Projecting a non-Abelian SU(2) vacuum gauge field - a pure gauge constructed from the group element U - onto a fixed (electromagnetic) direction in isospace gives rise to a nontrivial magnetic field, with nonvanishing magnetic helicity, which coincides with the winding number of U. Although the helicity is not conserved under Maxwell (vacuum) evolution, it retains one-half its initial value at infinite time
It has been suggested that the weak magnetic field hosted by the intergalactic medium in cosmic void...
Magnetic helicity, $H$, measures magnetic linkages in a volume. The early theoretical development of...
It is well known that Yang-Mills theory in vacuum has a perturbative instability to spontaneously fo...
Electroweak baryogenesis proceeds via changes in the non-Abelian Chern-Simons number. It is argued t...
Primordial magnetic fields may account for all or part of the fields observed in galaxies. We consid...
We reconsider the topological interpretation of magnetic helicity for magnetic fields in open domain...
We reconsider the topological interpretation of magnetic helicity for magnetic fields in open domain...
CONTEXT: Relative magnetic helicity is conserved by magneto-hydrodynamic evolution even in the prese...
We have carried out numerical simulations of freely decaying magnetohydrodynamic (MHD) turbulence in...
The central result of this thesis is the solution of a decades-old problem in magnetohydrodynamic (M...
Context. Magnetic helicity has the remarkable property of being a conserved quantity of ideal magnet...
The topological underpinning of magnetic fields connected to a planar boundary is naturally describe...
We study the possibility that primordial magnetic fields generated in the transition between inflati...
Relative magnetic helicity is a gauge-invariant quantity suitable for the study of the magnetic heli...
The broad variety of ways in which magnetic helicity affects astrophysical systems, in particular dy...
It has been suggested that the weak magnetic field hosted by the intergalactic medium in cosmic void...
Magnetic helicity, $H$, measures magnetic linkages in a volume. The early theoretical development of...
It is well known that Yang-Mills theory in vacuum has a perturbative instability to spontaneously fo...
Electroweak baryogenesis proceeds via changes in the non-Abelian Chern-Simons number. It is argued t...
Primordial magnetic fields may account for all or part of the fields observed in galaxies. We consid...
We reconsider the topological interpretation of magnetic helicity for magnetic fields in open domain...
We reconsider the topological interpretation of magnetic helicity for magnetic fields in open domain...
CONTEXT: Relative magnetic helicity is conserved by magneto-hydrodynamic evolution even in the prese...
We have carried out numerical simulations of freely decaying magnetohydrodynamic (MHD) turbulence in...
The central result of this thesis is the solution of a decades-old problem in magnetohydrodynamic (M...
Context. Magnetic helicity has the remarkable property of being a conserved quantity of ideal magnet...
The topological underpinning of magnetic fields connected to a planar boundary is naturally describe...
We study the possibility that primordial magnetic fields generated in the transition between inflati...
Relative magnetic helicity is a gauge-invariant quantity suitable for the study of the magnetic heli...
The broad variety of ways in which magnetic helicity affects astrophysical systems, in particular dy...
It has been suggested that the weak magnetic field hosted by the intergalactic medium in cosmic void...
Magnetic helicity, $H$, measures magnetic linkages in a volume. The early theoretical development of...
It is well known that Yang-Mills theory in vacuum has a perturbative instability to spontaneously fo...