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#' Estimation algorithms available for \pkg{rstanarm} models
#'
#' @name available-algorithms
#'
#' @section Estimation algorithms:
#' The modeling functions in the \pkg{rstanarm} package take an \code{algorithm}
#' argument that can be one of the following:
#' \describe{
#' \item{\strong{Sampling} (\code{algorithm="sampling"})}{
#' Uses Markov Chain Monte Carlo (MCMC) --- in particular, Hamiltonian Monte
#' Carlo (HMC) with a tuned but diagonal mass matrix --- to draw from the
#' posterior distribution of the parameters. See \code{\link[rstan:stanmodel-method-sampling]{sampling}}
#' (\pkg{rstan}) for more details. This is the slowest but most reliable of the
#' available estimation algorithms and it is \strong{the default and
#' recommended algorithm for statistical inference.}
#' }
#' \item{\strong{Mean-field} (\code{algorithm="meanfield"})}{
#' Uses mean-field variational inference to draw from an approximation to the
#' posterior distribution. In particular, this algorithm finds the set of
#' independent normal distributions in the unconstrained space that --- when
#' transformed into the constrained space --- most closely approximate the
#' posterior distribution. Then it draws repeatedly from these independent
#' normal distributions and transforms them into the constrained space. The
#' entire process is much faster than HMC and yields independent draws but
#' \strong{is not recommended for final statistical inference}. It can be
#' useful to narrow the set of candidate models in large problems, particularly
#' when specifying \code{QR=TRUE} in \code{\link{stan_glm}},
#' \code{\link{stan_glmer}}, and \code{\link{stan_gamm4}}, but is \strong{only
#' an approximation to the posterior distribution}.
#' }
#' \item{\strong{Full-rank} (\code{algorithm="fullrank"})}{
#' Uses full-rank variational inference to draw from an approximation to the
#' posterior distribution by finding the multivariate normal distribution in
#' the unconstrained space that --- when transformed into the constrained space
#' --- most closely approximates the posterior distribution. Then it draws
#' repeatedly from this multivariate normal distribution and transforms the
#' draws into the constrained space. This process is slower than meanfield
#' variational inference but is faster than HMC. Although still an
#' approximation to the posterior distribution and thus \strong{not recommended
#' for final statistical inference}, the approximation is more realistic than
#' that of mean-field variational inference because the parameters are not
#' assumed to be independent in the unconstrained space. Nevertheless, fullrank
#' variational inference is a more difficult optimization problem and the
#' algorithm is more prone to non-convergence or convergence to a local
#' optimum.
#' }
#' \item{\strong{Optimizing} (\code{algorithm="optimizing"})}{
#' Finds the posterior mode using a C++ implementation of the LBGFS algorithm.
#' See \code{\link[rstan:stanmodel-method-optimizing]{optimizing}} for more details. If there is no prior
#' information, then this is equivalent to maximum likelihood, in which case
#' there is no great reason to use the functions in the \pkg{rstanarm} package
#' over the emulated functions in other packages. However, if priors are
#' specified, then the estimates are penalized maximum likelihood estimates,
#' which may have some redeeming value. Currently, optimization is only
#' supported for \code{\link{stan_glm}}.
#' }
#' }
#'
#' @seealso \url{https://mc-stan.org/rstanarm/}
#'
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