Impact of Lyman alpha pressure on metal-poor dwarf galaxies
  Understanding the origin of strong galactic outflows and the suppression of
star formation in dwarf galaxies is a key problem in galaxy formation. Using a
set of radiation-hydrodynamic simulations of an isolated dwarf galaxy embedded
in a $10^{10}\,M_\odot$ halo, we show that the momentum transferred from
resonantly scattered Lyman-$\alpha$ (Lya) photons is an important source of
stellar feedback which can shape the evolution of galaxies. We find that Lya
feedback suppresses star formation by a factor of two in metal-poor galaxies by
regulating the dynamics of star-forming clouds before the onset of supernova
explosions (SNe). This is possible because each Lya photon resonantly scatters
and imparts 10-300 times greater momentum than in the single scattering limit.
Consequently, the number of star clusters predicted in the simulations is
reduced by a factor of $\sim 5$, compared to the model without the early
feedback. More importantly, we find that galactic outflows become weaker in the
presence of strong Lya radiation feedback, as star formation and associated SNe
become less bursty. We also examine a model in which radiation field is
arbitrarily enhanced by a factor of up to 10, and reach the same conclusion.
The typical mass loading factors in our metal-poor dwarf system are estimated
to be $\sim5-10$ near the mid plane, while it is reduced to $\sim1$ at larger
radii. Finally, we find that the escape of ionizing radiation and hence the
reionization history of the Universe is unlikely to be strongly affected by Lya
feedback.
