A. P. Mehta, C. Reichhardt, C. J. Olson, and Franco Nori*
Department of Physics, The University of Michigan, Ann Arbor,
Michigan 48109-1120
(Received 4 September 1998)
River basins as diverse as the Nile, the Amazon, and the Mississippi
satisfy certain topological invariants known as Horton's Laws.
Do these macroscopic (up to 103 km) laws extend to the micron scale?
Through realistic simulations, we analyze the
morphology and statistical properties of networks
of vortex flow in flux-gradient-driven superconductors.
We derive a phase diagram of the different
network morphologies, including one in which
Horton's laws of length and stream number are
obeyed - even though these networks are about
109 to 1015 times smaller than geophysical river basins.
[S0031-9007(98)08235-0]
PACS numbers: 64.60.Ht, 74.60.Ge, 92.40.Fb
The nature of river
basins [1-4],
including their physical structure and evolution,
has been a problem of major interest to civilized
societies throughout history. Horton's laws are
perhaps one of the most intriguing
properties of river networks [1-4].
In order to apply them to a network, the individual streams
composing the network must be identified and labeled with an order
number, as in the top left corner of Fig. 1(a).
The lowest order streams are the smallest outlying tributaries on the
edges of the network, according to the Strahler ordering scheme.
At each point where two tributary streams join, a new stream begins.
Whenever two tributaries of the same order meet, the outgoing
stream has an order number one higher than that of the tributaries.
If two tributaries of different orders meet, the outgoing stream
has the same order number as the higher ordered tributary.
Eventually, all streams in the network combine to form the
highest order (main) stream.
The number of streams of order w is Nw,
while Lw is the average length of streams of order w.
Horton's laws state that the bifurcation ratio
RB and the length ratio RL, given by
RB=Nw/Nw+1 and
RL=Lw+1/Lw,
are constant, or independent of w.
These ratios also provide the
fractal dimension [1-3]
of the rivers
DF
log RB/log RL.
Geophysical river basins [1-3]
typically have values of
RB
4 and
RL
2.
Do these (Horton's) laws apply to microscopic landscapes?
Here we present evidence that these macroscopic laws are
obeyed at the microscopic scale by riverlike networks
of flowing quantized magnetic flux.

3
/2
[7]); and (c) dense
(when pinning is much weaker than fvv;
i.e., for B > 2
,
or at any field for low fp).
Here, np=0.75/
.
The matching field
occurs when the number of
vortices Nv equals the number of pinning sites Np.
is used to quantify the relative strength
of pinning versus vortex-vortex repulsion [7].
Vortex River Basins. - Near the depinning transition,
magnetic vortices in type-II
superconductors move in intricate flow patterns that have been
seen both in computer simulations
and in experiments, including fingerlike or dendritic shapes
as well as the filamentary flow of vortices in riverlike paths
and networks
(see, e.g., [5-7], and
references therein).
Despite the ubiquity of the river-like pathways produced by the
vortex motion, very little work has been done towards
characterizing the morphology of these flow patterns.
Moreover, concepts and ideas used for decades to characterize
geophysical river basins have not been applied
to the study of the microscopic flow through tree-shaped
channel networks. This is surprising since the underlying physics
of vortex and geological rivers offers striking similarities:
driven nonequilibrium dissipative systems displaying branched
(or ramified) transport among
metastable states on a rough landscape [8].
One is driven by the Lorentz force and the other by gravity.
Like geophysical rivers, vortex flow basins exhibit
sinuosity (i.e., tortuosity), anabranching, braiding, occasional
sudden floods, and other features that make them remarkably
similar to geophysical rivers [1].
Indeed, some satellite photographs of river basins are
strikingly similar to the channels produced by vortex motion.
However, significant differences also exist, including:
flow direction,
quantized flux flow versus continuum water flow,
compressible vortex lattice versus incompressible fluid,
negligible inertia with overdamped vortex dynamics versus massive fluid,
nonerosional versus erosional landscape,
peripheral flux sources versus uniform rain, and
correlated long-range versus short-range interactions
(so the rapidly varying vortex-vortex repulsion
landscape smooths out the underlying static pinscape).
This strongly-correlated vortex dynamics generates flux motion
that can be either continuous-flow-type, like water, or
intermittent stick-slip-type motion - depending on the
balance of forces.
Also, vortices typically move over relatively flat
landscapes with many divots, as opposed to the
mountain-range-like very rough landscapes
of some geophysical rivers.
Moreover, vortex river basins occur inside materials
at approximate scales between 1 to 100
m,
much smaller than geophysical river basins
(of up to 103 km) - and also spanning a smaller
range of length scales.
Thus, given these numerous similarities and differences,
it is very unclear a priori which macroscopic
results carry over to the microscopic domain.
