
2 FRANK R ¨
OSLER AND CHRISTIANE TRETTER
The urgent need to classify computational problems in spectral theory in the SCI Hierarchy is further
substantiated by parallel research on challenges in spectral approximation such as spectral pollution or
spectral invisibility and methods to avoid them, see e.g. [10], [11]. In recent years, since the fundamental
work [6] which contains a detailed study on computing the spectra and pseudospectra of bounded matrix
operators on `2pNqas well as results on computing spectra and pseudospectra of Schr¨odinger operators
with potentials satisfying a uniform BV bound (cf. [6, Thm. 8.3, 8.5]), the SCI theory has been further
developed in multiple directions. We mention the works [17,19,39] on matrix operators; [5,18] on
solving PDEs; [20] on the computation of spectral measures, and [7,8] on the computation of scattering
resonances.
While many of the above works obtained results on the (nonrelativistic) Schr¨odinger equation, no
SCI results seem to exist so far on relativistic models, such as the Klein-Gordon or Dirac equations. The
present article begins to fill this gap: we study the spectral problem for the Klein-Gordon equation in the
framework of the SCI Hierarchy. The novelty of this contribution is computational, physically relevant
as well as mathematical. Indeed, the spectral problem for the Klein-Gordon equation is non-standard
in the sense that one is lead to the study of quadratic operator pencils rather than classical eigenvalue
equations which lead to linear monic pencils. Moreover, essential spectrum is not only present but it is
not semi-bounded; even bounded symmetric potentials may create complex eigenvalues in addition to the
two unbounded rays of real essential spectrum. Accordingly, new methods are needed to study spectral
computation which require an intimate interplay of analysis and numerics with operator theory. The
development and evaluation of these techniques, along with corresponding implementable algorithms,
are the focus of this article.
In the next two subsections we present our main results on the computational spectral problem for the
Klein-Gordon equation and we introduce the SCI hierarchy allowing us to interpret our results therein.
1.1. The Klein-Gordon equation. In quantum mechanics the Klein-Gordon equation
(1.1) ˆ´´´i~B
Bt´eϕ¯2
`c2´´i~∇´e
c
~
A¯2
`m2c4˙U“0
describes the motion of a relativistic spinless particle with mass mand charge ein an electromagnetic
field with scalar potential ϕand vector potential ~
A; here cis the speed of light and ~is the Planck
constant. If we separate time by setting Upx, tq“: eiλ{~tupxq,xPRd,tPR, normalize cto 1, let Vbe
the multiplication operator by eϕ in L2pRdqand A0:“p´i~∇´e~
Aq2, then (1.1) leads to a quadratic
eigenvalue problem in λ, which we will cast in a more abstract framework.
To this end, let pH,x¨,¨yq be a separable Hilbert space, let A0be a nonnegative operator on Hand
H0:“A0`m2with mą0. If Vis a symmetric operator with dom H1{2
0Ădom V, the operator
V H´1{2
0is bounded in H. Then the quadratic eigenvalue problem associated with (1.1) is of the form
TVpλqu“0, λPC, where the Klein-Gordon operator polynomial (or pencil) in His given by
TVpλq:“H0´ pV´λq2,dom TVpλq “ dom H0, λ PC.
If we assume that S:“V H´1{2
0“S0`S1with a strict contraction S0and compact S1, as in [28], [29],
[30], then it is well-known that the essential spectrum of TVhas a gap around 0 and that the non-real
spectrum of TVis discrete, see [28], [29]. Moreover, one can show that if S0“0, then the essential
spectrum of TVis given by the half lines p´8,´msYrm, 8q and any other spectral points are discrete
eigenvalues. We ensure that S0“0 by making the following assumptions throughout the paper.
Hypothesis 1.1. Unless otherwise stated, assume that H“L2pRdq, and ~
A“0, i.e. A0“ ´∆,
dompA0q “ H2pRdq. Moreover, assume that
(i) VPW1,ppRdqfor some pąd,
(ii) there exists a constant Mą0 such that
}V}W1,ppRdqďM, |Vpxq| ď Mp1` |x|2q´1
2for all xPRd.(HM)
It is easy to see from the Fr´echet-Kolmogorov-Riesz theorem [34, Th. XIII.66] that Hypothesis 1.1
implies compactness of V H´1{2
0and thus S0“0. Therefore
σesspTVq “ σesspT0q“tλPC|λ2PσpH0qu “ ´aσpH0q Y aσpH0q,