Definition (Sub-Gaussian Random Variable). A random variable X X X is called a sub-gaussian random variable, if it exhibits one of the following equivalent properties: let K i > 0 , i ∈ [ 5 ] K_i > 0, i \in [5] K i > 0 , i ∈ [ 5 ] be absolute constants.
The tails of X X X satisfyPr [ ∣ X ∣ ≥ t ] ≤ 2 exp ( − t 2 K 1 2 ) , ∀ t ≥ 0.
\Pr[|X| \ge t]
\le 2 \exp \left(− \frac{t^2}{K_1^2} \right), \quad \forall t \ge 0.
Pr [ ∣ X ∣ ≥ t ] ≤ 2 exp ( − K 1 2 t 2 ) , ∀ t ≥ 0.
The moments of X X X satisfy∥ X ∥ L p = ( E ∣ X ∣ p ) 1 / p ≤ K 1 p ⋅ Γ ( p / 2 ) p ≤ K 2 p , ∀ p ≥ 1.
\Vert X \Vert_{L^p}
= ( \mathbb{E}|X|^p )^{1/p}
\le K_1 \sqrt[p]{p \cdot \Gamma(p / 2)}
\le
K_2 \sqrt{p},
\quad \forall p \ge 1.
∥ X ∥ L p = ( E ∣ X ∣ p ) 1/ p ≤ K 1 p p ⋅ Γ ( p /2 ) ≤ K 2 p , ∀ p ≥ 1.
The MGF of X 2 X^2 X 2 satisfiesE exp ( λ 2 X 2 ) ≤ exp ( K 3 2 λ 2 ) ∀ λ s.t. , ∣ λ ∣ ≤ 1 / K 3 .
\mathbb{E} \exp(\lambda^2 X^2)
\le \exp(K_3^2 \lambda^2)
\quad \forall \lambda \, \text{ s.t. }, \, |\lambda| \le 1 / K_3 .
E exp ( λ 2 X 2 ) ≤ exp ( K 3 2 λ 2 ) ∀ λ s.t. , ∣ λ ∣ ≤ 1/ K 3 .
The MGF of X 2 X^2 X 2 is bounded at some point, namelyE exp ( X 2 / K 4 2 ) ≤ 2.
\mathbb{E} \exp(X^2 / K_4^2) \le 2.
E exp ( X 2 / K 4 2 ) ≤ 2.
Moreover, if E [ X ] = 0 \mathbb{E} [ X ] = 0 E [ X ] = 0 then properties 1 - 4 are also equivalent to the following property.
The MGF of X X X satisfiesE exp ( λ X ) ≤ exp ( K 5 2 λ 2 ) ∀ λ ∈ R .
\mathbb{E} \exp(\lambda X) \le \exp(K_5^2 \lambda^2)
\quad \forall \lambda \in \mathbb{R}.
E exp ( λ X ) ≤ exp ( K 5 2 λ 2 ) ∀ λ ∈ R .
Proof.
1 → 2 : 1 \rightarrow 2: 1 → 2 :
E [ ∣ X ∣ p ] = ∫ 0 ∞ Pr [ ∣ X ∣ p ≥ t ] d t = ∫ 0 ∞ Pr [ ∣ X ∣ ≥ t 1 / p ] d t ≤ ∫ 0 ∞ 2 ⋅ exp ( − t 2 / p K 1 2 ) d t u = t 2 / p / K 1 2 → t = K 1 p u p / 2 = ∫ 0 ∞ 2 ⋅ K 1 p ⋅ ( p / 2 ) ⋅ u p / 2 − 1 e − u d u = K 1 p ⋅ p ⋅ Γ ( p / 2 )
\begin{aligned}
\mathbb{E} \big[ |X|^p \big]
&= \int_0^\infty \Pr\big[ |X|^p \ge t \big] \, d t \\
&= \int_0^\infty \Pr\big[ |X| \ge t^{1 / p} \big] \, d t \\
&\le \int_0^\infty 2 \cdot \exp \left(− \frac{t^{2/ p}}{K_1^2} \right) \, d t & u = t^{2/p} / K_1^2 \rightarrow t = K_1^p u^{p / 2} \\
&= \int_0^\infty 2 \cdot K_1^p \cdot (p / 2) \cdot u^{p / 2 - 1} e^{-u} \, d u \\
&= K_1^p \cdot p \cdot \Gamma(p / 2)
\end{aligned}
E [ ∣ X ∣ p ] = ∫ 0 ∞ Pr [ ∣ X ∣ p ≥ t ] d t = ∫ 0 ∞ Pr [ ∣ X ∣ ≥ t 1/ p ] d t ≤ ∫ 0 ∞ 2 ⋅ exp ( − K 1 2 t 2/ p ) d t = ∫ 0 ∞ 2 ⋅ K 1 p ⋅ ( p /2 ) ⋅ u p /2 − 1 e − u d u = K 1 p ⋅ p ⋅ Γ ( p /2 ) u = t 2/ p / K 1 2 → t = K 1 p u p /2 Applying the Stirling's approximation of Γ ( x ) ≤ x x \Gamma(x) \le x^x Γ ( x ) ≤ x x , and taking the p p p root of both sides given
E [ ∣ X ∣ p ] ≤ K 1 ⋅ p p ⋅ p / 2 .
