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Episode Transcript
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Speaker 1 (00:00):
Hi everyone, and welcome back to the morning round. But
we are alive once again. It is Wednesday, September eighteenth.
Those of you that want to join in with me
on the chat, you're most definitely welcome to do. So.
Let's look at what we have on the table where
we left off Monday and Tuesday, and we're speaking of
lower mass black holes. Our star is what we're looking
(00:21):
at and leaving off with time curvature and two massive
objects in orbit, and yesterday be stating well, Monday me stating, well,
this massive object it will be greater than the Sun
now and it does not have to be orbiting, it
(00:46):
does not have to be within the orbit of this
star war that we're speaking of. Specifically, I spoke yesterday
about different types of gravity because it took us to
where the rate is took up what we focused on
our start now in our stars calculation, the radius taken
us to different types of gravity. We are using gravity, radiation,
(01:20):
gas and dust as our main ingredients. Well, the foundation
of our ingredients, our main ingredients as our statey as
of yesterday are it is the galaxy clusters most specifically,
and that's the second major secondary primary object cause we're
gonna get to the first primary object. Also this second
(01:42):
primary object that is not an orbit that is, but
it's taking place and taking a part of space and
place regarding bringing into our start, bringing back into the
core of our start. Our stated yesterday, this is where
all the information is. Most of the information is here,
and this is when we get in different types of gravity.
So we are speaking about modified gravity here. Now let's
(02:06):
look at this and talk about the information that is
coming from our galaxy clusters, and we're speaking of irregular
clusters accounting for the space time curvature, because remember it
bought us back to space time curvature. It brought us
back to the two massive objects, one being the Sun,
(02:28):
the other one being the galaxy clusters themselves. So in
accounting for that time curvature, and we'll getting to the
time curvature tomorrow or on Friday, But let's look at
this first here and why it is happening and the
ingredients that makes it so in us deciding based on
pulling into our star White Draft Star, Replica Star, Neutron Star,
(02:53):
and two draft stars, and what line stands up regarding
the ingredients are making that the problem ability of and
within the bounds of what can be drawn in now,
and we're gonna see why those were chosen as the
probability of what could be drawn into our lower mass
(03:13):
black hole into our star that we're focused on. Remember
their outcome probability probability Replica star, neutron star, two drawer stars. Now,
yesterday we talked about what the outcome probability of with
the super and nova type lass and that dust that
(03:34):
outcome probability of being white draw star. But let's get deeper,
because we haven't look at d or even beginning to
look at the galaxy customs themselves, and the dust and
the particles coming from that is where the light comes
from and the light scatter comes from. Because remember our
(03:55):
obviously with a with explosive stars such as are what
we're dealing where it will not be emitting any light.
So and but because we're dealing with spotification, also there's
a lot that's going on there that plays a role
in and that plays a role in this space curvature
because we're also looking at time scales that are quite
(04:17):
different and ages of the dying stars and how long
they've been in their death processes and what that makes
regarding what the star is emitting and what is being
thrown out into the atmosphere and what is being changed
through spotification and through the gravitational pull of this massive, secondary,
(04:44):
most massive object, even though it's the secondary, looking at
it the secondary object, what the potential that it holds
as it relates to time curature and what is being
about into our star And we'll look at that also.
So let's look at this we're talking about. We're speaking
of regular galaxies, and you all understand why irregular galaxies
we're speaking on spouse most specifically within irregular galaxies now
(05:08):
containing a lot of gas and dust, because that's what
our primary structural focus is structure, the structural focused radiation, gas, gravity, dust.
We're gonna talk about magnetism also when we get to
that now. So I want to back back with our supernova,
with our particle collision regarding our start self now and
(05:31):
it being laxed in the type of dust and we
did our aging with our own specific star and the
type of dust material and energy that it emits now,
So is it in that particle collision that is separate
in amongst itself because when we're talking about age stars now,
(05:55):
and in dying stars, they are under a different law
of physics regarding their age and where they are positioned
within the within space. So that does of those supernovas
contain a different age, a different space time continuum, and
(06:15):
different laws of physics, meaning different potentials of what they
can do as it relates to us pulling in. And
you have to remember that within these explosions, because that's
where we're speaking of space. Explosions start explosion, and within
these collisions and colliding with what is external to it
(06:38):
within space, that material, that energy, that the type of
energy release, and we're talking about radiation and those collisions
and what they create, but also spoification because remember we
know that the tidal forces of lower mass black black
holes are very strong, so they have very strong tidal
(06:58):
forces in that spotification and creating a bending. But through
our calculations we see that it's not a bending per se.
It's a straight line. And we from Monday, when I
first laid everything out on the table, I know the
first doubts were like, Okay, this creates the chaos and
not the stated Well, well, it depends. It depends on
(07:22):
what their ingredients are and where they're coming from with
this space, you know, and whether the the chaos it
creates a very chaotic environment, whether the chaos is diminished
through what the particles pass through as they're circulating in space,
what they lose. So we know a lot of mass
is loss through these types of there's more mass loss
(07:46):
and through these types of evaporate evaporations and explosions and
through what they colloud with, so there's more mass loss.
