MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus, B. Tabone, G.P. Rosotti, G. Lodato, P.J. Armitage, A.J. Cridland, & E.F. van Dishoeck, MNRAS Letters, 512, L74 (2022)
Secular evolution of MHD wind-driven discs: analytical solutions in the expanded alpha-framework, B. Tabone, G.P. Rosotti, A.J. Cridland, P.J. Armitage, & G. Lodato, MNRAS, 512, 2290 (2022)
Global 3D radiation hydrodynamic simulations of proto-Jupiter's convective envelope, Z. Zhu, Y.-F. Jiang, H. Baehr, A.N. Youdin, P.J. Armitage & R.G. Martin, MNRAS, 508, 453 (2021)
Boundary layer circumplanetary accretion: How fast could an unmagnetized planet spin up through its disk?, J. Dong, Y.-F. Jiang & P.J. Armitage, ApJ, 921, id. 54 (2021)
A Bayesian neural network predicts the dissolution of compact planetary systems, M. Cranmer et al., PNAS, 118, issue 40, id. 2026053118 (2021)
Lecture notes on accretion disk physics (arXiv only)
Visualizing the kinematics of planet formation, Disk Dynamics Collaboration
Physical processes in protoplanetary disks (Armitage, 45th Saas-Fee Advanced Course "From Protoplanetary Disks to Planet Formation")
A brief overview of planet formation (Armitage, short introduction for the Handbook of Exoplanets)
Dynamics of protoplanetary disks (Armitage, ARA&A, 2011)
Lecture notes on the formation and early evolution of planetary systems (arXiv only)
Beyond work I enjoy hiking, often combined with photography. My main focus is landscapes, but over the years I've also made trips to photograph bears in some spectacular spots in Alaska.