\mathbb{E} \big[ |X|^p \big] \le K_1 \cdot \sqrt[p]{p} \cdot \sqrt{p / 2}.
E [ ∣ X ∣ p ] ≤ K 1 ⋅ p p ⋅ p /2 . 2 → 3 : 2 \rightarrow 3: 2 → 3 :
By monotone convergence theorem,
E exp ( λ 2 X 2 ) = E ( 1 + ∑ n ∈ N + λ 2 n X 2 n n ! ) = 1 + ∑ n ∈ N + E ( λ 2 n X 2 n n ! ) ≤ 1 + ∑ n ∈ N + ( λ 2 K 1 2 ) n ⋅ 2 n ⋅ Γ ( n ) n ! since E ∣ X ∣ 2 n ≤ K 1 2 n ⋅ 2 n ⋅ Γ ( 2 n / 2 ) ≤ 1 + 2 ⋅ ∑ n ∈ N + ( λ 2 K 1 2 ) n = 1 + 2 K 1 2 λ 2 1 − K 1 2 λ 2 provided that K 1 2 λ 2 < 1 = 1 + K 1 2 λ 2 1 − K 1 2 λ 2 = exp ( 3 ⋅ K 1 2 λ 2 ) , 1 + x 1 − x ≤ e 3 x , ∀ x ∈ [ 0 , 4 / 5 ] .
\begin{aligned}
\mathbb{E} \exp(\lambda^2 X^2)
&= \mathbb{E} \left( 1 + \sum_{n \in \mathbb{N}^+} \frac{\lambda^{2n} X^{2n}}{ n! } \right) \\
&= 1 + \sum_{n \in \mathbb{N}^+} \mathbb{E} \left( \frac{\lambda^{2n} X^{2n}}{ n! } \right) \\
&\le 1 + \sum_{n \in \mathbb{N}^+} \frac{ ( \lambda^2 K_1^2 )^n \cdot 2n \cdot \Gamma(n) }{ n! }
& \text{since } \mathbb{E} |X|^{2n} \le K_1^{2n} \cdot 2 n \cdot \Gamma(2n / 2) \\
&\le 1 + 2 \cdot \sum_{n \in \mathbb{N}^+} (\lambda^2 K_1^2 )^n \\
&= 1 + \frac{2 K_1^2 \lambda^2}{1 - K_1^2 \lambda^2} & \text{provided that } K_1^2 \lambda^2 < 1 \\
&= \frac{1 + K_1^2 \lambda^2}{1 - K_1^2 \lambda^2} \\
&= \exp(3 \cdot K_1^2 \lambda^2), & \frac{1 + x}{1 - x} \le e^{3x}, \, \forall x \in [0, 4 / 5].
\end{aligned}
E exp ( λ 2 X 2 ) = E ( 1 + n ∈ N + ∑ n ! λ 2 n X 2 n ) = 1 + n ∈ N + ∑ E ( n ! λ 2 n X 2 n ) ≤ 1 + n ∈ N + ∑ n ! ( λ 2 K 1 2 ) n ⋅ 2 n ⋅ Γ ( n ) ≤ 1 + 2 ⋅ n ∈ N + ∑ ( λ 2 K 1 2 ) n = 1 + 1 − K 1 2 λ 2 2 K 1 2 λ 2 = 1 − K 1 2 λ 2 1 + K 1 2 λ 2 = exp ( 3 ⋅ K 1 2 λ 2 ) , since E ∣ X ∣ 2 n ≤ K 1 2 n ⋅ 2 n ⋅ Γ ( 2 n /2 ) provided that K 1 2 λ 2 < 1 1 − x 1 + x ≤ e 3 x , ∀ x ∈ [ 0 , 4/5 ] . 3 → 4 : 3 \rightarrow 4: 3 → 4 :
Taking λ = 1 / K 3 \lambda = 1 / K_3 λ = 1/ K 3 in property 3 proves property 4.
4 → 1 : 4 \rightarrow 1: 4 → 1 :
By Markov's inequality, we have
Pr [ ∣ X ∣ ≥ t ] = Pr [ X 2 / K 4 2 ≥ t 2 / K 4 2 ] = Pr [ exp ( X 2 / K 4 2 ) ≥ exp ( t 2 / K 4 2 ) ] ≤ E exp ( X 2 / K 4 2 ) exp ( t 2 / K 4 2 ) ≤ 2 exp ( − t 2 / K 4 2 ) .
\begin{aligned}
\Pr[|X| \ge t]
&= \Pr[X^2 / K_4^2 \ge t^2 / K_4^2] \\
&= \Pr[\exp (X^2 / K_4^2 ) \ge \exp( t^2 / K_4^2 )] \\
&\le \frac{ \mathbb{E} \exp(X^2 / K_4^2) }{ \exp( t^2 / K_4^2 ) } \\
&\le 2 \exp( - t^2 / K_4^2 ).