So there is a minimizing due to the mass loss
of the chaos that one will proposed, that superposed that
that they will create. Now, so we're going back over
here and and looking at this these different this different
(08:10):
type of gravity because as I stated in the end
of of yesterday's presentation that the cluster galaxies is where
all the information is held now and the explosions there
to dyeing stars within those galaxies also, and the where
in our yesterday we were talking about supermassive supermassive object
(08:36):
in orbit of these supermassive will have to be calculated,
and we're gonna s talk about why that calculation will
will disperse the type of material and why those calculation
outcomes will disperse the type of material and energy and
also corresponds with modified gravity and it pulling into the
(09:00):
direction even though it is not within the orbit of
our star, of our black hole. And when we're the
pulling end, because remember with our star that the the
is we get, the gravitational pull is we get, but
(09:22):
we're drawing back into the core. So now we know
that irregular galaxies contain a lot of gas and dust.
Now the type of gas and dust, the type of
dust most specifically with this project, would be the most
(09:45):
significant because what do we gather from dust? We're speaking
about cosmic dust, dust particles. We gather the age the
beginning or as is it close to the beginning of
the universe in which it sits, and that is determined
by calculations of the dust itself, the particles within the dust,
(10:10):
and that lets us know the laws of physics pertaining
to the specific dying stars that we're looking at within
the the in the cluster galaxies. Because we're looking at
the dying stars within the cluster galaxies, we're looking at
material change material but material so now so, and we
(10:35):
know that we're looking at that because it leads to
the birth of new stars. And we're pulling into our
black hole into our star. So we're speaking about this
super massive galaxy cluster. You may have already done your
calculations on the masterly of it because we spoke about volume.
I spoke about volume on Monday and the importance of volume.
(11:04):
So that the the the cosmic d the dust of
these we already have the dust from the type that
soup and over regarding our own starring particle collision. Spogification
emits its own dust when when when different types of
material collide with this space orbiting around the black hole.
(11:30):
Now so is so we're we're speaking of the dust
from our dying stars within the cluster galaxies. That's that's
what we're focused on within the galaxies because they account
this type of gravity, cause we're speaking about modified gravity,
different types of gravity. As I stated yesterday, this this
(11:51):
type of gravity and the irregular clusters that we're dealing with,
and the rate is regardless. Spogification and we calculate it
being stretched out is what also accounts for a time curvature.
It accounts for time curvature here, but time curatures also
(12:12):
accounted for around our black hole and this spotification that
is going through regarding the material that is thrown out
through the explosion and the spotification that it's gone through
with the material that was released, and we talked about
that on Monday, material being released, and we calculate material
release by the age of the star and by what,
(12:38):
and that lets us know the potential of what. The
start the potential of what lets us know the direct
capability of the star regarding physics, and it also lets
us lets us know the potential of new capability because
we're talking about we're speaking about the birth of new stars,
(12:59):
but through spot vacation the new potential. Okay, now, so
that's that on is on that dust Lanel part while
we focus on this dust from our galaxies and the
DIN starts here now accounting more here with our supercluster,
(13:22):
accounting more here for space time curvature. But also this
is where time scales come into play now and time
scales coming into play because the calculation of the volume
(13:42):
volume calculation were we with the with the radius calculation,
we're speaking of schwatsh Our radius because we're speaking of
field equations. Because we remember, we're dealing with radiation and
we're talking about the radiation fil we're dealing with radiation
(14:06):
just all over the place is what this is radiation, gas,
gravity and dust. And remember we're talking about white draft star,
Revelu star, neutron star, or two draft stars. Now we're
gonna get into where two draft stars come into play.
We already yesterday got into where the white draft came
(14:27):
into play. Now with the with the type last dust
and the calculations brought to white draft star. Now, so
now we're gonna get into where neutron star could come
into the play. It come into play, excuse me, so
with our cosmic dust it's bringing it brings our focus
(14:49):
towards the dying stars now in the in the in
the clusters of missions of longer wave length radiation. Now
it could be this is where it takes our focus
to time scals in space time, not so much to
(15:10):
time curvature, but it takes our focus to time scals
space time and that within dying stars with these types
of galaxy galaxy clusters specifically can create strong gravitational ways
and ripples. Now, and we're speaking of a super massive object,
(15:40):
our secondary object being galaxy clusters, not orbiting, not within
the orbit or of our lower mass black hole. Now,
and what makes this hold a possibility now because with
these types of galaxies and their clusters and were irregular
(16:04):
but spiral, and different types of gravity, modified gravity being
within it. These calculations coming from schwartz Child radius in
our field equations regarding the mass of the black hole
(16:26):
that our own star now so and also this radius
and volume connects us to the modified gravity within the
within our galaxy clusters and the stars there. It tells
us a lot about age and the physics, the laws
(16:54):
of physics within these galaxies and where they come from.
It tells us about the collisions and what have changed
them because they would have met their own spotification through
explosions and colliding with one another. We're speaking of us
(17:18):
supermassive clusters here. There's much destruction. And that's where Monday
it came into. When we're first presenting this and laying
it on the table, it came into, Okay, that's well,
that's a lot of CRE's. You're creating a well, because
(17:42):
we're falling back into space time with this, that's creating
a lot of chaotic energy in the atmosphere. We are
well because we're coming from each direction, We're coming from
radiation gas, different types of gravity and different types of dust.
