A first principles explanation for the density limit in magnetized plasmas

TL;DR

This paper presents a first principles microscopic model explaining the density limit in magnetized plasmas, showing that the maximum density is proportional to the square of the magnetic field and matches empirical data well.

Contribution

It introduces a simple first principles model that predicts the plasma density limit in tokamaks, linking it to fundamental electrodynamics without adjustable parameters.

Findings

Derived a density limit law proportional to B^2

The theoretical limit agrees well with empirical data

Identified the loss of collective behavior in continuum approximation

Abstract

Fusion research on magnetic confinement is confronted with a severe problem concerning the electron densities ne to be used in fusion devices. Indeed, high densities are mandatory for obtaining large efficiencies, whereas it is empirically found that catastrophic disruptive events occur for densities exceeding a maximal one n^M_e. On the other hand, despite the large theoretical work there is no widely accepted, first principles model for the density limit (see [1], abstract). Here, we propose a simple microscopic model of a magnetized plasma suited for a tokamak, for which the existence of a density limit is proven. This property turns out to be a general collective feature of electrodynamics of point charges, which is lost in the continuum approximation. The law we find is n^M_e = 1.74 1/(me c^2) B^2/ \mu_0, (1), where \mu_0 is the vacuum permeability, c the speed of light, me the electron mass, and B the magnetic field. As shown in Fig. 1, the theoretical limit (big circles) is in rather good agreement with the empirical data, actually a surprisingly good one for a model based on first principles, with no adjustable parameter.