Become a supporter of this podcast: https://www.spreaker.com/podcast/the-morning-ramble--3016702/support.
Mark as Played
Transcript
Episode Transcript
Available transcripts are automatically generated. Complete accuracy is not guaranteed.
Speaker 1 (00:00):
However, wan and welcome back to the morning. Remember we
alive once again. Today is Thursday, September nineteenth. Let's see
what we have laying on the table where the calculations
have taken us some very interesting stuff. Now, I a
most definitely be highlighting it in my writing that you
all can expect. We we left I wanna go back
(00:23):
here where we left off, cause this is the most
important part, what one of them, all.
Speaker 2 (00:29):
Of it is highly important.
Speaker 1 (00:30):
Remember where we are, uh, our our foundational ingredients radiation, gas, gravity,
dust in the introduction of magnetism yesterday. So doy's the
foundation of our primary structural is what we'll call it,
(00:56):
what our ingredients will sit upon, and.
Speaker 2 (00:58):
What's the driving for words behind them? Now?
Speaker 1 (01:02):
And we we turned to focus onto the secondary massive
object that is not in orbit of our of our
star now and I stated that this is where the
information is it. It is a heap of information here,
(01:23):
uh uh, loads of information, very telling. So let's go
ahead and pick up cause I wanna focus now on
We're gonna leave that b.
Speaker 2 (01:32):
But we know that we're dealing with.
Speaker 1 (01:34):
A modified gravity, meaning different types of gravity, and we
have the radiation coming from a m a month to
the places were already gonna over that regarding our own
little mass black star and the radiation there also the
(01:55):
radiation from the explosions within our secondary massive object, which
it is is secondary because of distance, because remember it
is not in the same orbit of the primary. The
primary yet to be identified. But we're gonna get to
talk about that and this identification and will maybe we'll
(02:16):
speak about its identification tomorrow be cause, but the attention
brings us here, the calculations actually bringing us here, and
it being our primary focus now, the primary focus going
towards it and identifying it. Now, let's see what the
information coming from our clusters.
Speaker 2 (02:38):
Very telling.
Speaker 1 (02:39):
Now let's start with the rate is cause this popification
is very important with us focused on the time curvature
and the different directions that this time curature is coming from,
which makes it.
Speaker 2 (02:55):
With which takes the thought back to when our presented
this on Monday of this is a lot of a
lot of chaos, you know, and it just creates chaos.
Speaker 1 (03:09):
And I stated that, well, the chaos can be minimized
based on what the particles will encounter as they are
ejected released into the atmosphere. Now and we're dealing with
types of gravity coming from multily direction but modified gravities
that are going through a multul change, especially with our
(03:31):
with our cluster galaxies and the stars that we're using
there in their explosions in that material and what it
encounters in orbit around where these explosions happen, what the
materials encounter, and what makes of the new material because
remember we're drawing in and we have the gravitational force
to gravitational pull from multile the rerection.
Speaker 2 (03:52):
For that to happen.
Speaker 1 (03:53):
Now, So now even though our own the star is
obviously weakened, but it with the of force around it,
is able.
Speaker 2 (04:02):
To neutralize itself.
Speaker 1 (04:09):
In a way that it still connects itself with this
core and can pull in the particles that would be
necessary to help us come to our conclusion of replica star,
neutron star, or two drawstars. And I know Monday, when
I introduced this, it was that two drawtstars was like
(04:31):
a question mark of how would that come to pass,
what calculations would make that and necessarid, well, that's what
we're gonna be speaking of today. Case last night calculations
brought that up as one of the conclusions we already
had where Monday when I introduced this, and I stayd well,
we would be dealing with because of the radiation, the
(04:53):
type of radiation that we're dealing with or dealing with
type different types of radiation that you all will know,
the different types of gases that we're dealing with. And
we've done the calculation for our radiation and gases and
the different types of gravity we went into our modified gravity.
What on Tuesday when I stayed there will be different
types of gravity and the dusts from our supernova our
explosions with the supernovas are coming from different different space times.
(05:19):
So and that's just the dust the particles that were
needed cause we're needed because we're bringing.
Speaker 2 (05:23):
Into our star now.
Speaker 1 (05:26):
Okay, So so don's where Monday even knowing when I presented,
is that we're speaking of what type of star?
Speaker 2 (05:37):
What would this bringing into?
Speaker 1 (05:39):
What would it make Replica star, Neutron star or two
door stars.
Speaker 2 (05:43):
Now we the Neutron star, we've.
Speaker 1 (05:47):
Had what we've had d with the calculations. I feel
that I think that it was from yesterday or was
it from Tuesday where it showed up why r Door
star White Door star would be a a potential based
(06:10):
on the ingredients and the calculations that are being used.
Speaker 2 (06:14):
Okay, so now, but that Y, we had not introduced
yet our.
Speaker 1 (06:19):
Massive object, our primary massive object. And I call it
this well, our secondary massive object. So I call it
this secondary massive object, as I stated Y, due to
distance and then and then I I I called the
primary massive object the primary massive object due to its
distance and it being closer in in the in the
(06:42):
gravity it well, it being it being closer to our
start to our black hole. So that's what I'm meaning
when I'm saying primary massive object, secondary massive object. Now
let's go cause w W, let's go over here. Last
night takes us to the spotification and we're we used
(07:07):
the swatch our rats because and also we use the
field equations now because and it shows a type of
time curvature.
Speaker 2 (07:22):
And the surprising part is that we're.
Speaker 1 (07:25):
Dealing with different time curvatures come from different space times.
Now regarding the material ages of the stars and the
material that they present into the atmosphere during these explosions,
(07:49):
and what these material meets and where speaking of spoglifications
specifically here, So it takes us here to.
Speaker 2 (07:58):
Back to looking at the the the.
Speaker 1 (08:01):
Radius calculations last night. It puts our focus on this
spotification now and in the age of our star and
the mass calculations which.
Speaker 2 (08:16):
We spoke about yesterday.
Speaker 1 (08:18):
And it it caused us to look at our start again.
Speaker 2 (08:23):
And this spocification.
Speaker 1 (08:31):
Now here is where because remember when we s when
these when with with the introduction of our our secondary
massive object, the introduction of those particles in the atmosphere
meeting gravitation of being poor towards the primary massive object
(08:52):
that is yet to be identified, is when the the
instability happens.
Speaker 2 (08:57):
Is when what one can and E spat.
Speaker 1 (09:03):
From the first introduction of the work or Monday, what
was my was Marvel calls, Okay, this is uh a
lot of chaotic energy within the within the environment. So
is so calculating the This is where the instability is encountered.
Speaker 2 (09:21):
Here is in the in the the rate of instability.
It takes us into a paradox.