So that's that what our see constitute with space time
curvature time scales, which are different in space time itself
(18:13):
when you're when when it when the focus is the
electromagnetic field and talking about radiation here and the different
degrees and levels also calculated. Whoever, because we're talking about
custom Gaalley and different degrees of stars start ages here
in their collisions, we're talking about explosions. Our star is
(18:34):
quite clear because it's singularly now when we're talking about
the galaxy clustures, we're speaking of b is of years
of start death, we're speaking of bees of years of
(18:57):
time scales. We're speaking of different beings of years of
different space time quantums, laws of physics. So there's a
a lot here. So that's why d I there there's
(19:19):
a lot here with this objective and objective being narrow
white draft Star Replica Star two draws stars, a neutron star,
you know, not white drest store replica Star Neutron Star
two draws Stars. Okay, And and we knew this on
Monday because I mentioned volume, and I knew that there
(19:43):
was volume coming from somewhere, and that lets us know
that there were two massive objects amongst our own uh
black hole, A A soun type, and we're gonna talk
about that son type also, as I state, this will
(20:05):
be included in the end depth in depth scientific writings
of my work. Now we're gonna we're gonna talk about
that son type. Okay, a sun type, A type of
massive massive object that could be Son adjacent. A type
(20:37):
of massive object here that could be Son adjacent because
why well, because of its calculations being able to produce
material that falls back into space time. Mm hm. This
(21:01):
is all of this is also wild money when it
was let When it we uh introduced it and laid
it on the table here, the first thought that would
have came to mind would have been, well, we're talking
about uh, very chaotic environments, much destruction due to heat
and hot gas. There my structures radiation, gas, gravity, and dust.
(21:25):
As I mentioned yesterday, we're into magnetism because we know
that and it's not even magnetism because of this sposification
and because of the the lower mass black hole that
we're speaking of. In the weakening of it, we're at
its core core depletion. But lit you we with calculating
(21:47):
age in it telling about the laws of physics within
our star's environment and the laws of physicity terms the
potential to draw in are start not emitting any light,
but with the cluster galaxies that we're looking at, specifically here,
(22:13):
scattering of light is coming from these particles, this dust here,
the scattering of light of dying stars within these galaxies
and their potential due to the laws of physical laws
of nature of what they were. It brings space time
(22:39):
into play and the potential for creating strong gravitational wood
waves excuse me, and ripples and giving birth the new stars.
Also the potential for the birth of new stars. With
what we have laid on the table. When I'm saying
we are a meaning me, you know. But what we
have on the table is it's coming from a multitude
(23:05):
of ingredients. Accept it sap the energy that was released
and the material released from our own start, our own
dying star. It doesn't come from there. That's why we're talking.
We're speaking of gravity. They're different types of gravity. Why
(23:35):
this spotification in this specific event calculates as stretched out,
I have no idea. Now, let's let's talk about these
(23:56):
d dying stars a month. Because we're speaking of dying
stars within this cluster galaxy. But we're speaking of specific
dying stars amongst dying stars in the cluster galaxy. Now
in in the age and we we on money, we
spe we spoke about universe as we know obviously know
(24:20):
how to calculate that based on the the dying stars
potential the death radius volume. Now, so it's so we're
talking about high density with our own no infinite density.
(24:41):
So we're speaking of the start the core when we're
speaking about our own star, own black hole or lower
mass m mass loss through the through evaporation. So we're
(25:03):
speaking of core in the core, and that could account
the structure of our own what was a star. Okay,
the structure at its core could account well in the
(25:23):
spotification around it after the material that is thrown out
in the injury beliezers could account for the what's outside
of it that has been thrown out in the atmosphere
could account for the gravitational poel towards it. Because remember
(25:44):
speaking of different types of gravity, be modified gravity. Remember
we know that gravity is mass and density dependent, and
we would calculate the mass and in density of the
stars the sell to see what potential ho they hold
regarding the laws of physicis or what they were. What
(26:09):
would be left after explosion and their material being exploded
into the atmosphere along with gas and energy energy comes in.
How how how what we're speaking of when we with
the galaxy clusters when they draw close, because they have
(26:35):
strong gravitational waves and rifles even with even but also
with so that would be about they have the longer
wave of wavelength of radiation, also radiation meeting radiation. That's
where money. It was about the chaotic environment. It would
(26:55):
be different types of radiation because we're talking about speaking
of different time space times here lows of mobility and
we're speaking of it which we'll correspond to age and
beginning now, so that would be its see our own
(27:22):
HO cap C calculations with our own star. Now we
have to go into HO calculations with these stars within
these this custom galaxy, and that would let us know
the th P, the w potential meaning what they were
not potential, the significance of what they were and what
(27:44):
they hold in capability of potential. Now, after the material
is released through explosion, we tell a sup and over
dust also hearing, but different type of dusts. The dust
from type laps from our own star, the black hole.
(28:08):
It would be different from the dust supernova's explosions, dust
hear from these cause we're talk we're speaking of customs
of galaxies that are have a gravity had a gravitational
pool towards one another through bees of years. And we
can't just throw bes of years out there. We have
to get an exact calculation of of what years so
(28:30):
that we can cause did did what that information holds
d what was and what was holds what they were
in the ability capability, laws of physics, laws of gravity,
laws of continuum, space time, curvature, time scals, so within
(29:02):
the so let's we we have to separate dying stars
here within these cluster galaxies from other dying stars because well,
because there's a lot of this structure. I want to
go back to d to the swatch Child rad is
(29:25):
here with our own massive black hole and where and
what in the atmosphere around it, but it has foification there.
That radius is very important because it lets us know
what the what the perimeter is holding. Now we're circulating
within the atmosphere amongst it, and it lets us know
(29:48):
also how this primary massive object that is it's primary
because it's closer. We're talking about distance. We talked spoke
about distance yesterday. It's primary only because it's closer now.
