Note on bigravity and dark matter

It could maybe seem somehow insubstantial to consider an actual increase in computing power produced merely by a change in representation, consid- ering that computable functions

Here we can verify what we believe constitutes a paradox: the necessity of con- siderations of an ethical kind is imposed, but from that tradition of Economic Theory whose

Following their approach, we define the Fekete points on M and show their connection with the interpolating and M-Z families and prove the asymptotic equidistribution of the

By comparing the predicted rotation curves with observations of dwarf and low surface brightness galaxies, we show that the pressure from dark matter annihilation may improve

The results have been used to constrain the pair production of dark matter particles in models with a heavy mediator, and large extra dimensions in the context of the

The lightest neutralino, ˜ χ 0 1 , is usually assumed to be the LSP, unless R-parity is not conserved, because it is the only MSSM particle which can make a good cold dark

As we have seen, even though the addition of a cosmological constant to Einstein’s eld equations may be the simplest way to obtain acceleration, it has its caveats. For this rea-

We have solved this problem by designing an optimal filter with minimal mode- mixing of the resonant mode to the axion field, which consists on a cascade of cavities connected