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Article

Exponential Bounds for the Density of the Law of the Solution of an SDE with Locally Lipschitz Coefficients

Department of Mathematics and Statistics, Grant MacEwan University, 5-103C, 10700-104 Ave., Edmonton, AB T5J 4S2, Canada
Mathematics 2025, 13(5), 798; https://doi.org/10.3390/math13050798
Submission received: 30 November 2024 / Revised: 17 February 2025 / Accepted: 25 February 2025 / Published: 27 February 2025
(This article belongs to the Special Issue Advances in Probability Theory and Stochastic Analysis)

Abstract

:
Under the uniform Hörmander hypothesis, we study the smoothness and exponential bounds of the density of the law of the solution of a stochastic differential equation (SDE) with locally Lipschitz drift that satisfies a monotonicity condition. We extend the approach used for SDEs with globally Lipschitz coefficients and obtain estimates for the Malliavin covariance matrix and its inverse. Based on these estimates and using the Malliavin differentiability of any order of the solution of the SDE, we prove exponential bounds of the solution’s density law. These results can be used to study the convergence of implicit numerical schemes for SDEs.

1. Introduction

We use Malliavin calculus to study the smoothness and exponential bounds for the density of the law of the solution of a stochastic differential equation (SDE) with a locally Lipschitz drift that satisfies a monotonicity condition. These exponential bounds are important, for example, to study the convergence rate of numerical schemes [1] for approximating the solutions of the SDE. SDEs with non-globally Lipschitz coefficients appear in models for financial securities and various models for dynamical systems [2,3,4].
We consider the SDE
d X ( t ) = b ( X ( t ) ) d t + σ ( X ( t ) ) d W ( t ) , X ( 0 ) = x R d , t [ 0 , T ] , T > 0 ,
where W ( t ) is an m-dimensional Brownian motion defined on the filtered complete probability space Ω , F , { F t } t 0 , P , and b : R d R d , σ : R d R d × m . We make the following assumptions for the coefficients b and σ :
C: 
b and σ have derivatives of any order k with polynomial growth. More precisely, for any order k 1 and any multi-index α = ( α 1 , , α d ) with | α | = α 1 + + α d = k , there exist L b , k > 0 , L σ , k > 0 and N b , k 0 , N σ , k 0 , with N σ , 1 = 0 , such that for any x R d we have
| α b ( x ) | L b , k 1 + | x | N b , k , | α σ ( x ) | L σ , k 1 + | x | N σ , k .
M: 
There exists L b > 0 such that for any x 1 , x 2 R d we have
< x 1 x 2 , b ( x 1 ) b ( x 2 ) > L b | x 1 x 2 | 2
P: 
There exist L b , 0 0 and N 1 such that for any x 1 , x 2 R d we have
| b ( x 1 ) b ( x 2 ) | 2 L b , 0 ( 1 + | x 1 | 2 N 2 + | x 2 | 2 N 2 ) | x 1 x 2 | 2
Supposing that b and σ are globally Lipschitz, C , all their derivatives have polynomial growth, and Hörmander’s hypothesis holds; in [5], it is shown that the strong solution of (1) is Malliavin-differentiable for any order and it is non-degenerate at any fixed positive time. Furthermore, an estimate for the Malliavin covariance matrix (Theorem 2.17 [5]) is used to show that the law of the solution of the SDE is absolutely continuous with respect to the Lebesgue measure, its density is infinity differentiable, and exponential bounds are proven under the uniform Hörmander hypothesis.
There are several approaches to extend these results for SDEs with non-globally Lipschitz coefficients. In [6], assuming that the coefficients of the SDE are smooth and non-degenerate on an open domain D, estimations of the Fourier transform are used to show that the law of the solution has a smooth density and upper bounds for this density are given. In [7], the Sobolev regularity of strong solutions with respect to the initial value is established for SDEs with local Sobolev and super-linear growth coefficients. For SDEs driven by fractional Brownian motions, in [8] it is shown that the density of the law of the solution is smooth and admits an upper sub-Gaussian bound in the rough case.
For SDEs with random coefficients with drifts satisfying locally Lipschitz and monotonicity conditions, in [9] the concepts of ray absolute continuity and stochastic Gâteaux differentiability are used to prove Malliavin differentiability and absolute continuity of the solution’s law. In [10], we extend this result and under assumptions C, M, and P we show Malliavin differentiability of any order. Here, under assumptions C, M, and P we use the results in [9,10] to obtain an estimate for the Malliavin covariance matrix similar to the one in Theorem 2.17 in [5]. If, in addition, the uniform Hörmander hypothesis holds, we prove that the solution of the SDE is non-degenerate and we obtain exponential bounds for the density of the law of the solution of the SDE.
Recently, Malliavin calculus was used to study the convergence of various numerical schemes for SDEs with non-globally Lipschitz coefficients [11,12]. Without the global Lipschitz assumption, the Euler numerical scheme is no longer convergent [2], but under assumptions C, M, and P, the mean square convergence of a class of fully implicit methods is proven in [13]. In [1], the exponential bounds of the density obtained in [5] for SDEs with globally Lipschitz coefficients are used to find an expansion of the error for the explicit Euler scheme. An application of the results presented in this paper is to extend these results for fully implicit symplectic methods for stochastic Hamiltonian systems with coefficients satisfying assumptions C, M, and P.
The paper is organized as follows. In the next section, we present some results regarding the Malliavin differentiability of the solution of the SDE. Section 3 includes preliminary results about the Malliavin matrix and the statement of the main result. In Section 4, we include estimates for the Malliavin matrix, and based on these estimates in Section 5 we prove the exponential bounds for the density of the law of the solution of the SDE (1).

2. Notation and Results About Malliavin Differentiability

We denote by f the gradient of a differentiable function f : R d R , and for a vector-valued function v : R d R d let v denote the matrix with components v i , j ( x ) = v i ( x ) x j , i , j = 1 , , d . For any multi-index α = ( α 1 , , α d ) with length | α | = α 1 + + α d , let α denote the partial derivative of order | α | . If ϕ is a smooth function, we denote by x α ϕ ( t , x , y ) the derivation with respect to the coordinates of x, where t and y are fixed.
For a vector v R l , we denote by | v | : = i = 1 l v i 2 1 2 the Euclidean norm, and if A = ( a i j ) is an l 1 × l 2 matrix we denote by | A | : = i = 1 l 1 j = 1 l 2 a i j 2 1 2 the Frobenius norm. For two vectors u , v R l , we denote < u , v > = i = 1 l u i v i , and for two l 1 × l 2 matrices A , B , < A , B > = i = 1 l 1 j = 1 l 2 a i j b i j denotes the Frobenius inner product.
We consider the Banach space C ( [ 0 , T ] ) , · , where C ( [ 0 , T ] ) : = { ϕ : [ 0 , T ] R , ϕ uniformly continuous and bounded } , ϕ = sup x [ 0 , T ] | ϕ ( x ) | , and we denote C 0 ( [ 0 , T ] ) : = { ϕ C ( [ 0 , T ] ) , ϕ ( 0 ) = 0 } . We define C p ( R l ) : = { ϕ C ( R l ) , ϕ and all its derivatives are functions with polynomial growth }.
For any open set E R d and n N , we denote C b n ( E , R d ) = { f C n ( E , R d ) , f and all its derivatives of order at most n are bounded } with the norm f C b n ( E , R d ) = max 0 i n sup x E | x i f ( x ) | .
Let Ω , F , { F t } t 0 , P be a filtered probability space. For any separable Banach space ( E , · ) , we denote L p ( Ω ; E ) = { X : Ω E , X is F -measurable and X p = E [ X p ] 1 / p < } . Let L be the subset of bounded random variables with norm X L = e s s sup ω Ω | X ( ω ) | .
Let S p ( [ 0 , T ] , R d ) = { ( Y t ) t [ 0 , T ] stochastic processes, Y t R d , that are { F t } t [ 0 , T ] , adapted, and Y S p = E [ | Y p ] 1 / p = E [ sup t [ 0 , T ] | Y ( t ) | p ] 1 / p < } . Let S ( [ 0 , T ] , R d ) = p 1 S p ( [ 0 , T ] , R d ) .

