4Phases of SLE
III Schramm--Loewner Evolutions
4 Phases of SLE
We now study some basic properties of
SLE
κ
. Our first goal will be to prove the
following theorem:
Theorem. SLE
κ
is a simple curve if κ ≤ 4, and is self-intersecting if κ > 4.
When proving this theorem, we will encounter the Bessel stochastic differential
equation, and so we shall begin by understanding this SDE and the associated
Bessel process.
Definition
(Square Bessel process)
.
Let
X
= (
B
1
, . . . , B
d
) be a
d
-dimensional
standard Brownian motion. Then
Z
t
= kX
t
k
2
= (B
1
t
)
2
+ (B
2
t
)
2
+ ··· + (B
d
t
)
2
is a square Bessel process of dimension d.
The square Bessel process satisfies a stochastic differential equation, which
we can obtain from Itˆo’s formula. Itˆo’s formula tells us
dZ
t
= 2B
1
t
dB
1
t
+ ··· + 2B
d
t
dB
d
t
+ d ·dt.
For reasons that will become clear soon, we define
Y
t
=
Z
t
0
B
1
s
dB
1
s
+ ··· + B
d
s
dB
d
s
Z
1/2
s
.
Then tautologically, we have
dZ
t
= 2Z
1/2
t
dY
t
+ d ·dt.
Observe that
Y
t
is a continuous local martingale, and the quadratic variation is
equal to
[Y ]
t
=
Z
t
0
(B
1
s
)
2
+ ··· + (B
d
s
)
2
Z
s
ds = t.
By the L´evy characterization,
Y
T
is a standard Brownian motion. So we can
write
Lemma.
dZ
t
= 2Z
1/2
t
d
˜
B
t
+ d ·dt.
where
˜
B is a standard Brownian motion.
This is called the square Bessel stochastic differential equation of dimension
d.
Ultimately, we are interested in the Bessel process, i.e. the square root of the
square Bessel process.
Definition
(Bessel process)
.
The Bessel process of dimension
d
, written BES
d
,
is
U
t
= Z
1/2
t
.
Applying Itˆo’s formula, we have
dU
t
=
1
2
Z
−1/2
t
dZ
t
−
1
8
Z
−3/2
t
d[Z]
t
The square Bessel SDE lets us understand the first term, and we can calculate
[Z]
t
= 4Z
t
dt
Simplifying, this becomes
Lemma.
dU
t
=
d − 1
2
U
−1
t
dt + d
˜
B
t
.
This is the Bessel stochastic differential equation of dimension d.
Observe that we can make sense of this equation for any
d ∈ R
, not necessarily
integral. However, the equation only makes sense when
U
t
6
= 0, and
U
−1
t
fails
to be Lipschitz as
U
t
→
0. To avoid this problem, we say this is defined up to
when it hits 0.
Proposition. Let d ∈ R, and U
t
a BES
d
.
(i) If d < 2, then U
t
hits 0 almost surely.
(ii) If d ≥ 2, then U
t
doesn’t hit 0 almost surely.
This agrees with what we expect from the recurrence of Brownian motion,
for integral
d
. In particular, for
d
= 2, a Brownian motion gets arbitrarily close
to 0 infinitely often, so we expect that if we are just a bit lower than
d
= 2, we
would hit 0 almost surely.
Proof. The proof is similar to the proof of recurrence of Brownian motion. For
a ∈ R
>0
, we define
τ
a
= inf{t ≥ 0 : U
t
= a}.
We then consider
P
[
τ
b
< τ
a
], and take the limit
a →
0 and
b → ∞
. To do so, we
claim
Claim. U
2−d
t
is a continuous local martingale.
To see this, we simply compute using Itˆo’s formula to get
dU
2−d
t
= (2 − d)U
1−d
t
dU
t
+
1
2
(2 − d)(1 −d)U
−d
t
d[U]
t
= (2 − d)U
1−d
t
d
˜
B
t
+
(2 − d)(d −1)
2U
t
U
1−d
t
dt +
1
2
(2 − d)(1 −d)U
−d
t
dt
= (2 − d)U
1−d
t
d
˜
B
t
.
Therefore
U
t
is a continuous local martingale. Since
U
t∧τ
a
∧τ
b
is bounded, it is a
true martingale, and so optional stopping tells us
U
2−d
0
= E[U
2−d
τ
a
∧τ
b
] = a
2−d
P[τ
a
< τ
b
] + b
2−d
P[τ
b
< τ
a
].
– If d < 2, we set a = 0, and then
U
2−d
0
= b
2−d
P[τ
b
< τ
0
].
Dividing both sides as b, we find that
U
0
b
2−d
= P[τ
b
< τ
0
].
Taking the limit b → ∞, we see that U
t
hits 0 almost surely.
– If d > 2, then we have
P[τ
a
< τ
b
] =
U
0
a
2−d
−
b
a
2−d
P[τ
b
< τ
a
] → 0
as a → 0 for any b and U
0
> 0. So we are done in this case.
–
If
d
= 2, then our martingale is just constant, and this analysis is useless.