Speaker 1 (09:31):
Because remember we spoke about the the speed being close
to the speed of lights and I mentioned slicing on Tuesday,
and I mentioned time dilations on Tuesday because of the gravity,
the gravitational pull of the particles, and we're speaking of
(09:54):
the the particles, the energy releasing the particles from our
start from the the the the lower massed black hole.
Because we when the massive object which is the the
the secondary massive object, which are the clusters.
Speaker 2 (10:12):
When that when those particles meet and and are.
Speaker 1 (10:17):
Gravitationally pulled into the field, cause remember they're out of
they're not in the same orbit the there the secondary
massive object is not in the same object in the
same orbit as the primary. When they meet, it creates
This is the first introduction of the instability, and it
(10:39):
takes us into a a a paradox, and that's what
the slicing that I introduced on Tuesday happens. It takes place,
and that causes us to focus our attention to.
Speaker 2 (10:59):
To the stars.
Speaker 1 (11:03):
This would be the initial introduction of time curvature outside
of the gravitational field of the of the secondary massive
objects which are our customers, and outside of the primary
massive object which is yet to be identified, but it's
(11:24):
closer to our lower mass black.
Speaker 2 (11:26):
Hole to our start. So we have what was what
does that mean?
Speaker 1 (11:30):
Where we have time curvature coming from three primary directions.
Speaker 2 (11:40):
And that's big die is very significant.
Speaker 1 (12:01):
Because our unidentified well yet to be identified primary massive
object is closer. That's close to our lower mass black
star accounts for time curvature.
Speaker 2 (12:16):
Even though within its radius.
Speaker 1 (12:19):
Weaker gravity is encountered. Okay, bg GU. We have a
lot going on that we have spotification going on.
Speaker 2 (12:26):
So it is that's where the I.
Speaker 1 (12:30):
Not instability, that's where there the chaos that one would
expect when this was first introduced is encountered, and there's
something that will have to be identified amongst the material.
Speaker 2 (12:53):
But t W between our star.
Speaker 1 (12:57):
And the primary massive object that's in this orbit, they're
close together, their distance is closer than our custers are.
There's something in between our lower mass black hole and
this primary massive object that they're in the same rate,
(13:23):
they're in the same ratus, or the distance is closer
than it is for our secondary our customs, but there's
something that needs to be identified between the two.
Speaker 2 (13:43):
There's some type of.
Speaker 1 (13:47):
Energy combination, radiation combination, gas combination, particle combination that has
been created from the material that has been released in
the energy that has been released from our exposure of
our own star and this spotification what it.
Speaker 2 (14:07):
Was meant with, there's a something that has.
Speaker 1 (14:12):
Been id, some something that has been something that is
to be encountered there as the as the particles are
pulled towards the the the our start. And we'll have
to look at those calculations that night to see what
(14:34):
it is. And it's gonna be easy to see what
it is. Why would it be easy to see what
it is?
Speaker 2 (14:40):
Well, because of the slicing that has been introduced.
Speaker 1 (14:48):
And the two dark star theory that was introduced on Monday,
and what they will consist of what their particle composition
would be, and that can give a that's an idea of.
Speaker 2 (15:01):
What would be between.
Speaker 1 (15:04):
What infusion is between some like a particle infusion something
unidentified here that is also accountable for a type of
accountable for a type of space curvature. But it's between
our primary massive object and.
Speaker 2 (15:24):
Between our start what was and what is to be
our start and and we also have yet to look.
But in this tape, this puts our.
Speaker 1 (15:39):
Attention on our primary massive object that's close to our star,
because it puts on us our tension. They're on identifying
and identifying what this massive object is and I and
I stated that it is Sun similar and identifying it
(16:00):
is important here at this point because the identification shows
the capacity. It shows the capacity because now we're speaking
about time, we're speaking about space time, space time curvature,
we're also speaking about time scales, and we're also speaking
about dilations.
Speaker 2 (16:17):
Here time dilations, and.
Speaker 1 (16:20):
They're all very distinct because of the type of radiation, gas, gravity.
Speaker 2 (16:25):
And dust particles we're speaking of.
Speaker 1 (16:33):
So their tension puts on it identifying of what this
primary object is and what is what the spotification has
created between the two that the massive that the cluster
galaxies with particles will encounter.
Speaker 2 (16:52):
And go through a then different type of spotification.
Speaker 1 (16:59):
As it's pull it towards, as those particles are put
towards our.
Speaker 2 (17:03):
Our lower mass black hole.
Speaker 1 (17:11):
Even with the radar instability, it it takes our attention.
Speaker 2 (17:17):
It puts our attention on the time dilations.
Speaker 1 (17:25):
In it creating that instability, It creating that well, the
instability would be the time dilations. It creating a type
of uh of a a K chaotic.
Speaker 2 (17:36):
But not a really radical response.
Speaker 1 (17:38):
The radical response is encountered as the particles are drawn
gravitationally pulled towards magnetized now at this point magnetized towards
the massive object that is close to our star is
where the the kind of a er er erradic response
(17:58):
U T to D is spoglification is.
Speaker 2 (18:02):
Wor didn account for the radic response.
Speaker 1 (18:09):
Because remember I've stated already on I think it was
on Tuesday, Monday or Tuesday, I talked about the quantum
fluctuations that were regardless spogification, that is near the atmosphere
of our primary massive object, and that's where everybody.
Speaker 2 (18:30):
That spent it. When I first introduced this on Monday, Okay.
Speaker 1 (18:33):
This was j This is creating ako the atmosphere, and
it sure is, but this was when.
Speaker 2 (18:37):
The chaos is encountered. But the chaos is also minimized.
Speaker 1 (18:41):
Because with the because the rate of instability could be
calculated with the encountering of well, with the initial encountering
of the of the particles and our.
Speaker 2 (19:00):
Of our black star.
Speaker 1 (19:01):
And the the clusters here, it's like initially there's a
A A A the the rate of instability. That's when
we have the time dilations, and that's encountered. And while
the the time dilations encountered here well, because remember we
stated that the injections of s, the the injection of
(19:21):
certain stars within these explosives of our cluster galaxies would
not be usable material, but those that are still b
but those the material that is still accountable for the
scattering of lights is where that material that is thrown
(19:43):
out into the atmosphere was thrown out into the atmosphere
at at after these it this explosion within these clusters
for these stars, the account encountering of material from our
own low mass black star is where the instability state
takes place, and that's where we'll have the time dilations there.
(20:03):
And when the time dilations, that's what we're looking at,
things like well w based on our ho calculations of
the age of our own own star. In this material,
it would we would look at things like what one
would look at as time travel wa not even time travel,
it would be the experience of.
Speaker 2 (20:27):
Multi dimensional space.