By conducting realistic simulations of slowly driven vortices moving over many samples, we have identified several distinct network phases. These vortex basins appear in the initial penetrating front of vortices [6,7]. Remarkably, we find that for a wide range of parameters networks of vortex channels obey Horton's laws just as geophysical river networks do. This is remarkable, given the many physical differences between basins of flux quanta and geophysical rivers and that they move over very different types of potential-energy landscapes. Unlike previous work, here we first present a detailed list of analogies and differences between river basins and networks of vortex channels. Afterwards, we present the first morphological phase diagram for vortex motion. Finally, we analyze the hierarchical structure of the vortex channels.
Simulation. -
We model a transverse 2D
slice (in the x-y plane) of an infinite zero-field-cooled T=0
superconducting slab containing flux-gradient-driven 3D rigid
vortices that are parallel to the sample edge
[6,7].
Vortices are added at the surface
at periodic time intervals, and enter the superconducting slab
under the force of their own mutual repulsion [6,7].
The slab is
36
x 36
in size, where
is
the penetration depth.
The vortex-vortex repulsive interaction is correctly modeled by a
modified Bessel function, K1(r/
).
The vortices also interact with 972 nonoverlapping attractive parabolic
wells of radius
=0.3
.
The density of pins np is
np=0.75/
. All pins in
a given sample have the same maximum pinning force fp, which ranged
from fp=0.3f0 to
fp=6.0f0 in 13 different samples.
For each sample type, we considered five realizations of disorder.
Thus, the five points at each pinning force, delineating
the broad crossover boundary between Hortonian and braided
phases in Fig. 2, refer to these five realizations of disorder.
A sixth point, indicating the average value from the five trials,
is not visible when it overlaps with another point.
We measure all forces in units of
f0=
/8
,
magnetic fields in units of
/
,
and lengths in units of the penetration depth
.
Here,
is the flux quantum.
The overdamped equation of vortex motion is
fi=fivv+fivp=
vi,
where the total force fi on vortex i (due to other
vortices fivv,
and pinning sites fivp)
is given by
Here,
is the Heaviside step function,
ri (vi)
is the location (velocity) of the ith vortex,
rk(p)
is the location of the kth pinning site,
is
the pinning site radius, Np (Nv)
is the number of pinning sites
(vortices),
=(ri-rj)/|ri-rj|,
=(ri-rk(p))/|ri-rk(p)|,
and we take
=1.
Morphological Characterization. -
In order to identify and characterize the vortex river networks formed
as the flux-gradient-driven front initially penetrates the sample,
we divide our simulation area into a 300 x 300 grid.
Each time a vortex enters a grid element, the counter associated
with that element is incremented. All grid elements that are
visited at least once by a vortex are considered part of
the network [6].
The maximum number of vortices in the sample is approximately 1200.
The pinning density np and radius
were kept constant at
np=0.75/
and
=0.3
,
while the pinning
force fp varied from sample to sample.
We also performed additional
simulations in which fp was kept constant and np varied
from np=0.15/
to np=2.15/
.

(thus, here
=0.75
/
).
In regions of very low pinning force, dense
vortex river networks dominate.
For higher pinning fp's, the Hortonian
rivers become braided when B grows.
For samples with significant amount of pinning, it is
the initial front (with low local density of
field lines B, B < 3
/2
[7],
and thus dominant pinning force fp) which branches
out in a Hortonian manner. Behind this initial front
follows the (intermediate-B) braided region. Further
behind, follows the (large-B) dense-flux regime.
The inset shows the shift in the
Horton-braided boundary fp=3.0f0
as the pinning density, np, is changed.
As np is increased, the Horton-braided
boundary shifts towards higher B.
The broad crossover boundaries are in the region of triangles and
rhombuses. The (power-law fit) lines are just guides to the eye.
The dense-braided crossover at high fields (dashed line)
is an extrapolation of the power-law-fit for low fields;
the former is very difficult to compute because it requires
a large number of vortices monitored over very long times.
We observed three distinct vortex river network morphologies,
depending on the local magnetic field B
and the pinning force fp,
as indicated in one of our main results:
the "morphological phase diagram" in Fig. 2.
In Fig. 1
the vortex trajectories are presented for the three
morphologies. In samples with low pinning force values,
fp
0.75f0
(see Fig. 2),
vortices flow throughout the sample, producing dense
vortex river basins. These become space-filling
for large times - or large fields since
the external field is slowly ramped up.
An example of the vortex channels in this regime,
as they appear after 160 000 MD steps, is shown in
Fig. 1(c).
If the simulation is
allowed to proceed for a larger number of MD steps, the
channels eventually fill the entire region shown in
Fig. 1(c).
For stronger pinning,
fp
1.0f0,
and low vortex densities
B
/
3
/2,
we observe branched "Hortonian" river networks that follow
Horton's laws of stream number and length
[see Fig. 1(a)].
At higher magnetic fields
B
/
3
/2,
the vortex rivers become highly braided or
interconnected and are no longer Hortonian in morphology
[see Fig. 1(b)].
Unlike the dense networks of Fig 1(c), where
preferred vortex paths are uncommon,
in the braided regime vortices consistently
move along certain pathways, while in some areas of
the sample vortex motion rarely occurs.
