Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

NONLINEAR EVOLUTION OF RAYLEIGH-TAYLOR INSTABILITY IN A RADIATION-SUPPORTED ATMOSPHERE

Journal Article · · Astrophysical Journal
;  [1];  [2]
  1. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)
  2. Canadian Institute for Theoretical Astrophysics, Toronto, ON M5S3H4 (Canada)
The nonlinear regime of Rayleigh-Taylor instability (RTI) in a radiation supported atmosphere, consisting of two uniform fluids with different densities, is studied numerically. We perform simulations using our recently developed numerical algorithm for multi-dimensional radiation hydrodynamics based on a variable Eddington tensor (VET) as implemented in Athena, focusing on the regime where scattering opacity greatly exceeds absorption opacity. We find that the radiation field can reduce the growth and mixing rate of RTI, but this reduction is only significant when radiation pressure significantly exceeds gas pressure. Small-scale structures are also suppressed in this case. In the nonlinear regime, dense fingers sink faster than rarefied bubbles can rise, leading to asymmetric structures about the interface. By comparing the calculations that use a VET versus the Eddington approximation, we demonstrate that anisotropy in the radiation field can affect the nonlinear development of RTI significantly. We also examine the disruption of a shell of cold gas being accelerated by strong radiation pressure, motivated by models of radiation driven outflows in ultraluminous infrared galaxies. We find that when the growth timescale of RTI is smaller than acceleration timescale, the amount of gas that would be pushed away by the radiation field is reduced due to RTI.
OSTI ID:
22167131
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 763; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

Direct simulation Monte Carlo investigation of the Rayleigh-Taylor instability
Journal Article · Tue Aug 30 20:00:00 EDT 2016 · Physical Review Fluids · OSTI ID:1339256

Spike deceleration and bubble acceleration in the ablative Rayleigh-Taylor instability
Journal Article · Tue Dec 14 23:00:00 EST 2010 · Physics of Plasmas · OSTI ID:21532097

Bubble Acceleration in the Ablative Rayleigh-Taylor Instability
Journal Article · Sun Nov 19 23:00:00 EST 2006 · Physical Review Letters · OSTI ID:895299