Pis’ma v ZhETF, vol. 110, iss. 12, pp. 812 - 813
© 2019 December 25
Optical properties of px + ipy superconductors with strong impurities
P. A. Ioselevich+∗1), P. M. Ostrovsky∗×
+National Research University Higher School of Economics, 101000 Moscow, Russia
L. D. Landau Institute for Theoretical Physics, 119334 Moscow, Russia
×Max-Planck-Institute for Solid State Research, 70569 Stuttgart, Germany
Submitted 15 November 2019
Resubmitted 27 November 2019
Accepted 27
November 2019
DOI: 10.1134/S0370274X19240081
Observation of the polar Kerr effect in Sr2RuO4
impurity band consisting of Yu-Shiba-Rusinov (YSR)
[1] has lead to theoretical studies of the Hall response
type bound states hosted by the impurities [10-12]. We
σxy(ω) in px + ipy-wave superconductors [2-9]. A non-
derive a semi-circle-shaped density of states centered√
zero σxy implied by the Kerr effect requires either a
at E0 with the bandwidth w =
8nimpΔ| sin3 δ|/πν.
multi-band structure or impurities in the superconduc-
This is valid in the limit of a well-resolved band, w ≪
tor. So far only weak impurities have been considered.
≪E0, Δ - E0.
We generalize existing theory to strong impurities, con-
Equations (2), (3) also describe smoothing of the
sidering their effect on the spectrum of the chiral su-
Bardeen-Cooper-Schrieffer cusp in the density of states
perconductor and on its Hall response in the limit of
at energies close to Δ. This happens on the energy scale
strong, point-like impurities of low concentration nimp.
n2imp/Δν2 which is parametrically smaller than the YSR
Point-like impurities are parametrized by their scat-
bandwidth w.
tering phase δ in the s-channel. It enters the T matrix,
The density of states resulting from Eqs. (2), (3) is
which describes scattering off a single impurity in a clean
illustrated by Fig. 1.
metal to all orders in its potential,
1
T0 =
,
(1)
πν(isignImE - τ3 cotδ)
where E is energy, ν is metallic density of state and τ3
acts in Nambu space. To describe a disordered super-
conducting state, we write down the Dyson equation
G-1 = G-1S - nimp
T,
(2)
where GS = (E - τ3ξ(p) -
Δ)-1 is the clean supercon-
ducting Green’s function with
Δ=Δ(τ1px - τ2py)/|p|
being the px + ipy order parameter.
T is a T matrix
describing scattering in the disordered superconducting
Fig. 1. (Color online) Density of states of the supercon-
state. It is related to T0 via
ductor with strong point-like impurities at cos δ = 0.7,
nimp = 0.06Δν. The semi-circle shape of the YSR impu-
T -T0 =
T( G - G0)T0,
(3)
rity band is distorted due to vicinity to the continuum
where G0
= (E - τ3ξ)-1 is the clean normal-state
Having established the effects of strong impurities
Green’s function. Together, Eqs. (2), (3) form a self-
on the spectrum, we turn to the calculation of σxy(ω).
consistent equation set on the disorder-averaged ob-
The leading contribution in small nimp is given by the
jects
G,T. Solving these, we find that
G(E) exhibits
diagram on the inset of Fig. 2. It contains all orders of
a short cut at energies close to E0 = Δcosδ, where
scattering off a single impurity, with the shaded trian-
Δ is the superconducting gap. This indicates a sub-gap
gles representing T matrices. Calculating the diagram,
1)e-maol: pioselevich@itp.ac.ru
we arrive at
812
Письма в ЖЭТФ том 110 вып. 11 - 12
2019
Optical properties of px + ipy superconductors with strong impurities
813
nimpe2v2Δsin3 δ
R(x ± i0) = (2Δ2 - E0x - x2) ×
σxy(ω) =
×
4
arccos
[
]
,
|x| < Δ,
× R(E0 + ω + i0) + R(E0 - ω - i0) - 2R(E0) ,
(4)
π
Δ2 - x2
x
arccosh
Δ
,
x > Δ,
(5)
×
π
x2 - Δ2
where R(x) is a cumbersome integral (see full text) de-
x
iπ - arccosh
pending on the ratios of x and the three energy pa-
 ∓
Δ
,
x < -Δ.
rameters E0, Δ, and temperature T. The function R(x)
π
x2 - Δ2
is real for |x| < Δ but acquires an imaginary part at
Only the threshold process at ω = Δ + E0 survives at
|x| > Δ. This leads to threshold behavior in σxy(ω) as
T = 0, as seen on Fig.2.
seen on Fig.2. As ω is increased, an imaginary part in
Experiment [1] was limited to ω ∼ 1 eV. In this limit,
σxy first appears at ω = Δ - E0. This threshold corre-
ω ≫ Δ,T we obtain
sponds to processes where occupied YSR states are ion-
nimpe2v2Δsin3 δ
σxy(ω) = -
×
ized into the continuum, and hence this process is sup-
[
3
]
E0
4E0
ω
pressed as ∼ exp(-E0/T ) at low temperatures T ≪ E0.
× itanh
+
ln
(6)
2T
πω
max{Δ, T }
The second threshold appears at ω = Δ + E0 and cor-
responds to Cooper pairs being optically excited into a
In the low-T , weak impurity limit, T ≪ Δ, E0 → Δ,
pair of YSR quasiparticle and continuum quasiparticle.
this reproduces [7] up to parameters used to describe
This process is not thermally activated and therefore
the impurities.
survives at T → 0.
In conclusion, we have considered strong point-like
impurities in px + ipy superconductors. We have shown
such impurites to produce a YSR-type impurity band at
E0 = Δcosδ. We have calculated the anomalous Hall re-
sponse σxy as a function of temperature and frequency.
At high frequencies ω ≫ Δ, T its behavior is similar
to that of weak impurities, while behavior at ω ∼ Δ
is much richer, exhibiting thresholds at ω = Δ - E0
and ω = Δ + E0. The first corresponds to the onset
of ionization of YSR states into the continuum and is
thermally activated while the second involves creation
of continuum + YSR quasiparticle pairs and survives at
T = 0.
This work was supported by the Basic Research Pro-
gram of Higher School of Economics.
Fig. 2. (Color online) Imσxy(ω) (solid lines) and Reσxy(ω)
Full text of the paper is published in JETP Letters
(dashed lines) in a.u. at Δ = 1, E0 = 0.6. Black lines are
journal. DOI: 10.1134/S0021364019240019
at T = 0 while red lines are at T = 0.1. Inset: diagram
representing σxy(ω) in the linear order in nimp
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vated, therefore at low temperatures our result is rele-
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vant up to exponentially small ω ∼ exp(-#E0/T ). Note
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that σxy(ω) shows no features at ω = 2Δ indicating
10. L. Yu, Acta Phys. Sin. 21, 75 (1965).
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that processes where two continuum quasiparticles are
(1968).
created are irrelevant to the Hall response.
12. A. Rusinov, Sov. Phys. JETP 29, 1101 (1969).
At zero temperature, the function R(x) simplifies to
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2019