2.1. Malliavin Calculus

Let Ω = C 0 [ 0 , T ] , R m = { ω : [ 0 , T ] R m , ω = ( ω 1 , , ω m ) ,   ω i C 0 ( [ 0 , T ] ) , i = 1 , , m } be the canonical Wiener space, and W : = ( W t 1 , , W t m ) t [ 0 , T ] be the canonical Wiener process defined as W t i ( ω ) : = ω t i for any ω Ω , i = 1 , , m . We set F 0 as the natural filtration of W, P the Wiener measure, and F = { F t } t [ 0 , T ] the usual augmentation (which is right-continuous and complete) of F 0 . In this setting, W is a standard Brownian motion.
We denote by H : = L 2 ( [ 0 , T ] ; R m ) = { f : [ 0 , T ] R m Borel-measurable and 0 T | f ( s ) | 2 d s < } , and the canonical inner product is
< f , g > H : = 0 T < f ( s ) , g ( s ) > d s = i = 1 m 0 T f i ( s ) g i ( s ) d s , f , g H .
Let H be the Cameron–Martin space:
H : = { h : [ 0 , T ] R m , h Ω , there exists h ˙ H , such that h ( t ) = 0 t h ˙ ( s ) d s , t [ 0 , T ] }
For h H , we denote by h ˙ a version of its Radon–Nykodym density with respect to the Lebesgue measure. For any Hilbert space K we define L p ( K ) = { f : Ω K , f is F T -measurable and f L p ( K ) p : = ( E [ f K p ) 1 / p < } . Let
W ( h ) : = 0 T h ˙ s d W s : = i = 1 m 0 T h ˙ s i d W s i , h H .
Following [14], we set
S : = { F : Ω R , F = f ( W ( h 1 ) , , W ( h n ) ) , f C b ( R n ) , h i H , i = 1 , , n , for some n N , n 1 }
For any F S we define the Malliavin derivative D F : Ω H by
D F : = i = 1 n i f ( W ( h 1 ) , , W ( h n ) ) h i .
We identify D F with the stochastic process { D t F } t [ 0 , T ] , where D t F R m and
D t F ( ω ) = i = 1 n i f ( W ( h 1 ) ( ω ) , , W ( h n ) ( ω ) ) h i ( t ) , ( t , ω ) [ 0 , T ] × Ω .
D t j F denotes the jth component of D t F . We denote by D 1 , p , p 1 the closure of S with respect to the semi-norm
F 1 , p : = E [ | F | p ] + E [ D F H p 1 / p ,
and we set D 1 , = p 2 D 1 , p .
The kth order Malliavin derivative D k F : Ω H k is defined iteratively and its components are D t 1 , , t k j 1 , , j k F : = D t k j k D t 1 j 1 F , with ( t 1 , , t k ) [ 0 , T ] k , j 1 , , j k { 1 , , m } . For the Nth order Malliavin derivative, D N , p , p 1 is the closure of S with the semi-norm
F N , p : = E | F | p + i = 1 N E D i F H i p 1 / p = F L p ( Ω ) p + i = 1 N D i F L p Ω ; L 2 ( [ 0 , T ] i , R m ) p 1 p .
We set D = p 2 i 1 D i , p
The definition of Malliavin derivative can be extended to mappings G : Ω E , where ( E , · E ) is a separable Banach space ([9]). We consider the family
S E : = { G : Ω E , G = j = 1 k F j e j , F j S , e j E for some k N , k 1 }
S E is dense in L p ( F ; E ; P ) [9]. For any G S E we define the Malliavin derivative D G : Ω H E by
D G : = j = 1 k D F j e j
We denote by D 1 , p ( E ) , p 1 the closure of S E with respect to the semi-norm
G 1 , p , E : = E [ G E p ] + E [ D G H E p 1 / p ,

2.2. The Solution of the SDE

Assumption C and N σ , 1 = 0 imply that b is locally Lipschitz and σ is globally Lipschitz. Moreover, from assumptions C, M, and P we obtain that there exists C > 0 such that for any x , y R d ,
y x b ( x ) y L b | y | 2 ,
| σ ( x ) | 2 C ( 1 + | x | 2 ) ,
| x σ ( x ) | 2 C ,
| b ( x ) | 2 C ( 1 + | x | 2 N ) ,
| x b ( x ) | 2 C ( 1 + | x | 2 N b , 1 ) .
From assumption C, (6), and Theorems 3.6 in [15], we know that there exists a unique global solution X ( t , 0 , x ) of the SDE (1). From Theorems 9.1 and 9.5 in [15], we know that X ( t , 0 , x ) t 0 is a time-homogeneous { F t } t 0 -adapted Markov process and we have
E 0 T | X ( t , 0 , x ) | 2 d t < .
Moreover, from Theorem 4.1 in [15] we know that for any p 2 there exists a constant α p > 0 such that we have
E | X ( t , 0 , x ) | p 2 p 2 2 1 + | x | p e p α p t , t [ 0 , T ] .
From Theorem 2.2 in [9], we know that the map t X ( t ) ( ω ) is P almost surely continuous, and for any p 2 we have X S p : = S p ( [ 0 , T ] , R d ) and there exists C > 0 depending on p, b, and σ such that
E sup t [ 0 , T ] | X ( t , 0 , x ) | p < C ( | x | p + 1 ) .
From inequalities Equations (6)–(9), (12), and assumption C, for any multi-index α = ( α 1 , , α d ) and any p 2 we obtain
E sup t [ 0 , T ] | α b ( X ( t ) ) | p < , E sup t [ 0 , T ] | α σ ( X ( t ) ) | p < .
From Corollary 3.5 and Theorem 3.21 in [9], we know that X is Malliavin-differentiable and D X S p [ 0 , T ] , L 2 ( [ 0 , T ] ) for any p 2 :
E sup t [ 0 , T ] 0 T | D s X ( t ) | 2 d s p / 2 <
Thus, from (12) and (14) we have X D 1 , p ( S p ) for any p 2 , so X D 1 , ( S p ) = p 2 D 1 , p ( S p ) . Thus, similarly with the case in Theorem 2.2.1 in [16] of globally Lipschitz coefficients, for any t [ 0 , T ] we have X ( t ) D 1 , .
For any fixed s [ 0 , T ] and i = 1 , , m , from (6), (5), (10), and Theorem 2.5 in [9], we have for any p 2 ,
E sup t [ 0 , T ] | D s i X ( t ) | p C E | σ i ( X ( s , 0 , x ) ) | p C 1 + E | X ( s ) ) | p
This and (11) imply that for any t [ 0 , T ] and any p 2 ,
X ( t , 0 , x ) 1 , p p = E [ | X ( t , 0 , x ) | p ] + E 0 T | D s X ( t , 0 , x ) | 2 d s p / 2 C 1 , p ( T ) ( 1 + | x | p ) ,
where C 1 , p ( T ) > 0 depends on p, T, b, and σ .
In [10], we extend this result and show that under assumptions C, M, and P, X i ( t ) belongs to D for all t [ 0 , T ] , and i = 1 , , d . Moreover, for any t [ 0 , T ] , p 2 , k = 1 , 2 , , there exist C k , p ( T ) , β k , p > 0 depending on p, k, T, b, and σ such that
X ( t , 0 , x ) k , p p C k , p ( T ) ( 1 + | x | β k , p ) .

