Energy of the retarded gravity field in a collapse of a mass shell: the energy is significant
In the case of a collapsing sphere, the retarded field steals energy from the kinetic energy of the collapse.
Suppose that retardation keeps time running at a fraction h / 2 faster at the center of the collapsing shell than it would run if the signal speed were infinite. Then most of the retardation energy is stored in the interaction of the mass near the center, M, and the retarded field. The energy is
~ h / 2 * M c²,
that is, linear in h.
If there is no mass near the center, the energy of the retarded field might be similar to the analogous electric field. Another way to estimate the energy of the gravity field is to calculate the pseudotensor. Generally, the energy density is quadratic in h.
Mark Hindmarsh (2018) gives the following approximate formula for the energy density of gravitational waves:
The dot means the derivative over time. The brackets ⟨ ... ⟩ denote an average over an entire wave. The components hij are differences from the flat Minkowski metric.
Let us calculate a very rough estimate for the collapse into a neutron star. We assume that the mass 3 * 10³⁰ kg forms a thin shell. What is the energy of the retarded gravity field inside the shell?
In the previous blog post we calculated that h₀₀ ≈ 0.13 at the center, that is, time runs 6.4% faster at the center than for a flat metric.
Let us assume that the metric becomes flat when the signal to the center reaches from the radius r = 10 km of the neutron star which just formed. Then
dh₀₀ / dt = h₀₀ c / r.
The energy density of the retarded gravity field is something like
egw = c² / (32 π G) * h₀₀² c² / r²
= c⁴ / (32 π G) * h₀₀² / r²,
and the total energy
E = 1/24 * c⁴ / G * h₀₀² * r
= 1/24 * 8 * 10³³ * 1.5 * 10¹⁰
* 0.13² * 10⁴ J
= 8 * 10⁴⁴ J.
This is interesting. The energy is of the same order of magnitude as we calculated in the previous blog post (13 versus 8) from the interaction of the mass near the center and the retarded gravity field (gravity potential).
Maybe the radial metric g₁₁ is stretched, too? In that case the energy density ggw must be doubled.
The energy of the pure retarded gravity field, without any mass in it, is significant!
What is the energy of the retarded field if we calculate it from the analogous electric field?
In the force formula,
G ~ 1 / (4 π ε₀).
The energy density of a gravity field is then
e = 1 / (8 π G) * Eg²,
where Eg is the strength of the gravity field (force / mass).
If the potential is h₀₀ / 2 * c² over a distance of r = 10 km, the field strength is
Eg = h₀₀ / 2 * c² / r.
The energy density of the retarded gravity field is then
e = c⁴ / (32 π G) * h₀₀² / r²
= egw.
We see that the energy density e agrees with the one which we calculated from the formula for gravitational waves!
Does the energy of the retarded gravity field approach the total released energy in a collapse into a black hole?
The gravitational energy released in a collapse into a neutron star of a mass 3 * 10³⁰ kg is roughly 300 * 10⁴⁴ J. The energy in the retarded gravity field is something like 13 * 10⁴⁴ J – not a very large portion of the total energy.
What if the collapse would go further, so that the system becomes a black hole? Could the energy of the retarded field approach the total energy released in the collapse?
As the shell approaches the Schwarzschild radius r = 4.5 km, its speed approaches c.
signal
----------------------------------------------->
--> 0.4 c --> c
| | ×
r = 10 km r = 4.5 km center
potential potential
-0.2 c² -c²
Let the shell at r = 10 km send a signal to the center. When the signal arrives, the shell is already close to the Schwarzschild radius r = 4.5 km. But the observer at the center thinks that the radius is 6 km.
The potential difference at the center versus close to the shell is then ~ 0.5 c². Then
h₀₀ / 2 * c² = 0.5 c²,
or h₀₀ = 1. The energy of the retarded gravity field is
E = 1/24 * c⁴ / G * h₀₀² * r.
The energy is (1 / 0.13)² * 0.45 = 30 times that which we calculated in the previous section, or 240 * 10⁴⁴ J.
The potential energy released is
M c² = 3 * 10³⁰ * 9 * 10¹⁶ J
= 2700 * 10⁴⁴ J.
Our calculation is extremely crude. It shows that the energy of the retarded gravity field approaches a significant portion of the released potential energy when a shell collapses into a black hole.
This suggests that in the reverse process, an explosion, the retarded gravity field might boost the expansion speed greatly, which might explain "dark energy" in the universe.
An explosion of a mass shell
Can a retarded gravity field release energy enough, so that it could accelerate the expansion?
In a collapse, some of the energy goes to the retarded field, so that kinetic energy grows slower. But kinetic energy does not decrease at any point.
Let us then imagine an explosion of a shell. As the shell expands, gravity slows down its expansion. A clock at the center "thinks" that the shell has expanded more than it actually has. The clock ticks faster than it would if the speed of signals were infinite.
Let us assume that the speed of the expansion approaches some constant value v > 0 as the radius r becomes very large.
signal
-------------------->
0.4 c <-- <-- c
| | ×
r = 10 km rs = 4.5 km center
potential potential
-0.2 c² -c²
Above we have the start of an expansion from an almost-black-hole. When the center receives the signal, a clock there "deduces" that the shell is at r = 9 km. But the velocity of the shell has already fallen substantially. Let us guess that the shell is at r = 8 km.
