Home > Research > Publications & Outputs > Friction domination with superconducting strings
View graph of relations

Friction domination with superconducting strings

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Friction domination with superconducting strings. / Dimopoulos, Konstantinos; Davis, Anne-Christine.
In: Physical Review D, Vol. 57, No. 2, 15.01.1998, p. 692-701.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Dimopoulos, K & Davis, A-C 1998, 'Friction domination with superconducting strings', Physical Review D, vol. 57, no. 2, pp. 692-701. https://doi.org/10.1103/PhysRevD.57.692

APA

Vancouver

Dimopoulos K, Davis A-C. Friction domination with superconducting strings. Physical Review D. 1998 Jan 15;57(2):692-701. doi: 10.1103/PhysRevD.57.692

Author

Dimopoulos, Konstantinos ; Davis, Anne-Christine. / Friction domination with superconducting strings. In: Physical Review D. 1998 ; Vol. 57, No. 2. pp. 692-701.

Bibtex

@article{d4124da1586247f091a82decd1b8f117,
title = "Friction domination with superconducting strings",
abstract = "We investigate the evolution of a superconducting string network with arbitrary, constant string current in the friction dominated regime. In the absence of an external magnetic field the network always reaches a scaling solution. However, for string current stronger than a critical value, it is different than the usual horizon scaling of the nonsuperconducting string case. In this case the friction domination era never ends. Whilst the superconducting string network can be much denser than usually assumed, it can never dominate the universe energy density. It can, however, influence the cosmic microwave background radiation and the formation of large scale structure. When embedded in a primordial magnetic field of sufficient strength, the network never reaches scaling and, thus, eventually dominates the universe evolution.",
author = "Konstantinos Dimopoulos and Anne-Christine Davis",
year = "1998",
month = jan,
day = "15",
doi = "10.1103/PhysRevD.57.692",
language = "English",
volume = "57",
pages = "692--701",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "2",

}

RIS

TY - JOUR

T1 - Friction domination with superconducting strings

AU - Dimopoulos, Konstantinos

AU - Davis, Anne-Christine

PY - 1998/1/15

Y1 - 1998/1/15

N2 - We investigate the evolution of a superconducting string network with arbitrary, constant string current in the friction dominated regime. In the absence of an external magnetic field the network always reaches a scaling solution. However, for string current stronger than a critical value, it is different than the usual horizon scaling of the nonsuperconducting string case. In this case the friction domination era never ends. Whilst the superconducting string network can be much denser than usually assumed, it can never dominate the universe energy density. It can, however, influence the cosmic microwave background radiation and the formation of large scale structure. When embedded in a primordial magnetic field of sufficient strength, the network never reaches scaling and, thus, eventually dominates the universe evolution.

AB - We investigate the evolution of a superconducting string network with arbitrary, constant string current in the friction dominated regime. In the absence of an external magnetic field the network always reaches a scaling solution. However, for string current stronger than a critical value, it is different than the usual horizon scaling of the nonsuperconducting string case. In this case the friction domination era never ends. Whilst the superconducting string network can be much denser than usually assumed, it can never dominate the universe energy density. It can, however, influence the cosmic microwave background radiation and the formation of large scale structure. When embedded in a primordial magnetic field of sufficient strength, the network never reaches scaling and, thus, eventually dominates the universe evolution.

U2 - 10.1103/PhysRevD.57.692

DO - 10.1103/PhysRevD.57.692

M3 - Journal article

VL - 57

SP - 692

EP - 701

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 2

ER -