There are various ways to find the moments of the T-distribution, but the simplest method is to use the mixture representation using the normal distribution. If $T$ has a Student's T distribution with $\varphi$ degrees-of-freedom then we can write it via the mixture $T|\lambda \sim \text{N}(0, \tfrac{1}{\lambda})$ with $\lambda \sim \text{Ga}(\tfrac{\varphi}{2}, \tfrac{\varphi}{2})$ (i.e., as a mixture of normal distributions where the precision is gamma distributed). Using this mixture representation the density function for the Student's T distribution can be written as the integral:
$$\begin{equation} \begin {aligned}
\text{St}(t|\varphi)
&= \int \limits_0^\infty \text{N}(t|0,\tfrac{1}{\lambda}) \text{Ga}(\lambda|\tfrac{\varphi}{2},\tfrac{\varphi}{2}) \ d \lambda.
\end{aligned} \end{equation}$$
Using this mixture representation, the raw moments of $T$ can be obtained via the law of iterated expectation, using the known moments of the normal distribution. The conditional moments are:
$$\mathbb{E}(T^k|\lambda) = \int \limits_{-\infty}^\infty t^k \text{ N}(t|0,\tfrac{1}{\lambda}) \text{ } dt = \begin{cases}
0 & & \text{if } k \text{ is odd}, \\[6pt]
\frac{k!}{2^{k/2}(k/2)!} \lambda^{-k/2} & & \text{if } k \text{ is even}. \\[6pt]
\end{cases}$$
For values $k \geqslant \varphi$ the moments of the T distribution do not exist. For odd values $0<k<\varphi$ the moments are zero and for even values $0<k<\varphi$ the moments are:
$$\begin{equation} \begin {aligned}
\mathbb{E}(T^k) = \mathbb{E}( \mathbb{E}(T^k | \lambda ) )
&= \int \limits_0^\infty \frac{k!}{2^{k/2}(k/2)!} \lambda^{-k/2} \text{ Ga}(\lambda|\tfrac{\varphi}{2},\tfrac{\varphi}{2}) \text{ } d\lambda \\[6pt]
&= \int \limits_0^\infty \frac{k!}{2^{k/2}(k/2)!} \lambda^{-k/2} \cdot \frac{\varphi^{\varphi/2}}{2^{\varphi/2} \Gamma(\tfrac{\varphi}{2})} \lambda^{\varphi/2-1} \exp \Big( -
\frac{\varphi}{2} \lambda \Big) \text{ } d\lambda \\[6pt]
&= \frac{k!}{2^k (k/2)!} \cdot \frac{\Gamma(\tfrac{\varphi-k}{2})}{\Gamma(\tfrac{\varphi}{2})} \cdot \varphi^{k/2} \\
&\quad \quad \quad \quad \times \int \limits_0^\infty \frac{\varphi^{(\varphi-k)/2}}{2^{(\varphi-k)/2} \Gamma(\tfrac{\varphi-k}{2})} \lambda^{(\varphi-k)/2-1} \exp \Big( -\frac{\varphi}{2} \lambda \Big) \text{ } d\lambda \\[6pt]
&= \frac{k!}{2^k (k/2)!} \cdot \frac{\Gamma(\tfrac{\varphi-k}{2})}{\Gamma(\tfrac{\varphi}{2})} \cdot \varphi^{k/2} \int \limits_0^\infty \text{Ga}(\lambda|\tfrac{\varphi-k}{2},\tfrac{\varphi}{2}) \text{ } d\lambda \\[6pt]
&= \frac{k!}{2^k (k/2)!} \cdot \frac{\Gamma(\tfrac{\varphi-k}{2})}{\Gamma(\tfrac{\varphi}{2})} \cdot \varphi^{k/2} \\[6pt]
&= \frac{\Gamma(\tfrac{k+1}{2})}{\sqrt{\pi}} \cdot \frac{\Gamma(\tfrac{\varphi-k}{2})}{\Gamma(\tfrac{\varphi}{2})} \cdot \varphi^{k/2}. \\[6pt]
&= \frac{\Gamma(\tfrac{k+1}{2})}{\sqrt{\pi}} \cdot \frac{\varphi^{k/2}}{\prod_{i=1}^{k/2} (\tfrac{\varphi}{2}-i)}. \\[6pt]
\end{aligned} \end{equation}$$
Application of this formula for the even moments yields:
$$\begin{equation} \begin{aligned}
\mathbb{E}(T^2) &= \frac{\varphi}{\varphi-2} & & & \text{for } \varphi > 2, \\[6pt]
\mathbb{E}(T^4) &= \frac{3 \varphi^2}{(\varphi-2) (\varphi-4)} & & & \text{for } \varphi > 4, \\[6pt]
\mathbb{E}(T^6) &= \frac{15 \varphi^3}{(\varphi-2) (\varphi-4) (\varphi-6)} & & & \text{for } \varphi > 6. \\[6pt]
\end{aligned} \end{equation}$$
You can now obtain the kurtosis, etc., via algebraic manipulation of the raw moments. In particular, the kurtosis is:
$$\begin{equation} \begin{aligned}
\mathbb{Kurt}(T) = \frac{\mathbb{E}(T^4)}{\mathbb{E}(T^2)^2}
&= \frac{3 \varphi^2}{(\varphi-2) (\varphi-4)} \Big/ \Big( \frac{\varphi}{\varphi-2} \Big)^2 \\[6pt]
&= \frac{3 (\varphi-2)}{\varphi-4} \\[6pt]
&= \frac{3 \varphi - 6}{\varphi-4} \\[6pt]
&= \frac{3 \varphi - 12}{\varphi-4} + \frac{6}{\varphi-4} \\[6pt]
&= 3 + \frac{6}{\varphi-4}. \\[6pt]
\end{aligned} \end{equation}$$
self-study
tag should appear in your question. First and third moments (assuming $\nu$ is large enough) are obvious by symmetry. For second and fourth moments, you can use the representation $X=\mu+\sigma\times Z/\sqrt{W/\nu}$ where $Z$ is standard normal and $W$ is $\chi^2_\nu$. $\endgroup$v
is large enough the distribution converges to a normal. But how do you get it by not givingv
a value? $\endgroup$