activity
20142025
most citedExtending and Calibrating the Velocity dependent One-Scale model for Cosmic Strings with One Thousand Field Theory Simulations

40 citations · 153 across the 11 of their papers we have counts for

collaborators

12 papers

hep-ph2025

Domain wall evolution beyond quartic potentials: The Sine-Gordon and Christ-Lee potentials

R. Heilemann, M. C. Rosa, J. R. C. C. C. Correia +1

Domain walls are the simplest type of topological defects formed at cosmological phase transitions, and one of the most constrained. Their studies typically assume a quartic double…

hep-ph2024

Evolution of current-carrying string networks

J. R. C. C. C. Correia, C. J. A. P. Martins, F. C. N. Q. Pimenta

Cosmic string networks are expected to form in early Universe phase transitions via the Kibble mechanism and are unavoidable in several Beyond the Standard Model theories. While mo…

astro-ph.CO2022★ 8 cited

Multitension strings in high-resolution U(1)U(1) simulations

J. R. C. C. C. Correia, C. J. A. P. Martins

Topological defects are a fossil relic of early Universe phase transitions, with cosmic strings being the best motivated example. While in most cases one studies Nambu-Goto or Abel…

astro-ph.CO2021

High resolution calibration of string network evolution

J. R. C. C. C. Correia, C. J. A. P. Martins

The canonical velocity-dependent one-scale (VOS) model for cosmic string evolution contains a number of free parameters which cannot be obtained ab initio. Therefore it must be cal…

astro-ph.CO2021★ 13 cited

High resolution calibration of the cosmic strings velocity dependent one-scale model

J. R. C. C. C. Correia, C. J. A. P. Martins

The canonical velocity-dependent one-scale (VOS) model for cosmic string evolution must be calibrated using high resolution numerical simulations, We exploit our state of the art g…

astro-ph.CO2020★ 15 cited

Quantifying the effect of cooled initial conditions on cosmic string network evolution

J. R. C. C. C. Correia, C. J. A. P. Martins

Quantitative studies of the evolution and cosmological consequences of networks of cosmic strings (or other topological defects) require a combination of numerical simulations and…

physics.comp-ph2020

Abelian-Higgs cosmic string evolution with multiple GPUs

J. R. C. C. C. Correia, C. J. A. P. Martins

Topological defects form at cosmological phase transitions by the Kibble mechanism. Cosmic strings and superstrings can lead to particularly interesting astrophysical and cosmologi…

astro-ph.CO2019★ 40 cited

Extending and Calibrating the Velocity dependent One-Scale model for Cosmic Strings with One Thousand Field Theory Simulations

J. R. C. C. C. Correia, C. J. A. P. Martins

Understanding the evolution and cosmological consequences of topological defect networks requires a combination of analytic modeling and numerical simulations. The canonical analyt…

physics.comp-ph2018★ 12 cited

Abelian-Higgs Cosmic String Evolution with CUDA

J. R. C. C. C. Correia, C. J. A. P. Martins

Topological defects form at cosmological phase transitions by the Kibble mechanism, with cosmic strings and superstrings having the most interesting phenomenology. A rigorous analy…

astro-ph.CO2018★ 22 cited

Effects of biases in domain wall network evolution. II. Quantitative analysis

J. R. C. C. C. Correia, I. S. C. R. Leite, C. J. A. P. Martins

Domain walls form at phase transitions which break discrete symmetries. In a cosmological context they often overclose the universe (contrary to observational evidence), although o…

physics.comp-ph2017★ 11 cited

General purpose graphics-processing-unit implementation of cosmological domain wall network evolution

J. R. C. C. C. Correia, C. J. A. P. Martins

Topological defects unavoidably form at symmetry breaking phase transitions in the early Universe. To probe the parameter space of theoretical models and set tighter experimental c…

hep-ph2014★ 32 cited

Effects of Biases in Domain Wall Network Evolution

J. R. C. C. C. Correia, I. S. C. R. Leite, C. J. A. P. Martins

We study the evolution of various types of biased domain wall networks in the early universe. We carry out larger numerical simulations than currently available in the literature a…