Speaker 1 (20:30):
At calculated giving points within time. Because when where we
are focused on, as I stated yesterday, as of yesterday,
focus on the laws of physics that govern these stars
and in their explosions, in the laws of physics that
govern their explosions, based on the bids of years that
(20:51):
they've been in the process of exploding of dying. So
we're speaking of the potential that I stated of their capability.
Speaker 2 (20:58):
Well, we're not in the potential that capability, but their actual.
Speaker 1 (21:01):
Capabilities when they were stars and the potential that it
still holds after the explosions with it, the potential that
holds within some stars after the explosions, and the material
being released in the atmosphere, and what the Spokul occasion
can create, as.
Speaker 2 (21:15):
It relates to its is is adding into the creation
of new stars and the material necessary for that to happen.
So we we know that we will be looking.
Speaker 1 (21:35):
At material, that is, particles that are have gone through
U processes based on their environment. With the addition of
the ingredients of what creates it gives birth to new stars.
(22:02):
And that's why our outcome as of Monday when this
was introduced Replica Star, Neutron Star two dark Stars.
Speaker 2 (22:08):
As of yet we do not know.
Speaker 1 (22:10):
I obviously that would be in my writing when I
put all this together with the calculations in the final.
Speaker 2 (22:18):
Completion.
Speaker 1 (22:23):
So is, and because when we look at time caricature
also in the fascination of it, our our modified gravity
also accounts for the time curvature. We have our unidentified
well yet to be identified, primary massive object that's close
to our lower massive blackness, the.
Speaker 2 (22:40):
Whole account of a ta R account of time curvature.
Speaker 1 (22:43):
Also, even though we h it has a w.
Speaker 2 (22:47):
I, there the the weak of gravity as.
Speaker 1 (22:48):
An encounter, but that would be a necessary ingredient. And
we have something that even even with its unidentified spotification
that has happened between the two between our lower mass.
Speaker 2 (22:59):
Black hole and the in the.
Speaker 1 (23:00):
The unidentified object that is within its orbit. It it's
creation can create a a a very erratic atmosphere as
it's pulling, as the gravitational pull and the mandatory towards
our black hole is happening, it will create a very chaotic, erratic,
(23:23):
but necessary change. And why would that chaotic erratic be encountered. Well,
because we're talking about space time now and we're talking
about we're speaking of of different It's because we're speaking
of these custom galaxies, primarily him, and we're we're speaking
of different time scals, different time dilations, different laws of
(23:47):
physics that govern the age and the aging of the
stars and their beginnings and what they were consistent w
what they consist of, what their particles consist of from
the beginning, and that's what's accounting for the time their
(24:09):
time curvature of all of that is accounting for the
time curvature the.
Speaker 2 (24:13):
I it's it it it could be experienced with time. Obnestly,
it would be experienced.
Speaker 1 (24:19):
With the with the the time it would be the
time would be slowed down. But it would also uh
s a celerate time.
Speaker 2 (24:27):
Now this is acceleration of time.
Speaker 1 (24:28):
It create it accounts for the erratic energy also because
of their encountering the unidentified whatever is between that has
been created by this spotification between our black hole and
our primary object that is in its orbit during the
same orbit.
Speaker 2 (24:48):
So time would be experienced quite k quite well.
Speaker 1 (25:01):
That would be a W that would be account for
the for the time being experienced as m the multi
dimensional experiencing of time, as opposed to where that could
account for a type UH that is in itself a
type of time travel.
Speaker 2 (25:16):
I Y is where.
Speaker 1 (25:30):
Where that T where that type of erratic composition.
Speaker 2 (25:35):
Is necessary for the output of.
Speaker 1 (25:37):
Two dog star repelical start a neutron star, But which
would it be. What we spoke about today focused on
the two door stars, but yesterday we talked about the
introdutional neutron star and what focused on that. This combination
of what we have laying on the table and then
(25:58):
tools that we spoke about the white door star right,
the output of the ingredients unknown and and why would
(26:22):
we still unknown what? Because we have our massive object,
our primary massive object that's in that's not at their
furthest distance and distance have distance hasn't has already been
calculated of our massive object is in this unidentified in
whatever is between that the spotification has already created and
what the particles will be encountering as they come towards.
Speaker 2 (26:46):
Our start.
Speaker 1 (27:01):
Because remember with our the clusters is the longer wavelength
of radiation emissions in that B which I all of
this aids in.
Speaker 2 (27:12):
The the gravitational pull behind. But why is the gravity
of peach.
Speaker 1 (27:16):
Why is the gravitational pool behind the particles?
Speaker 2 (27:20):
Why is it behind as opposed to the particles being
pulled forward?
Speaker 1 (27:26):
Well, we'll know that wants well it it It could
be because of the modified gravity that we're using that
would occur in c in these types of cluster galaxy,
and we're talking we're speaking of irregular clusters and the
the weakening, the weakening of the gravitational pull or the
(27:47):
completely weakening, cause we have a lot of mass loss
through evaporation and explosion. It the the weakening of our
lower mass black hole.
Speaker 2 (27:56):
But the tidal forces are very uh very we have very.
Speaker 1 (27:59):
Strong title forceys and and but why is the and
this is a question that the identifying of the primary
massive object can answer and also what is here? So
but it can answer it. There has to be something
(28:24):
with this radiation in our customs that is causing the
w that that is cr that is CAUs that's where
the paradox is. Also it's like it is causing the
(28:46):
pull quotation, Oh well push is is causing a push
and where it's speaking about the close to the speed
of light would.
Speaker 3 (28:57):
Be speed uh uh th this push could be related
to a.
Speaker 1 (29:11):
Modified velocity that is coming from behind. Why do why
does this appear to be due to a type of
radiation A A type of radiation which wouldn't be s
(29:39):
isn't surprising because the radiation age would come from the
the earliest space time and the ages of these coastal
galaxies and the stars here that were that we're focused
on in their explosions and their particles, So would be
a type of radiation that is is like a like
behind the part particles like a type of a type
(30:02):
of a t it a lot of a little type
of type of.
Speaker 4 (30:10):
Uh.
Speaker 2 (30:10):
It's it.
Speaker 1 (30:13):
It appears as a type of velocity that is coming
from behind or something, but it's the The focus is
on the radiation regarding that specifically. And that's why I
(30:39):
stated on Wednesday that this is where the information is
when we when our uh t at tension was uh
turned to the when our focus was turned to the
cluster galaxies, this is where the information is a lot
of telling information when we identify this this primary uh
this primary massive object also this close to our black.
Speaker 2 (30:56):
Hole, and what will being countered by these particles from
then the cluster.
Speaker 1 (31:03):
Galaxies, what they will encounter regardles what this specification has
has bought about in the atmosphere.
Speaker 2 (31:13):
So that's why Monday, when I introduced this as yuh
you know radio as where when.
