Massive Black Hole Definition:
A massive black hole is a black hole with a single core resulting from a supernova event.
Reminder: “The Universe cannot compress Energy indefinitely because there is no infinite Energy anywhere in the Universe (not even the possibility of infinite Energy density at a point). This restriction leads us to conclude that a state of Matter with a maximum density MUST exist.
I name this state of maximum Matter density “
Dachus” (derived from the Hebrew word for compressed.) I use the term “
Dachus density” to denote this maximal density” [
1].
I denote Dachus density by
[
1]
Reminder: “Continual compression of Matter within a black hole ultimately compresses its Matter until it reaches Dachus density within a non-zero volume in the center of the black hole. As the Matter inside the black hole compresses to its maximum degree, it reaches a state where any further compression only contributes to the expansion of the black hole’s core size, which maintains its Dachus state.
Remark: The concept of a black hole without a singularity challenges the calculations of esteemed physicists who predict singularities at the core of black holes. However, it is essential to note that these calculations, which suggest the existence of singularities as a mathematical necessity, did not account for the possibility of an upper limit to matter density. Consequently, the conclusion that geodesics inside a black hole inevitably converge at a singularity is invalid” [
1].
All massive black holes have a core at Dachus density: .In this context, represents the distance from the center of the black hole to the radius where the maximal possible density begins to decrease.
During the supernova contraction phase, the gravitational attraction force is so big that it overcomes the tremendous deflecting centrifugal force of the elementary particles and creates a massive black hole with a small core at its center in Dachus density. In this core, all Energy compresses to the Dachus state, and the elementary particles lose their identity as elementary particles; they stop spinning because, in the Dachus state, there is no room for movement (the constituents of the black hole’s core do not move in relation to each other), and all that remains of them are their charges. After creating the massive black hole, the mighty gravitational attraction forces keep bending the space-time curvature around the core, causing any Energy near the core to join the core and then compressing it up to the Dachus density. (This is how a massive black hole’s core grows.)
Aside: Are there circumstances in which a black hole’s core shrinks?
Discussion: There are two possibilities: When anti-Matter encounters its corresponding Matter at the core’s rim, they annihilate each other, and some of the Matter charges may spread outside the core because of the kinetic Energy discharged—emanating from the incoming anti-Matter Universe part. On very rare occasions, a surge of very intense uncertainty-related Energy hits the core’s rim, and if it is intense enough, it tears away some charges from the core’s rim. Both these occurrences can reduce the core size. Note: These two occurrences describe what can happen at the black hole’s core rim. However, the same occurrences can also happen between the core and the black hole’s border or at the border of the black hole. If these events occur at the black hole’s rim, the size of the black hole will decrease.
Most massive black holes’ cores rotate relativistically fast, maintaining some of their pre-supernovae star’s angular momentum, which had maintained the angular momentum of the revolving dust cloud that precedes them.
Short-range forces (of quarkic (aka color) and weak charges) do not affect massive black holes at their borders because their charge’s diminishing points (range) are less than the massive black holes’ event horizons. Negative and positive electric charges appear in equal quantities and negate each other, so they do not influence the event horizon of the massive black hole.
Therefore, I will use the Kerr equation for the event horizons: , where R is the massive black hole radius.
The calculations presented here assume a spherical shape for the black hole’s core. I have not considered the slight flattening of the core at its poles near the spin axis, which occurs when the black hole spins at a very high rate, forming a slightly oblated spheroid.
How big are the cores and horizons of spinning Massive black holes?
To answer, I will use two examples. The first black hole, Cygnus X-1, is a massive black hole in Cygnus’s constellation. It has 21.2 ± 2.2 Solar Masses [
3]. The second black hole is a supermassive black hole in the center of the Milky Way galaxy—Sagittarius A* with
solar Masses [
4].
I will calculate the Dachus core radius using .
is extremely small (it can be more than 48 orders of magnitude smaller than the Massive black hole event horizon radius in the case of Cygnus X-1—see table below.) When calculating the event horizon radius and its volume, I can assume that (almost) all the black hole Mass resides in its core. Thus, I can treat the Mass of a Massive black hole as a point Mass in the following angular momentum calculations. Assuming the black hole rotates very relativistically
[
5],
Remark: The observed Mass
already includes the relativistic effects.
Observations show that for Cygnus X-1:
[
6].
Observations show that for Sagittarius A*:
[
7].
Equation (1) Event horizon radius for a rotating massive black hole
where “
v” is the linear velocity at the equator of the spinning black hole.
is the boundary of the black hole.
We know very little about the Energy density distribution between the Dachus core and the rest of the massive black hole enveloping the core, except that most of the Massive black hole Energy is in the core. I name the volume between the black hole’s core and rim: the “Black Hole Mantle.” The black hole mantle must revolve very fast due to the relativistically fast rotating Dachus core that drags the Energy encompassing it. As we look further from the core, the revolving Energy speed inside the massive black hole decreases—but not too much, as seen in the two examples I presented in which the revolution speed of the entire black hole is very large.
Table 1.
Sizes comparison for Dachus core versus the entire black hole event horizon for highly relativistically rotating massive black holes.
Table 1.
Sizes comparison for Dachus core versus the entire black hole event horizon for highly relativistically rotating massive black holes.
Star |
Solar Masses |
|
Radius [m] |
Volume [m3] |
Cygnus X-1 |
|
|
|
Sagittarius A* |
|
|
|
Star |
|
Radius [Km] |
Volume [Km3] |
Cygnus X-1 |
|
|
Sagittarius A* |
|
|
The massive black hole’s core is a speck inside its total size. Cygnus X-1’s Dachus core volume is approximately times smaller than its event horizon volume, and Sagittarius A*‘s Dachus core volume is approximately times smaller than its event horizon volume.