C.J. Olson Reichhardt and M.B. Hastings
Center for Nonlinear Studies and Theoretical Division,
Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
(Received 15 July 2003; published 15 April 2004)
We propose an experiment for directly constructing and locally probing topologically entangled states of superconducting vortices which can be performed with present-day technology. Calculations using an elastic string vortex model indicate that as the pitch (the winding angle divided by the vertical distance) increases, the vortices approach each other. At values of the pitch higher than a maximum value the entangled state becomes unstable to collapse via a singularity of the model. We provide predicted experimental signatures for both vortex entanglement and vortex cutting. The local probe we propose can also be used to explore a wide range of other quantities.
DOI: 10.1103/PhysRevLett.92.157002 PACS numbers: 74.25.Qt, 74.25.Sv
The high superconducting transition temperatures of
compounds such as
YBa2Cu3O(7-
)
(YBCO) and
BiSr2Ca2CuO8 (BSCCO)
lead to a very rich set of behaviors of the
magnetic vortices which
form inside the material in the presence of an applied magnetic
field. Thermal fluctuations are significant over a wide range of the
(H,T) phase diagram [1],
causing the lattice of stiff vortex lines to
melt well below Tc. The nature of this molten state has remained
a subject of intense debate. Since there can be significant
thermally-induced wiggling along the length of the vortex in the
liquid state, Nelson proposed that neighboring vortex lines may
become entangled with each other, in analogy with a superfluidity
transition in a boson system [2].
This entanglement could produce a dramatic viscocity increase
[3-5],
similar to that which occurs for entangled polymers.
This would enhance vortex pinning by random disorder in the sample,
so that the resistivity
would drop in the entangled state.
In order for the vortices to entangle, it is crucial that neighboring lines not cut through each other easily [6,7] and reconnect into a disentangled state. Estimates of the cutting barrier vary widely [3,5,8-12], ranging from 50kBT to of order kBT, leaving the question of whether vortices can easily cut in the liquid state unresolved. Numerical simulations performed in limits ranging from the low-field London regime to the high-field lowest Landau level regime have proven similarly ambiguous, with some simulations interpreted as providing evidence for entanglement [13] and others interpreted as showing that the lines cut and do not entangle [10,11,14,15]. The simulations are limited both by the models chosen and by the system size. Boson models lack long-range interactions along the vortex line, which can stiffen the vortices and might reduce entanglement. [8,16,17]. In the frustrated 3D XY model, there are multiple ways to define a path followed by a vortex line, some of which are consistent with entanglement, and others which are not [14].
Since theoretical and numerical evidence for entanglement have proven inconclusive up to this point, it is natural to turn to experiments to resolve the issue. Unfortunately experimental evidence for or against entanglement [18-21] has also proven ambiguous, both because the experimental measures are indirect, and because there is considerable variation in the definition of entanglement [22], such as equating entanglement with the onset of plasticity [18]. Thus, despite more than a decade of theoretical, numerical, and experimental studies, the question of whether vortices can form an entangled state has not yet been convincingly answered.
Here we propose a direct experimental test of vortex entanglement by means of a local magnetic force microscope (MFM) probe which can unambiguously determine whether it is possible for two vortices to wind around each other without cutting. We consider conditions that are as favorable as possible for entanglement: low vortex density, weak background pinning, and low temperatures, which should increase the barrier to flux cutting. We propose using the MFM tip to produce the simplest possible entangled state, two vortices wound around each other, and show theoretically that the forces involved in creating the entangled state can be measured with current technology. Should the vortices cut rather than entangling, a distinct force signature will be observed. If entanglement does not occur in this limit, it seems unlikely to occur in the higher density, higher temperature conditions near the melting transition. In addition to testing entanglement, this local MFM probe can be used to measure a wide range of other quantities, such as vortex line tension, local pinning force, and local shear forces.

