INCLUDING AN EXTENSION
$\psi_o$ is, as mentioned previously, the normalisation constant which is calculated by doing the integral $\int_V|\psi|^2dV$ and setting its value equal to 1 (hence normalization). This will give you the equation for $\psi_o$. If your interest is to find the probablity amplitude for a particle in a volume V, for example, then you get the equation
$$\int_V|\psi|^2dV = |\psi_o|^2 V = 1\quad,$$
which gives you
$$\psi_o = \frac{1}{\sqrt{V}}\quad,$$
and this is the normalization constant for the probability amplitude $\psi$. Thus you will write
$$\psi(\textbf{r})= \frac{1}{\sqrt{V}}\exp[i(\textbf{k}\cdot\textbf{r}-\omega t)]\quad.$$
For a particle in infinitely large volume, the probability amplitude is zero. I.e $\psi_0=0$. So the probability to find the particle at a particular position is zero.
I hope this helps understand the difference between these two.
This question has been asked before in a different format, answers were given. In the light of your reworded question consider this:
EXTENSION:
The general solution to Schrodinger equation for a free-particle in 1-D (as in your question) is
$\psi(x)=\psi_0e^{i(kx-\omega t)}$
The point with this question is that it puts down arbitrary wave functions and asks how to normalise them. No problem with that, but to normalize the wave function you need to know the boundaries of the problem, hence the boundary conditions.
Assuming you have a ‘box’ of side L in the $x$-axis, the normalisation will give you $\psi_0=\frac{1}{\sqrt {L}}$ so that
$\psi(x)=\frac {1}{\sqrt {L}}e^{i(kx-\omega t)}$
If you now wish to see what will happen to the wave function if $L$ goes to infinity, you must take into consideration the fact that the phase factor is finite, so that it results in $\psi_0=0$ and the whole wave function is zero. This means, as said above, you have no chance of finding the particle at a particular point along the $x$-axis.
In the genuine case where the particle wave-function does occupy the whole of the $x$-axis (the whole volume in the general case,) then, the particle has well defined momentum, hence energy ( it is a stationary state,) but let us focus on the space dimension for simplicity. This means that in the momentum space, the wave function must be $\delta (p^/-p) $ function. This gives the standard $\delta$-function normalisation of the wave function as I mentioned in a previous communication. In other words, we do a Fourier transformation of the plane wave (the above wave function) with the condition that L goes to infinity, and this produces the correct sharp momentum value as indicated by the $\delta$-function
$\psi_k (x)=\frac {1}{\sqrt{2\pi}}e^{i(kx)}$
The limit L going to infinity has already been taken into account in the Fourier transform, hence the $2\pi$ in the normalisation coefficient.
It is very important to understand that the wf must reflect the uncertainty principle. For this reason, a free particle is often described by a wave packet, as mentioned in other answers, with a Gaussian profile. For a particle that is initially confined in a region of width $w_0$, and then is let free, the Gaussian profile expands, and the equation of evolution of the width is given by standard quantum mechanics (there is some good theory about it, see: Stephen Gasiorowicz page 67-70, David Bohm page: 45-47, for example.) Eventually, over time, the wave function reduces to a plane wave-a free particle wave function.