Detailed study of defect models for cosmic structure formation
We calculate predictions from wide class of `active' models of cosmic\nstructure formation which allows us to scan the space of possible defect\nmodels. We calculate the linear ...
We calculate predictions from wide class of `active' models of cosmic\nstructure formation which allows us to scan the space of possible defect\nmodels. We calculate the linear ...
The treatment of first-order phase transitions for standard grand unified theories is shown to break down for models with radiatively induced spontaneous symmetry breaking. It i...
h-index: Number of publications with at least h citations each.