But and then the secondary object, which is the massive,
(30:08):
which is the guidless becausure, its super massive guidless becausure,
is the primary as it relates to material, but still
with its gravitational pull towards this environment here and it
being gravitationally pulled there, it is change happens because there
(30:29):
it would meet a different type of spotification that will
align itself with the adjacent I don't know why it
comes out the calculations as son adjacent or adjacent, but
has the ingredients necessary to affect time curvature specifically, So
(31:00):
did these coming towards our massive our lord mass black
hole the guidance in questure they go through a different
type of regenerant constant but change. And I spoke about
(31:32):
speed of light on Monday, and I stated that it's
equivalent to close to the speed of light, not the
speed of light itself. Because we're telling about speed, we're
also talking speaking about distant. So there was this knowing
through the calculations that we were speaking about distant but
(31:53):
out of orbit distant and that's where our secondary comes in.
But secondary only because of distance. This is having to
be calculated obviously because we need exact because of the
space times that these galaxy clusters belong to and within
them stars and collisions and we're and and magnetizing towards
(32:18):
one another. We're talking about different types of gravity and
what they belong to in in individual clusters. So this
is this is a had significant ingredients and yesterday our
ended things. What this is where the information is here
(32:42):
and we know that we can pinpoint here galaxy clusters
separating dying stars from one another. Compuses about galaxy age,
the start age, excuse me, and that will bring in
the laws of physics of what was and potential as
it relates to the material and in type of energy
(33:06):
release and that is created different through collisions within the
godless and then where they came from within whatever universe is.
And the scattering of light, the scattered like being are
a very important ingredient. So that's an accomplishment cause remember
(33:32):
we're drawn in like we're drawing in material. That's an accomplishment.
Speaker 2 (33:44):
There, I id it.
Speaker 1 (33:58):
It's highly fast. How these different these different types of gravity.
Speaker 3 (34:03):
They aid in the day aid in the accounting for
a time curvature, a highly unique.
Speaker 1 (34:29):
Well phenomena would be occurring and highly unique phenomena regarding
replica star, neutron star, and two dr stars. Now we're
gonna speak about because a lot of information is here.
So this is where the this is where the calculation
take us one place to the next. This is talk
(34:50):
about the distinguishment amongst age, the age of dying stars
and where it takes us and that matter that is
thrown out into space, and it taken us towards the
neutron stars. It also taken us towards white dort stars,
(35:17):
which isn't surprising because we're speaking of galaxy closer to
that can and in collisions, and we're speaking of u
of material that we're gravitationally pulled magnetized towards one another.
That this is whe're getting the heavy duty magnetism and
(35:46):
and it's due to different reason beings. And it goes
back to the calculations of beginning and what these clusters
have passed through and pass within past past, within most
(36:11):
importantly or significantly through this gravitational pull and this magnetism
that slightly. That that slightly I don't know how to
(36:38):
state this, that that's because there is a duality here
that slightly plays a role in their space time continue
(36:59):
and plays a role in them falling back into space
time curvature or the reality there. So we know that
our the foundation of our framework wor we're dealing with radiation, gas, gravity,
dust with the galaxy club clusters in our calculations, we
(37:24):
now at magnetism and we're gonna have to figure the
degrees of magnetism and which of these dining stars have
d the d what is there for lack of a
better world capability towards drawing in towards them. That's why
(37:45):
it's it's separating the dining stars from one another, cause uh,
there's been like many of them are or or hold
a lot of lower energy gas. Man of them to
destroy through radiation also and and that means that they
(38:09):
they they don't hold the I and it would be
due to their beginning in which we have to be
calculated is the beginning, not any of the Y Y
universe now that they would belong to, and that would
be correspond with their fields that they will belong to
also is and then the introduction to fields that are
(38:33):
radia radioactive fields because no radiation and when you're speaking
of the galaxy customs such as this and these types
of explosions, is a high there. There's a lot of
radiation there. So it kind of kind of takes one
that those out of the game now. So is so
(38:57):
it taken us to neutrons start because remember we're dealing
with high radiation gas gravity, and that's so everybody would
have known from that that we're we're speaking about the
birth of new Star. Okay, and we're pulling towards it's
just obviously when you look at the see radiation, gas,
gravity and dust. Okay, that's the birth of new Star.
So and I'll stay that on Monday now and mentioned
(39:17):
it yesterday again, so now is it is? And then
we're speaking of the rigidity of replica star, Neutron star
or two draw stars and and why is that rigidity there? Well,
(39:38):
it's constrained, not rigidity, but there's a constraining. It is
becoming more constrained when we introduced now that we're onto
the galaxies, it's uh, the customer galaxies, and it's introduction.
It's now about the the constrained in it lining up
with white jaws with two draw stars replica star or nutrition.
(40:02):
It's like there's because now we're getting into the laws
of what the stars were governed by the potential of
what the particles hold out the explosion cosmic dust, they're
changed through spotification. There's changed well in the different in
(40:26):
the different types of gravity that they would be constrained
by laws of gravity, the tax of radiation that is
omitted coming from different space times, time scales, and also
(40:53):
the massive object that they would be introduced too. That
it's close to our start and it is son of Jakin,
and we'll have to do calculations that lets us know
why it is it is son of Jason and why
it is not the sign a son. The The beauty
(41:28):
of it all is the the where we get our
scattered scattering of light here m h.
Speaker 4 (41:47):
When we're speaking of particles, there's a part of light.
It's part of light.
Speaker 1 (42:03):
Okay, Well, we will continue and continue to see where
the math takes us until next time. Thanks for listening.
