Revisiting relaxation in globular clusters

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• Chris Hamilton (DAMTP)
• Friday 15 June 2018, 11:30-12:30
• Kavli Large Meeting Room, Kavli Building.

If you have a question about this talk, please contact ma557.

The classical (Spitzer-Chandrasekhar) theory of cluster relaxation is unsatisfactory because it involves the Coulomb logarithm and completely neglects the cluster’s self-gravity. A modern alternative is the Balescu-Lenard (BL) equation, which has no such ill-defined parameter and includes self-gravity. The BL equation has recently explained the secular evolution of collisionless stellar discs. In this talk I will review the classical theory and demonstrate its pitfalls, showing at each stage why the BL equation does a better job. I will then present the first application of the BL formalism to spherical systems. I will show how the BL flux through action space differs from the corresponding classical flux, and discuss what a complete theory of cluster relaxation might entail.

This talk is part of the Galaxies Discussion Group series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology, Astrophysics and General Relativity
• Galaxies Discussion Group
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Kavli Large Meeting Room, Kavli Building

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