Speaker 1 (31:18):
I introduced it as replica starting neutron start two dorch stars, radiation, gas,
gravity and dust, the first that came to mind was
this is is chaos and I s I I still
see it as what it is, just still calculated as
(31:41):
instability where necessary and erratic.
Speaker 2 (31:49):
Encounters. This is where encounters happen now when.
Speaker 1 (31:53):
We introduce the Custer galaxies, and then there there the
the pull, the gravitational pull towards this massive object in
our black and lower mass black hole. Okay, this is
where encounters come. This is where we're speaking about time curvature.
(32:15):
This is where we're speaking about time skills. This is
where we're spaking about time dilations, but in a very
erratic phenomenal way, because each of these spaces in time
has their own inputs and and have been due to
these explosions effect that time or had an effect on
(32:42):
time and had an effect on the experience in of time.
Time scials even come into play, the dilation of time,
the dilations of time, the time dilation, the time skills
E even come to play with I I I is
the well more so, the instability brings that in in
(33:26):
s and this spotification has had the effect on the
time dilations is created in effect on TI on the
time dilation. There's that instability encounter like is the type
of instability. This is where we get into unknown in
(33:50):
encounters of particles and wh why the uh why the
encounters unknown?
Speaker 2 (33:57):
Well, because we know that parts are coded with.
Speaker 1 (34:03):
Laws of physics, gravity laws, from their beginnings, spacetime age
of their beginnings, what they were capable of as it
relates to time and to get in the galaxies that
they are related to, what their explosions changed regarding that,
(34:30):
and what they encountered within the atmosphere after these explosions.
Speaker 2 (34:36):
It creates a very a very It creates an environment.
Speaker 1 (34:42):
That is conducive for the birthing of new stars.
Speaker 2 (34:48):
The environment is set up for it. But what type?
Speaker 1 (34:56):
And that's why I introduces on Monday with that was
the question replica star, neutron star or two door stars?
Speaker 2 (35:07):
What type?
Speaker 1 (35:26):
And it's very interesting the way that these ingredients create
an experiencing of time.
Speaker 2 (35:34):
It is and.
Speaker 1 (35:39):
Associates itself for me with a type of what one
can look at as being the equivalent or as close
to time travel as one would get.
Speaker 2 (35:53):
Is that then that would be.
Speaker 1 (35:55):
The experience of the of of space, that menial or
a multi dimensional experiencing of time because we have curvature
(36:26):
coming from a much to the spears here and we're
dealing with the much to the different ages of stars
(36:47):
and laws of physics regarding what their not potentials were.
But what we're dealing with that. We the potentials are
are are what we're dealing with as we're pulling in now.
What they were regarding their h old age is what
their laws of physics are, what they are capable as
(37:11):
relates to space, time, age, and the overall renewal coding
for the creation of new.
Speaker 2 (37:27):
Giving birth to new stars.
Speaker 1 (37:32):
The potential that they hold comes from their the laws
of physics of what governed them when they were stars
before their their cycle started, and that comes from their
age old age, the age of their beginning, where they
(37:56):
the age of.
Speaker 2 (37:56):
Where they sit in the cosmos from the beginning.
Speaker 1 (38:16):
Even with I mentioned slicing on Tuesday, and it takes
us to and because I spoke about volume, is the
volume took us the slicing when when we do the
volume calculation, it takes to slicing now. And that's where
the two dark stars comes in. In the in in
the time the time dilations come in is of the
(38:42):
slowing down of time, but also the simultane is giving
birth particle energy.
Speaker 2 (38:50):
It comes in.
Speaker 1 (38:51):
It's that's where that in that instability is what causes
the creation of that to happen, or that is that
instability is that creation happening.
Speaker 2 (39:03):
Now with this.
Speaker 1 (39:04):
Erratic with this, with the erratic this, you know, it's
like what what what could that be?
Speaker 2 (39:13):
What will that create?
Speaker 1 (39:16):
Because there's an unknown creation already dead between our lower
massive black hole and our unidentified.
Speaker 2 (39:25):
Primary massive object.
Speaker 1 (39:26):
There's already something that there's there between those two that
has been created through spotifcation. We have used the tension
calculations to to identify this our primary massive object. Well,
(40:00):
the tension calculations would take us too that there's something
that would be have the that else that is there
that will be encountered that creates an erratic environment. All
this is associated with this type of time curvature, the
(40:21):
type of time curvature that are A A A A
object of this size would create with it being in
distance of our lower massive black hole. So we would
be speaking of time being experienced as with with this calculation,
(41:05):
after the pass through of what would be encountered.
Speaker 2 (41:11):
T, time is experienced as unilateral as a as a
type of it. It creates a.
Speaker 1 (41:28):
Time scale that is d that is conducive for experiencing.
Speaker 5 (41:45):
What one would look at is time travel.
Speaker 1 (42:07):
But the identifying what is encountered that w and with
th T th What is encountered these A particles, what
type of particles that would be producing for that regarding
the particles that are being encountered and that c those combinations,
what would be the cause and the way that that
(42:36):
to get that answer is identifying our primary massive object
as in orbit.
Speaker 2 (42:43):
Without low mass black star, without low mass black hole.
(43:07):
What we do know is that.
Speaker 1 (43:11):
This combination the combination of radiation, and we're dealing with
different combination of r types of radiation. We know that
with the different types of gases that we're dealing with,
the the modified gravity, so it's different types of gravity,
the magnetism and a type of velocity back from from
behind that it is.
Speaker 2 (43:32):
What we do know is these are k conducive and greed.
Speaker 1 (43:35):
These energies, these ingredients are conducive for the birthing of
new starts. That is, it's it's about age career with
this time curvature is a speaking of age.
Speaker 2 (43:47):
It's about age.
Speaker 1 (43:50):
And laws of physics ability capability, that's physics laws capability, ability,
initial capability and the time of inception beginning.
Speaker 2 (44:08):
And that capability working well with.
Speaker 1 (44:12):
This type of expression out into the atmosphere.
Speaker 2 (44:15):
This type of injury release, material release, radiation. It working
well with it so that.
Speaker 1 (44:23):
This type of birth can happen, and it is being
pulled into our lower mass black hole.
Speaker 2 (44:31):
It's being pulled towards.
Speaker 4 (44:33):
It is what we have here.
Speaker 1 (44:56):
Okay, when we're gonna go ahead and conclude things until
next time.
Speaker 2 (45:00):
Next for listening by
However, wan and welcome back to the morning. Remember we
alive once again. Today is Thursday, September nineteenth. Let's see
what we have laying on the table where the calculations
have taken us some very interesting stuff. Now, I a
most definitely be highlighting it in my writing that you
all can expect. We we left I wanna go back
(00:23):
here where we left off, cause this is the most
important part, what one of them, all.
