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Dirac matter

Condensed matter system

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Definition

Members of the class of Dirac matter differ significantly in nature. However, all examples of Dirac matter are unified by similarities within the algebraic structure of an effective theory describing them.

General

The general definition of Dirac matter is a condensed matter system where the quasi-particle excitations can be described in curved spacetime by the generalised Dirac equation:

[iℏvDγaeaμdμ(p)−mvD2]Ψ=0.

In the above definition dμ denotes a covariant vector depending on the (d+1)-dimensional momentum p (d space +1 time dimension), eaμ is the vierbein describing the curvature of the space, m the quasi-particle mass and vD the Dirac velocity. Note that since in Dirac matter the Dirac equation gives the effective theory of the quasiparticles, the energy from the mass term is mvD2, not the rest mass mc2 of a massive particle. γμ refers to a set of Dirac matrices, where the defining for the construction is given by the anticommutation relation,

{γμ,γν}=γμγν+γνγμ=ημνId.

ημν is the Minkowski metric with signature (+ - - -) and Id is the d×d-dimensional unit matrix. In all equations, implicit summation over a and μ is used (Einstein convention). Furthermore, Ψ is the wavefunction. The unifying feature of all Dirac matter is the matrix structure of the equation describing the quasi-particle excitations.

In the limit where dμ(p)=Dμ, i.e. the covariant derivative, conventional Dirac matter is obtained. However, this general definition allows the description of matter with higher order dispersion relations and in curved spacetime as long as the effective Hamiltonian exhibits the matrix structure specific to the Dirac equation.

Common (conventional)

The majority of experimental realisations of Dirac matter to date are in the limit of dμ(p)=Dμ which therefore defines conventional Dirac matter in which the quasiparticles are described by the Dirac equation in curved space-time,

[iℏvDγaeaμDμ−mvD2]Ψ=0.

Here, Dμ denotes the covariant derivative. As an example, for the flat metric, the energy of a free Dirac particle differs significantly from the classical kinetic energy where energy is proportional to momentum squared:

FreeDiracparticle:E=±ℏ2vD2k2+m2c4Kineticenergy:E=m|v|22=|k|22m.

The Dirac velocity vD gives the gradient of the E−k dispersion at large momenta k, m is the mass of particle or object. In the case of massless Dirac matter, such as the fermionic quasiparticles in graphene or Weyl semimetals, the energy-momentum relation is linear,

E(k)=ℏvD|k|

Therefore, conventional Dirac matter includes all systems that have a linear crossing or linear behavior in some region of the energy-momentum relation. They are characterised by features that resemble an 'X', sometimes tilted or skewed and sometimes with a gap between the upper ∨ and lower ∧ parts (the turning points of which become rounded if the origin of the gap is a mass term).

The general features and some specific examples of conventional Dirac matter are discussed in the following sections.

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