\end{aligned}
Pr [ ∣ X ∣ ≥ t ] = Pr [ X 2 / K 4 2 ≥ t 2 / K 4 2 ] = Pr [ exp ( X 2 / K 4 2 ) ≥ exp ( t 2 / K 4 2 )] ≤ exp ( t 2 / K 4 2 ) E exp ( X 2 / K 4 2 ) ≤ 2 exp ( − t 2 / K 4 2 ) . 3 → 5 3 \rightarrow 5 3 → 5 (when ∣ λ ∣ ⋅ K 3 ≤ 1 |\lambda| \cdot K_3 \le 1 ∣ λ ∣ ⋅ K 3 ≤ 1 ):
Since e x ≤ x + e x 2 , ∀ x ∈ R e^x \le x + e^{x^2}, \forall x \in R e x ≤ x + e x 2 , ∀ x ∈ R , we have
E exp ( λ X ) ≤ E ( λ X + exp ( λ 2 X 2 ) ) = E ( exp ( λ 2 X 2 ) ) ≤ exp ( K 3 2 λ 2 ) .
\begin{aligned}
\mathbb{E} \exp(\lambda X)
&\le \mathbb{E} \left( \lambda X + \exp(\lambda^2 X^2) \right) \\
&= \mathbb{E} \left( \exp(\lambda^2 X^2) \right) \\
&\le \exp(K_3^2 \lambda^2).
\end{aligned}
E exp ( λ X ) ≤ E ( λ X + exp ( λ 2 X 2 ) ) = E ( exp ( λ 2 X 2 ) ) ≤ exp ( K 3 2 λ 2 ) . 4 → 5 4 \rightarrow 5 4 → 5 (when ∣ λ ∣ ⋅ K 3 ≥ 1 |\lambda| \cdot K_3 \ge 1 ∣ λ ∣ ⋅ K 3 ≥ 1 ):
Since λ X ≤ ( X 2 / K 3 2 + λ 2 ⋅ K 3 2 ) / 2 \lambda X \le (X^2 / K_3^2 + \lambda^2 \cdot K_3^2) / 2 λ X ≤ ( X 2 / K 3 2 + λ 2 ⋅ K 3 2 ) /2 , we have
E exp ( λ X ) ≤ E exp ( X 2 / K 3 2 + λ 2 ⋅ K 3 2 2 ) = exp ( λ 2 ⋅ K 3 2 2 ) ⋅ E exp ( X 2 / K 3 2 2 ) ≤ exp ( λ 2 ⋅ K 3 2 2 ) exp ( 1 2 ) exp ( λ 2 ⋅ K 3 2 ) ,
\begin{aligned}
\mathbb{E} \exp(\lambda X)
&\le \mathbb{E} \exp \left( \frac{X^2 / K_3^2 + \lambda^2 \cdot K_3^2}{2} \right) \\
&= \exp \left( \frac{\lambda^2 \cdot K_3^2}{2} \right) \cdot \mathbb{E} \exp \left( \frac{X^2 / K_3^2 }{2} \right) \\
&\le \exp \left( \frac{\lambda^2 \cdot K_3^2}{2} \right) \exp \left( \frac{1}{2} \right) \\
& \exp \left( \lambda^2 \cdot K_3^2 \right),
\end{aligned}
E exp ( λ X ) ≤ E exp ( 2 X 2 / K 3 2 + λ 2 ⋅ K 3 2 ) = exp ( 2 λ 2 ⋅ K 3 2 ) ⋅ E exp ( 2 X 2 / K 3 2 ) ≤ exp ( 2 λ 2 ⋅ K 3 2 ) exp ( 2 1 ) exp ( λ 2 ⋅ K 3 2 ) , where the final inequality follows as λ 2 K 3 2 ≥ 1 \lambda^2 K_3^2 \ge 1 λ 2 K 3 2 ≥ 1 .
5 → 1 : 5 \rightarrow 1: 5 → 1 :
When λ > 0 \lambda > 0 λ > 0 ,
Pr [ X ≥ t ] = Pr [ exp ( λ X ) ≥ exp ( λ t ) ] ≤ exp ( − λ t ) ⋅ E exp ( λ X ) ≤ exp ( − λ t + K 5 2 λ 2 ) = exp ( − t 2 4 K 5 2 ) choosing λ = 1 / ( 2 K 5 2 ) .
\begin{aligned}
\Pr[X \ge t]
&= \Pr[ \exp(\lambda X) \ge \exp(\lambda t) ] \\
&\le \exp(- \lambda t) \cdot \mathbb{E} \exp(\lambda X) \\
&\le \exp( - \lambda t + K_5^2 \lambda^2 ) \\
&= \exp \left( - \frac{t^2}{4 K_5^2} \right)
& \text{ choosing } \lambda = 1 / (2 K_5^2).
