
Career
- 2005- : Professor of Mathematical Physics, Universityof Cambridge
- 1988-2005: Professor of Mathematics and Astronomy, Queen Mary, University of London
Research
John Papaloizou is a member of the Department of Applied Mathematics and Theoretical Physics . He works in the Astrophysical fluid dynamics research group. His current research interests are in the dynamics of astrophysical disks, planet formation and the early evolution of planetary systems.
Selected Publications
Publications
A planet on an inclined orbit as an explanation of the warp in the beta Pictoris disc
– Monthly Notices of the Royal Astronomical Society
(1997)
292,
896
(doi: 10.1093/mnras/292.4.896)
Bending instabilities in magnetized accretion discs
– Monthly Notices of the Royal Astronomical Society
(1997)
292,
631
(doi: 10.1093/mnras/292.3.631)
Non-adiabatic tidal forcing of a massive, uniformly rotating star — II. The low-frequency, inertial regime
– Monthly Notices of the Royal Astronomical Society
(1997)
291,
633
(doi: 10.1093/mnras/291.4.633)
Non-adiabatic tidal forcing of a massive, uniformly rotating star .3. Asymptotic treatment for low frequencies in the inertial regime
– Monthly Notices of the Royal Astronomical Society
(1997)
291,
651
(doi: 10.1093/mnras/291.4.651)
On the stability of an accretion disc containing a toroidal magnetic field: the effect of resistivity
– Monthly Notices of the Royal Astronomical Society
(1997)
287,
771
(doi: 10.1093/mnras/287.4.771)
Causal viscosity in accretion disc boundary layers
– Monthly Notices of the Royal Astronomical Society
(1997)
487,
125
(doi: 10.1093/mnras/285.2.239)
The hydrodynamical response of a tilted circumbinary disc: linear theory and non-linear numerical simulations
– Monthly Notices of the Royal Astronomical Society
(1997)
285,
288
(doi: 10.1093/mnras/285.2.288)
Causal viscosity in accretion disc boundary layers
– Monthly Notices of the Royal Astronomical Society
(1997)
285,
239
(doi: 10.1093/mnras/285.2.239)
On the nature of strange modes in massive stars
– Monthly Notices of the Royal Astronomical Society
(1997)
284,
821
(doi: 10.1093/mnras/284.4.821)
- <
- 17 of 28