Gravitating Perfect Fluid Solution & Mass/Energy Total

  • Thread starter Mentz114
  • Start date
In summary, there exists a static spherically symmetric perfect fluid solution of the EFE with energy-momentum tensor ##diag(\rho,p,p,p)##. The mass/energy total of this PF is given by ##M_s = 8\pi\ m_s##, which is equal to the Schwarzschild parameter ##m_s## in terms of the parameters a and b. The pressure terms in the EMT do not contribute to the mass due to the cancellation of positive pressure and negative gravitational binding energy. This solution is realistic as the radius of the ball can be varied by changing the parameter a.
  • #1
Mentz114
5,432
292
There is a static spherically symmetric perfect fluid solution of the EFE where the energy-momentum tensor is ##diag(\rho,p,p,p)## with ##\rho=b\,\left( 2\,b\,{r}^{2}+3\,a\right) /{\left( 2\,b\,{r}^{2}+a\right) }^{2}## and ##p={b}/({2\,b\,{r}^{2}+a})##. a and b are parameters with b>0 and 0<a<1. On the surface ##r=\sqrt{(1-a)/(2b)}\equiv r_{max}## the PF metric coincides with the Schwarzschild exterior, as long as the Schwarzschild parameter m has the value ##m_s= {\sqrt{1-a}\,\left( 1-a\right) }/( {4\,\sqrt{2b}})##.

Calculating ##M_s## the mass/energy total of the PF
[tex]\begin{align*}
M_s &=\ 4\pi\int_0^{r_{max}} r^2\rho\ dr = 4\pi\left[ \frac{\,b\,{r}^{3}}{2\,b\,{r}^{2}+a} \right]_0^{r_{max}}\\
&= \frac{\sqrt{2}\,\pi\,\sqrt{1-a}\,\left( 1-a\right) }{\sqrt{b}}\\
&= 8\pi\ m_s
\end{align*}
[/tex]
This seems most satisfactory but raises the question - what happened to the pressure terms in the EMT ? It appears that the integral of the energy density accounts for all the exterior vacuum curvature. Is this an anomaly or am I right to be surprised ?

(Actually I was very glad when the integral turned out like this - until the question of the pressure appeared).
 
Physics news on Phys.org
  • #2
Mentz114 said:
what happened to the pressure terms in the EMT ?

Heuristically, the positive contribution of the pressure to the mass is exactly canceled by the negative contribution of gravitational binding energy to the mass. The easiest way I know of to see how that works is to look at the Komar mass integral, in which ##\rho + 3 p## appears in the integrand, but also the "redshift factor" ##\sqrt{1 - 2m(r) / r}## appears, and the two contributions cancel each other when the integral is computed over the entire volume of the object.
 
  • #3
PeterDonis said:
Heuristically, the positive contribution of the pressure to the mass is exactly canceled by the negative contribution of gravitational binding energy to the mass. The easiest way I know of to see how that works is to look at the Komar mass integral, in which ##\rho + 3 p## appears in the integrand, but also the "redshift factor" ##\sqrt{1 - 2m(r) / r}## appears, and the two contributions cancel each other when the integral is computed over the entire volume of the object.
Thanks. That could account for it. I'll check out the KM integral.

This PF is more realistic than I first thought because the radius of the ball can be set to any multiple of 2m by a suitable choice of parameter a. As a-> 0 so rmax -> 4m, and as a->1 so rmax increases without bound.
 
Last edited:

1. What is a gravitating perfect fluid solution?

A gravitating perfect fluid solution is a theoretical model used in physics to describe the behavior of a perfect fluid (a fluid with no viscosity or heat conduction) in the presence of gravity. It is often used in the study of general relativity and cosmology.

2. What is the mass/energy total in a gravitating perfect fluid solution?

The mass/energy total in a gravitating perfect fluid solution refers to the total amount of matter and energy present in the system. In general relativity, mass and energy are considered to be equivalent and are combined into a single quantity known as the stress-energy tensor.

3. How is a gravitating perfect fluid solution different from other fluid models?

A gravitating perfect fluid solution is different from other fluid models in that it takes into account the effects of gravity on the fluid. This allows for the inclusion of gravitational potential energy and the curvature of spacetime in the fluid's behavior.

4. Can a gravitating perfect fluid solution be used to model real-world systems?

While a gravitating perfect fluid solution is a useful theoretical model, it may not accurately describe all real-world systems. In some cases, other factors such as viscosity or heat conduction may need to be taken into account. However, it can still provide valuable insights and predictions in many situations.

5. What are some applications of gravitating perfect fluid solutions?

Gravitating perfect fluid solutions have a wide range of applications in physics, particularly in the study of cosmology and astrophysics. They are used to model the behavior of matter and energy in the universe, including the formation of galaxies, the evolution of the universe, and the behavior of black holes.

Similar threads

  • Special and General Relativity
Replies
4
Views
276
  • Special and General Relativity
Replies
5
Views
1K
  • Special and General Relativity
Replies
2
Views
574
  • Special and General Relativity
Replies
0
Views
2K
  • Special and General Relativity
Replies
1
Views
844
  • Special and General Relativity
Replies
1
Views
820
  • Special and General Relativity
Replies
8
Views
1K
  • Special and General Relativity
Replies
10
Views
709
  • Special and General Relativity
Replies
29
Views
1K
  • Special and General Relativity
Replies
13
Views
1K
Back
Top