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Primordial magnetic fields in false vacuum inflation

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Primordial magnetic fields in false vacuum inflation. / Davis, Anne-Christine; Dimopoulos, Konstantinos.
In: Physical Review D, Vol. 55, No. 12, 15.06.1997, p. 7398-7414.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Davis, A-C & Dimopoulos, K 1997, 'Primordial magnetic fields in false vacuum inflation', Physical Review D, vol. 55, no. 12, pp. 7398-7414. https://doi.org/10.1103/PhysRevD.55.7398

APA

Vancouver

Davis A-C, Dimopoulos K. Primordial magnetic fields in false vacuum inflation. Physical Review D. 1997 Jun 15;55(12):7398-7414. doi: 10.1103/PhysRevD.55.7398

Author

Davis, Anne-Christine ; Dimopoulos, Konstantinos. / Primordial magnetic fields in false vacuum inflation. In: Physical Review D. 1997 ; Vol. 55, No. 12. pp. 7398-7414.

Bibtex

@article{f37fa85687a9472e83b82827b4c920c3,
title = "Primordial magnetic fields in false vacuum inflation",
abstract = "We show that, during false vacuum inflation, a primordial magnetic field can be created, sufficiently strong to seed the galactic dynamo and generate the observed galactic magnetic fields. Considering the inflaton dominated regime, our field is produced by the Higgs-field gradients, resulting from a grand unified phase transition. The evolution of the field is followed from its creation through to the epoch of structure formation, subject to the relevant constraints. We find that it is possible to create a magnetic field of sufficient magnitude, provided the phase transition occurs during the final 5 e-foldings of the inflationary period.",
author = "Anne-Christine Davis and Konstantinos Dimopoulos",
year = "1997",
month = jun,
day = "15",
doi = "10.1103/PhysRevD.55.7398",
language = "English",
volume = "55",
pages = "7398--7414",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "12",

}

RIS

TY - JOUR

T1 - Primordial magnetic fields in false vacuum inflation

AU - Davis, Anne-Christine

AU - Dimopoulos, Konstantinos

PY - 1997/6/15

Y1 - 1997/6/15

N2 - We show that, during false vacuum inflation, a primordial magnetic field can be created, sufficiently strong to seed the galactic dynamo and generate the observed galactic magnetic fields. Considering the inflaton dominated regime, our field is produced by the Higgs-field gradients, resulting from a grand unified phase transition. The evolution of the field is followed from its creation through to the epoch of structure formation, subject to the relevant constraints. We find that it is possible to create a magnetic field of sufficient magnitude, provided the phase transition occurs during the final 5 e-foldings of the inflationary period.

AB - We show that, during false vacuum inflation, a primordial magnetic field can be created, sufficiently strong to seed the galactic dynamo and generate the observed galactic magnetic fields. Considering the inflaton dominated regime, our field is produced by the Higgs-field gradients, resulting from a grand unified phase transition. The evolution of the field is followed from its creation through to the epoch of structure formation, subject to the relevant constraints. We find that it is possible to create a magnetic field of sufficient magnitude, provided the phase transition occurs during the final 5 e-foldings of the inflationary period.

U2 - 10.1103/PhysRevD.55.7398

DO - 10.1103/PhysRevD.55.7398

M3 - Journal article

VL - 55

SP - 7398

EP - 7414

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 12

ER -