About
The self force problem is ubiquitous in astrophysics and cosmology. It is defined by the following situation. An object moves in contact with an external system (S), which may or may not break Poincare invariance. The motion of the object deforms S which then back-reacts on the particle and changes its dynamics. When S is Poincare invariant this is often called "Radiation Reaction Forces" while when it S violates this symmetry it often called (incompletely) "Dynamical Friction". In this talk I will introduce an effective field theory which can describe both cases in the context. This theory turns out to have an interesting renormalization group flow in the context of the Schwinger Keldysh formalism and allows one to calculate in a systematic way for any choice of S.
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The talk
Credits and licence
- Institution
- CERN
- Speaker
- Ira Rothstein
- Year
- 2026
- Language
- English
- Source
- CERN
- Licence
- CERN, as CERN states it. CERN's terms
- Attribution
- © CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
- Who can watch
- CERN gives no rating. Invisible Network shows it to Teens profiles and older, judged from what the source says about it. How courses are placed