Hydrostatic equilibrium violated in the sun

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SUMMARY

The discussion centers on the implications of a 0.01% violation of hydrostatic equilibrium in the Sun, specifically how this imbalance affects the Sun's radius. The relevant equations include the second derivative of radius with respect to time, expressed as d²r/dt² = -Gm/r² - 4πr²(∂P/∂m), and the dynamical timescale given by τ_dyn = √(R³/2GM). The net gravitational acceleration is calculated as g(net) = 2.7 x 10³ cm/s², indicating a significant inward pull on solar material. The discussion highlights the complexities of modeling such a scenario accurately.

PREREQUISITES
  • Understanding of hydrostatic equilibrium in astrophysics
  • Familiarity with gravitational force equations
  • Knowledge of pressure gradient concepts in stellar physics
  • Proficiency in differential equations and dynamical timescales
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  • Explore the implications of hydrostatic equilibrium in stellar evolution
  • Study the derivation and applications of the equations of state in astrophysics
  • Investigate numerical methods for simulating stellar dynamics
  • Learn about the role of pressure gradients in maintaining stellar stability
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Astronomers, astrophysicists, and students studying stellar dynamics and hydrostatic equilibrium will benefit from this discussion, particularly those interested in the stability and evolution of stars like the Sun.

AStaunton
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Hi there

Problem is:

if hydrostatic equilibrium were violated by .01% so that 0.01% of the gravitational force were imbalanced by the pressure gradient, estimate how long it would take the sun to change its radius by 10%.

My attempts at solving problem:

My feeling is that the following relation must be relevant:

\frac{d^{2}r}{dt^{2}}=-\frac{Gm}{r^{2}}-4\pi r^{2}\frac{\partial P}{\partial m}

and going by the problem posed, the pressure quantity should be .01 greater than the gravity quantity...

Also, I feel that the dynamical timescale is relevant here, the equation I have is:

\tau_{dyn}=\frac{R}{v_{esc}}=\sqrt{\frac{R^{3}}{2GM}}

But again, I am really stuck as to how to use these equations to solve this problem, any advice is greatly appreciated.
 
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Suppose the equilibrium between pressure and gravitational forces were violated by 0.01%, so that 0.01% of the gravitational force is not balanced by the pressure force. This means it would actually be
dP/dr = -ρg +10-4ρg
0.01% of the gravitational force could then pull the material inwards. For a gravitational acceleration of go = 2.7 x 104 cm s~2 the net acceleration would then be g(net) = 2.7 x 103 cms"2.
 
This thread is more than four years old - no point in reawakening it now.
 

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