Neutron starsThe ultimate goal of studying isospin physics via heavy-ion reactions with neutron-rich, stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear effective interac
We also show that two neutron stars in a binary have to be within 4% of each other in mass, for neutron stars sufficiently massive that they escape helium shell burning. For those that are so light that they do have helium shell burning, after a small correction for this, they must be...
Stars and stellar systems of all masses go through periods when they are surrounded by large amounts of circumstellar (CS) material in the form of gas and dust. These periods have different durations which mostly depend on the objects’ masses and orbital separations in multiple systems. The ...
This put in evidence the main limits of a system based on fossil fuels, that are limited on our planet and whose combustion is at the bases of major air pollution and of the green-house effect mostly due to CO2 intense emissions. The predicted effects of the latter are dramatic, as ...