Speaker 2 (00:29):
Of it is highly important.
Speaker 1 (00:30):
Remember where we are, uh, our our foundational ingredients radiation, gas, gravity,
dust in the introduction of magnetism yesterday. So doy's the
foundation of our primary structural is what we'll call it,
(00:56):
what our ingredients will sit upon, and.
Speaker 2 (00:58):
What's the driving for words behind them? Now?
Speaker 1 (01:02):
And we we turned to focus onto the secondary massive
object that is not in orbit of our of our
star now and I stated that this is where the
information is it. It is a heap of information here,
(01:23):
uh uh, loads of information, very telling. So let's go
ahead and pick up cause I wanna focus now on
We're gonna leave that b.
Speaker 2 (01:32):
But we know that we're dealing with.
Speaker 1 (01:34):
A modified gravity, meaning different types of gravity, and we
have the radiation coming from a m a month to
the places were already gonna over that regarding our own
little mass black star and the radiation there also the
(01:55):
radiation from the explosions within our secondary massive object, which
it is is secondary because of distance, because remember it
is not in the same orbit of the primary. The
primary yet to be identified. But we're gonna get to
talk about that and this identification and will maybe we'll
(02:16):
speak about its identification tomorrow be cause, but the attention
brings us here, the calculations actually bringing us here, and
it being our primary focus now, the primary focus going
towards it and identifying it. Now, let's see what the
information coming from our clusters.
Speaker 2 (02:38):
Very telling.
Speaker 1 (02:39):
Now let's start with the rate is cause this popification
is very important with us focused on the time curvature
and the different directions that this time curature is coming from,
which makes it.
Speaker 2 (02:55):
With which takes the thought back to when our presented
this on Monday of this is a lot of a
lot of chaos, you know, and it just creates chaos.
Speaker 1 (03:09):
And I stated that, well, the chaos can be minimized
based on what the particles will encounter as they are
ejected released into the atmosphere. Now and we're dealing with
types of gravity coming from multily direction but modified gravities
that are going through a multul change, especially with our
(03:31):
with our cluster galaxies and the stars that we're using
there in their explosions in that material and what it
encounters in orbit around where these explosions happen, what the
materials encounter, and what makes of the new material because
remember we're drawing in and we have the gravitational force
to gravitational pull from multile the rerection.
Speaker 2 (03:52):
For that to happen.
Speaker 1 (03:53):
Now, So now even though our own the star is
obviously weakened, but it with the of force around it,
is able.
Speaker 2 (04:02):
To neutralize itself.
Speaker 1 (04:09):
In a way that it still connects itself with this
core and can pull in the particles that would be
necessary to help us come to our conclusion of replica star,
neutron star, or two drawstars. And I know Monday, when
I introduced this, it was that two drawtstars was like
(04:31):
a question mark of how would that come to pass,
what calculations would make that and necessarid, well, that's what
we're gonna be speaking of today. Case last night calculations
brought that up as one of the conclusions we already
had where Monday when I introduced this, and I stayd well,
we would be dealing with because of the radiation, the
(04:53):
type of radiation that we're dealing with or dealing with
type different types of radiation that you all will know,
the different types of gases that we're dealing with. And
we've done the calculation for our radiation and gases and
the different types of gravity we went into our modified gravity.
What on Tuesday when I stayed there will be different
types of gravity and the dusts from our supernova our
explosions with the supernovas are coming from different different space times.
(05:19):
So and that's just the dust the particles that were
needed cause we're needed because we're bringing.
Speaker 2 (05:23):
Into our star now.
Speaker 1 (05:26):
Okay, So so don's where Monday even knowing when I presented,
is that we're speaking of what type of star?
Speaker 2 (05:37):
What would this bringing into?
Speaker 1 (05:39):
What would it make Replica star, Neutron star or two
door stars.
Speaker 2 (05:43):
Now we the Neutron star, we've.
Speaker 1 (05:47):
Had what we've had d with the calculations. I feel
that I think that it was from yesterday or was
it from Tuesday where it showed up why r Door
star White Door star would be a a potential based
(06:10):
on the ingredients and the calculations that are being used.
Speaker 2 (06:14):
Okay, so now, but that Y, we had not introduced
yet our.
Speaker 1 (06:19):
Massive object, our primary massive object. And I call it
this well, our secondary massive object. So I call it
this secondary massive object, as I stated Y, due to
distance and then and then I I I called the
primary massive object the primary massive object due to its
distance and it being closer in in the in the
(06:42):
gravity it well, it being it being closer to our
start to our black hole. So that's what I'm meaning
when I'm saying primary massive object, secondary massive object. Now
let's go cause w W, let's go over here. Last
night takes us to the spotification and we're we used
(07:07):
the swatch our rats because and also we use the
field equations now because and it shows a type of
time curvature.
Speaker 2 (07:22):
And the surprising part is that we're.
Speaker 1 (07:25):
Dealing with different time curvatures come from different space times.
Now regarding the material ages of the stars and the
material that they present into the atmosphere during these explosions,
(07:49):
and what these material meets and where speaking of spoglifications
specifically here, So it takes us here to.
Speaker 2 (07:58):
Back to looking at the the the.
Speaker 1 (08:01):
Radius calculations last night. It puts our focus on this
spotification now and in the age of our star and
the mass calculations which.
Speaker 2 (08:16):
We spoke about yesterday.
Speaker 1 (08:18):
And it it caused us to look at our start again.
Speaker 2 (08:23):
And this spocification.
Speaker 1 (08:31):
Now here is where because remember when we s when
these when with with the introduction of our our secondary
massive object, the introduction of those particles in the atmosphere
meeting gravitation of being poor towards the primary massive object
(08:52):
that is yet to be identified, is when the the
instability happens.
Speaker 2 (08:57):
Is when what one can and E spat.
Speaker 1 (09:03):
From the first introduction of the work or Monday, what
was my was Marvel calls, Okay, this is uh a
lot of chaotic energy within the within the environment. So
is so calculating the This is where the instability is encountered.
Speaker 2 (09:21):
Here is in the in the the rate of instability.
It takes us into a paradox.
Speaker 1 (09:31):
Because remember we spoke about the the speed being close
to the speed of lights and I mentioned slicing on Tuesday,
and I mentioned time dilations on Tuesday because of the gravity,
the gravitational pull of the particles, and we're speaking of
(09:54):
the the particles, the energy releasing the particles from our
start from the the the the lower massed black hole.
Because we when the massive object which is the the
the secondary massive object, which are the clusters.
Speaker 2 (10:12):
When that when those particles meet and and are.