Bite
Hi everyone, and welcome back to the morning round. But
we are alive once again. It is Wednesday, September eighteenth.
Those of you that want to join in with me
on the chat, you're most definitely welcome to do. So.
Let's look at what we have on the table where
we left off Monday and Tuesday, and we're speaking of
lower mass black holes. Our star is what we're looking
(00:21):
at and leaving off with time curvature and two massive
objects in orbit, and yesterday be stating well, Monday me stating, well,
this massive object it will be greater than the Sun
now and it does not have to be orbiting, it
(00:46):
does not have to be within the orbit of this
star war that we're speaking of. Specifically, I spoke yesterday
about different types of gravity because it took us to
where the rate is took up what we focused on
our start now in our stars calculation, the radius taken
us to different types of gravity. We are using gravity, radiation,
(01:20):
gas and dust as our main ingredients. Well, the foundation
of our ingredients, our main ingredients as our statey as
of yesterday are it is the galaxy clusters most specifically,
and that's the second major secondary primary object cause we're
gonna get to the first primary object. Also this second
(01:42):
primary object that is not an orbit that is, but
it's taking place and taking a part of space and
place regarding bringing into our start, bringing back into the
core of our start. Our stated yesterday, this is where
all the information is. Most of the information is here,
and this is when we get in different types of gravity.
So we are speaking about modified gravity here. Now let's
(02:06):
look at this and talk about the information that is
coming from our galaxy clusters, and we're speaking of irregular
clusters accounting for the space time curvature, because remember it
bought us back to space time curvature. It brought us
back to the two massive objects, one being the Sun,
(02:28):
the other one being the galaxy clusters themselves. So in
accounting for that time curvature, and we'll getting to the
time curvature tomorrow or on Friday, But let's look at
this first here and why it is happening and the
ingredients that makes it so in us deciding based on
pulling into our star White Draft Star, Replica Star, Neutron Star,
(02:53):
and two draft stars, and what line stands up regarding
the ingredients are making that the problem ability of and
within the bounds of what can be drawn in now,
and we're gonna see why those were chosen as the
probability of what could be drawn into our lower mass
(03:13):
black hole into our star that we're focused on. Remember
their outcome probability probability Replica star, neutron star, two drawer stars. Now,
yesterday we talked about what the outcome probability of with
the super and nova type lass and that dust that
(03:34):
outcome probability of being white draw star. But let's get deeper,
because we haven't look at d or even beginning to
look at the galaxy customs themselves, and the dust and
the particles coming from that is where the light comes
from and the light scatter comes from. Because remember our
(03:55):
obviously with a with explosive stars such as are what
we're dealing where it will not be emitting any light.
So and but because we're dealing with spotification, also there's
a lot that's going on there that plays a role
in and that plays a role in this space curvature
because we're also looking at time scales that are quite
(04:17):
different and ages of the dying stars and how long
they've been in their death processes and what that makes
regarding what the star is emitting and what is being
thrown out into the atmosphere and what is being changed
through spotification and through the gravitational pull of this massive, secondary,
(04:44):
most massive object, even though it's the secondary, looking at
it the secondary object, what the potential that it holds
as it relates to time curature and what is being
about into our star And we'll look at that also.
So let's look at this we're talking about. We're speaking
of regular galaxies, and you all understand why irregular galaxies
we're speaking on spouse most specifically within irregular galaxies now
(05:08):
containing a lot of gas and dust, because that's what
our primary structural focus is structure, the structural focused radiation, gas, gravity, dust.
We're gonna talk about magnetism also when we get to
that now. So I want to back back with our supernova,
with our particle collision regarding our start self now and
(05:31):
it being laxed in the type of dust and we
did our aging with our own specific star and the
type of dust material and energy that it emits now,
So is it in that particle collision that is separate
in amongst itself because when we're talking about age stars now,
(05:55):
and in dying stars, they are under a different law
of physics regarding their age and where they are positioned
within the within space. So that does of those supernovas
contain a different age, a different space time continuum, and
(06:15):
different laws of physics, meaning different potentials of what they
can do as it relates to us pulling in. And
you have to remember that within these explosions, because that's
where we're speaking of space. Explosions start explosion, and within
these collisions and colliding with what is external to it
(06:38):
within space, that material, that energy, that the type of
energy release, and we're talking about radiation and those collisions
and what they create, but also spoification because remember we
know that the tidal forces of lower mass black black
holes are very strong, so they have very strong tidal
(06:58):
forces in that spotification and creating a bending. But through
our calculations we see that it's not a bending per se.
It's a straight line. And we from Monday, when I
first laid everything out on the table, I know the
first doubts were like, Okay, this creates the chaos and
not the stated Well, well, it depends. It depends on
(07:22):
what their ingredients are and where they're coming from with
this space, you know, and whether the the chaos it
creates a very chaotic environment, whether the chaos is diminished
through what the particles pass through as they're circulating in space,
what they lose. So we know a lot of mass
is loss through these types of there's more mass loss
(07:46):
and through these types of evaporate evaporations and explosions and
through what they colloud with, so there's more mass loss.