In this case, we consider
log U
t
and perform the same analysis to obtain
the desired conclusion.
Now take an SLE
κ
curve. For x ∈ R, consider the process
V
x
t
= g
t
(x) − U
t
= g
t
(x) − g
t
(γ(t)).
Essentially by definition,
x
starts being in
A
t
when
V
x
t
= 0 (formally, we need
to take limits, since x is not in H). We thus define
τ
x
= inf{t ≥ 0 : V
x
t
= 0}.
This is then the time
γ
cuts
x
off from
∞
. We thus want to understand
P
[
τ
x
< ∞
].
We can calculate
dV
x
t
= d(g
t
(x) − U
t
) =
2
g
t
(x) − U
t
dt −
√
κ dB
t
=
2
V
x
t
dt −
√
κ dB
t
.
This looks almost like the Bessel SDE, but we need to do some rescaling to write
this as
d
V
x
t
√
κ
=
2/κ
V
×
t
/
√
κ
dt + d
˜
B
t
,
˜
B
t
= −B
t
.
So we get that
V
×
t
/
√
κ ∼ BES
d
, with
d
= 1 + 4
/κ
. Thus, our previous result
implies
P[τ
x
< ∞] =
(
1 κ > 4
0 κ ≤ 4
.
Theorem. SLE
κ
is a simple curve if κ ≤ 4, and is self-intersecting if κ > 4.
Proof.
If
κ ≤
4, consider the probability that
γ
(
t
+
n
) hits
γ
([0
, n
]). This is
equivalently the probability that
γ
(
t
+
n
) hits
∂A
n
. This is bounded above by
the probably that
g
n
(
γ
(
t
+
n
))
− U
n
hits
∂H
. But by the conformal Markov
property, g
n
(γ(t + n)) −U
n
is an SLE
κ
. So this probability is 0.
If
κ >
4, we want to reverse the above argument, but we need to be a bit
careful in taking limits. We have
lim
n→∞
P[γ(t) ∈ [−n, n] for some t] = 1.
On the other hand, for any fixed n, we have
lim
m→∞
P[g
m
(A
m
) − U
m
⊇ [−n, n]] = 1.
The probability that SLE
κ
self-intersects is
≥ P[g
m
(A
m
) − U
m
⊇ [−n, n] and g
m
(γ(t + m)) −U
m
∈ [−n, n] for some t].
By the conformal Markov property,
g
m
(
γ
(
t
+
m
))
− U
m
is another
SLE
κ
given
F
m
. So this factors as
P[g
m
(A
m
) − U
m
⊇ [−n, n]]P[γ(t) ∈ [−n, n] for some t].
Since this is true for all
m
and
n
, we can take the limit
m → ∞
, then the limit
n → ∞ to obtain the desired result.
It turns out there are two further regimes when κ > 4.
Theorem. If κ ≥ 8, then SLE
κ
is space-filling, but not if κ ∈ (4, 8).
This will be shown in the second example sheet. Here we prove a weaker
result:
Proposition. SLE
κ
fills ∂H iff κ ≥ 8.
To phrase this in terms of what we already have, we fix
κ >
4. Then for any
0 < x < y, we want to understand the probability
g(x, y) = P[τ
x
= τ
y
].
where we assume 0
< x < y
. If
τ
x
=
τ
y
, this means the curve
γ
cuts
x
and
y
from
∞
ft the same time, and hence doesn’t hit [
x, y
]. Conversely, if
P
[
τ
x
=
τ
y
] = 0,
then with probability one,
γ
hits (
x, y
), and this is true for all
x
and
y
. Thus,
we want to show that g(x, y) > 0 for κ ∈ (4, 8), and g(x, y) = 0 for κ ≥ 8.
To simplify notation, observe that
g
(
x, y
) =
g
(1
, y/x
) as
SLE
κ
is scale-
invariant. So we may assume x = 1. Moreover, we know
g(1, r) → 0 as r → ∞,
since P[τ
1
< t] → 1 as t → ∞, but P[τ
r
< t] → 0 as r → ∞ for t fixed.
Definition (Equivalent events). We say two events A, B are equivalent if
P[A \ B] = P[B \ A] = 0,
Proposition. For r > 1, the event {τ
r
= τ
1
} is equivalent to the event
sup
t<τ
1
V
r
t
− V
1
t
V
1
t
< ∞. (∗)
Proof.
If (
∗
) happens, then we cannot have that
τ
1
< τ
r
, or else the supremum
is infinite. So (
∗
)
⊆ {τ
1
=
τ
r
}
. The prove the proposition, we have to show that
P
τ
1
= τ
r
, sup
t<τ
1
V
r
t
− V
1
t
V
1
t
= ∞
= 0.
For M > 0, we define
σ
M
= inf
t ≥ 0 :
V
r
t
− V
1
t
V
1
t
≥ M
.
It then suffices to show that
P
M
≡ P
τ
1
= τ
r
sup
t<τ
1
V
r
t
− V
1
t
V
1
t
≥ M
= P[τ
1
= τ
r
| σ
M
< τ
1
] → 0 as M → ∞.