Speaker 1 (10:17):
Gravitationally pulled into the field, cause remember they're out of
they're not in the same orbit the there the secondary
massive object is not in the same object in the
same orbit as the primary. When they meet, it creates
This is the first introduction of the instability, and it
(10:39):
takes us into a a a paradox, and that's what
the slicing that I introduced on Tuesday happens. It takes place,
and that causes us to focus our attention to.
Speaker 2 (10:59):
To the stars.
Speaker 1 (11:03):
This would be the initial introduction of time curvature outside
of the gravitational field of the of the secondary massive
objects which are our customers, and outside of the primary
massive object which is yet to be identified, but it's
(11:24):
closer to our lower mass black.
Speaker 2 (11:26):
Hole to our start. So we have what was what
does that mean?
Speaker 1 (11:30):
Where we have time curvature coming from three primary directions.
Speaker 2 (11:40):
And that's big die is very significant.
Speaker 1 (12:01):
Because our unidentified well yet to be identified primary massive
object is closer. That's close to our lower mass black
star accounts for time curvature.
Speaker 2 (12:16):
Even though within its radius.
Speaker 1 (12:19):
Weaker gravity is encountered. Okay, bg GU. We have a
lot going on that we have spotification going on.
Speaker 2 (12:26):
So it is that's where the I.
Speaker 1 (12:30):
Not instability, that's where there the chaos that one would
expect when this was first introduced is encountered, and there's
something that will have to be identified amongst the material.
Speaker 2 (12:53):
But t W between our star.
Speaker 1 (12:57):
And the primary massive object that's in this orbit, they're
close together, their distance is closer than our custers are.
There's something in between our lower mass black hole and
this primary massive object that they're in the same rate,
(13:23):
they're in the same ratus, or the distance is closer
than it is for our secondary our customs, but there's
something that needs to be identified between the two.
Speaker 2 (13:43):
There's some type of.
Speaker 1 (13:47):
Energy combination, radiation combination, gas combination, particle combination that has
been created from the material that has been released in
the energy that has been released from our exposure of
our own star and this spotification what it.
Speaker 2 (14:07):
Was meant with, there's a something that has.
Speaker 1 (14:12):
Been id, some something that has been something that is
to be encountered there as the as the particles are
pulled towards the the the our start. And we'll have
to look at those calculations that night to see what
(14:34):
it is. And it's gonna be easy to see what
it is. Why would it be easy to see what
it is?
Speaker 2 (14:40):
Well, because of the slicing that has been introduced.
Speaker 1 (14:48):
And the two dark star theory that was introduced on Monday,
and what they will consist of what their particle composition
would be, and that can give a that's an idea of.
Speaker 2 (15:01):
What would be between.
Speaker 1 (15:04):
What infusion is between some like a particle infusion something
unidentified here that is also accountable for a type of
accountable for a type of space curvature. But it's between
our primary massive object and.
Speaker 2 (15:24):
Between our start what was and what is to be
our start and and we also have yet to look.
But in this tape, this puts our.
Speaker 1 (15:39):
Attention on our primary massive object that's close to our star,
because it puts on us our tension. They're on identifying
and identifying what this massive object is and I and
I stated that it is Sun similar and identifying it
(16:00):
is important here at this point because the identification shows
the capacity. It shows the capacity because now we're speaking
about time, we're speaking about space time, space time curvature,
we're also speaking about time scales, and we're also speaking
about dilations.
Speaker 2 (16:17):
Here time dilations, and.
Speaker 1 (16:20):
They're all very distinct because of the type of radiation, gas, gravity.
Speaker 2 (16:25):
And dust particles we're speaking of.
Speaker 1 (16:33):
So their tension puts on it identifying of what this
primary object is and what is what the spotification has
created between the two that the massive that the cluster
galaxies with particles will encounter.
Speaker 2 (16:52):
And go through a then different type of spotification.
Speaker 1 (16:59):
As it's pull it towards, as those particles are put
towards our.
Speaker 2 (17:03):
Our lower mass black hole.
Speaker 1 (17:11):
Even with the radar instability, it it takes our attention.
Speaker 2 (17:17):
It puts our attention on the time dilations.
Speaker 1 (17:25):
In it creating that instability, It creating that well, the
instability would be the time dilations. It creating a type
of uh of a a K chaotic.
Speaker 2 (17:36):
But not a really radical response.
Speaker 1 (17:38):
The radical response is encountered as the particles are drawn
gravitationally pulled towards magnetized now at this point magnetized towards
the massive object that is close to our star is
where the the kind of a er er erradic response
(17:58):
U T to D is spoglification is.
Speaker 2 (18:02):
Wor didn account for the radic response.
Speaker 1 (18:09):
Because remember I've stated already on I think it was
on Tuesday, Monday or Tuesday, I talked about the quantum
fluctuations that were regardless spogification, that is near the atmosphere
of our primary massive object, and that's where everybody.
Speaker 2 (18:30):
That spent it. When I first introduced this on Monday, Okay.
Speaker 1 (18:33):
This was j This is creating ako the atmosphere, and
it sure is, but this was when.
Speaker 2 (18:37):
The chaos is encountered. But the chaos is also minimized.
Speaker 1 (18:41):
Because with the because the rate of instability could be
calculated with the encountering of well, with the initial encountering
of the of the particles and our.
Speaker 2 (19:00):
Of our black star.
Speaker 1 (19:01):
And the the clusters here, it's like initially there's a
A A A the the rate of instability. That's when
we have the time dilations, and that's encountered. And while
the the time dilations encountered here well, because remember we
stated that the injections of s, the the injection of
(19:21):
certain stars within these explosives of our cluster galaxies would
not be usable material, but those that are still b
but those the material that is still accountable for the
scattering of lights is where that material that is thrown
(19:43):
out into the atmosphere was thrown out into the atmosphere
at at after these it this explosion within these clusters
for these stars, the account encountering of material from our
own low mass black star is where the instability state
takes place, and that's where we'll have the time dilations there.
(20:03):
And when the time dilations, that's what we're looking at,
things like well w based on our ho calculations of
the age of our own own star. In this material,
it would we would look at things like what one
would look at as time travel wa not even time travel,
it would be the experience of.
Speaker 2 (20:27):
Multi dimensional space.
Speaker 1 (20:30):
At calculated giving points within time. Because when where we
are focused on, as I stated yesterday, as of yesterday,
focus on the laws of physics that govern these stars
and in their explosions, in the laws of physics that
govern their explosions, based on the bids of years that
(20:51):
they've been in the process of exploding of dying. So
we're speaking of the potential that I stated of their capability.
Speaker 2 (20:58):
Well, we're not in the potential that capability, but their actual.
Speaker 1 (21:01):
Capabilities when they were stars and the potential that it
still holds after the explosions with it, the potential that
holds within some stars after the explosions, and the material
being released in the atmosphere, and what the Spokul occasion
can create, as.