and the system is isotropic.
We use as our definition of an entangled vortex state the picture
originally proposed by Nelson, in which vortices behave like elastic
lines that cannot easily cut through each other
[2].
We consider a layered superconductor containing two closely spaced magnetic
dots at the bottom of the sample
[23] (dark circles in Fig. 1)
A mobile magnetic dot is introduced to the top of the sample
in the form of a magnetic MFM tip (open circle in Fig. 1).
An optional additional magnetic dot
can be added at the top of the sample to pin one of the vortices.
We assume that there is a sufficiently small externally applied
magnetic field that there are only two vortex lines within the region of
interest, an area a few
on a side,
where
is the London
penetration depth of the material. The magnetic
dots attract the vortices, so that the top and bottom positions of the
vortices are fixed at the dot locations.
As the MFM is moved along the surface of the sample, it
drags the top of one vortex with a directly measurable force.
When the MFM tip moves in a circular path around the fixed upper dot,
the two vortices wind together, producing an entangled state. In
Fig. 1(b), we illustrate one possible entangled vortex configuration, obtained
numerically as described below. As the winding angle increases,
the force required to drag the vortex further around increases according
to a form derived below. If the vortices cut, this force will abruptly
drop. Thus, using such an experiment, it is possible to directly probe
whether vortex entanglement can occur.
To estimate the force required to entangle a pair of linelike vortices, we represent the vortex lines as one-dimensional elastic strings that cannot cross. Such a model may be applicable in the London limit at low fields B < 0.2Bc2, although the lack of long-range interactions along the z axis is a notable limitation [8,16,17]. The vortex configuration is determined by a balance of the interaction energy, which drives the strings apart, and the elastic energy, which pulls the strings together to reduce their length as they are wound. Thus, the greater the pitch (defined as the rate of change of winding angle per vertical distance), the closer the vortices approach, as they seek the preferred spacing that minimizes their free energy. Even if they are held radially away from the preferred spacing, as is shown at the top of Fig. 1(b), they approach the preferred spacing within the middle of the sample, leading to the roughly constant spacing in the middle of the sample as shown. This applies up to a certain pitch; beyond that pitch, we will show that the vortices are unstable to a collapse. A similar instability in a related model was discussed in Ref. [9]. The existence within the model of a collapse of the entangled state at a singularity when the vortices approach each other too closely raises the question of whether the entangled state can exist in other experimental situations where the vortices are driven closer than this distance.
Elastic string model.-
We consider two vortices, at positions
with
,
giving the position in the plane as a function of the vertical distance z.
As a starting point, we consider the free energy
from the elastic string model [2]:
(1)
with
=(
/4
)2,

We fix the boundary conditions on the vortex position at the
top (z=L) and the bottom (z=0) of the sample, and then minimize
the free energy (1) to find the positions of the vortex in between.
To specify these positions, we need eight real numbers,
two for each vortex at the
top and another two for each vortex at the bottom. To simplify, let
us fix two of these coordinates by setting
(0)+
(0)=0; thus,
the origin of the coordinate system is set at the midpoint of the two
vortices at the bottom of the sample.
We note that if a given pair of functions
(z) minimize the
free energy for given boundary conditions
(L), then the functions
(z)+
z
also minimize the free energy for a different set of boundary
conditions:
(L)+
L.
Thus, it suffices to consider only the
case in which also
(L)+
(L)=0,
as then all other boundary
conditions at the top can also be obtained. In this case, for
all z, r1(z)+r2(z)=0.
Thus, introduce coordinates with
r1(z)=[r(z) cos(
(z)),
r(z) sin(
(z))]
and r2(z)=-r1(z).
For the boundary conditions, we fix r(0), r(L),
(0),
(L).
Then, the extremization of the free energy yields equations of motion:
, (2)
, (3)
Exploiting an analogy of
this system to a particle evolving in time, the first equation is the
familiar conservation of angular momentum, with some constant J.
There exist solutions with constant vortex spacing, r(z), and pitch,
.
To find these, set
in the
equations of motion to obtain
(4)
This gives the preferred pitch as a function of spacing,
by a balance between elastic energy of one vortex and interaction
energy between two. For small r, this reduces to
From this one can show that for
small spacing in the isotropic system
(
=
)
the vortices cross at an angle of
/2,
as expected [9].
While this scenario seems reasonable, there is a major caveat:
Eq. (4) describes a minimum of the free energy
for small pitch, but for
larger pitch [above the maximum of the torque curve, Fig. 2(b)],
it describes only an extremum and is unstable to a collapse
of the vortices. To show this, we
find, by differentiating the free energy twice, that for stability
at fixed J, we need
(5)
When Eq. (5) vanishes, at
r
1.19
,
the system is marginal. For smaller r, the system is unstable to
perturbations.
In this case, the repulsion between the vortices is unable to overcome
the elastic energy, and the two vortices will be driven together, meeting
at a singularity for some z with r(z)=0.
Only a finite energy cost is paid to have
the two vortices meet at a point, while an arbitrary amount of winding
can be accomplished at that point with no free energy cost.
Within an elastic string model,
it can be shown that for any vortex-vortex interaction energy which
diverges less strongly than 1/r2
there is an instability of this nature
for sufficiently small r. The marginal
r
1.19
corresponds to the maximum of
the torque curve, giving a maximal torque on each vortex
equal to
(0.536...)
, and a
minimal stable spacing of
2r
2.39
.
The presence of a surrounding vortex lattice would further reduce
the stability
[10].