\end{aligned}
Pr [ X ≥ t ] = Pr [ exp ( λ X ) ≥ exp ( λ t )] ≤ exp ( − λ t ) ⋅ E exp ( λ X ) ≤ exp ( − λ t + K 5 2 λ 2 ) = exp ( − 4 K 5 2 t 2 ) choosing λ = 1/ ( 2 K 5 2 ) . When λ < 0 \lambda < 0 λ < 0 ,
Pr [ X ≤ − t ] = Pr [ exp ( λ X ) ≥ exp ( λ t ) ] ≤ exp ( − λ t ) ⋅ E exp ( λ X ) ≤ exp ( − λ t + K 5 2 λ 2 ) = exp ( − t 2 4 K 5 2 ) choosing λ = 1 / ( 2 K 5 2 ) .
\begin{aligned}
\Pr[X \le -t]
&= \Pr[ \exp(\lambda X) \ge \exp(\lambda t) ] \\
&\le \exp(- \lambda t) \cdot \mathbb{E} \exp(\lambda X) \\
&\le \exp( - \lambda t + K_5^2 \lambda^2 ) \\
&= \exp \left( - \frac{t^2}{4 K_5^2} \right)
& \text{ choosing } \lambda = 1 / (2 K_5^2).
\end{aligned}
Pr [ X ≤ − t ] = Pr [ exp ( λ X ) ≥ exp ( λ t )] ≤ exp ( − λ t ) ⋅ E exp ( λ X ) ≤ exp ( − λ t + K 5 2 λ 2 ) = exp ( − 4 K 5 2 t 2 ) choosing λ = 1/ ( 2 K 5 2 ) . □ \square □
Remark. If
E exp ( λ X ) ≤ exp ( K 5 2 λ 2 ) ∀ λ ∈ R ,
\mathbb{E} \exp(\lambda X) \le \exp(K_5^2 \lambda^2)
\quad \forall \lambda \in \mathbb{R},
E exp ( λ X ) ≤ exp ( K 5 2 λ 2 ) ∀ λ ∈ R , then it holds that
E [ X ] = 0 , and E [ ∣ X ∣ k ] ∈ O ( k ! ) , ∀ k ∈ N + .
\mathbb{E} [ X ] = 0, \quad \text{ and } \quad \mathbb{E} [ |X|^k ] \in O(k!), \, \forall k \in \mathbb{N}^+.
E [ X ] = 0 , and E [ ∣ X ∣ k ] ∈ O ( k !) , ∀ k ∈ N + .
Proof.
Since exp ( ∣ λ X ∣ ) ≤ exp ( − λ X ) + exp ( λ X ) \exp(|\lambda X|) \le \exp(-\lambda X) + \exp(\lambda X) exp ( ∣ λ X ∣ ) ≤ exp ( − λ X ) + exp ( λ X ) , it holds that exp ( ∣ λ X ∣ ) \exp(|\lambda X|) exp ( ∣ λ X ∣ ) is integrable and
E exp ( ∣ λ X ∣ ) ≤ 2 ⋅ exp ( K 5 2 λ 2 ) .
\mathbb{E} \exp(|\lambda X|)
\le 2 \cdot \exp(K_5^2 \lambda^2).
E exp ( ∣ λ X ∣ ) ≤ 2 ⋅ exp ( K 5 2 λ 2 ) . It follows that E exp ( ∣ X ∣ ) ∈ O ( 1 ) \mathbb{E} \exp(|X|) \in O(1) E exp ( ∣ X ∣ ) ∈ O ( 1 ) .
Since ∣ X ∣ k ≤ k ! ⋅ exp ( ∣ X ∣ ) |X|^k \le k! \cdot \exp(|X|) ∣ X ∣ k ≤ k ! ⋅ exp ( ∣ X ∣ ) , it is integrable and
E ∣ X ∣ k ∈ O ( k ! ) .
\mathbb{E} |X|^k \in O(k!).
E ∣ X ∣ k ∈ O ( k !) . Further, as for each n ∈ N n \in \mathbb{N} n ∈ N , it holds that
∑ k = 0 n λ k X k k ! ≤ ∑ k = 0 n ∣ λ ∣ k ∣ X ∣ k k ! ≤ exp ( ∣ λ X ∣ ) ,
\sum_{k = 0}^n \frac{\lambda^k X^k}{k!}
\le \sum_{k = 0}^n \frac{|\lambda|^k |X|^k}{k!}
\le \exp(|\lambda X|),
k = 0 ∑ n k ! λ k X k ≤ k = 0 ∑ n k ! ∣ λ ∣ k ∣ X ∣ k ≤ exp ( ∣ λ X ∣ ) , by dominated convergence theorem, we have
1 + λ E [ X ] + λ 2 2 E [ X 2 ] + ∑ k = 3 ∞ λ k E [ X k ] k ! = E exp ( λ X ) ≤ exp ( K 5 2 λ 2 ) = 1 + K 5 2 λ 2 + ∑ k = 2 ∞ ( K 5 λ ) 2 k k ! .
1 + \lambda \mathbb{E}[X] + \frac{\lambda^2}{2} \mathbb{E}[X^2] + \sum_{k = 3}^\infty \frac{\lambda^k \mathbb{E}[X^k] }{k!}
= \mathbb{E} \exp(\lambda X)
\le \exp(K_5^2 \lambda^2)
= 1 + K_5^2 \lambda^2 + \sum_{k = 2}^\infty \frac{ (K_5\lambda)^{2k} }{k!}.
