[PDF] Top 20 Hall equilibria with toroidal and poloidal fields: application to neutron stars

... in neutron star crusts have tended to focus on the natural approach of starting with an ini- tial field and following its evolution under the joint action of the Hall effect and ... See full document

... stratified stars, numerical magnetohydrodynamics simulations have shown that arbi- trary initial magnetic fields evolve into stable equilibrium configurations, usually containing nearly axisymmetric, linked ... See full document

... main-sequence stars, white dwarfs, and neutron stars are known to possess stable, large-scale magnetic fi ...magnetohydrodynamic equilibria can exist in non-barotropic, stably ... See full document

... Magnetic fields in upper main-sequence stars, white dwarfs and neutron stars are known to persist for time-scales comparable to their ...non-barotropic stars, ... See full document

... magneto-hydrostatic equilibria appear to exist in stars whenever the matter in their interior is stably stratified (not ...These equilibria are not force-free and not required to ... See full document

... field with a possibly realistic, axially symmetric configuration in a solid star with non-uniform electron ...2) and specialize it to the two inde- pendent scalar functions determining the ... See full document

... order to study the possible presence of instabilities, Rheinhardt & Geppert (2002) studied a homogeneous plane- parallel model and performed a perturbation analysis against a background field that lies ... See full document

... on to show how these extremely strong fields are actually weak in terms of their effects on the stellar ...magnetic stars on the upper main sequence and magnetic white dwarfs, which have similar total ... See full document

... bulge stars is compared to the results of stable-light- curve RRab stars in M3 in ...bulge stars in this plot indicates that they are similar to the variables in M3, ...I- and ... See full document

... required to reach magnetohy- drostatic quasi-equilibrium, the neutrons and charged particles move relative to each other with different velocities and are af- fected by collisional ... See full document

... necessary to separate insoluble excipi- ...extraction with SPE-SCX resin in order to eliminate its interference on the absorbance of the ...found to be highly precise, having a relative ... See full document

... This thesis is devoted to the characterization of a search method for continuous gravitational wave signals from unknown sources - neutron stars that do not beam a radio signal in Earth’[r] ... See full document

... consistent and predictive description of quantum gravity is a long-standing ...us to derive equations for the running of couplings of an effective average action without any power expansion in the ... See full document

... fluids and fluid mixtures, Part II, IUPAC, Commission on Thermodynamics, Elsevier, ...equilibrium and stability analysis using homotopy continuation in the complex ...Computers and Chemical ... See full document

... close to the isochrone at a distance of approximately 10 ...spread, and population size, this filamentary structure is suggestive of the 9 kpc Sgr Tidal Stream predicted by the LM10 ...interesting ... See full document

... disks with spherical symmetry in the inner regions, two stellar sech 2 thick disks, a gaseous exponential disk, and a spherical structure associated with the dark matter ...bar and the ... See full document

... measured and calculated paths in the power versus incore delta-I surveillance plot, as registered every 5 minutes along 32 hours, during a routine operating procedure at partial power, for valves testing, in cycle ... See full document

... performing and improving our pasper code and we needed some variable stars to check the performance of our ...B and Be star variables in the low metallicity environment of the ... See full document

... illuminated and non ‑ illuminated ...intensity and exposure time ...similar and their minima are located at the square sides, the absolute value in the non‑illuminated face is one order of magnitude ... See full document

... ment and Na within the two groups, which would be expected if these elements are all produced by the same AGB stars of higher ...However, stars with initial masses >3 M will evolve in 300 ... See full document