What is a Plummer Sphere Exactly?

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In summary, a plummer sphere is a specific model for the density and gravitational potential distribution in a spherical halo of matter. It is often used in N-body simulations to soften gravity at close distance scales, preventing point particles from scattering too strongly off each other. The density distribution is given by the formula \rho(r)=\frac{3M}{4\pi a^3}\frac{1}{(1+\frac{r^2}{a^2})^{5/2}} and the gravitational potential is \Phi(r)=\frac{-GM}{\sqrt{r^2+a^2}}. The parameter "a" is an arbitrary value, but can be thought of as the radius of the halo or the "softening
  • #1
sderamus
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I assume it is a sphere with "handles" stretching out from the side - somewhat like a galaxy as that is where I have seen the term. I searched in vain in old Physics texts but could not find what it is exactly.

TIA

Sterling
 
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A plummer sphere is just a particular model for density/gravitational potential distribution in a spherical halo of matter. The density distribution is given by:

[tex]\rho(r)=\frac{3M}{4\pi a^3}\frac{1}{(1+\frac{r^2}{a^2})^{5/2}}[/tex]

The gravitational potential is

[tex]\Phi(r)=\frac{-GM}{\sqrt{r^2+a^2}}[/tex]

The plummer potential is often used in N-body simulations to "soften" gravity at small distance scales. This is needed to prevent the point particles (which are used as an approximation to extended objects) from scattering too strongly off of one another on close approach.
 
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  • #3
SpaceTiger said:
A plummer sphere is just a particular model for density/gravitational potential distribution in a spherical halo of matter. The density distribution is given by:

[tex]\rho(r)=\frac{3M}{4\pi a^3}\frac{1}{(1+\frac{r^2}{a^2})^{5/2}}[/tex]

The gravitational potential is

[tex]\Phi(r)=\frac{-GM}{\sqrt{r^2+a^2}}[/tex]

The plummer potential is often used in N-body simulations to "soften" gravity at small distance scales. This is needed to prevent the point particles (which are used as an approximation to extended objects) from scattering too strongly off of one another on close approach.

Thanks, Tiger. I saw the gravitational potential equation in the text. But what is "a" exactly? Is it the radius of the halo?

TIA

Sterling
 
  • #4
sderamus said:
Thanks, Tiger. I saw the gravitational potential equation in the text. But what is "a" exactly? Is it the radius of the halo?

Just an arbitrary parameter in the Plummer formula. It can be thought of roughly as the radius of the halo, since the potential approaches that of a point mass beyond that radius. In the context of N-Body simulations, "a" will be called the "softening length".
 

1. What is a Plummer Sphere?

A Plummer Sphere is a theoretical model of a star cluster that is used to study the dynamics of stars within the cluster. It is named after the British astronomer Herbert Dingle Plummer, who first proposed the model in 1911.

2. How is a Plummer Sphere different from other models of star clusters?

A Plummer Sphere assumes that the stars within the cluster have a constant density distribution, which means that the number of stars per unit volume remains the same throughout the cluster. This is different from other models that assume different density distributions, such as a Gaussian or King profile.

3. What factors influence the shape and size of a Plummer Sphere?

The shape and size of a Plummer Sphere are primarily influenced by the total mass of the cluster and the velocity dispersion of the stars within it. A higher mass or higher velocity dispersion will result in a larger and more elongated Plummer Sphere.

4. What is the significance of using a Plummer Sphere in studying star clusters?

A Plummer Sphere is a simple and widely used model that allows scientists to study the dynamics of star clusters and make predictions about their evolution over time. It also provides a good starting point for more complex models that incorporate additional factors, such as binary star interactions.

5. Are there any limitations to using a Plummer Sphere in studying star clusters?

Yes, there are some limitations to using a Plummer Sphere. For example, it assumes a spherically symmetric cluster and does not take into account the effects of external forces or disruptions from passing stars. It also does not account for the presence of dark matter, which is believed to play a significant role in the dynamics of star clusters.

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