On the first page of Ustunel's lecture notes, he defines the Wiener measure in the following way:
Let $W = C_0([0,1]), \omega \in W, t\in [0,1]$, define $W_t(\omega) = \omega(t)$. If we denote by $\mathcal{B}_t = \sigma\{W_s; s\leq t\}$, then there is one and only one measure $\mu$ on $W$ such that
1) $\mu \{W_0(\omega) = 0\} = 1$
2) $\forall f \in C_b^{\infty}$, the stochastic process $$(t, \omega ) \mapsto f(W_t(\omega)) - \dfrac{1}{2}\int_0^tf''(W_s(\omega))ds$$
is a $(\mathcal{B}_t, \mu)$-martingale. $\mu$ is called the Wiener measure
I am more familiar with the definition which supposes that we have already a Brownian motion $B_t$ available and then define $$\nu\left(\{\omega: \omega_{t_1} \in A_1, \cdots, \omega_{t_n} \in A_ n\}\right) = P(B_{t_1} \in A_1, \cdots, B_{t_n} \in A_ n)$$
My question is why $\mu$ and $\nu$ are the same? Of couree if we begin with $\nu$ and use Its's formula, we can see the two conditions defning $\mu$ are verified. But if we begin with the definition of $\mu$, how can we verify the condition defining $\nu$?
In addition, in Ustunel's notes, he first presented his definition of Wiener measure then introduced stochastic integral. So I am wondering if there is a way to begin with the definition of $\mu$, then to show $\mu$ satisfies the condition defining $\nu$ without using stochastic integral.
Of course I will still appreciate it if you help me show $\mu \implies \nu$ using stochastic integral.
Thank you!