Tiago Floriano

A Brief Introduction To Black Holes: From Newton to String Theory (English Edition: for United States, Germany, United Kingdom, Canada, Italy, India and Brazil)

The end of some stars could be to become a nebula after a cataclysmic explosion, creating an environment conducive to the formation of new stars and seeding the nearby objects with the chemical elements that constituted it, or to become a neutron star, depending on what. left over from the explosion. Another possibility, depending on how heavy the star is, which no longer has the strength to overcome gravity, is to collapse gravitationally and become a black hole. In A Brief Introduction To Black Holes we will explore all the particularities of these incredible objects that have intrigued us for centuries!