A self-consistent reduced model for dusty magnetorotationally unstable discs

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 423:1 (2012) 437-443

Authors:

Emmanuel Jacquet, Steven Balbus

MAPPING THE GALACTIC CENTER WITH GRAVITATIONAL WAVE MEASUREMENTS USING PULSAR TIMING

The Astrophysical Journal American Astronomical Society 752:1 (2012) 67

Authors:

Bence Kocsis, Alak Ray, Simon Portegies Zwart

Gas pile-up, gap overflow, and Type 1.5 migration in circumbinary disks: application to supermassive black hole binaries

(2012)

Authors:

Bence Kocsis, Zoltan Haiman, Abraham Loeb

Gas pile-up, gap overflow, and Type 1.5 migration in circumbinary disks: general theory

(2012)

Authors:

Bence Kocsis, Zoltan Haiman, Abraham Loeb

Zero-Turbulence Manifold in a Toroidal Plasma

ArXiv 1203.6455 (2012)

Authors:

EG Highcock, AA Schekochihin, SC Cowley, M Barnes, FI Parra, CM Roach, W Dorland

Abstract:

Sheared toroidal flows can cause bifurcations to zero-turbulent-transport states in tokamak plasmas. The maximum temperature gradients that can be reached are limited by subcritical turbulence driven by the parallel velocity gradient. Here it is shown that q/ε(magnetic field pitch/inverse aspect ratio) is a critical control parameter for sheared tokamak turbulence. By reducing q/ε, far higher temperature gradients can be achieved without triggering turbulence, in some instances comparable to those found experimentally in transport barriers. The zero-turbulence manifold is mapped out, in the zero-magnetic-shear limit, over the parameter space (γ_E, q/ε, R/L_T), where γ_E is the perpendicular flow shear and R/L_T is the normalised inverse temperature gradient scale. The extent to which it can be constructed from linear theory is discussed.