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Gravitational systems with variable mass: galaxy merger

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Author(s):
Tiago Amancio da Silva
Total Authors: 1
Document type: Master's Dissertation
Press: Campinas, SP.
Institution: Universidade Estadual de Campinas (UNICAMP). Instituto de Física Gleb Wataghin
Defense date:
Examining board members:
Patricio Anibal Letelier Sotomayor; Vilson Tonin Zanchin; Pedro Cunha de Holanda
Advisor: Patricio Anibal Letelier Sotomayor; Orlando Luis Goulart Peres
Abstract

We study the process of galactic merger, where galaxies are regarded as compact objects with time-dependent masses. This study is made through the analysis of the system's orbit. For this purpose, we consider the gravitational problem of two bodies exchanging mass with a surrounding atmosphere. The Gylden-Mestschersky problem is reviewed in order to be used as a reference for that problem. We propose some models of mass variation, based on a hydrodynamics analogy and on a microscopic analysis of the system. The two-body problem considered is applied to the three-boby problem of varying masses. We found stationary solutions corresponding to the ones of the usual constant masses problem (AU)

FAPESP's process: 07/01207-7 - Galaxy merger: a dynamic systems analysis approach
Grantee:Tiago Amancio da Silva
Support Opportunities: Scholarships in Brazil - Master