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Related papers: Open string tachyon is the stringy inflaton

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We study a simple model of p-adic closed and open strings. It sheds some light on the dynamics of tachyon condensation for both types of strings. We calculate the effect of static and decaying D-brane configurations on the closed string…

High Energy Physics - Theory · Physics 2009-11-10 Nicolas Moeller , Martin Schnabl

In this paper we give an exact analytic solution for tachyon condensation in the modified (picture 0) cubic superstring field theory. We prove the absence of cohomology and, crucially, reproduce the correct value for the D-brane tension.…

High Energy Physics - Theory · Physics 2009-11-18 Theodore Erler

In this thesis we review the fundamental framework of boundary string field theory (BSFT) and apply it to the tachyon condensation on non-BPS systems in the superstring theory. The boundary string field theory can be regarded as a natural…

High Energy Physics - Theory · Physics 2007-05-23 Tadaoki Uesugi

We show that the naive application of the Kibble mechanism seriously underestimates the initial density of cosmic superstrings that can be formed during the annihilation of D-branes in the early universe, as in models of brane-antibrane…

High Energy Physics - Theory · Physics 2009-11-10 Neil Barnaby , Aaron Berndsen , James M. Cline , Horace Stoica

We discuss the problem of tachyon condensation in the framework of background independent open string field theory. We show, in particular, that the computation of the string field theory action simplifies considerably if one looks at…

High Energy Physics - Theory · Physics 2009-10-31 L. Cornalba

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…

High Energy Physics - Theory · Physics 2007-05-23 Huan-Xiong Yang

Inflationary cosmology has provided a predictive and phenomenologically very successful scenario for early universe cosmology. Attempts to implement inflation using scalar fields, however, lead to models with serious conceptual problems. I…

Astrophysics · Physics 2007-05-23 Robert H. Brandenberger

It is widely believed that string theory easily allows for a QCD axion in the cosmologically favoured mass range. The required small decay constant, $f_a\ll M_P$, can be implemented by using a large compactification volume. This points to…

High Energy Physics - Theory · Physics 2022-10-19 Michele Cicoli , Arthur Hebecker , Joerg Jaeckel , Manuel Wittner

This is a short review of string cosmology. We wish to connect string-scale physics as closely as possible to observables accessible to current or near-future experiments. Our possible best hope to do so is a description of inflation in…

High Energy Physics - Theory · Physics 2015-12-07 Alexander Westphal

We review applications of string theory to cosmology, from primordial times to the present-day accelerated expansion. Starting with a brief overview of cosmology and string compactifications, we discuss in detail moduli stabilisation,…

High Energy Physics - Theory · Physics 2023-05-08 Michele Cicoli , Joseph P. Conlon , Anshuman Maharana , Susha Parameswaran , Fernando Quevedo , Ivonne Zavala

These lectures provide an introduction to the subject of tachyon condensation in the open bosonic string. The problem of tachyon condensation is first described in the context of the low-energy Yang-Mills description of a system of multiple…

High Energy Physics - Theory · Physics 2007-05-23 Washington Taylor

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

Although the formulas of tachyon inflation correspond to those of the inflation driven by the ordinary scalar field, there is obvious difference between them, which can not be neglected. We calculate the scalar and tensor perturbation of…

High Energy Physics - Theory · Physics 2014-11-18 Xin-zhou Li , Dao-jun Liu , Jian-gang Hao

We consider the dynamics of the open string tachyon condensation in a framework of the cubic fermionic String Field Theory including a non-minimal coupling with closed string massless modes, the graviton and the dilaton. Coupling of the…

High Energy Physics - Theory · Physics 2009-01-06 I. Ya. Aref'eva , A. S. Koshelev

In spite of its great phenomenological success, current models of scalar field-driven inflation suffer from important unresolved conceptual issues. New fundamental physics will be required to address these questions. String theory is a…

High Energy Physics - Theory · Physics 2008-11-26 Robert H. Brandenberger

We use open string field theory to study the dynamics of unstable branes in the bosonic string theory, in the background of a generic linear dilaton. We find a simple exact solution describing a dynamical interpolation between the…

High Energy Physics - Theory · Physics 2008-03-11 Simeon Hellerman , Martin Schnabl

Thermal inflation was proposed as a mechanism to dilute the density of cosmological moduli. Thermal inflation is driven by a complex scalar field possessing a large vacuum expectation value and a very flat potential, called a `flaton'. Such…

Cosmology and Nongalactic Astrophysics · Physics 2023-04-13 Robert Brandenberger , Aline Favero

Superstring theory has continued to develop at a rapid clip in the past few years. Following a quick review of some of the major discoveries prior to 1998, this talk focuses on a few of the more recent developments. The topics I have chosen…

High Energy Physics - Theory · Physics 2007-05-23 John H. Schwarz

The inflationary scenario has become the paradigm of early universe cosmology, and - in conjuction with ideas from superstring theory - has led to speculations about an "inflationary multiverse". From a point of view of phenomenology, the…

Cosmology and Nongalactic Astrophysics · Physics 2012-05-09 Robert Brandenberger

Towards the end of the brane inflationary epoch in the brane world, cosmic strings (but not texture, domain walls or monopoles) are copiously produced during brane collision. These cosmic strings are D$p$-branes with $(p-1)$ dimensions…

High Energy Physics - Theory · Physics 2009-11-07 Saswat Sarangi , S. -H. Henry Tye