Infalling ultra-faint dwarfs as emissaries of the Axiverse
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| Main Authors: | , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| author | Pozo, A. Broadhurst, T. Luu, H. N. Smoot, G. Umetsu, K. Chiueh, T. Schive, H. -Y. Emami, R. Hernquist, L. Mocz, P. Vogelsberger, M. |
| author_facet | Pozo, A. Broadhurst, T. Luu, H. N. Smoot, G. Umetsu, K. Chiueh, T. Schive, H. -Y. Emami, R. Hernquist, L. Mocz, P. Vogelsberger, M. |
| contents | Recent discoveries of ultra-faint dwarf galaxies (UFDs) infalling onto the Milky Way, namely Leo K \& M at $r \simeq 450$kpc, considerably strengthens the case that UFDs constitute a distinct galaxy class that is inherently smaller and fainter, and metal-poorer than the classical dwarf spheroidals (dSph). This distinction is at odds with the inherent continuity of galaxy halo masses formed under scale-free gravity for any standard dark-matter (DM) model. Here, we show that distinct galaxy classes do evolve in cosmological simulations of multiple light bosons representing the ``Axiverse'' proposal of string theory, where a discrete mass spectrum of axions is generically predicted to span many decades in mass. In this context, the
observed UFD class we show corresponds to a relatively heavy boson of $3\times 10^{-21}$ eV, including Leo K \& M, whereas a lighter axion of $10^{-22}$ eV comprises the bulk of DM in all larger galaxies including the dSphs. Although Leo M is larger in size than Leo K, we predict its velocity dispersion to be smaller $(\simeq 1.7$km/s) than that of Leo K $(\simeq 4.5$km/s) because of the inverse de Broglie scale dependence on momentum. This scenario can be definitively tested using millisecond pulsars close to the Galactic center, where the Compton frequencies of the heavy and light bosons imprint monotone timing residuals that may be detected by the Square Kilometre Array (SKA) on timescales of approximately one week and four months, respectively. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2506_16915 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Infalling ultra-faint dwarfs as emissaries of the Axiverse Pozo, A. Broadhurst, T. Luu, H. N. Smoot, G. Umetsu, K. Chiueh, T. Schive, H. -Y. Emami, R. Hernquist, L. Mocz, P. Vogelsberger, M. Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies Recent discoveries of ultra-faint dwarf galaxies (UFDs) infalling onto the Milky Way, namely Leo K \& M at $r \simeq 450$kpc, considerably strengthens the case that UFDs constitute a distinct galaxy class that is inherently smaller and fainter, and metal-poorer than the classical dwarf spheroidals (dSph). This distinction is at odds with the inherent continuity of galaxy halo masses formed under scale-free gravity for any standard dark-matter (DM) model. Here, we show that distinct galaxy classes do evolve in cosmological simulations of multiple light bosons representing the ``Axiverse'' proposal of string theory, where a discrete mass spectrum of axions is generically predicted to span many decades in mass. In this context, the observed UFD class we show corresponds to a relatively heavy boson of $3\times 10^{-21}$ eV, including Leo K \& M, whereas a lighter axion of $10^{-22}$ eV comprises the bulk of DM in all larger galaxies including the dSphs. Although Leo M is larger in size than Leo K, we predict its velocity dispersion to be smaller $(\simeq 1.7$km/s) than that of Leo K $(\simeq 4.5$km/s) because of the inverse de Broglie scale dependence on momentum. This scenario can be definitively tested using millisecond pulsars close to the Galactic center, where the Compton frequencies of the heavy and light bosons imprint monotone timing residuals that may be detected by the Square Kilometre Array (SKA) on timescales of approximately one week and four months, respectively. |
| title | Infalling ultra-faint dwarfs as emissaries of the Axiverse |
| topic | Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2506.16915 |