If Dark Matter is Fuzzy, the First Stars Form in Massive Pancakes
Published in ApJL, 2022
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Recommended citation: Kulkarni M., Visbal E., Bryan G. L., Li X., 2022, ApJL, 941, 18
Publications
Robust field-level inference with dark matter halos
Published in arXiv e-prints, 2022
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Recommended citation: Shao H., et al., 2022a, arXiv e-prints, p. arXiv:2209.06843
What is the halo mass function in a fuzzy dark matter cosmology?
Published in MNRAS, 2022
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Recommended citation: Kulkarni, M. & Ostriker, J. P. 2022, MNRAS, 510, 1425
The Critical Dark Matter Halo Mass for Population III Star Formation: Dependence on Lyman-Werner Radiation, Baryon-dark Matter Streaming Velocity, and Redshift
Published in ApJ, 2021
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Recommended citation: Kulkarni M., Visbal E., Bryan G. L., 2021, ApJ, 917, 40
Fragmentation in Population III Galaxies Formed through Ionizing Radiation
Published in ApJ, 2019
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Recommended citation: Kulkarni, M., Visbal, E., & Bryan, G. L. 2019, ApJ, 882, 178