So there is a minimizing due to the mass loss
of the chaos that one will proposed, that superposed that
that they will create. Now, so we're going back over
here and and looking at this these different this different
(08:10):
type of gravity because as I stated in the end
of of yesterday's presentation that the cluster galaxies is where
all the information is held now and the explosions there
to dyeing stars within those galaxies also, and the where
in our yesterday we were talking about supermassive supermassive object
(08:36):
in orbit of these supermassive will have to be calculated,
and we're gonna s talk about why that calculation will
will disperse the type of material and why those calculation
outcomes will disperse the type of material and energy and
also corresponds with modified gravity and it pulling into the
(09:00):
direction even though it is not within the orbit of
our star, of our black hole. And when we're the
pulling end, because remember with our star that the the
is we get, the gravitational pull is we get, but
(09:22):
we're drawing back into the core. So now we know
that irregular galaxies contain a lot of gas and dust.
Now the type of gas and dust, the type of
dust most specifically with this project, would be the most
(09:45):
significant because what do we gather from dust? We're speaking
about cosmic dust, dust particles. We gather the age the
beginning or as is it close to the beginning of
the universe in which it sits, and that is determined
by calculations of the dust itself, the particles within the dust,
(10:10):
and that lets us know the laws of physics pertaining
to the specific dying stars that we're looking at within
the the in the cluster galaxies. Because we're looking at
the dying stars within the cluster galaxies, we're looking at
material change material but material so now so, and we
(10:35):
know that we're looking at that because it leads to
the birth of new stars. And we're pulling into our
black hole into our star. So we're speaking about this
super massive galaxy cluster. You may have already done your
calculations on the masterly of it because we spoke about volume.
I spoke about volume on Monday and the importance of volume.
(11:04):
So that the the the cosmic d the dust of
these we already have the dust from the type that
soup and over regarding our own starring particle collision. Spogification
emits its own dust when when when different types of
material collide with this space orbiting around the black hole.
(11:30):
Now so is so we're we're speaking of the dust
from our dying stars within the cluster galaxies. That's that's
what we're focused on within the galaxies because they account
this type of gravity, cause we're speaking about modified gravity,
different types of gravity. As I stated yesterday, this this
(11:51):
type of gravity and the irregular clusters that we're dealing with,
and the rate is regardless. Spogification and we calculate it
being stretched out is what also accounts for a time curvature.
It accounts for time curvature here, but time curatures also
(12:12):
accounted for around our black hole and this spotification that
is going through regarding the material that is thrown out
through the explosion and the spotification that it's gone through
with the material that was released, and we talked about
that on Monday, material being released, and we calculate material
release by the age of the star and by what,
(12:38):
and that lets us know the potential of what. The
start the potential of what lets us know the direct
capability of the star regarding physics, and it also lets
us lets us know the potential of new capability because
we're talking about we're speaking about the birth of new stars,
(12:59):
but through spot vacation the new potential. Okay, now, so
that's that on is on that dust Lanel part while
we focus on this dust from our galaxies and the
DIN starts here now accounting more here with our supercluster,
(13:22):
accounting more here for space time curvature. But also this
is where time scales come into play now and time
scales coming into play because the calculation of the volume
(13:42):
volume calculation were we with the with the radius calculation,
we're speaking of schwatsh Our radius because we're speaking of
field equations. Because we remember, we're dealing with radiation and
we're talking about the radiation fil we're dealing with radiation
(14:06):
just all over the place is what this is radiation, gas,
gravity and dust. And remember we're talking about white draft star,
Revelu star, neutron star, or two draft stars. Now we're
gonna get into where two draft stars come into play.
We already yesterday got into where the white draft came
(14:27):
into play. Now with the with the type last dust
and the calculations brought to white draft star. Now, so
now we're gonna get into where neutron star could come
into the play. It come into play, excuse me, so
with our cosmic dust it's bringing it brings our focus
(14:49):
towards the dying stars now in the in the in
the clusters of missions of longer wave length radiation. Now
it could be this is where it takes our focus
to time scals in space time, not so much to
(15:10):
time curvature, but it takes our focus to time scals
space time and that within dying stars with these types
of galaxy galaxy clusters specifically can create strong gravitational ways
and ripples. Now, and we're speaking of a super massive object,
(15:40):
our secondary object being galaxy clusters, not orbiting, not within
the orbit or of our lower mass black hole. Now,
and what makes this hold a possibility now because with
these types of galaxies and their clusters and were irregular
(16:04):
but spiral, and different types of gravity, modified gravity being
within it. These calculations coming from schwartz Child radius in
our field equations regarding the mass of the black hole
(16:26):
that our own star now so and also this radius
and volume connects us to the modified gravity within the
within our galaxy clusters and the stars there. It tells
us a lot about age and the physics, the laws
(16:54):
of physics within these galaxies and where they come from.
It tells us about the collisions and what have changed
them because they would have met their own spotification through
explosions and colliding with one another. We're speaking of us
(17:18):
supermassive clusters here. There's much destruction. And that's where Monday
it came into. When we're first presenting this and laying
it on the table, it came into, Okay, that's well,
that's a lot of CRE's. You're creating a well, because
(17:42):
we're falling back into space time with this, that's creating
a lot of chaotic energy in the atmosphere. We are
well because we're coming from each direction, We're coming from
radiation gas, different types of gravity and different types of dust.
