TY - JOUR
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.
UR - https://www.scopus.com/pages/publications/0037158745
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
EP - 7
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 -