For low pinning forces in the dense network regime, vortex motion occurs both interstitially (with the vortices moving only in the areas between pinning sites) and by means of depinning. If vortex depinning is occurring in a landscape with traps of comparable strength, no favored paths for flux motion can form, leading to the observed dense pathways. The Hortonian and braided regimes arise once the pinning is strong enough that predominantly interstitial motion occurs. That is, pinned vortices almost never depin. Other vortices are prevented from moving close to a pinned vortex by the vortex-vortex repulsion, which has a longer (by nearly 2 orders of magnitude) range than the attraction of each pinning site. Since there are regions of the sample (i.e., at or near pinned vortices) where flux motion does not occur, the flow of the moving vortices must be concentrated in certain well-defined regions or rivers, leading to the formation of either Hortonian or braided rivers.

.
(b) The length ratio RL and
DF/dc=log RB/log RL,
versus the pinning force, fp.
The stream dimension, dc, is one.
Only the trend in the fractal dimension DF
can be observed from above because the error bars for
RL and DF/dc are
0.1. The lines are
power-law best fit curves, which only provide a guide to the eye.
The formula for DF
gives values slightly above
2, because it assumes that Horton's laws hold
at all length scales, while our vortex basins
only span a very limited range of length scales.
The broad crossover between Hortonian and braided rivers
occurs when the flux density has increased enough that
a large fraction of the pinning sites are occupied.
In Fig. 2, the crossover region
increases from
B
0.9
/
for
fp=1.0f0, to
B
1.3
/
for fp=6.0f0.
In each case, the crossover occurs at vortex densities
higher
(3
/2
B < 2
)
than the matching field
=0.75
/
,
when Np=Nv [11].
This is in agreement with the results for the inset of
Fig. 2, which shows that the
transition from Hortonian rivers to braided rivers
occurs at higher vortex densities as np
(and thereby the matching field) is increased.
Additional support for this interpretation comes from
examining the fraction Rups of
unoccupied pinning sites [Fig. 3(a)].
At the matching field,
=0.75
/
,
only about 65% of the pins are occupied [7,11].
The pins are not fully occupied until a field of
B
1.4
/
2
is applied - when
the potential energy landscape experienced by the
moving vortices becomes much more uniform.

Horton Analysis. -
In order to determine whether the vortex river networks we observe obey
Horton's laws, we performed Hortonian analysis on five different
realizations of disorder for each of eight different pinning forces
fp falling within the Hortonian regime. In each trial, a branching
river was identified for analysis. The numbers
Nw and lengths Lw
of streams of order w= 1 to 4 were recorded
[9].
Representative plots of the
type used to determine the length ratio,
RL=Lw+1/Lw, and the bifurcation ratio,
RB=Nw/Nw+1,
are shown in Fig. 4.
In the best fit exponential regressions used to extract
RL and RB,
the average correlation coefficient was 0.99, indicating a good
fit to the Hortonian relationships.
The average values for RB and RL throughout the Hortonian
river region were
RB=3.99
0.18 and
RL=2.04
0.12, in excellent agreement with
geophysical rivers [1,10].
The characteristics of the Hortonian river networks are dependent on the pinning force fp. In Fig. 3(b) we plot the length ratios RL, and fractal dimensions DF, for each pinning force in the Hortonian region. The braching ratio (not shown) is roughly constant as fp is varied. Changing the pinning force alters the ease with which individual vortices can be depinned, and thereby changes RL and Df/dc. As the pinning force decreases, it is more likely that some vortices will be depined and form new pathways of vortex motion. This will decrease the length of the higher order rivers by cutting short how far the vortex channels propagate before bifurcating. Therefore RL will decrease with decreasing fp. Since a larger number of paths are created the Df will increase with decreasing fp, in agreement with Fig. 3(b).
In conclusion, we have analyzed the morphologies of flux-flow channels slowly driven to its marginally stable state, as a function of flux density and disorder strength. We have identified three distinct morphologies [12] which include: A (large B) dense network regime, where flow can occur anywhere; a braided network regime, where flow is restricted to certain regions; and a (low B) Hortonian network regime, where Horton's laws of length and branching ratio are obeyed in agreement with geophysical rivers. Indeed, it seems promising to analyze tree-shaped channel flow at the microscopic level adapting concepts that have already been successful in treating macroscopic river basins. These types of analysis are largely unexplored. The direction and success of such an approach constitutes an open and fascinating area.
C. J. O. (APM) acknowledges support from the GSRP of the microgravity division of NASA (NSF-REU). We thank the Maui Supercomputer Center, R. Riolo, and the UM-PSCS for providing computing resources. We thank F. Marchesoni, M. Bretz, E. Somfai, D. Tarboton, and S. Peckham for their useful comments.
. This type of collective
correlated motion is absent from the simple
random topological network models.
Also, the lack of "uniform rain" and erosion inside
materials, common in river basin models,
makes it difficult to make comparisons with
previous work on river basins. Moreover, there is no
consensus on the precise conditions required to obtain
Horton's laws at the macroscopic level (let alone at the
microscopic quantum regime). These issues are beyond
the scope of this paper and will be explored elsewhere.
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