So that's that what our see constitute with space time
curvature time scales, which are different in space time itself
(18:13):
when you're when when it when the focus is the
electromagnetic field and talking about radiation here and the different
degrees and levels also calculated. Whoever, because we're talking about
custom Gaalley and different degrees of stars start ages here
in their collisions, we're talking about explosions. Our star is
(18:34):
quite clear because it's singularly now when we're talking about
the galaxy clustures, we're speaking of b is of years
of start death, we're speaking of bees of years of
(18:57):
time scales. We're speaking of different beings of years of
different space time quantums, laws of physics. So there's a
a lot here. So that's why d I there there's
(19:19):
a lot here with this objective and objective being narrow
white draft Star Replica Star two draws stars, a neutron star,
you know, not white drest store replica Star Neutron Star
two draws Stars. Okay, And and we knew this on
Monday because I mentioned volume, and I knew that there
(19:43):
was volume coming from somewhere, and that lets us know
that there were two massive objects amongst our own uh
black hole, A A soun type, and we're gonna talk
about that son type also, as I state, this will
(20:05):
be included in the end depth in depth scientific writings
of my work. Now we're gonna we're gonna talk about
that son type. Okay, a sun type, A type of
massive massive object that could be Son adjacent. A type
(20:37):
of massive object here that could be Son adjacent because
why well, because of its calculations being able to produce
material that falls back into space time. Mm hm. This
(21:01):
is all of this is also wild money when it
was let When it we uh introduced it and laid
it on the table here, the first thought that would
have came to mind would have been, well, we're talking
about uh, very chaotic environments, much destruction due to heat
and hot gas. There my structures radiation, gas, gravity, and dust.
(21:25):
As I mentioned yesterday, we're into magnetism because we know
that and it's not even magnetism because of this sposification
and because of the the lower mass black hole that
we're speaking of. In the weakening of it, we're at
its core core depletion. But lit you we with calculating
(21:47):
age in it telling about the laws of physics within
our star's environment and the laws of physicity terms the
potential to draw in are start not emitting any light,
but with the cluster galaxies that we're looking at, specifically here,
(22:13):
scattering of light is coming from these particles, this dust here,
the scattering of light of dying stars within these galaxies
and their potential due to the laws of physical laws
of nature of what they were. It brings space time
(22:39):
into play and the potential for creating strong gravitational wood
waves excuse me, and ripples and giving birth the new stars.
Also the potential for the birth of new stars. With
what we have laid on the table. When I'm saying
we are a meaning me, you know. But what we
have on the table is it's coming from a multitude
(23:05):
of ingredients. Accept it sap the energy that was released
and the material released from our own start, our own
dying star. It doesn't come from there. That's why we're talking.
We're speaking of gravity. They're different types of gravity. Why
(23:35):
this spotification in this specific event calculates as stretched out,
I have no idea. Now, let's let's talk about these
(23:56):
d dying stars a month. Because we're speaking of dying
stars within this cluster galaxy. But we're speaking of specific
dying stars amongst dying stars in the cluster galaxy. Now
in in the age and we we on money, we
spe we spoke about universe as we know obviously know
(24:20):
how to calculate that based on the the dying stars
potential the death radius volume. Now, so it's so we're
talking about high density with our own no infinite density.
(24:41):
So we're speaking of the start the core when we're
speaking about our own star, own black hole or lower
mass m mass loss through the through evaporation. So we're
(25:03):
speaking of core in the core, and that could account
the structure of our own what was a star. Okay,
the structure at its core could account well in the
(25:23):
spotification around it after the material that is thrown out
in the injury beliezers could account for the what's outside
of it that has been thrown out in the atmosphere
could account for the gravitational poel towards it. Because remember
(25:44):
speaking of different types of gravity, be modified gravity. Remember
we know that gravity is mass and density dependent, and
we would calculate the mass and in density of the
stars the sell to see what potential ho they hold
regarding the laws of physicis or what they were. What
(26:09):
would be left after explosion and their material being exploded
into the atmosphere along with gas and energy energy comes in.
How how how what we're speaking of when we with
the galaxy clusters when they draw close, because they have
(26:35):
strong gravitational waves and rifles even with even but also
with so that would be about they have the longer
wave of wavelength of radiation, also radiation meeting radiation. That's
where money. It was about the chaotic environment. It would
(26:55):
be different types of radiation because we're talking about speaking
of different time space times here lows of mobility and
we're speaking of it which we'll correspond to age and
beginning now, so that would be its see our own
(27:22):
HO cap C calculations with our own star. Now we
have to go into HO calculations with these stars within
these this custom galaxy, and that would let us know
the th P, the w potential meaning what they were
not potential, the significance of what they were and what
(27:44):
they hold in capability of potential. Now, after the material
is released through explosion, we tell a sup and over
dust also hearing, but different type of dusts. The dust
from type laps from our own star, the black hole.
(28:08):
It would be different from the dust supernova's explosions, dust
hear from these cause we're talk we're speaking of customs
of galaxies that are have a gravity had a gravitational
pool towards one another through bees of years. And we
can't just throw bes of years out there. We have
to get an exact calculation of of what years so
(28:30):
that we can cause did did what that information holds
d what was and what was holds what they were
in the ability capability, laws of physics, laws of gravity,
laws of continuum, space time, curvature, time scals, so within
(29:02):
the so let's we we have to separate dying stars
here within these cluster galaxies from other dying stars because well,
because there's a lot of this structure. I want to
go back to d to the swatch Child rad is
(29:25):
here with our own massive black hole and where and
what in the atmosphere around it, but it has foification there.
That radius is very important because it lets us know
what the what the perimeter is holding. Now we're circulating
within the atmosphere amongst it, and it lets us know
(29:48):
also how this primary massive object that is it's primary
because it's closer. We're talking about distance. We talked spoke
about distance yesterday. It's primary only because it's closer now.
