| The critical dark matter halo mass for Population III star formation: Dependence on Lyman–Werner radiation, baryon-dark matter streaming velocity, and redshift M Kulkarni, E Visbal, GL Bryan The Astrophysical Journal 917 (1), 40, 2021 | 67 | 2021 |
| What is the halo mass function in a fuzzy dark matter cosmology? M Kulkarni, JP Ostriker Monthly Notices of the Royal Astronomical Society 510 (1), 1425-1430, 2022 | 39 | 2022 |
| Fragmentation in Population III Galaxies Formed through Ionizing Radiation M Kulkarni, E Visbal, GL Bryan The Astrophysical Journal 882 (2), 178, 2019 | 13 | 2019 |
| If dark matter is fuzzy, the first stars form in massive pancakes M Kulkarni, E Visbal, GL Bryan, X Li The Astrophysical Journal Letters 941 (1), L18, 2022 | 9 | 2022 |
| A critical mass for Pop III stars: dependence on Lyman-Werner radiation, baryon/dark-matter streaming, and redshift M Kulkarni, E Visbal, GL Bryan American Astronomical Society Meeting Abstracts# 235 235, 153.07, 2020 | | 2020 |
| On the letter frequencies and entropy of written Marathi J Chipalkatti, M Kulkarni arXiv preprint arXiv:1707.08209, 2017 | | 2017 |
| Simulating the distribution of cosmological neutral hydrogen over cosmic times M KULKARNI | | 2015 |
