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Summer School on Gravitational - Wave Astronomy
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Tides in binary star systems Lecture 1
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Gravitational wave signal
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Interpretation: precise theoretical prediction
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Other objects
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Newtonian theory
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Useful identity
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Taylor expansion of some field Phix around z
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Symmetric trace-free tensor
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For any tensor TL
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Check
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Mass multipole moments
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Example of multipole moments
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In spherical coordinates
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Relation between n Land Yemtheta, phi:
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Example: relation between ni and Yimtheta, phi for i=x
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Potential in A's exterior
Description:
Explore the physics of tides in binary star systems in this comprehensive lecture from the Summer School on Gravitational-Wave Astronomy. Delve into the intricacies of gravitational wave signals, Newtonian theory, and mass multipole moments. Learn about Taylor expansions, symmetric trace-free tensors, and the relation between spherical harmonics and Cartesian coordinates. Gain insights into the potential in a star's exterior and its implications for binary systems. This lecture, delivered by Tanja Hinderer from the Max Planck Institute for Gravitational Physics, is part of a broader program covering various aspects of compact objects and gravitational wave astronomy.

Tides in Binary Star Systems - Lecture 1

International Centre for Theoretical Sciences
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