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We describe how the strings, which are classical solutions of the continuum three-dimensional U(1)+Higgs theory, can be studied on the lattice. The effect of an external magnetic field is also discussed and the first results on the string…

High Energy Physics - Lattice · Physics 2009-10-31 K. Kajantie , M. Laine , T. Neuhaus , J. Peisa , A. Rajantie , K. Rummukainen

Recently, the chiral superconductivity of the cosmic string in the axion model has gathered attention. The superconductive nature can alter the standard understanding of the cosmology of the axion model. For example, a string loop with a…

High Energy Physics - Phenomenology · Physics 2023-01-11 Masahiro Ibe , Shin Kobayashi , Yuhei Nakayama , Satoshi Shirai

Moduli fields are generally present in superstring--inspired models. They are typically characterized by masses of the order of the supersymmetry breaking scale and by interactions of gravitational strength to ordinary matter. If stable,…

High Energy Physics - Phenomenology · Physics 2009-11-07 Marco Peloso , Lorenzo Sorbo

I argue that string creation may have played a role in reheating the universe after inflation. For strings in four dimensions that arise from branes wrapping cycles in the extra dimensions, estimates from effective field theory show that…

High Energy Physics - Theory · Physics 2017-08-23 Steven S. Gubser

It is presented an exact solution of straight spinning cosmic strings in Brans-Dicke theory of gravitation. The possibility of the existence of closed timelike curves around these cosmic strings is analyzed. Furthermore, the stability about…

General Relativity and Quantum Cosmology · Physics 2022-08-30 S. Mittmann dos Santos , J. M. Hoff da Silva , J. L. Cindra

We first consider local cosmic strings in dilaton-axion gravity and show that they are singular solutions. Then we take a supermassive Higgs limit and present expressions for the fields at far distances from the core by applying a…

General Relativity and Quantum Cosmology · Physics 2014-11-17 Caroline Santos

We describe a new mechanism, whose ingredients are realised in string compactifications, for the formation of cosmic (super)string networks. Oscillating string loops grow when their tension $\mu$ decreases with time. If $2H + \dot{\mu}/\mu…

High Energy Physics - Phenomenology · Physics 2024-06-19 Joseph P. Conlon , Edmund J. Copeland , Edward Hardy , Noelia Sánchez González

We analyze all individual cosmic strings of various lengths in a large ensemble of the global cosmic string networks in the post-inflationary scenario, obtained from numerical simulations on a discrete lattice with $N^3 = 4096^3$. A strong…

High Energy Physics - Phenomenology · Physics 2025-09-19 Heejoo Kim , Minho Son

The spectrum of radially excited hadrons provides much information about the confinement forces in QCD. The confinement is realized most naturally in terms of the QCD string whose quantization gives rise to the radially excited modes. We…

High Energy Physics - Phenomenology · Physics 2013-08-30 S. S. Afonin , A. D. Katanaeva

We investigate properties of several string networks in $D < 10$ which carry electric currents as well as electrostatic charge densities. We show the electric-current conservations as well as the force-balance condition of the string…

High Energy Physics - Theory · Physics 2007-05-23 Alok Kumar , Sudipta Mukherji

We study the behaviour and consequences of cosmic string networks in contracting universes. They approximately behave during the collapse phase as a radiation fluids. Scaling solutions describing this are derived and tested against…

Astrophysics · Physics 2015-06-24 P. P. Avelino , C. J. A. P. Martins , C. Santos , E. P. S. Shellard

The authors study the quantum effect of self-interacting fields in the classical background of conical space, i.e. around a cosmic string with infinitesimal width. The renormalized value of $\langle\phi^2\rangle$ and energy-momentum tensor…

High Energy Physics - Theory · Physics 2019-12-18 Kiyoshi Shiraishi , Satoru Hirenzaki

The influence on cosmic string dynamics of fermionic massive bound states propagating in the vortex, and getting their mass only from coupling to the string forming Higgs field, is studied. Such massive fermionic currents are numerically…

High Energy Physics - Phenomenology · Physics 2009-11-07 Christophe Ringeval

We show that axions can be produced from Abelian-Higgs cosmic strings due to the axion-gauge coupling. The strong magnetic field is confined in the string, and the electric field is induced around the moving string, allowing axion…

High Energy Physics - Phenomenology · Physics 2026-04-29 Naoya Kitajima , Michiru Uwabo-Niibo

Cosmic strings are generic cosmological predictions of many extensions of the Standard Model of particle physics, such as a $U(1)^\prime$ symmetry breaking phase transition in the early universe or remnants of superstring theory. Unlike…

High Energy Physics - Phenomenology · Physics 2018-06-13 Yanou Cui , Marek Lewicki , David E. Morrissey , James D. Wells

We report on the energy-momentum correlators obtained with recent numerical simulations of the Abelian Higgs model, essential for the computation of cosmic microwave background and matter perturbations of cosmic strings. Due to significant…

Cosmology and Nongalactic Astrophysics · Physics 2017-02-28 David Daverio , Mark Hindmarsh , Martin Kunz , Joanes Lizarraga , Jon Urrestilla

We reconsider the effect of electromagnetic radiation from superconducting strings on cosmic microwave background (CMB) mu- and y-distortions and derive present (COBE-FIRAS) and future (PIXIE) constraints on the string tension, mu_s, and…

Cosmology and Nongalactic Astrophysics · Physics 2012-12-18 Hiroyuki Tashiro , Eray Sabancilar , Tanmay Vachaspati

We investigate the region of restored electroweak symmetry around a superconducting cosmic string coupled to the Weinberg-Salam model with an extra Higgs doublet. We show that the presence of the extra Higgs fields, and in particular their…

High Energy Physics - Phenomenology · Physics 2015-06-25 M. Trodden

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…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-01 R. P. L. Azevedo , C. J. A. P. Martins

Under certain conditions the collision and intercommutation of two cosmic strings can result in the formation of a third string, with the three strings then remaining connected at Y-junctions. The kinematics and dynamics of collisions of…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-17 D. A. Steer , Marc Lilley , Daisuke Yamauchi , Takashi Hiramatsu