TY - JOUR
T1 - Erratum
T2 - Generation of chiral asymmetry via helical magnetic fields (Physical Review D (2020) 101 (103028) DOI: 10.1103/PhysRevD.101.103028)
AU - Schober, Jennifer
AU - Fujita, Tomohiro
AU - Durrer, Ruth
N1 - Publisher Copyright:
© 2022 American Physical Society.
PY - 2022/3/15
Y1 - 2022/3/15
N2 - This is an erratum to the paper "Generation of chiral asymmetry via helical magnetic fields", published in Phys. Rev. D 101, 103028 (2020). In Figs. 10(d) and 10(h) of this publication, the labels indicate that the kinetic energy spectra Ekink are presented for runs R8mhd and R8, respectively. However, the data shown in Figs. 10(d) and 10(h) corresponds to the magnetic energy spectra Emagk. We present Emagk and Ekink for runs R8mhd and R8 in Fig. 1. In comparison to Emagk, the kinetic energy spectra generally span over a wider range of wave numbers k and have a lower amplitude. The error in the original publication does not affect its conclusion.
AB - This is an erratum to the paper "Generation of chiral asymmetry via helical magnetic fields", published in Phys. Rev. D 101, 103028 (2020). In Figs. 10(d) and 10(h) of this publication, the labels indicate that the kinetic energy spectra Ekink are presented for runs R8mhd and R8, respectively. However, the data shown in Figs. 10(d) and 10(h) corresponds to the magnetic energy spectra Emagk. We present Emagk and Ekink for runs R8mhd and R8 in Fig. 1. In comparison to Emagk, the kinetic energy spectra generally span over a wider range of wave numbers k and have a lower amplitude. The error in the original publication does not affect its conclusion.
UR - http://www.scopus.com/inward/record.url?scp=85127256460&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85127256460&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.105.069901
DO - 10.1103/PhysRevD.105.069901
M3 - Comment/debate
AN - SCOPUS:85127256460
SN - 2470-0010
VL - 105
JO - Physical Review D
JF - Physical Review D
IS - 6
M1 - 069901
ER -