1 + λ E [ X ] + 2 λ 2 E [ X 2 ] + k = 3 ∑ ∞ k ! λ k E [ X k ] = E exp ( λ X ) ≤ exp ( K 5 2 λ 2 ) = 1 + K 5 2 λ 2 + k = 2 ∑ ∞ k ! ( K 5 λ ) 2 k . When ∣ λ ∣ < 1 |\lambda| < 1 ∣ λ ∣ < 1 and λ → 0 \lambda \rightarrow 0 λ → 0 , clearly
∑ k = 2 ∞ ( K 5 λ ) 2 k k ! ∈ o ( λ 2 ) .
\sum_{k = 2}^\infty \frac{ (K_5\lambda)^{2k} }{k!} \in o(\lambda^2).
k = 2 ∑ ∞ k ! ( K 5 λ ) 2 k ∈ o ( λ 2 ) . Observe that
λ k E [ X k ] k ! ≤ λ k E [ ∣ X ∣ k ] k ! ∈ O ( λ k ) .
\frac{\lambda^k \mathbb{E}[X^k] }{k!}
\le \frac{\lambda^k \mathbb{E}[|X|^k] }{k!}
\in O(\lambda^k).
k ! λ k E [ X k ] ≤ k ! λ k E [ ∣ X ∣ k ] ∈ O ( λ k ) . Therefore,
∣ ∑ k = 3 ∞ λ k E [ X k ] k ! ∣ ∈ O ( λ 3 ) ∈ o ( λ 2 ) .
\left| \sum_{k = 3}^\infty \frac{\lambda^k \mathbb{E}[X^k] }{k!} \right|
\in O(\lambda^3) \in o(\lambda^2).
k = 3 ∑ ∞ k ! λ k E [ X k ] ∈ O ( λ 3 ) ∈ o ( λ 2 ) . Hence,
λ E [ X ] + λ 2 2 E [ X 2 ] + o ( λ 2 ) ≤ K 5 2 λ 2 + o ( λ 2 ) .
\lambda \mathbb{E}[X] + \frac{\lambda^2}{2} \mathbb{E}[X^2] + o(\lambda^2)
\le K_5^2 \lambda^2 + o(\lambda^2).
λ E [ X ] + 2 λ 2 E [ X 2 ] + o ( λ 2 ) ≤ K 5 2 λ 2 + o ( λ 2 ) . Taking λ > 0 \lambda > 0 λ > 0 and letting λ → 0 \lambda \rightarrow 0 λ → 0 gives E [ X ] ≤ 0 \mathbb{E}[X] \le 0 E [ X ] ≤ 0 .
Taking λ < 0 \lambda < 0 λ < 0 and letting λ → 0 \lambda \rightarrow 0 λ → 0 gives E [ X ] ≥ 0 \mathbb{E}[X] \ge 0 E [ X ] ≥ 0 .
It concludes that E [ X ] = 0 \mathbb{E} [ X ] = 0 E [ X ] = 0 , and therefore E [ X 2 ] ≤ 2 K 5 2 \mathbb{E}[X^2] \le 2 K_5^2 E [ X 2 ] ≤ 2 K 5 2 .
□ \square □
Definition. The sub-gaussian norm of X X X , denoted ∥ X ∥ ψ 2 \Vert X \Vert_{\psi_2} ∥ X ∥ ψ 2 , is defined to be the smallest K 4 K_4 K 4 in property 4, i.e.,
∥ X ∥ ψ 2 = inf { t > 0 : E exp ( X 2 / t 2 ) ≤ 2 } .
\Vert X \Vert_{\psi_2}
= \inf \{ t > 0: \mathbb{E} \exp( X^2 / t^2) \le 2 \}.
∥ X ∥ ψ 2 = inf { t > 0 : E exp ( X 2 / t 2 ) ≤ 2 } .
We first show that E exp ( X 2 / ∥ X ∥ ψ 2 2 ) ≤ 2 \mathbb{E} \exp( X^2 / \Vert X \Vert_{\psi_2}^2) \le 2 E exp ( X 2 /∥ X ∥ ψ 2 2 ) ≤ 2 .
Let t 1 , t 2 , t 3 , … t_1, t_2, t_3, \ldots t 1 , t 2 , t 3 , … be a decreasing sequence such that t i − ∥ X ∥ ψ 2 ≤ 1 / k t_i - \Vert X \Vert_{\psi_2} \le 1 / k t i − ∥ X ∥ ψ 2 ≤ 1/ k .
Then by monotone convergence theorem, we have
E exp ( X 2 / ∥ X ∥ ψ 2 2 ) = E lim i → ∞ exp ( X 2 / t i 2 ) = lim i → ∞ E exp ( X 2 / t i 2 ) ≤ 2.
\mathbb{E} \exp( X^2 / \Vert X \Vert_{\psi_2}^2)
= \mathbb{E} \lim_{i \rightarrow \infty} \exp( X^2 / t_i^2 )
= \lim_{i \rightarrow \infty} \mathbb{E} \exp( X^2 / t_i^2 )
\le 2.
