Pulsar emission: Langmuir modes in a relativistic multi-component plasma

TL;DR

This paper investigates the properties of Langmuir modes in a relativistic multi-component plasma around pulsars, revealing conditions that stabilize or destabilize these modes and their potential role in generating coherent radio emission.

Contribution

It introduces a detailed analysis of Langmuir modes in a relativistic multi-component plasma, highlighting how electron-positron flux influences plasma stability and mode characteristics.

Findings

Electron-positron flux can stabilize the plasma and extinguish Langmuir modes.

Multi-component Langmuir modes can have growth rates and wavenumbers much larger than ion-proton modes.

These modes likely contribute to plasma turbulence responsible for pulsar radio emission.

Abstract

Ions, protons and possibly a small flux of electrons and positrons are accelerated outward from the polar cap of a normal or millisecond pulsar whose rotational spin is antiparallel with its magnetic moment. The Langmuir modes of this relativistic plasma have several properties of significance for the origin of coherent radio emission. The characteristics of the mode are determined by the sequence of singularities in the dielectric tensor at real angular frequencies, which in turn is fixed by the electron-positron momentum distribution. We find that under a certain condition on its momentum distribution, an electron-positron flux two orders of magnitude smaller than the Goldreich-Julian flux stabilizes the plasma and extinguishes the mode. But more generally, both the growth rate and wavenumber of the multi-component Langmuir mode can be as much as an order of magnitude larger than those of the two-component ion-proton mode. It appears to be a further effective source for the plasma turbulence whose decay is probably responsible for the observed emission.