Charge-velocity-dependent one-scale linear model

@article{Martins2021ChargevelocitydependentOL,
  title={Charge-velocity-dependent one-scale linear model},
  author={Carlos J. A. P. Martins and Patrick Peter and I. Yu. Rybak and E. P. S. Shellard},
  journal={Physical Review D},
  year={2021}
}
C. J. A. P. Martins,1, 2, ∗ Patrick Peter,3, 4, † I. Yu. Rybak,1, 2, ‡ and E. P. S. Shellard4, § Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal Instituto de Astrofísica e Ciências do Espaço, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal GRεCO – Institut d’Astrophysique de Paris, CNRS & Sorbonne Université, UMR 7095 98 bis boulevard Arago, 75014 Paris, France Centre for Theoretical Cosmology, Department of Applied Mathematics and Theoretical Physics… 

Figures from this paper

References

SHOWING 1-10 OF 72 REFERENCES
Models for small-scale structure on cosmic strings. II. Scaling and its stability
We make use of the formalism described in a previous paper [Martins {\it et al.} Phys. Rev. D90 (2014) 043518] to address general features of wiggly cosmic string evolution. In particular, we
Extending and calibrating the velocity dependent one-scale model for cosmic strings with one thousand field theory simulations
Understanding the evolution and cosmological consequences of topological defect networks requires a combination of analytic modeling and numerical simulations. The canonical analytic model for defect
Approach to scaling in axion string networks
Mark Hindmarsh, 2, ∗ Joanes Lizarraga, † Asier Lopez-Eiguren, 4, ‡ and Jon Urrestilla § Department of Physics and Helsinki Institute of Physics, PL 64, FI-00014 University of Helsinki, Finland
Current-carrying cosmic string loop 3D simulation: Towards a reduction of the vorton excess problem
The dynamical evolution of superconducting cosmic string loops with specific equations of state describing timelike and spacelike currents is studied numerically. This analysis extends previous work
Logarithmic equation of state for superconducting cosmic strings
This investigation follows up the suggestion that the equation of state for superconducting cosmic strings provided by Witten's prototype biscalar field model can be well represented by an effective
Superconducting cosmic string: Equation of state for spacelike and timelike current in the neutral limit.
  • Péter
  • Physics
    Physical review. D, Particles and fields
  • 1992
The equation of state relating the tension {ital T} and the energy per unit length {ital U} of a cosmic string is investigated in the simplest nontrivial case, namely, that of a field theory with
Extending the velocity-dependent one-scale string evolution model
We provide a general overview of the velocity-dependent one-scale model for cosmic string evolution and discuss two further extensions to it. We introduce and justify a new ansatz for the momentum
Essentials of Classical Brane Dynamics
This paper provides a self-contained overview of the geometry and dynamics of relativistic brane models, of the category that includes point particle, string, and membrane representations for
Type I Abelian Higgs strings: Evolution and cosmic microwave background constraints
We present results from the first simulations of networks of Type I Abelian Higgs cosmic strings to include both matter and radiation eras and Cosmic Microwave Background (CMB) constraints. In Type I
...
1
2
3
4
5
...