E exp ( X 2 /∥ X ∥ ψ 2 2 ) = E i → ∞ lim exp ( X 2 / t i 2 ) = i → ∞ lim E exp ( X 2 / t i 2 ) ≤ 2. We restate the previous theorem in terms of the sub-gaussian norm.
Pr ( ∣ X ∣ ≥ t ) ≤ 2 exp ( − c t 2 / ∥ X ∥ ψ 2 ) , ∀ t ≥ 0 \Pr (|X| \ge t) \le 2 \exp( −c t^2 / \Vert X \Vert_{\psi_2} ), \quad \forall t \ge 0 Pr ( ∣ X ∣ ≥ t ) ≤ 2 exp ( − c t 2 /∥ X ∥ ψ 2 ) , ∀ t ≥ 0 ;
∥ X ∥ L p ≤ C p ∥ X ∥ ψ 2 , ∀ p ≥ 1 \Vert X \Vert_{L_p} \le C \sqrt{p} \Vert X \Vert_{\psi_2}, \quad \forall p \ge 1 ∥ X ∥ L p ≤ C p ∥ X ∥ ψ 2 , ∀ p ≥ 1
E exp ( X 2 / ∥ X ∥ ψ 2 ) ≤ 2 \mathbb{E} \exp(X^2 / \Vert X \Vert_{\psi_2} ) \le 2 E exp ( X 2 /∥ X ∥ ψ 2 ) ≤ 2 ;
if E [ X ] = 0 \mathbb{E} [ X ] = 0 E [ X ] = 0 then E exp ( λ X ) ≤ exp ( C λ 2 ∥ X ∥ ψ 2 ) , ∀ λ ∈ R \mathbb{E} \exp( \lambda X) \le \exp( C \lambda^2 \Vert X \Vert_{\psi_2} ) , \quad \forall \lambda \in \mathbb{R} E exp ( λ X ) ≤ exp ( C λ 2 ∥ X ∥ ψ 2 ) , ∀ λ ∈ R .
Here C , c > 0 C, c > 0 C , c > 0 are absolute constants.
Theorem. ∥ ⋅ ∥ ψ 2 \Vert \cdot \Vert_{\psi_2} ∥ ⋅ ∥ ψ 2 is a norm on the space of sub-gaussian random variables.
Proof.
Let X X X and Y Y Y be sub-gaussian random variables, and a = ∥ X ∥ ψ 2 , b = ∥ Y ∥ ψ 2 a = \Vert X \Vert_{\psi_2}, b = \Vert Y \Vert_{\psi_2} a = ∥ X ∥ ψ 2 , b = ∥ Y ∥ ψ 2 .
Then
E exp ( X + Y a + b ) 2 = E exp ( X a ⋅ a a + b + Y b ⋅ b a + b ) 2 ≤ E [ a a + b exp ( X a ) 2 + b a + b ⋅ exp ( Y b ) 2 ] ≤ 2.
\begin{aligned}
\mathbb{E} \exp \left( \frac{X + Y}{a + b} \right)^2
&= \mathbb{E} \exp \left( \frac{X}{a} \cdot \frac{a}{a + b} + \frac{Y}{b} \cdot \frac{b}{a + b} \right)^2 \\
&\le \mathbb{E} \left[ \frac{a}{a + b} \exp \left( \frac{X}{a} \right)^2
+ \frac{b}{a + b} \cdot \exp \left( \frac{Y}{b} \right)^2 \right]
\le 2.
\end{aligned}
E exp ( a + b X + Y ) 2 = E exp ( a X ⋅ a + b a + b Y ⋅ a + b b ) 2 ≤ E [ a + b a exp ( a X ) 2 + a + b b ⋅ exp ( b Y ) 2 ] ≤ 2. Hence,
∥ X + Y ∥ ψ 2 ≤ a + b = ∥ X ∥ ψ 2 + ∥ Y ∥ ψ 2 .
\Vert X + Y \Vert_{\psi_2}
\le a + b
= \Vert X \Vert_{\psi_2} + \Vert Y \Vert_{\psi_2}.
∥ X + Y ∥ ψ 2 ≤ a + b = ∥ X ∥ ψ 2 + ∥ Y ∥ ψ 2 . □ \square □
Theorem (Sums of independent sub-gaussians) Let X 1 , … , X N X_1, \ldots, X_N X 1 , … , X N be independent mean-zero sub-gaussian random variables.
Then ∑ i ∈ [ N ] X i \sum_{i \in [N]} X_i ∑ i ∈ [ N ] X i is also a sub-gaussian random variable, and
∥ ∑ i ∈ [ N ] X i ∥ ψ 2 2 ≤ C ⋅ ∑ i ∈ [ N ] ∥ X ∥ ψ 2 2
\left\Vert \sum_{i \in [N]} X_i \right\Vert_{\psi_2}^2
\le C \cdot \sum_{i \in [N]} \Vert X \Vert_{\psi_2}^2
i ∈ [ N ] ∑ X i ψ 2 2 ≤ C ⋅ i ∈ [ N ] ∑ ∥ X ∥ ψ 2 2 where C C C is an absolute constant.
