The Scales of Gravitational Lensing
F. De PaolisDepartment of Mathematics and Physics “Ennio De Giorgi”, University of Salento, CP 193, I-73100 Lecce, ItalyMosé GiordanoDepartment of Mathematics and Physics “Ennio De Giorgi”, University of Salento, CP 193, I-73100 Lecce, ItalyG. IngrossoDepartment of Mathematics and Physics “Ennio De Giorgi”, University of Salento, CP 193, I-73100 Lecce, ItalyL. ManniDepartment of Mathematics and Physics “Ennio De Giorgi”, University of Salento, CP 193, I-73100 Lecce, ItalyAchille NucitaDepartment of Mathematics and Physics “Ennio De Giorgi”, University of Salento, CP 193, I-73100 Lecce, ItalyF. StrafellaDepartment of Mathematics and Physics “Ennio De Giorgi”, University of Salento, CP 193, I-73100 Lecce, Italy
2016en
ABI
Аннотация
After exactly a century since the formulation of the general theory of relativity, the phenomenon of gravitational lensing is still an extremely powerful method for investigating in astrophysics and cosmology. Indeed, it is adopted to study the distribution of the stellar component in the Milky Way, to study dark matter and dark energy on very large scales and even to discover exoplanets. Moreover, thanks to technological developments, it will allow the measure of the physical parameters (mass, angular momentum and electric charge) of supermassive black holes in the center of ours and nearby galaxies.
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