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The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity

Posted By: AvaxGenius
The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity

The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity by Paul Ramond
English | EPUB (True) | 2023 | 408 Pages | ISBN : 3031179633 | 40.6 MB

The thesis tackles two distinct problems of great interest in gravitational mechanics — one relativistic and one Newtonian. The relativistic one is concerned with the "first law of binary mechanics", a remarkably simple variational relation that plays a crucial role in the modern understanding of the gravitational two-body problem, thereby contributing to the effort to detect gravitational-wave signals from binary systems of black holes and neutron stars. The work reported in the thesis provides a mathematically elegant extension of previous results to compact objects that carry spin angular momentum and quadrupolar deformations, which more accurately represent astrophysical bodies than mere point particles.

The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity

Posted By: AvaxGenius
The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity

The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity by Paul Ramond
English | PDF (True) | 2023 | 408 Pages | ISBN : 3031179633 | 7.2 MB

The thesis tackles two distinct problems of great interest in gravitational mechanics — one relativistic and one Newtonian. The relativistic one is concerned with the "first law of binary mechanics", a remarkably simple variational relation that plays a crucial role in the modern understanding of the gravitational two-body problem, thereby contributing to the effort to detect gravitational-wave signals from binary systems of black holes and neutron stars. The work reported in the thesis provides a mathematically elegant extension of previous results to compact objects that carry spin angular momentum and quadrupolar deformations, which more accurately represent astrophysical bodies than mere point particles.