The local speed of light is always $c$. By this I mean that if any observer anywhere measures the speed of light they will get the value $c$. It doesn't matter if they are accelerating or not.
However for an accelerating observer, even in flat spacetime, the speed of light at distant locations will not be $c$. The geometry of spacetime for an observer with constant accelerating $a$ is described by the Rindler metric:
$$ c^2d\tau^2 = \left(1 + \frac{a}{c^2}x \right)^2 c^2 dt^2 - dx^2 $$
We get the speed of light from this buy setting $d\tau = 0$, which gives us:
$$ \frac{dx}{dt} = c\,\left(1 + \frac{a}{c^2}x \right) \tag{1} $$
For negative $x$, i.e. in the opposite direction to the acceleration, the right hand side of equation (1) is less than $c$ so in this direction the velocity of light decreases. In the other direction the velocity of light increases.
This is essentially the same phenomenon described in Does gravity slow the speed that light travels?. For a stationary observer in a curved spacetime the geometry looks locally like Rindler space. Note the caveats I make in the linked question. The quantity calculated here is the coordinate velocity of light not the velocity measured by any observer.