In the Schwarzschild metric, the potential at a radius r is
(-1 + sqrt(1 - rs / r)) * c².
The potential at 9 km is -0.29 c², and at 8 km it is -0.34 c². Then h₀₀ = 0.1.
Let us calculate the energy of the retarded gravity field:
E = 1/24 * c⁴ / G * h₀₀² * r
= 1/24 * 81 * 10³² * 1.5 * 10¹⁰
* 1² / 10² * 8 * 10³
= 16 * 10⁴⁴ J.
The negative potential is -900 * 10⁴⁴ J at r = 8 km. The energy of the retarded field is not very large compared to this.
Is there any reason why we should assume that the potential at the center is very different from -0.29 c²? Maybe it should be zero?
A cosmological model is uniform: the retarded gravity field is visible only in "static" coordinates?
In the collapse to a neutron star, we claimed that the retarded gravity field holds a substantial energy. Our claim is based on the potential difference between the mass shell center and close to the shell.
But in the universe, no such potential differences seem to be present. However, the equipotential state happens in the comoving coordinates. In "static" coordinates, there is a potential difference. That difference slows down the expansion of the universe.
If dark energy is in the retarded gravity field, then that energy is visible in static coordinates.
Let us assume that the universe is a large uniform expanding ball, embedded in an asymptotically Minkowski space.
Let us assume that gravity behaves, for some reason, "uniformly" in comoving coordinates, so that the ball expands uniformly, just like in cosmological models.
We probably can study the center of the ball in such a way that we ignore other parts. We only look at the "observable universe" whose radius is something like 30 billion light-years.
Then our considerations above about an expanding mass shell are relevant. The main difference is that the shell expands at almost the speed of light, and its radius is huge.
E = 1/24 * c⁴ / G * h₀₀² * r.
The energy of the retarded field is linear in r for an almost-black-hole. The mass of a black hole is linear in r.
The mass inside a radius r is proportional to r³ in a cosmological model.
Can the retarded gravity field energy be released in a cascade?
Is there a reason why almost all the energy in the retarded gravity field should be released just now when the mass density of the universe is 0.3 times the "critical density"?
Yes: if the expansion no longer slows down, then all the energy in the retarded field must be released. Recall that the energy is there only because the expansion was slowing down. If the expansion slows down enough, it may start a cascade in which all the energy is released from the retarded field.
This would mean that the expansion of the universe may accelerate a little now, and then start slowing down again, as predicted by cosmological models. In the long run, the expansion, on the average, obeys cosmological models.
Let us try to estimate if the cascade happens in the expansion.
^ bulge
|
____ ___
\ _____ /
\ • / \ • /
v <-- --> v
weight weight
Let us first consider a rubber membrane model. A ring of weights expands, and the membrane between them bulges upward as the velocity of the weights, v, slows down.
Could it be that no cascade happens?
If the energy stored in the bulge is just a few percents of the negative potential energy, then probably no cascade occurs.
We need better models and ideas to explain dark energy.
The length contraction of the gravity field of a mass moving at almost c
\ /
\ /
m • --> ≈ c
/ \
/ \
"squeezed"
gravity field
Suppose that a mass shell expands almost at the speed c. If the gravity field behaves like the electric Coulomb field, then the gravity field is very much "squeezed" in the direction of the movement of m. The field of m is not much felt inside the shell. This would mean that the a clock at the center of the shell would not be much slowed down.
Does this make sense? If the shell is initially static, and the shell consists of photons, what happens?
The potential initially corresponds to a static shell. Then there is a pressure shock, as the shell is shot outward at the speed of light.
The center "knows" that the shell has moved far away, and can "calculate" the potential and adjust the clock rate accordingly.
If we shoot a photon shell at the speed of light toward the center, then the center does not "know" that it is at a lower potential as the shell approaches. In this case, a clock at the center should run at almost the rate of outer space. In this case, the gravity field behaves as it would be "squeezed", and not affect the center.
In the contracting case, the retarded gravity field can hold a lot of energy.
If the shell contracts at a velocity slightly less than c, an observer will receive a warning of the approaching shell wall early on.
Could it be that the speed of light inside the shell remains faster than at the shell? In that case, an observer at the center might see the contraction slowing down as the shell wall approaches?
We deduce the expansion speed of the universe from the redshift. In the case of a contracting universe, we look at the blueshift. The blueshift can, indeed, decrease if the clock rate at the shell wall slows down.
The redshift inside an expanding mass shell
^ bulge
|
o observer
____ ___
\ _____ /
\ • / \ • /
v <-- --> v
weight weight
Above is the rubber membrane model. Let us have an observer at the center, on the "bulge".
He sees a redshift in the receding shell. The redshift depends both on the velocity v and the rate of the clock on the bulge. If the bulge grows taller, then he sees a larger redshift.
*** WORK IN PROGRESS ***