3. The Main Result

From Theorem 4.9 in [9] we know that under assumptions C, M, and P the matrix-valued SDE
J ( t ) = I d + 0 t x b X ( s , 0 , x ) J ( s ) d s + 0 t x σ X ( s , 0 , x ) J ( s ) d W ( s ) ,
t [ 0 , T ] , has a unique solution J S p [ 0 , T ] , R d × d , p 2 , and for any t [ 0 , T ] the map x X ( t , 0 , x ) is differentiable P a.s. and as ϵ 0 ,
X ( t , 0 , x + ϵ h ) ( ω ) X ( t , 0 , x ) ( ω ) ϵ h J ( t ) ( ω ) P a . s . .
We consider the matrix-valued SDE
K ( t ) = I d 0 t K ( s ) x b X ( s , 0 , x ) < x σ , x σ > X ( s , 0 , x ) d s 0 t K ( s ) x σ X ( s , 0 , x d W ( s ) , t [ 0 , T ] .
From Theorem 2.5 and Propositions 4.13 and 4.14 in [9], we know that under assumptions C, M, and P we have K ( t ) J ( t ) = I d for all t [ 0 , T ] P a.s.. Consequently, the Jacobian matrix J ( t ) is P -a.s. invertible for any choice of t [ 0 , T ] , and J ( t ) 1 = K ( t ) P a.s.. In [9], it was noted that since y x b X ( s , 0 , x ) y is not bounded from above by a constant P a.s. for any choice of y with | y | = 1 , an explicit solution of Equation (19) can be written path-wise, but it might not have finite moments.
Let J s ( t ) = J ( t ) J ( s ) 1 , t > s . Under assumptions C, M, and P from Proposition 5.1 in [9], we know that we have
J s ( t ) = I d + s t x b X ( r , 0 , x ) J s ( r ) d r + s t x σ X ( r , 0 , x ) J s ( r ) d W ( r ) ,
and the Malliavin derivative of X can be expressed for t > s as D s X ( t , 0 , x ) = J s ( t ) σ ( X ( s , 0 , x ) ) . The Malliavin matrix Q ( t ) is defined by
Q ( t , x ) : = 0 t D s X ( t , 0 , x ) D s X ( t , 0 , x ) d s = J ( t ) C ( t , x ) J ( t )
C ( t , x ) : = 0 t J ( s ) 1 σ ( X ( s , 0 , x ) ) σ ( X ( s , 0 , x ) ) ( J ( s ) 1 ) d s
The Lie bracket of the C 1 ( R d , R d ) vector fields V = i = 1 d V i x i , U = i = 1 d U i x i is defined as [ V , U ] ( x ) = U ( x ) V ( x ) V ( x ) U ( x ) , where U = ( i U j ) i , j = 1 , d , V = ( i V j ) i , j = 1 , d are the Jacobian matrices of U and V, respectively. Let us denote σ 0 = b 1 2 i = 1 m j = 1 d σ j i j σ i and let σ 0 , …, σ m be the corresponding vector fields:
σ 0 ( x ) = i = 1 d σ i 0 ( x ) x i , σ j ( x ) = i = 1 d σ i j ( x ) x i , j = 1 , , m .
We construct by recurrence the sets Σ 0 = { σ j , j = 1 , , m } , Σ k = { [ σ j , V ] , j = 0 , , m , V Σ k 1 } , k 1 , and Σ = k = 1 Σ k . We denote by Σ k ( x ) the subset of R m obtained by freezing the variable x R d in the vector fields of Σ k . For x R d we consider Hörmander’s hypothesis:
  • H(x): The vector space S p a n { Σ ( x ) } = R d .
If we have the ellipticity condition at x R d , i.e., for A ( x ) = σ ( x ) σ ( x ) there exists C > 0 such that y A ( y ) y C | y | 2 for any y R d , then Hörmander’s hypothesis H(x) holds. The interesting applications appear when A ( x ) is degenerate at x.
Example 1.
It is easy to check that assumptions C, M, and P hold for the coefficients of the following stochastic version with multiplicative noise of the Ginzburg–Landau equation [2] used in the theory of superconductivity to describe a phase transition:
d X ( t ) = μ + η + 1 2 σ ¯ 2 X ( t ) λ X ( t ) 3 d t + σ ¯ X ( t ) d W ( t ) , X ( 0 ) = x 0 R ,
where t [ 0 , T ] , η 0 , μ , λ , σ ¯ > 0 . We have A ( x ) = σ ¯ x 2 , so A ( 0 ) = 0 . However, a simple calculation shows that Hörmander’s hypothesis H(x) holds for any x R .
As in the Appendix in [5], let A = { } i = 1 ( { 0 , , m } ) i . Given α = ( α 1 , , α i ) A { } , we define α * = α i and
α = , if i = 1 ( α 1 , , α i 1 ) , if i 2 .
Given α A , set
| α | = 0 if α = i if α ( { 0 , , m } ) i , α = 0 if α = | α | + card { j : α j = 0 } if | α | 1 .
We define T ( α ) and I ( α ) ( t ) inductively on | α | by
T ( α ) ( V ) = V if α = [ σ α * , T ( α ) ( V ) ] if α , , V C ( R d , R d ) I ( α ) ( t ) = 1 if α = , 0 t I ( α ) ( s ) d W α * ( s ) if | α | 1 ,
where we consider W 0 ( t ) = t , t [ 0 , T ] .
Given L 1 , we define for any x , η R d
V L ( x , η ) = k = 1 m α L 1 < T ( α ) ( σ k ) ( x ) , η > 2 , V L ( x ) = inf | η | = 1 V L ( x , η ) 1 .
Let
U L : = { x R d , V L ( x ) > 0 } , U = L = 1 U L
Notice that for L N * = { 1 , 2 , } , the hypothesis
  • H L (x): S p a n { ϕ ( x ) , ϕ i = 1 L Σ i } = R d
is equivalent with x U L . As in [1], we consider the following assumption:
  • UH: For some integer L 0 > 0 , we have C L 0 : = inf x R d V L 0 ( x ) > 0 .
Notice that assumption UH implies U = R d and Hörmander’s hypothesis H(x) is true for any x R d .
Suppose that H(x), C, M, and P hold. Based on assumption H(x), (13), Formulas (21) and (22) for the Malliavin matrix Q ( t , x ) , and proceeding as in the proof of Theorem 2.3.2 in [16], we can show that the Malliavin matrix Q ( t , x ) is invertible almost surely. Thus, since from (15) we also know that X ( t , 0 , x ) D 1 , p for any p 2 , this implies that the law of X ( t , 0 , x ) is absolutely continuous with respect to the Lebesgue measure (Theorem 2.2.1 in [16]). Here, we replace assumption H(x) with assumption UH and we obtain an exponential bound for the density of the law of X ( t , 0 , x ) with respect to the Lebesgue measure.
Theorem 1.
Let X be the solution of SDE (1) and suppose that the assumptions C, M, P, and UH hold. Then, for any t ( 0 , T ] and any x R d the law of the random vector X ( t , 0 , x ) is absolutely continuous with respect to the Lebesgue measure, and for the density y p t ( x , y ) the following inequalities hold:
p t ( x , y ) K 0 ( T ) ( 1 + | x | Q 0 ) t q 0 exp C 0 ( | x y | 1 ) 2 t ( 1 + | x | ) 2 N ,
y α p t ( x , y ) K α ( T ) ( 1 + | x | Q α ) t q α exp C α ( | x y | 1 ) 2 t ( 1 + | x | ) 2 N ,
for any x , y R d , t ( 0 , T ] , t 1 ( | y x | 1 ) / ( 4 M ( x ) ) , where N is as in (8) and M ( x ) = sup z B ( x , 1 ) { σ ( z ) | b ( z ) | } . Here, the non-decreasing functions K 0 and K α and the positive real numbers C 0 , C α , Q 0 , and Q α depend on L N * such that x U L , and on the coefficients b and σ.
The proof is included in Section 5.
Example 2.
For the coefficients of the SDE (23), a simple calculation shows that assumption UH holds with L 0 = 3 . Thus, we can apply Theorem 1 and obtain the exponential bounds (24) and (25).
Example 3.
The following SDE includes a family of nonlinear mean-reverting models for interest rates [4]:
d X ( t ) = μ λ X ( t ) 3 d t + σ ¯ X ( t ) d W ( t ) , X ( 0 ) = x 0 > 0 ,
where t [ 0 , T ] , μ , λ , σ ¯ > 0 . We can easily check that the assumptions C, M, P, and UH are met, so we can apply Theorem 1 and obtain the exponential bounds (24) and (25).

