Help with the Virial Theorem please

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    Theorem Virial theorem
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Discussion Overview

The discussion revolves around the application of the Virial Theorem to a star cluster system composed of stars and gas. Participants are exploring how to calculate the kinetic energy of the system under specific conditions, including assumptions about mass distribution and equilibrium.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Homework-related

Main Points Raised

  • One participant describes a star cluster consisting of stars and gas, with total masses denoted as M sub * and M sub g, respectively, and proposes that M sub g = f*M sub *.
  • The same participant asks how to calculate the kinetic energy in terms of r sub c, f, and M sub * for an unrotating and equilibrium system.
  • Another participant suggests using mathematical notation for clarity, indicating that the current format of equations is difficult to understand.
  • A later post mentions potential energy, introducing the variable omega without further context.

Areas of Agreement / Disagreement

The discussion remains unresolved, with no consensus on the approach to calculating kinetic energy or the specific equations to use.

Contextual Notes

Participants have not fully defined all variables or assumptions, and there may be dependencies on specific definitions of terms like kinetic energy and potential energy.

Alfie114
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TL;DR
I have a question about the virial theorem as applied to a cluster of stars.
Anyone able to help if I provide you with more details?
 
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:welcome:

You might need to provide a bit more detail about your question.
 
OK we have a star cluster (the system) which is made up from stars (total mass M sub *) and gas (total mass M sub g). The stars and gas are all distributed as spheres of constant density and a finite radius r sub c.

The total mass of the stars and the gas is different but we can assume that M sub g = f*M sub *

If the system is unrotating and in equilibrium how do we calculate the kinetic energy in terms of r sub c, f and M sub *?

We can take 2KE + PE = 0 where KE = (-3/5) (GM^2/R) and PE = (3kT/2)*n where n is the total number of particles = (M/mu*m sub H) where mu=1 and m sub H is the mass of a hydrogen atom.
 
Alfie114 said:
OK we have a star cluster (the system) which is made up from stars (total mass M sub *) and gas (total mass M sub g). The stars and gas are all distributed as spheres of constant density and a finite radius r sub c.

The total mass of the stars and the gas is different but we can assume that M sub g = f*M sub *

If the system is unrotating and in equilibrium how do we calculate the kinetic energy in terms of r sub c, f and M sub *?

We can take 2KE + PE = 0 where KE = (-3/5) (GM^2/R) and PE = (3kT/2)*n where n is the total number of particles = (M/mu*m sub H) where mu=1 and m sub H is the mass of a hydrogen atom.
You need to use math latex notation. Its hard to understand your equations like this.
 
Ok I've got these where omega is the potential energy
1575636887584.png
1575636809181.png
 

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