Gravitational wave emission from a magnetically deformed non barotropic neutron star

MD simulations in this and previous work has allowed us to propose a relation between the nature of the interactions at the interface and the observed properties of nanofluids:

As a strong field ligand, CO affects the magnetic state of MnPc in two ways: (i) it increases the splitting of the d orbitals, and thus favors the low spin configuration in the

When we apply a magnetic field above the upper critical field, we do not find any signature for the magnetic impurities. This shows that there is no strong exchange cou- pling

Our high- resolution images clearly show that the H 2 emission is not uniformly distributed in a torus around the central star as it has been interpreted from previous

In FM films with (twofold) uniaxial magnetic anisotropy (K U ), SO determines symmetric magnetoresistance (MR) responses around the magnetization easy-axis (e.a.) and hard-axis

The figure also shows the results obtained using a standard Newton-based optimization method, and with a GA method using a standard minimum-square objective function.. We can see that

A slowing down of the dynamics is observed as the particle concentration increases or the magnitude of the vertical magnetic field decreases.. When the amplitude of the horizontal

The axial magnetic effect describes the generation of an energy current parallel to an axial magnetic field B 5 (i.e., a magnetic field coupling with opposite signs to the left