4. Results About the Malliavin Matrix

Notice that we can write Equations (1), (17), (19), and (20) in Stratonovich form as follows:
X ( t ) = x + 0 t σ 0 ( X ( u ) ) d u + i = 1 m 0 t σ i ( X ( u ) ) d W i ( u ) ,
J ( t ) = I d + 0 t x σ 0 X ( s ) J ( s ) d s + i = 1 m 0 t x σ i X ( s ) J ( s ) d W i ( s ) ,
J 1 ( t ) = I d 0 t J 1 ( s ) x σ 0 X ( s ) d s i = 1 m 0 t J 1 ( s ) x σ i X ( s )     d W i ( s ) ,
J s ( t ) = I d + s t x σ 0 X ( r ) J s ( r ) d r + i = 1 m s t x σ i X ( r ) J s ( r ) d W i ( r ) .
Given V C ( R d , R d ) , we use Ito’s formula and Equations (27) and (29) (Equation 2.10 in [5], Equation 2.63, p. 130 in [16]) to obtain
J 1 ( t ) V ( X ( t ) ) = V ( x ) + 0 t J 1 ( s ) [ σ 0 , V ] ( X ( s ) ) d s + i = 1 m 0 t J 1 ( s ) [ σ i , V ] ( X ( s ) ) d W i ( s )
Theorem 2.
Suppose that assumptions C, M, and P hold. For any L 1 and 0 < ϵ 1 there exist C L , ϵ , λ ( L , ϵ ) , μ L , ϵ > 0 such that for all x R d and V C p ( R d , R d ) we have
J 1 ( t ) V ( X ( t ) ) = α L 1 T ( α ) ( V ) ( x ) I ( α ) ( t ) + R L ( t , x , V )
for K K 0 ( L , x , V ) > 1 , with
sup 0 < t < 1 P 1 t L 0 t / K | R L ( s , x , V ) | 2 d s 1 K L + 1 ϵ C L , ϵ exp λ ( L , ϵ ) K μ L , ϵ ( 1 + M ( x ) ) 2
with
M ( x ) = max { σ i C b 2 ( B ( x , 1 ) , R d ) , i = 0 , , m } max { T ( α ) ( V ) C b 0 ( B ( x , 1 ) , R d ) , | α | L + 1 }
The proof is included in Appendix A.
Theorem 3.
Suppose that assumptions C, M, and P hold. For any L 1 there exists C ( L ) , C ˜ ( L ) > 0 , λ ( L ) , λ ˜ ( L ) > 0 , and μ L , μ ˜ L ( 0 , 1 ] , all of them independent of σ 0 , , σ m , such that for all t ( 0 , 1 ] and all K 1 we have
P λ ˜ t K 1 / ( L + 1 ) , x t L 1 K C ˜ ( L ) exp λ ˜ L V L ( x ) L + 2 K μ ˜ L ( 1 + M ( x ) ) 2
P λ t K 1 / ( L + 1 ) , x t L 1 K C ( L ) exp λ L V L ( x ) L + 2 K μ L ( 1 + M ( x ) ) 2 ,
where
λ ˜ ( s , x ) = inf | η | = 1 < η , C ( s , x ) η > , λ ( s , x ) = inf | η | = 1 < η , Q ( s , x ) η >
M ( x ) = max { T ( α ) ( σ k ) C b 2 ( B ( x , 1 ) , R d ) , k = 0 , , m , | α | L + 1 }
The proof is given in Appendix B.
Let us denote
Δ ( t , x ) : = det Q ( t , x ) , Δ ˜ ( t , x ) : = det C ( t , x )
Equations (21), (22), and (36) imply that C ( t , x ) and Q ( t , x ) are positive semi-definite and both λ ˜ ( t , x ) and λ ( t , x ) are non-decreasing with respect to t.
Theorem 4.
Suppose that assumptions C, M, and P hold, and let L N * . For any p 1 there exists K ( L , p ) , μ ( L ) > 0 , also depending on the coefficients b and σ, such that we have for any t ( 0 , 1 ] and any x U L
E 1 Δ ( t , x ) p K ( L , p ) ( 1 + | x | 2 ) p μ ( L ) ( V L ( x ) 1 + 2 / L t ) p d L
Proof. 
We know from (22) that Q ( t , x ) is positive semi-definite, so that the smallest eigenvalue of Q ( t , x ) is equal with λ ( t , x ) , and we have ( λ ( t , x ) ) d det ( Q ( t , x ) ) . These imply that for any p 1 ,
E 1 ( Δ ( t , x ) ) p E 1 λ ( t , x ) p d .
Next, since t λ ( t , x ) is non-decreasing, from (35) we obtain for any t ( 0 , 1 ] and K 1 ,
P λ ( t , x ) t L 1 K P λ ( t / K 1 / ( L + 1 ) , x ) t L 1 K C ( L ) exp λ L V L ( x ) L + 2 K μ L ( 1 + M ( x ) ) 2 ,
where C ( L ) , λ L > 0 , μ L ( 0 , 1 ] , and M ( x ) are as in Theorem 3. Using this, we obtain
E 1 λ ( t , x ) p d = 0 p d y p d 1 P λ ( t , x ) 1 > y d y = 0 p d y p d 1 P λ ( t , x ) t L < 1 y t L d y = 0 1 / A p d y p d 1 P λ ( t , x ) t L < 1 y t L d y + 1 / A p d y p d 1 P λ ( t , x ) t L < 1 y t L d y p d 1 A p d + 1 / A p d y p d 1 C ( L ) exp λ L A y μ L ( 1 + M ( x ) ) 2 d y = p d 1 A p d + p d C ( L ) μ L 1 A p d 1 z ( p d ) / μ L 1 exp λ L z ( 1 + M ( x ) ) 2 d z p d 1 A p d + p d C ( L ) μ L 1 A p d 1 z k 1 exp λ L z ( 1 + M ( x ) ) 2 d z ,
where
A : = V L ( x ) L + 2 t L ( 0 , 1 ] , k = p d μ L + 1 1 .
By repeatedly applying integration by parts, we obtain
E 1 λ ( t , x ) p d C 1 ( L , p ) 1 A p d ( 1 + M ( x ) ) 2 p d / μ L + 1
From assumption C and (6)–(9) we obtain
M ( x ) 2 C 1 ( 1 + | x | 2 N ) .
This yields
E 1 λ ( t , x ) p d K ( L , p ) ( 1 + | x | 2 ) 2 N p d / μ L + N V L ( x ) 1 + 2 / L t p d L K ( L , p ) ( 1 + | x | 2 ) N p d ( 2 / μ L + 1 ) V L ( x ) 1 + 2 / L t p d L
Thus, substituting μ L ( 0 , 1 ] into (39) we obtain (38). □

