The horseshoe prior for, say, an unknown mean $\mu$ is expressed $$ \begin{align*} \mu_i | \lambda_i, \tau &\sim N(0, \lambda_i^2 \tau^2) \\ \lambda_i &\sim C^+(0,1) \end{align*} $$ where the prior on $\lambda_i$ can be equivalently stated as $\kappa_i := \frac{1}{1+\lambda_i^2} \sim$ Beta(.5,.5), and it is this distribution on $\kappa_i$ that has the horseshoe shape for which the scheme is named. In the normal mean model $y | \mu \sim N_d (\mu, I)$, the $\kappa_i$ say how much the MLE $y$ should be shrunk, and the philosophy of the horseshoe is that you want $\kappa_i$ to be near 0 to produce no shrinkage in signal components, or near 1 to produce strong shrinkage to 0 of noise components. Hence you'd like a prior on $\kappa_i$ that has its mass toward 0 and 1, like Beta(.5,.5).
However, Beta(b,b) for b in (0,1) will have the same horseshoe shape. $b$ approaching 0 will shift mass out of the middle toward 0 and 1, with limiting distribution Bernoulli(.5). $b$ approaching 1 will shift mass from the ends into the middle, approaching U(0,1).
Is there any work on using values of $b$ other than .5 in horseshoe priors? If so, what guides such choices?