Space-time is curved by the presence of massive bodies and this curvature influences the motion of the bodies themselves: this leads to a geometry in constant evolution. One of the consequences is that even light, supposed to be massless, bends its trajectory while passing close to a massive body. The study of light bending started in the XVIII century and a lot of progress was done so far. Gravitational lensing is an important tool in astrophysics and in cosmology widely used to study both populations of compact objects (including exoplanets, black holes and other stellar remnants), and extended objects, such as galaxies, clusters of galaxies and large-scale structures. Since most of the mysteries of our Universe do not show up in observations based on electromagnetic interactions, gravitational lensing is more and more employed to study the dark side of the Universe, including dark matter, dark energy, and any kind of exotic matter (such as wormholes) conjectured by theorists. In the introduction in Chapter 1 we run across the history of gravitational lensing through the explanation of the lens equation, the magnification of images, the description of critical curves and caustics, the binary lenses in the standard theory. In Chapter 2 we focus on gravitational lensing by objects with 1/rn potential giving a complete atlas of the critical curves and caustics in mixed binary systems such as pairs of galaxies with different halos, or cases in which one object is made up of exotic matter and the other one is a normal star or in the case of wormholes when they appear in non-isolated systems. After the amazing discoveries by the GRAVITY collaboration in the last few years on the star S2 orbiting the black hole Sgr A* in the center of the Milky Way, we present in Chapter 3 a detailed investigation of the impact of gravitational lensing on the reconstruction of stellar orbits around this massive black hole. Finally, in Chapter 4 we draw the conclusions of this thesis. [edited by Author]
Gravitational lensing by massive and Exotic objects / Silvia Pietroni , 2023 Feb 21., Anno Accademico 2021 - 2022. [10.14273/unisa-5332].
Gravitational lensing by massive and Exotic objects
Pietroni, Silvia
2023
Abstract
Space-time is curved by the presence of massive bodies and this curvature influences the motion of the bodies themselves: this leads to a geometry in constant evolution. One of the consequences is that even light, supposed to be massless, bends its trajectory while passing close to a massive body. The study of light bending started in the XVIII century and a lot of progress was done so far. Gravitational lensing is an important tool in astrophysics and in cosmology widely used to study both populations of compact objects (including exoplanets, black holes and other stellar remnants), and extended objects, such as galaxies, clusters of galaxies and large-scale structures. Since most of the mysteries of our Universe do not show up in observations based on electromagnetic interactions, gravitational lensing is more and more employed to study the dark side of the Universe, including dark matter, dark energy, and any kind of exotic matter (such as wormholes) conjectured by theorists. In the introduction in Chapter 1 we run across the history of gravitational lensing through the explanation of the lens equation, the magnification of images, the description of critical curves and caustics, the binary lenses in the standard theory. In Chapter 2 we focus on gravitational lensing by objects with 1/rn potential giving a complete atlas of the critical curves and caustics in mixed binary systems such as pairs of galaxies with different halos, or cases in which one object is made up of exotic matter and the other one is a normal star or in the case of wormholes when they appear in non-isolated systems. After the amazing discoveries by the GRAVITY collaboration in the last few years on the star S2 orbiting the black hole Sgr A* in the center of the Milky Way, we present in Chapter 3 a detailed investigation of the impact of gravitational lensing on the reconstruction of stellar orbits around this massive black hole. Finally, in Chapter 4 we draw the conclusions of this thesis. [edited by Author]I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