5. Proof of Theorem 1

Proof. 
From Theorem 4 we obtain that 1 / Δ ( t , x ) p 1 L p ( Ω , R ) , and since X ( t , 0 , x ) D , X ( t , 0 , x ) is non-degenerate for any t ( 0 , T 1 ] , x R d (see Definition 2.1.1 in [16]). Thus, we have the integration by parts formulas (Proposition 2.1.4 in [16]): for any ϕ C p ( R d ) , G D and any index α , there exists H α ( X ( t , 0 , x ) , G ) D such that
E [ α ϕ ( X ( t , 0 , x ) ) G ] = E [ ϕ ( ( X ( t , 0 , x ) ) H α ( X ( t , 0 , x ) , G ) ] .
Moreover, for any 1 < p < q 1 < there exist constants C p , q > 0 , β , γ > 1 and k 1 , k 2 N * such that
H α ( X ( t , 0 , x ) , G ) p C p , q 1 1 Δ ( t , x ) β k 1 D X ( t , 0 , x ) | α | , γ k 2 G | α | , q 1 .
Using this, it can be shown (Proposition 2.1.5 in [16]) that the density p t belongs to the Schwarz space S ( R d ) = { f : R d R : f C ( R d ) , sup x R d | x | k | α f ( x ) | < for any k 1 , and any index α }. Moreover, for any y = ( y 1 , , y d ) R d such that y i > 0 x i , i = 1 , , d , we have
p t ( x , y ) = E [ 1 I y ( X ( t , 0 , x ) ) H ( 1 , , 1 ) ( X ( t , 0 , x ) , 1 ) ] , I y = i = 1 d [ y i , ) .
Using the Cauchy–Schwarz inequality, (40), (38) in Theorem 4, and (16) we obtain that for any x R d , t ( 0 , T 1 ] ,
p t ( x , y ) E [ 1 I y ( X ( t , 0 , x ) ) ] 1 / 2 E [ | H ( 1 , , d ) ( X ( t , 0 , x ) , 1 ) | 2 ] 1 / 2 ( P ( X ( t , 0 , x ) I y ) ) 1 / 2 C 1 Δ ( t , x ) β k 1 D X ( t , 0 , x ) d , γ k 2 C K L ( t ) ( 1 + | x | Q ) t d L k 1 ( P ( X ( t , 0 , x ) I y ) ) 1 / 2 ,
where L N * is as in Theorem 4, K L ( · ) is non-decreasing, C > 0 , β , γ > 1 , and k 1 , k 2 N * .
Let
τ = inf s [ 0 , T ] { | X ( s , 0 , x ) x | 1 / 2 } T , ξ = inf s [ 0 , T ] { | X ( s , 0 , x ) x | 1 } T
If | y x | < 1 , we have
P ( X ( t , 0 , x ) I y ) ) = P i = 1 d { X i ( t , x ) y i } = P i = 1 d { X i ( t , x ) x i y i x i } P | X ( t , 0 , x ) x | | y x | P sup 0 s t ξ 0 s b ( X ( u , 0 , x ) ) d u + i = 1 m 0 s σ i ( X ( u , 0 , x ) ) d W i ( u ) | y x | P sup 0 s t ξ 0 s | b ( X ( u , 0 , x ) ) | d u + i = 1 m 0 s | σ i ( X ( u , 0 , x ) ) | d W i ( u ) | y x |
For s t ξ we have | X ( u , 0 , x ) x | 1 for any u [ 0 , s ] , so X ( u , 0 , x ) B ( x , 1 ) and | b ( X ( u , 0 , x ) ) | M ( x ) , | σ ( X ( u , 0 , x ) ) | M ( x ) for any u [ 0 , s ] . This implies
0 s b ( X ( u , 0 , x ) ) d u t M ( x ) | y x | / 2 ,
for any t | y x | / ( 2 M ( x ) ) . We also have
0 s | σ i ( X ( u , 0 , x ) ) | 2 d u M ( x ) 2 t , i = 1 , , m .
Hence, for any t | y x | / ( 2 M ( x ) ) we obtain
P sup 0 s t ξ 0 s | b ( X ( u , 0 , x ) ) | d u + i = 1 m 0 s | σ i ( X ( u , 0 , x ) ) | d W i ( u ) | y x | 2 d exp | y x | 2 8 d t M ( x ) 2
Here, we have applied Lemma 8.5 from Chapter V, Section 8 [17] for each component of X.
Similarly, if | y x | > 1
P ( X ( t , 0 , x ) I y ) ) P | X ( t , 0 , x ) x | | y x | P τ t = P sup 0 s t ξ | X ( s , 0 , x ) x | 1 / 2 = P sup 0 s t ξ 0 s b ( X ( u , 0 , x ) ) d u + i = 1 m 0 s σ i ( X ( u , 0 , x ) ) d W i ( u ) 1 / 2 P sup 0 s t ξ 0 s | b ( X ( u , 0 , x ) ) | d u + i = 1 m 0 s | σ i ( X ( u , 0 , x ) ) | d W i ( u ) 1 / 2
For s t ξ we have | X ( u , 0 , x ) x | 1 for any u [ 0 , s ] , so X ( u , 0 , x ) B ( x , 1 ) and | b ( X ( u , 0 , x ) ) | M ( x ) , | σ ( X ( u , 0 , x ) ) | M ( x ) for any u [ 0 , s ] . This implies
0 s b ( X ( u , 0 , x ) ) d u t M ( x ) 1 / 4 ,
for any t 1 / ( 4 M ( x ) ) . We also have
0 s | σ i ( X ( u , 0 , x ) ) | 2 d u M ( x ) 2 t , i = 1 , , m .
Hence, for any t 1 / ( 4 M ( x ) ) we obtain
P sup 0 s t ξ 0 s | b ( X ( u , 0 , x ) ) | d u + i = 1 m 0 s | σ i ( X ( u , 0 , x ) ) | d W i ( u ) 1 / 2 2 d exp 1 16 d t M ( x ) 2
Here, we have applied Lemma 8.5 in Chapter V, Section 8 [17] for each component of X.
Thus, we obtain for t ( | y x | 1 ) / ( 4 M ( x ) )
P ( X ( t , 0 , x ) I y ) ) 2 d exp ( | y x | 2 1 ) 16 d t M ( x ) 2
Notice that from (6) and (8) we obtain
M ( x ) 2 C sup z B ( x , 1 ) ( 1 + | z | ) 2 N C sup z B ( x , 1 ) ( 1 + | z x | + | x | ) 2 N C ( 2 + | x | ) 2 N 2 2 N C ( 1 + | x | ) 2 N
Substituting this into (42), we obtain, for t ( | y x | 1 ) / ( 4 M ( x ) ) ,
P ( X ( t , 0 , x ) I y ) ) C 1 exp C 2 ( | y x | 2 1 ) t ( 1 + | x | ) 2 N
This inequality and (41) imply (24) for t 1 ( | y x | 1 ) / ( 4 M ( x ) ) .
Next, we prove (25). From Proposition 2.1.5 [16] we know that for any index α , and for any y = ( y 1 , , y d ) R d such that y i > 0 x i , i = 1 , , d , we have
y α p t ( x , y ) = ( 1 ) | α | E 1 I y ( X ( t , 0 , x ) ) H α X ( t , 0 , x ) , H ( 1 , , 1 ) ( X ( t , 0 , x ) , 1 ) ,
where I y = i = 1 d [ y i , ) . Using this formula, the proof is similar to the proof of (24). □

6. Conclusions and Future Work

We have proved exponential bounds for the density of the law of the solution of the autonomous SDE (1). This result is based on the Malliavin differentiability of any order for the solution of (1) with coefficients satisfying the assumptions C, M, and P.
Here, we obtain exponential bounds for the density p t ( x , y ) and for its partial derivatives with respect to y. As future work, we plan to also find bounds for the partial derivatives with respect to x and t. This would fully extend the results in [5] to SDEs with non-globally Lipschitz coefficients. Moreover, as we have mentioned before, the exponential bounds for the density can be used to obtain an expansion of the error for numerical schemes. Symplectic methods for general stochastic Hamiltonian systems are fully implicit [18,19], and their convergence can be proved under non-globally Lipschitz assumptions. This paper was motivated by our interest in obtaining an expansion of the error for these symplectic schemes. In the stochastic case, there is no theoretical proof of the better long term accuracy of the symplectic schemes compared with non-symplectic ones, and the study of the error could be an important step in solving this problem.

Funding

This work was supported by the Natural Sciences and Engineering Research Council of Canada under Grant DG-2018-04449.

Data Availability Statement

Data sharing is not applicable to this article. The article describes entirely theoretical research.

Conflicts of Interest

The author declares no conflicts of interest.