But at time
σ
M
, we have
V
r
t
= (
M
+ 1)
V
1
t
, and
τ
1
=
τ
r
if these are cut off at
the same time. Thus, the conformal Markov property implies
P
M
= g(1, M + 1).
So we are done.
So we need to show that
P
sup
t<τ
1
V
r
t
− V
1
t
V
1
t
< ∞
(
> 0 κ ∈ (4, 8)
= 0 k ≥ 8
.
We will prove this using stochastic calculus techniques. Since ratios are hard, we
instead consider
Z
t
= log
V
r
t
− V
1
t
V
1
t
.
We can then compute
dZ
t
=
3
2
− d
1
(V
1
t
)
2
+
d − 1
2
V
r
t
− V
1
t
(V
1
t
)
2
V
r
t
dt −
1
V
1
t
dB
t
, Z
0
= log(r −1).
Here we can already see why κ = 8 is special, since it corresponds to d =
3
2
.
When faced with such complex equations, it is usually wise to perform a
time change. We define σ(t) by the equation
σ(0) = 0, dt =
dσ(t)
(V
1
σ(t)
)
2
.
So the map
t 7→
˜
B
t
= −
Z
σ(t)
0
1
V
1
s
dB
s
is a continuous local martingale, with
[
˜
B]
t
=
"
−
Z
σ(t)
0
1
V
1
s
dB
s
#
t
=
Z
σ(t)
0
1
(V
1
s
)
2
ds = t.
So by the L´evy characterization, we know that
˜
B
t
is a Brownian motion.
Now let
˜
Z
t
= Z
σ( t)
.
Then we have
d
˜
Z
t
=
"
3
2
− d
+
d − 1
2
V
r
σ(t)
− V
1
σ(t)
V
r
σ(t)
#
dt + d
˜
B
t
.
In integral form, we get
˜
Z
t
=
˜
Z
0
+
˜
B
t
+
3
2
− d
t +
d − 1
2
Z
t
0
V
r
σ(s)
− V
1
σ(s)
V
r
σ(s)
ds
≥
˜
Z
0
+
˜
B
t
+
3
2
− d
t.
Now if κ ≥ 8, then d = 1 +
4
κ
≤
3
2
. So we have
˜
Z
t
≥
˜
Z
0
+
˜
B
t
.
So we find that
sup
t
˜
Z
t
≥
˜
Z
0
+ sup
t
˜
B
t
= +∞.
So we find that
sup
t<τ
1
V
r
t
− V
1
t
V
1
t
= ∞.
So g(x, y) = 0 for all 0 < x < y if κ ≥ 8.
Now if κ ∈ (4, 8), we pick ε > 0 and set
r = 1 +
ε
2
.
Then we have
˜
Z
0
=
log
(
r −
1) =
log
(
ε/
2). We will show that for small
ε
, we have
g
(1
, r
)
>
0. In fact, it is always positive, which is to be shown on the example
sheet.
We let
τ = inf{t > 0 :
˜
Z
t
= log ε}.
Then
˜
Z
t∧τ
=
˜
Z
0
+
˜
B
t∧τ
+
3
2
− d
t ∧ τ +
d − 1
2
Z
t∧τ
0
V
r
σ(s)
− V
1
σ(s)
V
r
σ(s)
ds
≤
˜
Z
0
+
˜
B
t∧τ
+
3
2
− d
t ∧ τ +
d − 1
2
Z
t∧τ
0
e
˜
Z
s
ds
≤
˜
Z
0
+
˜
B
t∧τ
+
3
2
− d
t ∧ τ −
d − 1
2
(t ∧ τ)ε
=
˜
Z
0
t +
˜
B
t∧τ
+
3
2
− d
+
d − 1
2
ε
(t ∧ τ).
We let
Z
∗
t
=
˜
Z
0
t +
˜
B
t
+
3
2
− d +
d − 1
2
ε
t.
We then have shown that
Z
∗
t∧τ
≥
˜
Z
t∧τ
.
We assume that
ε >
0 is such that
3
2
− d +
d−1
2
ε
<
0. Then
Z
∗
t
is a Brownian
motion with a negative drift, starting from
log
ε
2
, so (by the second example
sheet), we have
P
sup
t≥0
Z
∗
t
< log ε
> 0.
So we know that
P
sup
t≥0
˜
Z
t
< log ε
> 0.
So we have
g
1, 1 +
ε
2
> 0.
This concludes the proof of the theorem.
SLE on other domains
So far, we only defined
SLE
κ
in the upper half plane
H
from 0 to
∞
. But we
can define SLE in really any simply connected domain. If
D ⊆ C
is a simply
connected domain, and
x, y ∈ ∂D
are distinct, then there exists a conformal
transformation ϕ : H → D with ϕ(0) = x and ϕ(∞) = y.
An
SLE
κ
in
D
from
x
to
y
is defined by setting it to be
γ
=
ϕ
(
˜γ
), where
˜γ
is an
SLE
κ
in
H
from 0 to
∞
. On the second example sheet, we check that this
definition is well-defined, i.e. it doesn’t depend on the choice of the conformal
transformation.