Attractions between charged colloidal spheres mediated by correlated absorbed ions
We describe arrangements of ions capable of producing short-range attractive interactions between pairs of charged colloidal spheres in the low
23 indexed results
We describe arrangements of ions capable of producing short-range attractive interactions between pairs of charged colloidal spheres in the low
The RunII physics program at the Tevatron started in spring 2001 with protons and antiprotons colliding at an energy of
The state-of-the-art of chemical evolution models for Irregular and Blue Compact galaxies is reviewed. The resulting scenarios for the initial
Thanks to the capabilities of modern telescopes and instrumentation, it is now possible to resolve single stars in external dwarf
The {\it best} chemical evolution models for the galactic disk computed by different groups with different assumptions are compared with
We investigate how the survival of dark matter satellites inside virialized halos depends on tidal stripping and dynamical friction. We
Figure rotation substantially increases the fraction of stochastic orbits in triaxial systems. This increase is most dramatic in systems with
The predictions of Galactic chemical evolution models for D and $^3$He are described in connection with those on the other
NGC6752 hosts in its halo PSR J1911-5958A, a newly discovered binary millisecond pulsar which is the most distant pulsar ever
The five millisecond pulsars that inhabit NGC 6752 display locations or accelerations remarkably different with respect to all other pulsars
In this paper we introduce the methodology used and the basic phases we followed to develop the Catalan WordNet, and
We explore, using an exact cooling code, the thermal evolution of a neutron star undergoing episodes of intense accretion, alternated
Within an adiabatic approximation, thermodynamical equilibrium and a small, nine dimensional, toroidal universe as initial conditions, we analyze the evolution
The stellar initial mass function and the stellar lifetimes are basic ingredients of chemical evolution models, for which different recipes
We investigate the statistical evolution of magnetic neutron stars recycled in Low Mass Binary (LMB) systems, simulating synthetic populations. Irrespective
We present an exact solution for a factorizable brane-world spacetime with two extra dimensions and explicit brane sources. The compactification
Methods are reported for the preparation of mixed-carboxylate versions of the [Mn12O12(O2CR)16(H2O)4] family of single-molecule magnets (SMMs). [Mn12O12(O2CCHCl2)8(O2CCH2But)8(H2O)3] (5) and
The thermal, spin and magnetic evolution of neutron stars in the old low mass binaries is first explored. Recycled to
If rotating core collapse leads to the formation of a proto-neutron star binary in super-close orbit, then the lighter star,
The maximally compact representation of a regular orbit is in terms of its action-angle variables. Computing the map between a
The chemical environment in circumstellar discs is a unique diagnostic of the thermal, physical and chemical environment. In this paper
Was the black hole in XTE J1118+480 ejected from a globular cluster or kicked away from the galactic disk?
This bibliography attempts to give a comprehensive overview of all the literature related to the Ashtekar connection and the Rovelli-Smolin