Appendix A. Proof of Theorem 2

Proof. 
The proof is similar with the proof of Theorem 2.12 in [5]. By repeated application of (31), we see that we have
J 1 ( t ) V ( X ( t ) ) = V ( x ) + i = 0 m 0 t J 1 ( s ) [ σ i , V ] ( X ( s ) ) d W i ( s ) = V ( x ) + i = 0 m [ σ i , V ] ( x ) 0 t 1 d W i ( s ) + i , j = 0 m 0 t 0 s J 1 ( s ) [ σ j , [ σ i , V ] ] ( X ( s ) ) d W j ( u ) d W i ( s ) = V ( x ) + i = 0 m [ σ i , V ] ( x ) 0 t 1 d W i ( s ) + i , j = 0 m [ σ j , [ σ i , V ] ] ( x ) 0 t 0 s 1 d W j ( u ) d W i ( s ) + i , j , k = 0 m 0 t 0 s 0 u J 1 ( s ) [ σ k , [ σ j , [ σ i , V ] ] ] ( X ( s ) ) d W k ( v ) d W j ( u ) d W i ( s ) = | α | L 1 T ( α ) ( V ) ( x ) I ( α ) ( t ) + | α | = L S ( α ) ( t , Z ( α ) )
where as in the proof of Theorem 2.12 [5], we set (see also Equation 2.63, p. 130 [16])
S ( α ) ( t , Z ( α ) ) = Z ( α ) ( t ) if α = , 0 t S ( α ) ( s , Z ( α ) ) d W α * ( s ) if | α | 1 , Z ( α ) ( t ) = J 1 ( t ) T ( α ) ( V ) ( X ( t ) ) = T ( α ) ( V ) ( x ) + i = 0 m 0 t J 1 ( s ) [ σ i , T ( α ) ( V ) ] ( X ( s ) ) d W i ( s ) = T ( α ) ( V ) ( x ) + i = 1 m 1 t J 1 ( s ) [ σ i , T ( α ) ( V ) ] ( X ( s ) ) d W i ( s ) + 0 t J 1 ( s ) ( [ σ 0 , T ( α ) ( V ) ] + 1 2 i = 1 m [ σ i , [ σ i , T ( α ) ( V ) ] ] ) ( X ( s ) ) d s
Notice that S ( α ) ( t , 1 ) = I ( α ) ( t ) .
From (A1), we have expansion (32) with
R L ( t , x , V ) = | α | = L S ( α ) ( t , Z ( α ) ) + α L | α | L 1 T ( α ) ( V ) ( x ) I ( α ) ( t )
For f C ( [ 0 , 1 ] ) , we have for any t ( 0 , 1 ] and K 1 ,
0 t / K | f ( s ) | 2 d s = 0 t / K | f ( s ) | s L / 2 ϵ / 4 2 s L ϵ / 2 d s sup 0 < s 1 / K | f ( s ) | s L / 2 ϵ / 4 2 0 t / K s L ϵ / 2 d s = 2 2 L ϵ + 2 sup 0 < s 1 / K | f ( s ) | 2 s L ϵ / 2 t K L ϵ / 2 + 1 2 2 L ϵ sup 0 < s 1 / K | f ( s ) | 2 s L ϵ / 2 t K L ϵ / 2 + 1
Hence, for any 0 < t 1 , K 1 we have
P 1 t L 0 t / K | R L ( s , x , V ) | 2 d s 1 K L + 1 ϵ P 2 2 L ϵ sup 0 < s 1 / K | R L ( s , x , V ) | 2 s L ϵ / 2 t 1 ϵ / 2 K ϵ / 2 P 2 2 L ϵ sup 0 < s 1 / K | R L ( s , x , V ) | 2 s L ϵ / 2 K ϵ / 2 P 2 2 L ϵ sup 0 < s 1 / K | R L ( s , x , V ) | s L / 2 ϵ / 4 2 K ϵ / 2 = P sup 0 < s 1 / K | R L ( s , x , V ) | s L / 2 ϵ / 4 2 L ϵ 2 1 / 2 K ϵ / 4 | α | = L P sup 0 < s 1 / K | S ( α ) ( s , Z ( α ) ) | s L / 2 ϵ / 4 K 1 + α L | α | L 1 P sup 0 < s 1 | T ( α ) ( V ) ( x ) I ( α ) ( s ) | s L / 2 ϵ / 4 K 1 ,
where K 1 = 2 L ϵ 2 1 / 2 K ϵ / 4 N , with N = card { α A , | α | = L } + card { α A , | α | L 1 , α L } .
To handle the terms of the first sum, let us define
Y i ( α ) ( s ) = J 1 ( s ) [ σ i , T ( α ) ( V ) ] ( X ( s ) ) , i = 1 , , m Y 0 ( α ) ( s ) = J 1 ( s ) [ σ 0 , T ( α ) ( V ) ] + 1 2 i = 1 m [ σ i , [ σ i , T ( α ) ( V ) ] ]
We obtain, for any α A , | α | = L ,
P sup 0 < s 1 / K | S ( α ) ( s , Z ( α ) ) | s L / 2 ϵ / 4 K 1 P sup 0 < s 1 / K | S ( α ) ( s , Z ( α ) ) | s α / 2 ϵ / 4 K 1 P sup 0 < s 1 / K | S ( α ) ( s , Z ( α ) ) | s α / 2 ϵ / 4 K 1 , sup 0 < s 1 / K | Z ( α ) ( s ) | K 2 , ( i = 1 m 0 1 / K | Y i ( α ) ( s ) | 2 d s ) 1 / 2 K 2 + P sup 0 < s 1 / K | Z ( α ) ( s ) | K 2 + P ( i = 1 m 0 1 / K | Y i ( α ) ( s ) | 2 d s ) 1 / 2 K 2 = : P 1 ( α ) + P 2 ( α ) + P 3 ( α ) ,
where K 2 = K 1 2 α K 1 2 2 L for a K large enough because L     α   2 | α | = 2 L . From Theorem A.5 [5] we know that there exist C ( L , ϵ ) > 0 , λ ( L , ϵ ) > 0 such that
P 1 ( α ) C ( L , ϵ ) exp λ 1 ( L , ϵ ) K 2 C ( L , ϵ ) exp λ 1 ( L , ϵ ) K 1 2 2 L .
Thus, there exist C 1 ( L , ϵ ) > 0 , λ 1 ( L , ϵ ) > 0 , μ 1 ( L , ϵ ) > 0 such that
| α | = L P 1 ( α ) C 1 ( L , ϵ ) exp λ 1 ( L , ϵ ) K μ 1 ( L , ϵ ) .
For K > 1 , let
τ = inf { s 0 : J 1 ( s ) I d | X ( s ) x | 1 / 2 } T ξ = inf { s 0 : J 1 ( s ) I d | X ( s ) x | 1 } T
We denote F ( s ) = ( X ( s ) , J 1 ( s ) ) . We have
P sup 0 < s 1 / K | Z ( α ) ( s ) Z ( α ) ( 0 ) | K 2 P sup 0 < s 1 / K | Z ( α ) ( s ) Z ( α ) ( 0 ) | K 2 , τ > 1 / K + P τ 1 / K P sup 0 < s 1 τ | Z ( α ) ( s ) Z ( α ) ( 0 ) | K 2 + P sup 0 < s 1 / K ξ | F ( s ) F ( 0 ) | 1 / 2
For a K large enough, we apply Lemma 8.5 in Chapter V, Section 8 [17] for each component of Z ( α ) and F and we obtain
P 2 ( α ) C 1 exp λ 1 K 2 / ( 1 + M ( x ) ) 2 + C 2 exp λ 2 K / ( 1 + M ( x ) ) 2
Notice that we have
P 3 ( α ) i = 1 m P 0 1 / K | Y i ( α ) ( s ) | 2 d s K 2 2 m i = 1 m P sup 0 < s 1 / K | Y i ( α ) ( s ) | 2 K 2 2 m i = 1 m P sup 0 < s 1 / K | Y i ( α ) ( s ) | 2 K 2 2 m = i = 1 m P sup 0 < s 1 / K | Y i ( α ) ( s ) | K 2 m
For Y i ( α ) , i = 1 , , m , we have an SDE similar to the one for Z ( α ) but with [ σ i , T ( α ) ( V ) ] replacing T ( α ) ( V ) , so we can treat P 2 ( α ) and the terms of P 3 ( α ) similarly.
Finally, since S ( α ) ( t , 1 ) = I ( α ) ( t ) , we obtain for any α A , | α | L 1 , α L
P sup 0 < s 1 | T ( α ) ( V ) ( x ) I ( α ) ( s ) | s L / 2 ϵ / 4 K 1 P sup 0 < s 1 | I ( α ) ( s ) | s L / 2 ϵ / 4 K 1 M ( x ) 2 P sup 0 < s 1 | S ( α ) ( s , 1 ) | s α / 2 ϵ / 4 K 1 2 M ( x ) 2
If K is large enough, using Theorem A.5 [5] we know that there exist C ( L , ϵ ) > 0 , λ ( L , ϵ ) > 0 and μ 1 ( L , ϵ ) > 0 such that
α L | α | L 1 P sup 0 < s 1 | T ( α ) ( V ) ( x ) I ( α ) ( s ) | s L / 2 ϵ / 4 K 1 C ( L , ϵ ) exp λ ( L , ϵ ) K μ 1 ( L , ϵ ) ( 1 + M ( x ) ) 2

