Using only the tools of basic physics, in this article the formation of stellar black holes has been analyzed, describing the evolutionary process followed by a star, starting from its formation to the conclusion of its permanence in the main sequence and to the subsequent gravitational collapse, which will lead, for very massive stars, to the formation of stellar black holes. In the last chapter, the possible types of classification of a black hole were analyzed, highlighting how super-massive black holes can be formed starting from stellar black holes in the galactic centers and dealing with other types of black holes, such as black holes. primordial that cosmological models predict arose after the Big Bang.

I buchi neri: analisi della loro formazione e classificazione / DI MARTINO, Ferdinando; Sessa, Salvatore. - In: PERIODICO DI MATEMATICA. - ISSN 2612-6745. - III:2(2021). [10.53159/PdM(IV).v3n2.045]

I buchi neri: analisi della loro formazione e classificazione

ferdinando di martino
;
salvatore sessa
2021

Abstract

Using only the tools of basic physics, in this article the formation of stellar black holes has been analyzed, describing the evolutionary process followed by a star, starting from its formation to the conclusion of its permanence in the main sequence and to the subsequent gravitational collapse, which will lead, for very massive stars, to the formation of stellar black holes. In the last chapter, the possible types of classification of a black hole were analyzed, highlighting how super-massive black holes can be formed starting from stellar black holes in the galactic centers and dealing with other types of black holes, such as black holes. primordial that cosmological models predict arose after the Big Bang.
2021
I buchi neri: analisi della loro formazione e classificazione / DI MARTINO, Ferdinando; Sessa, Salvatore. - In: PERIODICO DI MATEMATICA. - ISSN 2612-6745. - III:2(2021). [10.53159/PdM(IV).v3n2.045]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/864339
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