and (b) torque on the top end of each vortex
in units of

as a function of pitch
in units of
/
.
The dashed line denotes an unstable vortex configuration
above a pitch of approximately 0.378,
corresponding to a minimum
r
1.19
.
To find the force that would be detected by the MFM tip as the
vortices are wound around one another into an entangled state,
we first consider the large r case of Eq. (4)
when the entwined vortex configuration is stable. We fix the
total winding angle,

=
(L)-
(0),
and the values r(0),r(L).
The force that the
dragged vortex exerts on the MFM tip can be found by taking a derivative
of the free energy with respect to r and
. We find that the
angular torque on the top end of each vortex is
,
while the radial force
on each is
. The radial force will
vanish when r,
obey Eq. (4) at the top and
bottom of the sample, giving a solution with constant radius and
pitch
=(
(L)
-
(0))/L.
In Fig. 2 we plot the spacing and torque as a function
of pitch for this case.
Experimental implications.-
The magnitude of the angular force is large enough to be detected
experimentally in the constant pitch
configuration. For example, consider two vortices in a YBCO
sample. For this material,

0.2
,
where 
140 pN.
Thus, at the
maximum of the torque curve in Fig. 2, a torque of
(0.536)
at
=0.378
/
and r=1.19
gives a force of
0.45
28 pN.
This value is within the range of forces detectable with MFM, which
are as small as 0.4 pN [24].
In order to convert the pitch
plotted in Fig. 2
into the total angular displacement

imposed on the dragged vortex, we must know the thickness L of the
sample in the z direction. Assuming L=1
m
gives

=
L
=1.72
for
=0.378
.
In order to perform the experiment,
the angular force associated with entanglement should not exceed the
pinning force of the MFM tip, estimated to be of order
500 pN [25]. It should also be smaller than
the pinning force of the magnetic dot, which, following
Ref. [26],
can be roughly estimated as 200 pN for a Ni dot 40 nm thick and 250 nm in
diameter in YBCO.
To further reduce the angular force of entanglement,
a slightly different configuration can be used
in which the vortex spacing at the top and bottom of the sample is increased.
Solutions for this case can be found numerically from
Eqs. (2) and (3), but
an analytical solution exists in the following limit: the
vortex separation at the top and bottom is much greater than
and they are almost straight lines, while in the middle of the sample
the solution is close to a constant pitch solution of Eq. (4).
In this configuration the "lever arm" is increased,
enabling the angular force required to entangle the vortices
to be made arbitrarily small. The radial
force remains non-vanishing, and can be computed by minimizing the free
energy over the length l of the winding section at the center of the
sample. The result is that to produce a pitch of
0.378
requires a radial force of
0.25
16 pN.

as a function of
total winding angle

, obtained from
a simulation of pancake vortices.
In more highly anisotropic materials such as BSCCO, the elastic string model for the vortex lines is expected to break down due to the possibility of decoupling of vortex pancakes on adjacent layers. Consider an MFM tip bound to a pancake at the top of a vortex line in BSCCO. If this pancake decouples from the rest of the vortex line below, then the angular force as a function of angular displacement will not follow the form shown in Fig 2, but will instead be periodic in the winding angle, due to the interaction with the remaining stack of pancake vortices left behind. This is illustrated by a simulation of a pancake vortex system [27] of two isolated vortices in a BSCCO sample with 2000 layers and no periodic boundary conditions. The bottom pancake of each stack is held fixed while the upper pancake of one stack is driven at constant speed on a circular path. The force exerted by the rest of the pancakes on the driven pancake is shown in Fig. 3, and is two orders of magnitude smaller than the entanglement force in YBCO, placing it below the threshold of detection by MFM.
Discussion.- The local experimental probe that we propose can also be used to explore numerous other properties of the vortex system besides vortex entanglement. For example, in a geometry containing only one magnetic pin and one vortex line, the MFM tip can be used to measure the vortex line tension directly. If the line tension is known, the tip could be used to tear a vortex away from a (weaker) individual pin, such as a grain boundary, and the pinning force could be measured. By applying a transport current to the sample, the Lorentz force can be determined directly. Local rheology measurements are also possible in the vortex lattice state; for example, the local elastic constants can be probed by moving a single vortex back and forth around its lattice equilibrium position. The temperature dependence of both the elastic constants and the pinning energy could also be probed.
Conclusion.- We have proposed an experimental setup for constructing and probing entangled states of superconducting vortices, and shown that the forces associated with vortex entanglement are experimentally measurable. This kind of experimental setup can be generalized to other types of vortices, as in fluid turbulence. Within the elastic string model, we find that the entangled state is only stable up to a maximum pitch or minimum vortex spacing. The instabilities we have found raise the question of whether the entangled state can exist with a high density of vortices. To answer this question and to compare pancake and elastic string models, an experimental test of our proposal is desirable.
We thank C. Reichhardt for helpful discussions. This work was supported by the U.S. DOE under Contract No. W-7405-ENG-36.
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