Proof.
E exp ( λ ∑ i ∈ [ N ] X i ) = ∏ i ∈ [ N ] E exp ( λ X i ) ≤ ∏ i ∈ [ N ] exp ( C λ 2 ∥ X i ∥ ψ 2 2 ) = exp ( ∑ i ∈ [ N ] C λ 2 ∥ X i ∥ ψ 2 2 ) .
\begin{aligned}
\mathbb{E} \exp \left( \lambda \sum_{i \in [N]} X_i \right)
&= \prod_{i \in [N]} \mathbb{E} \exp \left( \lambda X_i \right) \\
&\le \prod_{i \in [N]} \exp \left( C \lambda^2 \Vert X_i \Vert_{\psi_2}^2 \right)
= \exp \left( \sum_{i \in [N]} C \lambda^2 \Vert X_i \Vert_{\psi_2}^2 \right).
\end{aligned}
E exp λ i ∈ [ N ] ∑ X i = i ∈ [ N ] ∏ E exp ( λ X i ) ≤ i ∈ [ N ] ∏ exp ( C λ 2 ∥ X i ∥ ψ 2 2 ) = exp i ∈ [ N ] ∑ C λ 2 ∥ X i ∥ ψ 2 2 . Hence, ∑ i ∈ [ N ] X i \sum_{i \in [N]} X_i ∑ i ∈ [ N ] X i is sug-gaussian, and ∥ X i ∥ ψ 2 2 ∈ O ( ∑ i ∈ [ N ] ∥ X i ∥ ψ 2 2 ) \Vert X_i \Vert_{\psi_2}^2 \in O( \sum_{i \in [N]} \Vert X_i \Vert_{\psi_2}^2 ) ∥ X i ∥ ψ 2 2 ∈ O ( ∑ i ∈ [ N ] ∥ X i ∥ ψ 2 2 ) .
□ \square □
Theorem (General Hoeffding Inequality).
Let X 1 , … , X N X_1, \ldots, X_N X 1 , … , X N be independent mean-zero sub-gaussian random variables.
Then,
Pr ( ∣ ∑ i ∈ [ N ] X i ∣ ≥ t ) ≤ 2 exp ( − c t 2 ∑ i ∈ [ N ] ∥ X ∥ ψ 2 2 ) , t ≥ 0.
\Pr \left( \left| \sum_{i \in [N]} X_i \right| \ge t \right)
\le 2 \exp \left( − \frac{c t^2}{\sum_{i \in [N]} \Vert X \Vert_{\psi_2}^2} \right),
\quad t \ge 0.
Pr i ∈ [ N ] ∑ X i ≥ t ≤ 2 exp ( − ∑ i ∈ [ N ] ∥ X ∥ ψ 2 2 c t 2 ) , t ≥ 0.
Proof.
This can be viewed as a corollary as the previous theorem.
□ \square □
Theorem (Khintchine’s inequality)
Let X 1 , … , X N X_1, \ldots, X_N X 1 , … , X N be independent sub-gaussian random variables with zero means and unit variances, and let a = ( a 1 , … , a N ) ∈ R N a = (a_1,\ldots,a_N) \in \mathbb{R}^N a = ( a 1 , … , a N ) ∈ R N .
Then for every p ∈ [ 2 , ∞ ) p \in [2, \infty) p ∈ [ 2 , ∞ ) we have
∥ a ∥ 2 ≤ ∥ ∑ i ∈ [ N ] a i X i ∥ L p ≤ C K p ∥ a ∥ 2
\Vert a \Vert_2
\le \left\Vert \sum_{i \in [N]} a_i X_i \right\Vert_{L_p}
\le C K \sqrt{p} \Vert a \Vert_2
∥ a ∥ 2 ≤ i ∈ [ N ] ∑ a i X i L p ≤ C K p ∥ a ∥ 2 where K = max i ∥ X i ∥ ψ 2 K = \max_i \Vert X_i \Vert_{\psi_2} K = max i ∥ X i ∥ ψ 2 and C C C is an absolute constant.
Proof.
First, since p ≥ 2 p \ge 2 p ≥ 2 , we have
∥ ∑ i ∈ [ N ] a i X i ∥ L p ≥ ∥ ∑ i ∈ [ N ] a i X i ∥ L 2 = ( E [ ( ∑ i ∈ [ N ] a i X i ) 2 ] ) 1 / 2 = ( ∑ i , j ∈ [ N ] E [ a i a j X i X j ] ) 1 / 2 = ∥ a ∥ 2 .
\begin{aligned}
\left\Vert \sum_{i \in [N]} a_i X_i \right\Vert_{L_p}
&\ge \left\Vert \sum_{i \in [N]} a_i X_i \right\Vert_{L_2} \\
&= \left( \mathbb{E} \left[ \left( \sum_{i \in [N]} a_i X_i \right)^2 \right] \right)^{1 / 2} \\
&= \left( \sum_{i, j \in [N]} \mathbb{E} \left[ a_i a_j X_i X_j \right] \right)^{1 / 2}
= \Vert a \Vert_2.
