Primordial magnetic fields from dark energy

Da Shin Lee; Wolung Lee; Kin Wang Ng

doi:10.1016/S0370-2693(02)02264-5

Primordial magnetic fields from dark energy

Da Shin Lee^*
, Wolung Lee
, Kin Wang Ng

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

24 Citations (Scopus)

Abstract

Evidences indicate that the dark energy constitutes about two thirds of the critical density of the universe. If the dark energy is an evolving pseudo scalar field that couples to electromagnetism, a cosmic magnetic seed field can be produced via spinoidal instability during the formation of large-scale structures.

Original language	English
Pages (from-to)	1-7
Number of pages	7
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	542
Issue number	1-2
DOIs	https://doi.org/10.1016/S0370-2693(02)02264-5
Publication status	Published - 2002 Aug 22
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/S0370-2693(02)02264-5

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title = "Primordial magnetic fields from dark energy",

abstract = "Evidences indicate that the dark energy constitutes about two thirds of the critical density of the universe. If the dark energy is an evolving pseudo scalar field that couples to electromagnetism, a cosmic magnetic seed field can be produced via spinoidal instability during the formation of large-scale structures.",

author = "Lee, \{Da Shin\} and Wolung Lee and Ng, \{Kin Wang\}",

note = "Funding Information: We would like to thank Daniel Boyanovsky and Hector de Vega for many interesting discussions and suggestions. This work of D.S.L. (W.L. and K.W.N.) was supported in part from National Science Council, ROC under the Grant NSC 90-2112-M-259-011 (NSC 89-2112-M-001-060).",

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doi = "10.1016/S0370-2693(02)02264-5",

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T1 - Primordial magnetic fields from dark energy

AU - Lee, Da Shin

AU - Lee, Wolung

AU - Ng, Kin Wang

N1 - Funding Information: We would like to thank Daniel Boyanovsky and Hector de Vega for many interesting discussions and suggestions. This work of D.S.L. (W.L. and K.W.N.) was supported in part from National Science Council, ROC under the Grant NSC 90-2112-M-259-011 (NSC 89-2112-M-001-060).

PY - 2002/8/22

Y1 - 2002/8/22

N2 - Evidences indicate that the dark energy constitutes about two thirds of the critical density of the universe. If the dark energy is an evolving pseudo scalar field that couples to electromagnetism, a cosmic magnetic seed field can be produced via spinoidal instability during the formation of large-scale structures.

AB - Evidences indicate that the dark energy constitutes about two thirds of the critical density of the universe. If the dark energy is an evolving pseudo scalar field that couples to electromagnetism, a cosmic magnetic seed field can be produced via spinoidal instability during the formation of large-scale structures.

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UR - https://www.scopus.com/pages/publications/0037158745#tab=citedBy

U2 - 10.1016/S0370-2693(02)02264-5

DO - 10.1016/S0370-2693(02)02264-5

M3 - Article

AN - SCOPUS:0037158745

SN - 0370-2693

VL - 542

SP - 1

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JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

IS - 1-2

ER -

Primordial magnetic fields from dark energy

Abstract

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