activity
20022026
most citedMagnetar Spindown, Hyper-Energetic Supernovae, and Gamma Ray Bursts

368 citations · 3.7k across the 79 of their papers we have counts for

collaborators
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16 papers · 1 filter

astro-ph2008★ 31 cited

The Effectiveness of the Kozai Mechanism in the Galactic Centre

P. Chang

I examine the effectiveness of Kozai oscillations in the centres of galaxies and in particular the Galactic centre using standard techniques from celestial mechanics. In particular…

astro-ph2008★ 20 cited

Migration of Star Clusters and Nuclear Rings

Glenn van de Ven, Philip Chang

Star clusters that form in nuclear rings appear to be at slightly larger radii than the gas. We argue that the star clusters move out from the gas in which they are formed because…

astro-ph2008★ 2 cited

Long Term Evolution of Magnetic Turbulence in Relativistic Collisionless Shocks

Philip Chang, Anatoly Spitkovsky, Jonathan Arons

We study the long term evolution of magnetic fields generated by an initially unmagnetized collisionless relativistic shock. Our 2D particle-in-cell numerical simulations…

astro-ph2008★ 48 cited

Convection during the Late Stages of Simmering in Type Ia Supernovae

Anthony L. Piro, Philip Chang

Following unstable ignition of carbon, but prior to explosion, a white dwarf (WD) in a Type Ia supernova (SN Ia) undergoes a simmering phase. During this time, a central convective…

astro-ph2008★ 14 cited

Gas Shepherding by an Infalling Satellite

P. Chang

I calculate the action of a satellite, infalling through dynamical friction, on a coplanar gaseous disk of finite radial extent. The disk tides, raised by the infalling satellite,…

astro-ph2007★ 198 cited

Long Term Evolution of Magnetic Turbulence in Relativistic Collisionless Shocks: Electron-Positron Plasmas

P. Chang, A. Spitkovsky, J. Arons

We study the long term evolution of magnetic fields generated by a collisionless relativistic shock which is initially unmagnetized. Our 2D particle-in-cell numerical simu…