activity
20172026
most citedResonant drag instability of grains streaming in fluids

74 citations · 103 across the 11 of their papers we have counts for

collaborators
Showing 2024Show all

8 papers · 1 filter

astro-ph.GA2024

Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe

Nadine H. Soliman, Philip F. Hopkins, Jonathan Squire

We propose a novel dust battery mechanism for generating seed magnetic fields in the early universe, in which charged dust grains are radiatively accelerated, inducing strong elect…

astro-ph.HE2024★ 7 cited

Rapid, strongly magnetized accretion in the zero-net-vertical-flux shearing box

Jonathan Squire, Eliot Quataert, Philip F. Hopkins

We show that there exist two qualitatively distinct turbulent states of the zero-net-vertical-flux shearing box. The first, which has been studied in detail previously, is characte…

astro-ph.GA2024

Are Stars Really Ingesting their Planets? Examining an Alternative Explanation

Nadine H. Soliman, Philip F. Hopkins

Numerous stars exhibit surprisingly large variations in their refractory element abundances, often interpreted as signatures of planetary ingestion events. In this study, we propos…

astro-ph.EP2024

The First Evidence of a Host Star Metallicity Cut-off In The Formation of Super-Earth Planets

Kiersten M. Boley, Jessie L. Christiansen, Jon Zink +7

Planet formation is expected to be severely limited in disks of low metallicity, owing to both the small solid mass reservoir and the low opacity accelerating the disk gas dissipat…

astro-ph.GA2024

Thermodynamics of Giant Molecular Clouds: The Effects of Dust Grain Size

Nadine H. Soliman, Philip F. Hopkins, Michael Y. Grudić

The dust grain size distribution (GSD) likely varies significantly across star-forming environments in the Universe, but its impact on star formation remains unclear. This ambiguit…

astro-ph.GA2024★ 8 cited

Playing with FIRE: A Galactic Feedback-Halting Experiment Challenges Star Formation Rate Theories

Shivan Khullar, Christopher D. Matzner, Norman Murray +4

Stellar feedback influences the star formation rate (SFR) and the interstellar medium of galaxies in ways that are difficult to quantify numerically, because feedback is an essenti…

astro-ph.GA2024★ 7 cited

Dust-Evacuated Zones Near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions

Nadine H. Soliman, Philip F. Hopkins, Michael Y. Grudić

Stars form within dense cores composed of both gas and dust within molecular clouds. However, despite the crucial role that dust plays in the star formation process, its dynamics i…

astro-ph.EP2024

Microphysical Regulation of Non-Ideal MHD in Weakly-Ionized Systems: Does the Hall Effect Matter?

Philip F. Hopkins, Jonathan Squire, Raphael Skalidis +1

The magnetohydrodynamics (MHD) equations plus 'non-ideal' (Ohmic, Hall, ambipolar) resistivities are widely used to model weakly-ionized astrophysical systems. We show that if grad…