Speaker 2 (21:15):
It relates to its is is adding into the creation
of new stars and the material necessary for that to happen.
So we we know that we will be looking.
Speaker 1 (21:35):
At material, that is, particles that are have gone through
U processes based on their environment. With the addition of
the ingredients of what creates it gives birth to new stars.
(22:02):
And that's why our outcome as of Monday when this
was introduced Replica Star, Neutron Star two dark Stars.
Speaker 2 (22:08):
As of yet we do not know.
Speaker 1 (22:10):
I obviously that would be in my writing when I
put all this together with the calculations in the final.
Speaker 2 (22:18):
Completion.
Speaker 1 (22:23):
So is, and because when we look at time caricature
also in the fascination of it, our our modified gravity
also accounts for the time curvature. We have our unidentified
well yet to be identified, primary massive object that's close
to our lower massive blackness, the.
Speaker 2 (22:40):
Whole account of a ta R account of time curvature.
Speaker 1 (22:43):
Also, even though we h it has a w.
Speaker 2 (22:47):
I, there the the weak of gravity as.
Speaker 1 (22:48):
An encounter, but that would be a necessary ingredient. And
we have something that even even with its unidentified spotification
that has happened between the two between our lower mass.
Speaker 2 (22:59):
Black hole and the in the.
Speaker 1 (23:00):
The unidentified object that is within its orbit. It it's
creation can create a a a very erratic atmosphere as
it's pulling, as the gravitational pull and the mandatory towards
our black hole is happening, it will create a very chaotic, erratic,
(23:23):
but necessary change. And why would that chaotic erratic be encountered. Well,
because we're talking about space time now and we're talking
about we're speaking of of different It's because we're speaking
of these custom galaxies, primarily him, and we're we're speaking
of different time scals, different time dilations, different laws of
(23:47):
physics that govern the age and the aging of the
stars and their beginnings and what they were consistent w
what they consist of, what their particles consist of from
the beginning, and that's what's accounting for the time their
(24:09):
time curvature of all of that is accounting for the
time curvature the.
Speaker 2 (24:13):
I it's it it it could be experienced with time. Obnestly,
it would be experienced.
Speaker 1 (24:19):
With the with the the time it would be the
time would be slowed down. But it would also uh
s a celerate time.
Speaker 2 (24:27):
Now this is acceleration of time.
Speaker 1 (24:28):
It create it accounts for the erratic energy also because
of their encountering the unidentified whatever is between that has
been created by this spotification between our black hole and
our primary object that is in its orbit during the
same orbit.
Speaker 2 (24:48):
So time would be experienced quite k quite well.
Speaker 1 (25:01):
That would be a W that would be account for
the for the time being experienced as m the multi
dimensional experiencing of time, as opposed to where that could
account for a type UH that is in itself a
type of time travel.
Speaker 2 (25:16):
I Y is where.
Speaker 1 (25:30):
Where that T where that type of erratic composition.
Speaker 2 (25:35):
Is necessary for the output of.
Speaker 1 (25:37):
Two dog star repelical start a neutron star, But which
would it be. What we spoke about today focused on
the two door stars, but yesterday we talked about the
introdutional neutron star and what focused on that. This combination
of what we have laying on the table and then
(25:58):
tools that we spoke about the white door star right,
the output of the ingredients unknown and and why would
(26:22):
we still unknown what? Because we have our massive object,
our primary massive object that's in that's not at their
furthest distance and distance have distance hasn't has already been
calculated of our massive object is in this unidentified in
whatever is between that the spotification has already created and
what the particles will be encountering as they come towards.
Speaker 2 (26:46):
Our start.
Speaker 1 (27:01):
Because remember with our the clusters is the longer wavelength
of radiation emissions in that B which I all of
this aids in.
Speaker 2 (27:12):
The the gravitational pull behind. But why is the gravity
of peach.
Speaker 1 (27:16):
Why is the gravitational pool behind the particles?
Speaker 2 (27:20):
Why is it behind as opposed to the particles being
pulled forward?
Speaker 1 (27:26):
Well, we'll know that wants well it it It could
be because of the modified gravity that we're using that
would occur in c in these types of cluster galaxy,
and we're talking we're speaking of irregular clusters and the
the weakening, the weakening of the gravitational pull or the
(27:47):
completely weakening, cause we have a lot of mass loss
through evaporation and explosion. It the the weakening of our
lower mass black hole.
Speaker 2 (27:56):
But the tidal forces are very uh very we have very.
Speaker 1 (27:59):
Strong title forceys and and but why is the and
this is a question that the identifying of the primary
massive object can answer and also what is here? So
but it can answer it. There has to be something
(28:24):
with this radiation in our customs that is causing the
w that that is cr that is CAUs that's where
the paradox is. Also it's like it is causing the
(28:46):
pull quotation, Oh well push is is causing a push
and where it's speaking about the close to the speed
of light would.
Speaker 3 (28:57):
Be speed uh uh th this push could be related
to a.
Speaker 1 (29:11):
Modified velocity that is coming from behind. Why do why
does this appear to be due to a type of
radiation A A type of radiation which wouldn't be s
(29:39):
isn't surprising because the radiation age would come from the
the earliest space time and the ages of these coastal
galaxies and the stars here that were that we're focused
on in their explosions and their particles, So would be
a type of radiation that is is like a like
behind the part particles like a type of a type
(30:02):
of a t it a lot of a little type
of type of.
Speaker 4 (30:10):
Uh.
Speaker 2 (30:10):
It's it.
Speaker 1 (30:13):
It appears as a type of velocity that is coming
from behind or something, but it's the The focus is
on the radiation regarding that specifically. And that's why I
(30:39):
stated on Wednesday that this is where the information is
when we when our uh t at tension was uh
turned to the when our focus was turned to the
cluster galaxies, this is where the information is a lot
of telling information when we identify this this primary uh
this primary massive object also this close to our black.
Speaker 2 (30:56):
Hole, and what will being countered by these particles from
then the cluster.
Speaker 1 (31:03):
Galaxies, what they will encounter regardles what this specification has
has bought about in the atmosphere.
Speaker 2 (31:13):
So that's why Monday, when I introduced this as yuh
you know radio as where when.
Speaker 1 (31:18):
I introduced it as replica starting neutron start two dorch stars, radiation, gas,
gravity and dust, the first that came to mind was
this is is chaos and I s I I still
see it as what it is, just still calculated as
(31:41):
instability where necessary and erratic.
Speaker 2 (31:49):
Encounters. This is where encounters happen now when.
Speaker 1 (31:53):
We introduce the Custer galaxies, and then there there the
the pull, the gravitational pull towards this massive object in
our black and lower mass black hole. Okay, this is
where encounters come. This is where we're speaking about time curvature.
