activity
20082013
most citedCharacterising the Gravitational Instability in Cooling Accretion Discs

212 citations · 216 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2013

The evolution of planetesimal swarms in self-gravitating protoplanetary discs

Joe Walmswell, Cathie Clarke, Peter Cossins

We investigate the kinematic evolution of planetesimals in self-gravitating discs, combining Smoothed Particle Hydrodynamical (SPH) simulations of the disc gas with a gravitational…

astro-ph.SR2010

The Nature of Angular Momentum Transport in Radiative Self-Gravitating Protostellar Discs

Duncan Forgan, Ken Rice, Peter Cossins +1

Semi-analytic models of self-gravitating discs often approximate the angular momentum transport generated by the gravitational instability using the phenomenology of viscosity. Thi…

astro-ph.IM2010★ 4 cited

Smoothed Particle Hydrodynamics

Peter J. Cossins

I present a review of Smoothed Particle Hydrodynamics (SPH), with the aim of providing a mathematically rigorous, clear derivation of the algorithms from first principles. The meth…

astro-ph.GA2009

The effects of opacity on gravitational stability in protoplanetary discs

Peter Cossins, Giuseppe Lodato, Cathie Clarke

In this paper we consider the effects of opacity regimes on the stability of self-gravitating protoplanetary discs to fragmentation into bound objects. Using a self-consistent 1-D…

astro-ph2008★ 212 cited

Characterising the Gravitational Instability in Cooling Accretion Discs

Peter Cossins, Giuseppe Lodato, Cathie Clarke

We perform numerical analyses of the structure induced by gravitational instabilities in cooling gaseous accretion discs. For low enough cooling rates a quasi-steady configuration…