosmological perturbations formalism in models with a single non-local scalar field originating from the string field theory description of the rolling tachyon dynamics. We construct the equation for the energy density…

High Energy Physics - Theory · Physics 2012-07-19 Alexey S. Koshelev , Sergey Yu. Vernov

We investigate cosmological dynamics of multiple tachyon fields with inverse square potentials. A phase-space analysis of the spatially flat FRW models shows that there exists power-law cosmological scaling solutions. We study the stability…

High Energy Physics - Theory · Physics 2007-05-23 Zong-Kuan Guo , Yuan-Zhong Zhang

We study dynamics of rolling tachyon and Abelian gauge field on unstable D-branes, of which effective action is given by Born-Infeld type nonlocal action. Possible cosmological evolutions are also discussed. In the Einstein frame of string…

High Energy Physics - Theory · Physics 2007-05-23 Chanju Kim , Hang Bae Kim , Yoonbai Kim , O-Kab Kwon

An overview is presented of some cosmological aspects of string theory. Recent developments are emphasised, especially the attempts to derive inflation or alternatives to inflation from the dynamics of branes in string theory. Time…

High Energy Physics - Theory · Physics 2008-11-26 F. Quevedo

We develop a technique for the reconstruction of the potential for a scalar field or a tachyon field, reproducing a given cosmological evolution in a closed and open isotropic cosmological models. Such potentials are explicitly written down…

General Relativity and Quantum Cosmology · Physics 2015-06-03 Alexander Y. Kamenshchik , Serena Manti

In this note I provide an extended version of the talk given at BW2011 workshop. The concise introduction to the non-local SFT motivated models is given with an emphasis on the non-local generalization of gravity. A number of open questions…

High Energy Physics - Theory · Physics 2012-02-10 Alexey S. Koshelev

We discuss the cosmological implications of some recent advances in understanding the dynamics of tachyon condensation in string theory.

High Energy Physics - Theory · Physics 2017-08-23 Gary Shiu

We consider the appearance of multiple scalar fields in SFT inspired non-local models with a single scalar field at late times. In this regime all the scalar fields are free. This system minimally coupled to gravity can be analyzed…

High Energy Physics - Theory · Physics 2011-01-24 Federico Galli , Alexey S. Koshelev
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