Output list
Journal article
Published 11/2023
Physics of Plasmas, 30, 11, 112701
Journal article
Influence of mass ablation on ignition and burn propagation in layered fusion capsules
Published 01/2023
Physics of Plasmas, 30, 1, 12704
Journal article
A mechanism for reduced compression in indirectly driven layered capsule implosions
Published 04/2022
Physics of Plasmas, 29, 4, 42704
Journal article
Experimental quantification of the impact of heterogeneous mix on thermonuclear burn
Published 02/01/2022
Physics of plasmas, 29, 2, 022702
Journal article
Published 03/2021
High Energy Density Physics, 38, 100929
Journal article
Experimental validation of shock propagation through a foam with engineered macro-pores
Published 01/2021
Physics of Plasmas, 28, 1, 012702
Journal article
First observation of increased DT yield over prediction due to addition of hydrogen
Published 01/2021
Physics of Plasmas, 28, 1, 012707
Journal article
Observation of persistent species temperature separation in inertial confinement fusion mixtures
Published 12/2020
Nature Communications, 11, 1, 544
Journal article
Published 10/2020
Physics of Plasmas, 27, 10, 102701
Journal article
Outflows from inflows: the nature of Bondi-like accretion
Published 01/01/2020
Monthly notices of the Royal Astronomical Society, 491, 1, L76 - L80
The classic Bondi solution remains a common starting point both for studying black hole growth across cosmic time in cosmological simulations and for smaller scale simulations of active galactic nuclei (AGN) feedback. In nature, however, there will be inhomogeneous distributions of rotational velocity and density along the outer radius (R-o) marking the sphere of influence of a black hole. While there have been many studies of how the Bondi solution changes with a prescribed angular momentum boundary condition, they have all assumed a constant density at R-o. In this Letter, we show that a non-uniform density at R-o causes a meridional flow and due to conservation of angular momentum, the Bondi solution qualitatively changes into an inflow-outflow solution. Using physical arguments, we analytically identify the critical logarithmic density gradient vertical bar partial derivative ln rho/partial derivative theta vertical bar above which this change of the solution occurs. For realistic R-o, this critical gradient is less than 0.01 and tends to 0 as R-o -> infinity. We show using numerical simulations that, unlike for solutions with an imposed rotational velocity, the accretion rate for solutions under an inhomogeneous density boundary condition remains constant at nearly the Bondi rate (M) over dot(B), while the outflow rate can greatly exceed (M) over dot(B).