(32:15):
This is where we're speaking about time skills. This is
where we're spaking about time dilations, but in a very
erratic phenomenal way, because each of these spaces in time
has their own inputs and and have been due to
these explosions effect that time or had an effect on
(32:42):
time and had an effect on the experience in of time.
Time scials even come into play, the dilation of time,
the dilations of time, the time dilation, the time skills
E even come to play with I I I is
the well more so, the instability brings that in in
(33:26):
s and this spotification has had the effect on the
time dilations is created in effect on TI on the
time dilation. There's that instability encounter like is the type
of instability. This is where we get into unknown in
(33:50):
encounters of particles and wh why the uh why the
encounters unknown?
Speaker 2 (33:57):
Well, because we know that parts are coded with.
Speaker 1 (34:03):
Laws of physics, gravity laws, from their beginnings, spacetime age
of their beginnings, what they were capable of as it
relates to time and to get in the galaxies that
they are related to, what their explosions changed regarding that,
(34:30):
and what they encountered within the atmosphere after these explosions.
Speaker 2 (34:36):
It creates a very a very It creates an environment.
Speaker 1 (34:42):
That is conducive for the birthing of new stars.
Speaker 2 (34:48):
The environment is set up for it. But what type?
Speaker 1 (34:56):
And that's why I introduces on Monday with that was
the question replica star, neutron star or two door stars?
Speaker 2 (35:07):
What type?
Speaker 1 (35:26):
And it's very interesting the way that these ingredients create
an experiencing of time.
Speaker 2 (35:34):
It is and.
Speaker 1 (35:39):
Associates itself for me with a type of what one
can look at as being the equivalent or as close
to time travel as one would get.
Speaker 2 (35:53):
Is that then that would be.
Speaker 1 (35:55):
The experience of the of of space, that menial or
a multi dimensional experiencing of time because we have curvature
(36:26):
coming from a much to the spears here and we're
dealing with the much to the different ages of stars
(36:47):
and laws of physics regarding what their not potentials were.
But what we're dealing with that. We the potentials are
are are what we're dealing with as we're pulling in now.
What they were regarding their h old age is what
their laws of physics are, what they are capable as
(37:11):
relates to space, time, age, and the overall renewal coding
for the creation of new.
Speaker 2 (37:27):
Giving birth to new stars.
Speaker 1 (37:32):
The potential that they hold comes from their the laws
of physics of what governed them when they were stars
before their their cycle started, and that comes from their
age old age, the age of their beginning, where they
(37:56):
the age of.
Speaker 2 (37:56):
Where they sit in the cosmos from the beginning.
Speaker 1 (38:16):
Even with I mentioned slicing on Tuesday, and it takes
us to and because I spoke about volume, is the
volume took us the slicing when when we do the
volume calculation, it takes to slicing now. And that's where
the two dark stars comes in. In the in in
the time the time dilations come in is of the
(38:42):
slowing down of time, but also the simultane is giving
birth particle energy.
Speaker 2 (38:50):
It comes in.
Speaker 1 (38:51):
It's that's where that in that instability is what causes
the creation of that to happen, or that is that
instability is that creation happening.
Speaker 2 (39:03):
Now with this.
Speaker 1 (39:04):
Erratic with this, with the erratic this, you know, it's
like what what what could that be?
Speaker 2 (39:13):
What will that create?
Speaker 1 (39:16):
Because there's an unknown creation already dead between our lower
massive black hole and our unidentified.
Speaker 2 (39:25):
Primary massive object.
Speaker 1 (39:26):
There's already something that there's there between those two that
has been created through spotifcation. We have used the tension
calculations to to identify this our primary massive object. Well,
(40:00):
the tension calculations would take us too that there's something
that would be have the that else that is there
that will be encountered that creates an erratic environment. All
this is associated with this type of time curvature, the
(40:21):
type of time curvature that are A A A A
object of this size would create with it being in
distance of our lower massive black hole. So we would
be speaking of time being experienced as with with this calculation,
(41:05):
after the pass through of what would be encountered.
Speaker 2 (41:11):
T, time is experienced as unilateral as a as a
type of it. It creates a.
Speaker 1 (41:28):
Time scale that is d that is conducive for experiencing.
Speaker 5 (41:45):
What one would look at is time travel.
Speaker 1 (42:07):
But the identifying what is encountered that w and with
th T th What is encountered these A particles, what
type of particles that would be producing for that regarding
the particles that are being encountered and that c those combinations,
what would be the cause and the way that that
(42:36):
to get that answer is identifying our primary massive object
as in orbit.
Speaker 2 (42:43):
Without low mass black star, without low mass black hole.
(43:07):
What we do know is that.
Speaker 1 (43:11):
This combination the combination of radiation, and we're dealing with
different combination of r types of radiation. We know that
with the different types of gases that we're dealing with,
the the modified gravity, so it's different types of gravity,
the magnetism and a type of velocity back from from
behind that it is.
Speaker 2 (43:32):
What we do know is these are k conducive and greed.
Speaker 1 (43:35):
These energies, these ingredients are conducive for the birthing of
new starts. That is, it's it's about age career with
this time curvature is a speaking of age.
Speaker 2 (43:47):
It's about age.
Speaker 1 (43:50):
And laws of physics ability capability, that's physics laws capability, ability,
initial capability and the time of inception beginning.
Speaker 2 (44:08):
And that capability working well with.
Speaker 1 (44:12):
This type of expression out into the atmosphere.
Speaker 2 (44:15):
This type of injury release, material release, radiation. It working
well with it so that.
Speaker 1 (44:23):
This type of birth can happen, and it is being
pulled into our lower mass black hole.
Speaker 2 (44:31):
It's being pulled towards.
Speaker 4 (44:33):
It is what we have here.
Speaker 1 (44:56):
Okay, when we're gonna go ahead and conclude things until
next time.
Speaker 2 (45:00):
Next for listening by
Popular Podcasts
Stuff You Should Know
If you've ever wanted to know about champagne, satanism, the Stonewall Uprising, chaos theory, LSD, El Nino, true crime and Rosa Parks, then look no further. Josh and Chuck have you covered.
Las Culturistas with Matt Rogers and Bowen Yang
Ding dong! Join your culture consultants, Matt Rogers and Bowen Yang, on an unforgettable journey into the beating heart of CULTURE. Alongside sizzling special guests, they GET INTO the hottest pop-culture moments of the day and the formative cultural experiences that turned them into Culturistas. Produced by the Big Money Players Network and iHeartRadio.
Dateline NBC
Current and classic episodes, featuring compelling true-crime mysteries, powerful documentaries and in-depth investigations. Follow now to get the latest episodes of Dateline NBC completely free, or subscribe to Dateline Premium for ad-free listening and exclusive bonus content: DatelinePremium.com