Presenter Information

Blake BottesiFollow

Start Date

April 2024

Location

2nd floor - Library

Abstract

Stars form when dense regions of molecular gas in our galaxy collapse due to their self-gravity. For this to occur, the magnetic field supporting these regions must diffuse out through a process known as ambipolar diffusion. We build on previous work by examining a one-dimensional self-gravitating gas with a polytropic equation of state (P∝ρε), considering cases that range from softer (ϵ<1) to stiffer (ϵ>1) than isothermal. Our results indicate that the diffusion time is not very sensitive to ϵ when stiffer than isothermal but is sensitive to ϵ when softer than isothermal. Additionally, the presence of magnetic and density fluctuations reduces the diffusion times, with the shortest diffusion times obtained for gases with large initial magnetic to gas pressure ratios and fairly soft equations of state. However, the diffusion time starts to increase significantly for ϵ ≲ 0.5, indicating that such soft equations of state are inconsistent with observations.

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Apr 17th, 4:00 PM Apr 17th, 4:45 PM

Ambipolar Diffusion with a Polytropic Equation of State

2nd floor - Library

Stars form when dense regions of molecular gas in our galaxy collapse due to their self-gravity. For this to occur, the magnetic field supporting these regions must diffuse out through a process known as ambipolar diffusion. We build on previous work by examining a one-dimensional self-gravitating gas with a polytropic equation of state (P∝ρε), considering cases that range from softer (ϵ<1) to stiffer (ϵ>1) than isothermal. Our results indicate that the diffusion time is not very sensitive to ϵ when stiffer than isothermal but is sensitive to ϵ when softer than isothermal. Additionally, the presence of magnetic and density fluctuations reduces the diffusion times, with the shortest diffusion times obtained for gases with large initial magnetic to gas pressure ratios and fairly soft equations of state. However, the diffusion time starts to increase significantly for ϵ ≲ 0.5, indicating that such soft equations of state are inconsistent with observations.

 

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