24 3 Brief Review of Models of High-Temperature Superconducting Cuprates
method. However, there are critical opinions for using the simple mean-field
approximation to the exotic spinon–holon picture. In the mean-field approx-
imation for the slave-boson or slave-fermion method, for example, the sum
of the average numbers of spinons and holons must be one. From this, the
average number of spinons becomes large in the underdoped region of holons
which contribute to superconductivity. According to the RVB theory and
thus the t–J model, the spinons contribute to the formation of large Fermi
surfaces. Thus the appearance of a large Fermi surface is expected for the
underdoped region. However, recent ARPES experiments by Yoshida et al.
[23, 24, 25] clearly shows that this is not the case. In this context, the jus-
tification of the t–J model by the mean-field approximation is questionable
unless one can obtain a direct experimental evidence for the existence of
spinon and holon excitation.
3.2.5 Spin Fluctuation Models
Starting from the single-band Hubbard model [98, 99, 100], the d–p model
[101], or an electron dispersion obtained from the “LDA-band calculations
plus Hubbard U ” (the LDA+U band calculations) by treating in a semi-
empirical formalism [102], another model has been introduced as regards the
mechanism of high-T
c
.
Near the half-filled level, strong Hubbard U repulsion between electrons
causes the enhanced q,ω-dependent spin susceptibility χ(q,ω). It takes a
large value around Q =(π/a,π/a)wherea denotes the lattice constant for
the CuO
2
plane. This fact reflects the nearly antiferromagnetic nature of the
system. This large spin fluctuation causes an “overall” attractive interaction
between quasi-particles with different spins, thus leading to the supercon-
ducting transition. Theories depending on such mechanisms are called “spin
fluctuation” models. Here we use the word “overall” in the above sentence
because the interaction caused by the antiferromagnetic spin fluctuation has
both repulsive and attractive components and it appears that in the k-space
it is always positive, i.e., repulsive. From the perturbation theory, the dressed
electron–electron interaction V
eff
is written in terms of U and χ(q,ω), and its
q-dependence is similar to that of χ(q,ω), i.e., it takes a small value around
q = 0, while it takes a very large value at q = Q =(π/a,π/a). Together
with the shape of the Fermi surface which has a large partial density of states
around (π/a, 0) and (0,π/a), we obtain d
x
2
−y
2
-wave superconductivity which
is consistent to the experimental results.
There are various models starting from the above mentioned picture. In
other words, these theories identify the origin of Cooper pair interaction in
HTSC with a large anti-ferromagnetic spin fluctuation of the system, but
they differ in their detail; they differ in the approximation methods to solve
a similar type of model Hamiltonians. These theories can explain normal
state properties of cuprates such as magnetic properties or optical responses.
In most of the theories of this category, they rely on strong antiferromagnetic