Appendix B. Proof of Theorem 3

Proof. 
This proof is similar to the proof of Theorem 2.17 [5]. From (22) and (36), notice that C ( t , x ) is positive semi-definite and both C ( t , x ) and λ ˜ ( t , x ) are non-decreasing with respect to t, so it is enough to prove (34) for K 1 large enough. Since for any a , b 0 we have ( a + b ) 2 a 2 / 2 b 2 , from (22) and (32) we have for any t ( 0 , 1 ] , K > 1 and η R d , | η | = 1 ,
< η , C ( t / K , x ) η > = k = 1 m 0 t / K < J ( s ) 1 σ k ( X ( s ) ) , η > 2 d s = k = 1 m 0 t / K < α L 1 T ( α ) ( σ k ) ( x ) I ( α ) ( s ) + R L ( s , x , σ k ) , η > 2 d s = k = 1 m 0 t / K < α L 1 T ( α ) ( σ k ) ( x ) I ( α ) ( s ) , η > + < R L ( s , x , σ k ) , η > 2 d s 1 2 k = 1 m 0 t / K < α L 1 T ( α ) ( σ k ) ( x ) I ( α ) ( s ) , η > 2 d s k = 1 m 0 t / K < R L ( s , x , σ k ) , η > 2 d s 1 2 k = 1 m 0 t / K < α L 1 T ( α ) ( σ k ) ( x ) , η > I ( α ) ( s ) 2 d s k = 1 m 0 t / K | R L ( s , x , σ k ) | 2 d s
This implies
inf | η | = 1 k = 1 m 0 t / K < α L 1 T ( α ) ( σ k ) ( x ) , η > I ( α ) ( s ) 2 d s 2 inf | η | = 1 < η , C ( t / K , x ) η > + 2 k = 1 m 0 t / K | R L ( s , x , σ k ) | 2 d s = 2 λ ˜ ( t / K , x ) + 2 k = 1 m 0 t / K | R L ( s , x , σ k ) | 2 d s
Let
M k ( x , η ) : = α L 1 < T ( α ) ( σ k ) ( x ) , η > 2
Since for any η R d , | η | = 1 ,
V L ( x , η ) = k = 1 m M k ( x , η ) V L ( x ) , α L 1 < T ( α ) ( σ k ) ( x ) , η > 2 M k ( x , η ) = 1
we obtain
inf | η | = 1 k = 1 m 0 t / K < α L 1 T ( α ) ( σ k ) ( x ) , η > I ( α ) ( s ) 2 d s = inf | η | = 1 k = 1 , M k ( x , η ) > 0 m M k ( x , η ) 0 t / K α L 1 < T ( α ) ( σ k ) ( x ) , η > M k ( x , η ) I ( α ) ( s ) 2 d s inf | η | = 1 k = 1 m M k ( x , η ) inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 = inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 inf | η | = 1 V L ( x , η ) inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 V L ( x )
Here, if M k ( x , η ) = 0 , then < T ( α ) ( σ k ) ( x ) , η > = 0 for any α L 1 , so the term corresponding to such a k is 0.
Thus, for any L 1 , (A2) yields for any ϵ ( 0 , 1 ) , t ( 0 , 1 ] , and K 1 ,
P λ ˜ ( t / K , x ) t L 1 K L + 1 ϵ P ( V L ( x ) 2 t L inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 1 t L k = 1 m 0 t / K | R L ( s , x , σ k ) | 2 d s 1 K L + 1 ϵ ) P ( 1 t L k = 1 m 0 t / K | R L ( s , x , σ k ) | 2 d s 1 K L + 1 ϵ ) + P ( V L ( x ) 2 t L inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 2 K L + 1 ϵ ) k = 1 m P ( 1 t L 0 t / K | R L ( s , x , σ k ) | 2 d s 1 m K L + 1 ϵ ) + P ( K t L inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 4 V L ( x ) K 1 ϵ )
By Theorem A.6 [5], there exist C 1 ( L , ϵ ) , μ 1 ( L , ϵ ) > 0 such that for all t ( 0 , 1 ] ,
P ( K t L inf 0 t / K α L 1 b α I ( α ) ( s ) 2 d s : α L 1 b α 2 = 1 4 V L ( x ) K 1 ϵ ) C 1 ( L , ϵ ) exp V L ( x ) K 1 ϵ 4 μ 1 ( L , ϵ )
By Theorem 2, there exist C 2 ( L , ϵ ) , λ 2 ( L , ϵ ) , μ 2 ( L , ϵ ) > 0 such that for all t ( 0 , 1 ] and K 1 large enough,
k = 1 m P ( 1 t L k = 1 m 0 t / K | R L ( s , x , σ k ) | 2 d s 1 m K L + 1 ϵ ) m C 2 ( L , ϵ ) exp λ 2 ( L , ϵ ) m 1 / ( L + 1 ϵ ) K μ 2 ( L , ϵ ) ( 1 + M ( x ) ) 2
Replacing K with K 1 / ( L + 1 ) and then taking ϵ = 1 / ( L + 2 ) and using V L ( x ) ) 1 , we obtain that there exist C ˜ ( L ) > 0 , λ ˜ ( L ) > 0 , and μ ˜ L > 0 , all of them independent of σ 0 , , σ m , such that for all t ( 0 , 1 ] and any K 1 large enough,
P λ ˜ ( t / K 1 / ( L + 1 ) , x ) t L 1 K P λ ˜ ( t / K 1 / ( L + 1 ) , x ) t L 1 K ( L + 1 ϵ ) / ( L + 1 ) C 1 ( L , ϵ ) exp V L ( x ) K ( 1 ϵ ) / ( L + 1 ) 4 μ 1 ( L , ϵ ) + m C 2 ( L , ϵ ) exp λ 2 ( L , ϵ ) m 1 / ( L + 1 ϵ ) K 1 / ( L + 1 ) μ 2 ( L , ϵ ) ( 1 + M ( x ) ) 2
C 1 ( L ) exp V L ( x ) K 1 / ( L + 2 ) 4 μ 1 ( L ) + m C 2 ( L ) exp λ 2 ( L ) m ( L + 2 ) / ( L 2 + 3 L + 1 ) K 1 / ( L + 1 ) μ 2 ( L ) ( 1 + M ( x ) ) 2 C 1 ( L ) exp 1 4 μ 1 ( L ) ( V L ( x ) ) L + 2 K μ 1 ( L ) / ( L + 2 ) ( 1 + M ( x ) ) 2 + m C 2 ( L ) exp λ 3 ( L ) ( V L ( x ) ) L + 2 K μ 2 ( L ) / ( L + 1 ) ( 1 + M ( x ) ) 2 C ˜ ( L ) exp λ ˜ L V L ( x ) L + 2 K μ ˜ L ( 1 + M ( x ) ) 2
For K 1 large enough we can consider μ ˜ L ( 0 , 1 ] .
Next, notice that for any η R d , | η | = 1 ,
< η , Q ( s , x ) η > = < J ( s ) η , C ( s , x ) J ( s ) η > = | J ( s ) η | 2 < J ( s ) η | J ( s ) η | , C ( s , x ) J ( s ) η | J ( s ) η | | J ( s ) η | 2 λ ˜ ( s , x )
Let
τ = inf { s 0 : J ( s ) I d 1 / 2 } T , τ 1 = inf { s 0 : J ( s ) I d 1 } T ξ = inf { s 0 : | X ( s ) x | 1 / 2 } T , ξ 1 = inf { s 0 : | X ( s ) x | 1 } T .
Notice that for s τ we have
| J ( s ) η | 2 = | ( J ( s ) I d ) η + η | 2 1 2 | η | 2 | ( J ( s ) I d ) η | 2 1 2 J ( s ) I d 2 | η | 2 1 2 1 4 = 1 4
Hence, for s τ and for any η R d , | η | = 1 ,
< η , Q ( s , x ) η > 1 4 λ ˜ ( s , x )
Thus, there exist C ( L ) > 0 , λ ( L ) > 0 , and μ L > 0 , all of them independent of σ 0 , , σ m , such that for all t ( 0 , 1 ) and all K 1 large enough we have
P λ t K 1 / ( L + 1 ) , x t L 1 K P λ ˜ t K 1 / ( L + 1 ) , x t L 4 K , τ > 1 K 1 / ( L + 1 ) + P τ 1 K 1 / ( L + 1 ) , ξ > 1 K 1 / ( L + 1 ) + P ξ 1 K 1 / ( L + 1 ) P λ ˜ t K 1 / ( L + 1 ) , x t L 4 K + P sup 0 < s τ 1 1 K 1 / ( L + 1 ) J ( s ) I d 1 / 2 , ξ > 1 K 1 / ( L + 1 )
+ P sup 0 < s ξ 1 1 K 1 / ( L + 1 ) | X ( s ) x | 1 / 2 C 0 ( L ) exp λ 0 ( L ) V L ( x ) L + 2 K μ 0 ( L ) ( 1 + M ( x ) ) 2 + C 1 ( L ) exp λ 1 ( L ) K 1 / ( L + 1 ) ( 1 + M ( x ) ) 2 + C 2 ( L ) exp λ 2 ( L ) K 1 / ( L + 1 ) ( 1 + M ( x ) ) 2 C 0 ( L ) exp λ 0 ( L ) V L ( x ) L + 2 K μ 0 ( L ) ( 1 + M ( x ) ) 2 + C 1 ( L ) exp λ 1 ( L ) V L ( x ) L + 2 K 1 / ( L + 1 ) ( 1 + M ( x ) ) 2 + C 2 ( L ) exp λ 2 ( L ) V L ( x ) L + 2 K 1 / ( L + 1 ) ( 1 + M ( x ) ) 2 C ( L ) exp λ L V L ( x ) L + 2 K μ L ( 1 + M ( x ) ) 2
Here, we have used V L ( x ) 1 , and for the first probability in the third inequality we have used (34) (we have 4 / K instead of 1 / K but we can adjust the constants from the beginning of the proof of (34)). For the second and third probabilities in the third inequality for a K > 1 large enough, we have applied Lemma 8.5 from Chapter V, Section 8 [17] for each component of X and J. □