But and then the secondary object, which is the massive,
(30:08):
which is the guidless becausure, its super massive guidless becausure,
is the primary as it relates to material, but still
with its gravitational pull towards this environment here and it
being gravitationally pulled there, it is change happens because there
(30:29):
it would meet a different type of spotification that will
align itself with the adjacent I don't know why it
comes out the calculations as son adjacent or adjacent, but
has the ingredients necessary to affect time curvature specifically, So
(31:00):
did these coming towards our massive our lord mass black
hole the guidance in questure they go through a different
type of regenerant constant but change. And I spoke about
(31:32):
speed of light on Monday, and I stated that it's
equivalent to close to the speed of light, not the
speed of light itself. Because we're telling about speed, we're
also talking speaking about distant. So there was this knowing
through the calculations that we were speaking about distant but
(31:53):
out of orbit distant and that's where our secondary comes in.
But secondary only because of distance. This is having to
be calculated obviously because we need exact because of the
space times that these galaxy clusters belong to and within
them stars and collisions and we're and and magnetizing towards
(32:18):
one another. We're talking about different types of gravity and
what they belong to in in individual clusters. So this
is this is a had significant ingredients and yesterday our
ended things. What this is where the information is here
(32:42):
and we know that we can pinpoint here galaxy clusters
separating dying stars from one another. Compuses about galaxy age,
the start age, excuse me, and that will bring in
the laws of physics of what was and potential as
it relates to the material and in type of energy
(33:06):
release and that is created different through collisions within the
godless and then where they came from within whatever universe is.
And the scattering of light, the scattered like being are
a very important ingredient. So that's an accomplishment cause remember
(33:32):
we're drawn in like we're drawing in material. That's an accomplishment.
Speaker 2 (33:44):
There, I id it.
Speaker 1 (33:58):
It's highly fast. How these different these different types of gravity.
Speaker 3 (34:03):
They aid in the day aid in the accounting for
a time curvature, a highly unique.
Speaker 1 (34:29):
Well phenomena would be occurring and highly unique phenomena regarding
replica star, neutron star, and two dr stars. Now we're
gonna speak about because a lot of information is here.
So this is where the this is where the calculation
take us one place to the next. This is talk
(34:50):
about the distinguishment amongst age, the age of dying stars
and where it takes us and that matter that is
thrown out into space, and it taken us towards the
neutron stars. It also taken us towards white dort stars,
(35:17):
which isn't surprising because we're speaking of galaxy closer to
that can and in collisions, and we're speaking of u
of material that we're gravitationally pulled magnetized towards one another.
That this is whe're getting the heavy duty magnetism and
(35:46):
and it's due to different reason beings. And it goes
back to the calculations of beginning and what these clusters
have passed through and pass within past past, within most
(36:11):
importantly or significantly through this gravitational pull and this magnetism
that slightly. That that slightly I don't know how to
(36:38):
state this, that that's because there is a duality here
that slightly plays a role in their space time continue
(36:59):
and plays a role in them falling back into space
time curvature or the reality there. So we know that
our the foundation of our framework wor we're dealing with radiation, gas, gravity,
dust with the galaxy club clusters in our calculations, we
(37:24):
now at magnetism and we're gonna have to figure the
degrees of magnetism and which of these dining stars have
d the d what is there for lack of a
better world capability towards drawing in towards them. That's why
(37:45):
it's it's separating the dining stars from one another, cause uh,
there's been like many of them are or or hold
a lot of lower energy gas. Man of them to
destroy through radiation also and and that means that they
(38:09):
they they don't hold the I and it would be
due to their beginning in which we have to be
calculated is the beginning, not any of the Y Y
universe now that they would belong to, and that would
be correspond with their fields that they will belong to
also is and then the introduction to fields that are
(38:33):
radia radioactive fields because no radiation and when you're speaking
of the galaxy customs such as this and these types
of explosions, is a high there. There's a lot of
radiation there. So it kind of kind of takes one
that those out of the game now. So is so
(38:57):
it taken us to neutrons start because remember we're dealing
with high radiation gas gravity, and that's so everybody would
have known from that that we're we're speaking about the
birth of new Star. Okay, and we're pulling towards it's
just obviously when you look at the see radiation, gas,
gravity and dust. Okay, that's the birth of new Star.
So and I'll stay that on Monday now and mentioned
(39:17):
it yesterday again, so now is it is? And then
we're speaking of the rigidity of replica star, Neutron star
or two draw stars and and why is that rigidity there? Well,
(39:38):
it's constrained, not rigidity, but there's a constraining. It is
becoming more constrained when we introduced now that we're onto
the galaxies, it's uh, the customer galaxies, and it's introduction.
It's now about the the constrained in it lining up
with white jaws with two draw stars replica star or nutrition.
(40:02):
It's like there's because now we're getting into the laws
of what the stars were governed by the potential of
what the particles hold out the explosion cosmic dust, they're
changed through spotification. There's changed well in the different in
(40:26):
the different types of gravity that they would be constrained
by laws of gravity, the tax of radiation that is
omitted coming from different space times, time scales, and also
(40:53):
the massive object that they would be introduced too. That
it's close to our start and it is son of Jakin,
and we'll have to do calculations that lets us know
why it is it is son of Jason and why
it is not the sign a son. The The beauty
(41:28):
of it all is the the where we get our
scattered scattering of light here m h.
Speaker 4 (41:47):
When we're speaking of particles, there's a part of light.
It's part of light.
Speaker 1 (42:03):
Okay, Well, we will continue and continue to see where
the math takes us until next time. Thanks for listening.
Bite
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