Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma

TL;DR

This study investigates how active black holes, cosmic rays, and baryonic feedback influence dark matter distribution in dwarf galaxies, revealing diverse profiles that help resolve small-scale challenges to the CDM model.

Contribution

It introduces new cosmological simulations showing the impact of AGN feedback and cosmic rays on dark matter profiles in dwarf galaxies, highlighting their role in the observed diversity.

Findings

AGN feedback causes cuspier or core-like profiles.

Cosmic rays significantly influence dark matter distributions.

Diverse dark matter profiles align with observed rotation curves.

Abstract

Dwarf galaxies have historically posed challenges to the cold dark matter (CDM) model and, while many of the so-called 'dwarf galaxy problems' have been mitigated by incorporating baryonic processes, the observed diversity of dwarf galaxy rotation curves remains a contentious topic. Meanwhile, the growing observational samples of active galactic nuclei (AGN) in dwarf galaxies have prompted a paradigm shift in our understanding of dwarf galaxy evolution, traditionally thought to be regulated by stellar feedback. In this study, we explore the potential role of AGN feedback in shaping dark matter distributions and increasing the diversity of dwarf galaxy rotation curves, using a new suite of cosmological zoom-in simulations of dwarf galaxies with the FIRE-3 model. Our findings indicate that the presence of active black holes (BHs) in dwarf galaxies can lead to diverse outcomes, ranging from cuspier to more core-like profiles. This variability arises from the dual role of BHs in providing additional feedback and regulating the extent of stellar feedback. Consistent with previous research, we find that AGN feedback is most impactful when cosmic ray (CR) modelling is included, with CRs from any source significantly influencing dark matter profiles. Overall, our results highlight that the interplay between stellar feedback, BHs, and CRs produces a broad spectrum of dark matter density profiles, which align with observed correlations between rotation curve shapes and baryonic dominance. This underscores the importance of including the full range of baryonic processes in dwarf galaxy simulations to address the persistent 'small-scale challenges' to the CDM paradigm.