  This study explores the potential for dark matter annihilation within brown
dwarfs, investigating an unconventional mechanism for neutrino production.
Motivated by the efficient accumulation of dark matter particles in brown
dwarfs through scattering interactions, we focus on a mass range above 10 GeV,
considering dark matter annihilation channels $\chi \chi \rightarrow \nu
\bar{\nu} \nu \bar{\nu}$ through long-lived mediators. Using the projected
sensitivity of IceCube Generation 2, we assess the detection capability of the
local population of brown dwarfs within 20 pc and exclude dark matter-nucleon
scattering with cross-sections as low as a few multiples of $10^{-36}~\rm
cm^{2}$.