References

  1. Bally, V.; Talay, D. The law of the Euler scheme for stochastic diferential equations I. Convergence rate of the distribution function. Probab. Theory Relat. Fields 1996, 104, 43–60. [Google Scholar] [CrossRef]
  2. Hutzenthaler, M.; Jentzen, A.; Kloeden, P. Strong and weak divergence in finite time of Euler’s method for stochastic differential equations with nonglobally Lipschitz continuous coefficients. Proc. R. Soc. Lond. Ser. A Math. Phys. Sci. 2011, 467, 1563–1576. [Google Scholar]
  3. Kloeden, P.; Platen, E. Numerical Solutions of Stochastic Differential Equations; Springer: Berlin, Germany, 1992. [Google Scholar]
  4. Mao, X.; Szpruch, L. Strong convergence rates for backward Euler–Maruyama method for non-linear dissipative-type stochastic differential equations with super-linear diffusion coefficients. Stochastics 2013, 85, 144–171. [Google Scholar] [CrossRef]
  5. Kusuoka, S.; Stroock, D. Applications of the Malliavin calculus, part II. J. Fac. Sci. Univ. Tokyo 1985, 32, 1–76. [Google Scholar]
  6. Marco, S.D. Smoothness and asymptotic estimates of densities for SDEs with locally smooth coefficients and applications to square root-type diffusions. Ann. Appl. Probab. 2011, 21, 1282–1321. [Google Scholar] [CrossRef]
  7. Xie, L.; Zhang, X. Sobolev differentiable flows of SDEs with local Sobolev and super-linear growth coefficients. Ann. Probab. 2016, 44, 3661–3687. [Google Scholar] [CrossRef]
  8. Baudoin, F.; Ouyang, C.; Tindel, S. Upper bounds for the density of solutions to stochastic differential equations driven by fractional Brownian motions. Ann. L’Institut Henri Poincaré Probab. Stat. 2014, 50, 111–135. [Google Scholar] [CrossRef]
  9. Imkeller, P.; dos Reis, G.; Salkeld, W. Differentiability of SDEs with drifts of super-linear growth. Electron. J. Probab. 2019, 24, 1–43. [Google Scholar] [CrossRef]
  10. Anton, C. Malliavian differentiablity and smoothness of density for SDES with locally Lipschitz coefficients. arXiv 2024, arXiv:2405.19482. [Google Scholar]
  11. Cui, J.; Hong, J.; Sun, L. Weak convergence and invariant measure of a full discretization for parabolic SPDEs with non-globally Lipschitz coefficients. Stoch. Process. Their Appl. 2021, 134, 55–93. [Google Scholar] [CrossRef]
  12. Chen, C.; Hong, J.; Lu, Y. Stochastic differential equations with piecewise continuous arguments: Markov property, invariant measure and numerical approximation. Discret. Contin. Dyn. Syst.-Ser. B 2023, 28, 765–807. [Google Scholar] [CrossRef]
  13. Tretyakov, M.V.; Zhang, Z. A fundamental mean-square convergence theorem for SDEs with locally Lipschitz coefficients and its applications. SIAM J. Numer. Anal. 2013, 51, 3135–3162. [Google Scholar] [CrossRef]
  14. Mastrolia, T.; Possamaï, D.; Réveillac, A. On the Malliavin differentiability of BSDEs. Ann. L’Institut Henri Poincaré Probab. Stat. 2017, 53, 464–492. [Google Scholar] [CrossRef]
  15. Mao, X. Stochastic Differential Equations and Applications, 2nd ed.; Woodhead Pubilshing: Philadelphia, PA, USA, 2011. [Google Scholar]
  16. Nualart, D. The Malliavin Calculus and Related Topics, 2nd ed.; Springer: Berlin/Heidelberg, Germany, 2006. [Google Scholar]
  17. Ikeda, N.; Watanabe, S. Stochastic Differential Equations and Diffusion Processes; Elsevier: New York, NY, USA, 1989. [Google Scholar]
  18. Deng, J.; Anton, C.; Wong, Y. High-order symplectic schemes for stochastic Hamiltonian systems. Commun. Cumput. Phys. 2014, 16, 169–200. [Google Scholar] [CrossRef]
  19. Anton, C.; Deng, J.; Wong, Y. Weak Symplectic Schemes for Stochastic Hamiltonian Equations. Electron. Trans. Numer. Anal. 2014, 43, 15. [Google Scholar]
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Anton, C. Exponential Bounds for the Density of the Law of the Solution of an SDE with Locally Lipschitz Coefficients. Mathematics 2025, 13, 798. https://doi.org/10.3390/math13050798

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Anton C. Exponential Bounds for the Density of the Law of the Solution of an SDE with Locally Lipschitz Coefficients. Mathematics. 2025; 13(5):798. https://doi.org/10.3390/math13050798

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Anton, Cristina. 2025. "Exponential Bounds for the Density of the Law of the Solution of an SDE with Locally Lipschitz Coefficients" Mathematics 13, no. 5: 798. https://doi.org/10.3390/math13050798

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Anton, C. (2025). Exponential Bounds for the Density of the Law of the Solution of an SDE with Locally Lipschitz Coefficients. Mathematics, 13(5), 798. https://doi.org/10.3390/math13050798

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