scispace - formally typeset
E

Eliot Quataert

Researcher at University of California, Berkeley

Publications -  242
Citations -  15951

Eliot Quataert is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Galaxy & Accretion (astrophysics). The author has an hindex of 66, co-authored 242 publications receiving 14271 citations. Previous affiliations of Eliot Quataert include University of California & UCB.

Papers
More filters
Journal ArticleDOI

Gyrokinetic turbulence: a nonlinear route to dissipation through phase space

TL;DR: In this paper, a conceptual framework for understanding kinetic plasma turbulence as a generalized form of energy cascade in phase space is presented, emphasizing that conversion of turbulent energy into thermodynamic heat is only achievable in the presence of some (however small) degree of collisionality.
Journal ArticleDOI

Accretion-Induced Collapse From Helium Star + White Dwarf Binaries

TL;DR: In this paper, the authors presented the first true binary simulations of He star + O/Ne white dwarf (WD) binaries, focusing on a $1.5 M_\odot$ He star in a 3 hour orbital period with O/NE WDs.
Journal ArticleDOI

The Impact of Type Ia Supernovae in Quiescent Galaxies. I. Formation of the Multiphase Interstellar Medium

TL;DR: In this paper, the authors proposed that uneven heating from Type Ia supernovae (SNe Ia), together with radiative cooling, can lead to the formation of the cool phase.
Journal ArticleDOI

When Should We Treat Galaxies as Isolated

TL;DR: In this article, the authors derive criteria for when disks can be well-approximated as "isolated" as a function of mass, redshift, and disk stability.
Journal ArticleDOI

Buoyancy instabilities in degenerate, collisional, magnetized plasmas

TL;DR: In this paper, the authors study analogous buoyancy instabilities in degenerate collisional plasmas, i.e., when the electron collision frequency is large compared to the electron cyclotron frequency, and show that the range of wavelengths that are unstable is independent of the magnetic field strength.