Synchrotron Firehose Instability

Journal article

Low density plasmas in curved spacetimes, such as those found in accretion flows around black holes, are challenging to model from first principles, owing to the large scale separation between the characteristic scales of the microscopic processes and large mean-free-paths comparable to the system sizes. Kinetic approaches become necessary to capture the relevant physics but lack the dynamic range to model the global characteristics of the systems. In this paper, we develop new covariant guiding center equations of motion for charges in general relativistic spacetimes that are computationally tractable. We decompose the particle motion into a fast gyration, which we integrate analytically and a slow drift of the guiding center, which can be solved numerically. We derive covariant conservation laws for the motions of the guiding centers and show, through a number of limiting cases, that the equations contain all known drift mechanisms. Finally, we present the general relativistic expressions for the various drift velocities in Schwarzschild spacetimes.Comment: Submitted to Ap

Authors: Zhdankin, V; Kunz, MW; Uzdensky, DA

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: American Astronomical Society
• Journal: The Astrophysical Journal
• Volume: 944
• Issue: 1
• Pages: 24-24
• Publication date: 2023-02-09
• DOI: 10.3847/1538-4357/acaf54
• EISSN: 1538-4357
• ISSN: 0004-637X
• Language: English
• Keywords: Magnetic field; Electron; Instability; Synchrotron radiation; Physics; Quantum mechanics; Electron cooling; Plasma; Nuclear physics; Atomic physics