On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Oxford University Press (OUP) 474:4 (2017) 5672-5683

Authors:

Nwc Leigh, Am Geller, B McKernan, Kes Ford, M-M Mac Low, J Bellovary, Z Haiman, W Lyra, J Samsing, M O'Dowd, B Kocsis, S Endlich

On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening

(2017)

Authors:

Nathan WC Leigh, Aaron M Geller, B McKernan, KES Ford, M-M Mac Low, J Bellovary, Z Haiman, W Lyra, J Samsing, M O'Dowd, B Kocsis, S Endlich

Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters

(2017)

Authors:

László Gondán, Bence Kocsis, Péter Raffai, Zsolt Frei

The TRAPPIST-1 system: Orbital evolution, tidal dissipation, formation and habitability

(2017)

Authors:

John CB Papaloizou, Ewa Szuszkiewicz, Caroline Terquem

Optimized up-down asymmetry to drive fast intrinsic rotation in tokamaks

Nuclear Fusion Institute of Physics 58:2 (2017) 026003

Authors:

Justin R Ball, Felix I Parra, M Landreman, Michael A Barnes

Abstract:

Breaking the up-down symmetry of the tokamak poloidal cross-section can significantly increase the spontaneous rotation due to turbulent momentum transport. In this work, we optimize the shape of flux surfaces with both tilted elongation and tilted triangularity in order to maximize this drive of intrinsic rotation. Nonlinear gyrokinetic simulations demonstrate that adding optimally-tilted triangularity can double the momentum transport of a tilted elliptical shape. This work indicates that tilting the elongation and triangularity in an ITER-like device can reduce the energy transport and drive intrinsic rotation with an Alfv\'{e}n Mach number on the order of $1\%$. This rotation is four times larger than the rotation expected in ITER and is sufficient to stabilize MHD instabilities. It is shown that this optimal shape can be created using the shaping coils of several experiments.