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Related papers: Cosmic Strings and Cosmic Superstrings

200 papers

In the context of brane world scenario, cosmic superstrings can be formed in D-brane annihilation at the end of the brane inflationary era. The cosmic superstring network has a scaling solution and the characteristic scale of the network is…

High Energy Physics - Theory · Physics 2009-11-10 Mairi Sakellariadou

Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In models which admit strings, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Robert H. Brandenberger

There are two main reasons for the recent renewal of interest in cosmic strings: Fundamental string-theory models suggest their existence; and there are at least two tentative observations of their possible effects. In this talk, I review…

Astrophysics · Physics 2007-05-23 T. W. B. Kibble

In the framework of Supersymmetric Grand Unified Theories (SUSY GUTs), the universe undergoes a cascade of symmetry breakings, during which topological defects can be formed. We address the question of the probability of cosmic string…

High Energy Physics - Phenomenology · Physics 2009-11-11 Jonathan Rocher

Recent developments in string theory suggest that cosmic strings could be formed at the end of brane inflation. Supergravity provides a realistic model to study the properties of strings arising in brane inflation. Whilst the properties of…

High Energy Physics - Theory · Physics 2009-11-11 Ph. Brax , C. van de Bruck , A. C. Davis , Stephen C. Davis

This is a short account, based on a talk given at the 2024 Moriond Cosmology Conference, of where and why string theory matters in early universe cosmology. It is written for a cosmology audience predisposed to be at best sceptical, and at…

Cosmology and Nongalactic Astrophysics · Physics 2024-05-30 Joseph P. Conlon

Many symmetry breaking patterns in grand unified theories (GUTs) give rise to cosmic strings that eventually decay when pairs of GUT monopoles spontaneously nucleate along the string cores. These strings are known as metastable cosmic…

High Energy Physics - Phenomenology · Physics 2024-01-23 Wilfried Buchmuller , Valerie Domcke , Kai Schmitz

A novel mechanism for the production of a cosmic network of fundamental superstrings based on a time-varying string tension has been recently proposed in the context of a kinating background driven by the volume modulus of string…

High Energy Physics - Theory · Physics 2025-03-17 Luca Brunelli , Michele Cicoli , Francisco G. Pedro

In this paper we will discuss how cosmic strings can be used to bridge the gap between the local geometry of our spacetime model and the global topology. The primary tool is the theory of foliations and surfaces, and together with…

Mathematical Physics · Physics 2017-03-22 Christopher L. Duston

Recent developments in cosmic strings are reviewed, with emphasis on unresolved problems.

High Energy Physics - Theory · Physics 2007-06-20 Alexander Vilenkin

Cosmic superstrings are introduced to non-experts. First D-branes and $(p,q)$ strings are discussed. Then we explain how tachyon condensation in the early universe may have produced F, D and $(p,q)$ strings. Warped geometries which can…

High Energy Physics - Theory · Physics 2007-05-23 Mahbub Majumdar

We describe the detailed study and results of high-resolution numerical simulations of string-induced structure formation in open universes and those with a non-zero cosmological constant. The effect from small loops generated from the…

Astrophysics · Physics 2009-09-25 J. H. P. Wu , P. P. Avelino , E. P. S. Shellard , B. Allen

The cosmic string is a useful probe of the early Universe and may give us a clue to physics at high energy scales where any artificial particle accelerators cannot reach. Although one of the most promising tools is the cosmic microwave…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Kohei Kamada , Yuhei Miyamoto , Jun'ichi Yokoyama

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

In a simple reanalysis of the KKLMMT scenario, we argue that the slow roll condition in the D3-anti-D3-brane inflationary scenario in superstring theory requires no more than a moderate tuning. The cosmic string tension is very sensitive to…

High Energy Physics - Theory · Physics 2008-11-26 Hassan Firouzjahi , S. -H. Henry Tye

This paper presents a review of the basic, model-independent differences between the pre-big bang scenario, arising naturally in a string cosmology context, and the standard inflationary scenario. We use an unconventional approach in which…

High Energy Physics - Theory · Physics 2010-04-06 M. Gasperini

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 study the formation and evolution of an interconnected string network in large-scale field-theory numerical simulations, both in flat spacetime and in expanding universe. The network consists of gauge U(1) strings of two different kinds…

High Energy Physics - Theory · Physics 2008-11-26 Jon Urrestilla , Alexander Vilenkin

A class of well-motivated models of inflation end by producing cosmic strings. The current status of efforts to calculate and observe the signals from such models are outlined, with a particular emphasis on cosmic strings, and on the Cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Mark Hindmarsh

We investigate cosmic strings arising from a hierarchical gauge symmetry breaking sequence, $\mathrm{SU}(2) \times \mathrm{U}(1) \rightarrow \mathrm{U}(1) \times \mathrm{U}(1) \rightarrow \mathrm{U}(1)' \rightarrow \text{Nothing}$. This…

High Energy Physics - Phenomenology · Physics 2025-06-19 Akifumi Chitose , Masahiro Ibe , Satoshi Shirai , Yaxuan Wen