\end{aligned}
i ∈ [ N ] ∑ a i X i L p ≥ i ∈ [ N ] ∑ a i X i L 2 = E i ∈ [ N ] ∑ a i X i 2 1/2 = i , j ∈ [ N ] ∑ E [ a i a j X i X j ] 1/2 = ∥ a ∥ 2 . Let X ≐ ∑ i ∈ [ N ] a i X i X \doteq \sum_{i \in [N]} a_i X_i X ≐ ∑ i ∈ [ N ] a i X i .
Then
∥ X ∥ ψ 2 2 ≤ ∑ i ∈ [ n ] ∥ a i X i ∥ ψ 2 2 = ∑ i ∈ [ n ] a i 2 ⋅ ∥ X i ∥ ψ 2 2 ≤ K 2 ⋅ ∥ a ∥ 2 2 .
\Vert X \Vert_{\psi_2}^2
\le \sum_{i \in [n]} \Vert a_i X_i \Vert_{\psi_2}^2
= \sum_{i \in [n]} a_i^2 \cdot \Vert X_i \Vert_{\psi_2}^2
\le K^2 \cdot \Vert a \Vert_2^2.
∥ X ∥ ψ 2 2 ≤ i ∈ [ n ] ∑ ∥ a i X i ∥ ψ 2 2 = i ∈ [ n ] ∑ a i 2 ⋅ ∥ X i ∥ ψ 2 2 ≤ K 2 ⋅ ∥ a ∥ 2 2 . It follows that
E [ ∣ X ∣ p ] ∈ O ( p ⋅ ∥ X ∥ ψ 2 ) ⊆ O ( p ⋅ K ⋅ ∥ a ∥ 2 ) .
\mathbb{E} [ |X|^p ]
\in O( \sqrt{p} \cdot \Vert X \Vert_{\psi_2} )
\subseteq O( \sqrt{p} \cdot K \cdot \Vert a \Vert_2 ).
E [ ∣ X ∣ p ] ∈ O ( p ⋅ ∥ X ∥ ψ 2 ) ⊆ O ( p ⋅ K ⋅ ∥ a ∥ 2 ) . □ \square □
Theorem (Centering). If X X X is a sub-gaussian random variable then X − E [ X ] X − \mathbb{E} [ X ] X − E [ X ] is sub-gaussian too and
∥ X − E [ X ] ∥ ψ 2 ≤ C ∥ X ∥ ψ 2 ,
\Vert X − \mathbb{E} [ X ] \Vert_{\psi_2}
\le C \Vert X \Vert_{\psi_2},
∥ X − E [ X ] ∥ ψ 2 ≤ C ∥ X ∥ ψ 2 , where C C C is an absolute constant.
Proof.
Since ∥ ⋅ ∥ ψ 2 \Vert \cdot \Vert_{\psi_2} ∥ ⋅ ∥ ψ 2 is a norm,
∥ X − E [ X ] ∥ ψ 2 ≤ ∥ X ∥ ψ 2 + ∥ E [ X ] ∥ ψ 2 .
\Vert X − \mathbb{E} [ X ] \Vert_{\psi_2}
\le \Vert X \Vert_{\psi_2} + \Vert \mathbb{E} [ X ] \Vert_{\psi_2}.
∥ X − E [ X ] ∥ ψ 2 ≤ ∥ X ∥ ψ 2 + ∥ E [ X ] ∥ ψ 2 . It remains to bound the second term.
By definition, we have
E [ exp ( ( E [ X ] ) 2 ( ( 1 / ln 2 ) 1 / 2 ⋅ E [ X ] ) 2 ) ] = 2 ,
\mathbb{E} \left[ \exp \left( \frac{(\mathbb{E} [ X ])^2}{ \big( (1 / \ln 2)^{1 / 2} \cdot\mathbb{E} [ X ] \big)^2} \right) \right] = 2,
E [ exp ( ( ( 1/ ln 2 ) 1/2 ⋅ E [ X ] ) 2 ( E [ X ] ) 2 ) ] = 2 , Therefore,
∥ E [ X ] ∥ ψ 2 = 1 ln 2 ⋅ E [ X ] ≤ 1 ln 2 ⋅ E ∣ X ∣ ∈ O ( ∥ X ∥ ψ 2 ) .
\begin{aligned}
\Vert \mathbb{E} [ X ] \Vert_{\psi_2}
&= \frac{1}{\sqrt{\ln 2}} \cdot \mathbb{E} [ X ]
\le \frac{1}{\sqrt{\ln 2}} \cdot \mathbb{E} | X |
\in O( \Vert X \Vert_{\psi_2} ).
\end{aligned}
∥ E [ X ] ∥ ψ 2 = ln 2 1 ⋅ E [ X ] ≤ ln 2 1 ⋅ E ∣ X ∣ ∈ O ( ∥ X ∥ ψ 2 ) . □ \square □
Reference
[1] R. Vershynin, High-Dimensional Probability: An Introduction with Applications in Data Science. in Cambridge Series in Statistical and Probabilistic Mathematics. Cambridge: Cambridge University Press, 2018.
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