CORE PHYSICS

a taxonomy






PREAMBLE

TAXONOMIC TABLE

GLOSSARY


Index

Taxa:
FUNDAMIDES

Taxon:
Teels

Taxon:
Teelons

Taxon
Teeloids


Taxa
PHOTIDES

Taxon:
Photons

Taxon:
Quarks


Taxa:
MORPHIDES

Taxon:
Electroids

Taxon:
Nucleons


Taxa:
NUCLIDES

Taxon:
Primalnuclides

Taxon:
Lithicnuclides

Taxon:
Ferricnuclides


Taxa:
STELLIDES

Taxon:
Protostars

Taxon:
Dwarfstars

Taxon:
Whitestars

Taxon:
Blackstars


Taxa:
GALACTIDES

Taxon:
Elliptogalaxies

Taxon:
Ellectrogalaxies

Taxon:
Nucleogalaxies


* * * * *

PREVIOUS ITERATIONS

The Blue Book (1996)

Principia Cosmologica
(2008)

Template
(2014)




 









































   





























































































































































































































































































































































Taxa
GALACTIDES


TAXA     Galactides     Objects with blackstars in their nuclei.

TAXON     Elliptogalaxies     Galactides with a one blackstar, standard, nucleus.
TAXON     Electrogalaxies     Galactides with a two blackstar, electroidal, nucleus.
TAXON     Nucleogalaxies     Galactides with a three blackstar, nucleonic, nucleus.

Revised:     4th May 2022




CONTENTS










BROUGHT FORWARD



GALACTIDES          A taxa.

This is a holding entry

Galactides is a taxa consisting of taxons with a peakmass high enough to maintain a holisphere. The taxa has three taxons:
  • Globulars     Galaxies in dominance adjacency to larger galaxies.
  • Galaxies     Galaxies in type adjacency to other galaxies.
  • Galactars     Clusters of type adjacent galaxies bound by their mutual gravitypull.



GLOBULAR          A taxon.

GLOBULAR     A taxon in the taxa Galactides. Globulars are galactides in dominance adjacency.

GALACTIDES     A taxa consisting of taxons that grow by accretion and maintain a holisphere until dissipation or stabilisation. The taxa has three taxons: globulars, galaxies, and galactars.

GLOBULAR FACTBASE     The globular factbase is not extensive. It is limited by observing distances and equipment inadequacy. Factbase expansions and revisions are expected.
GLOBULARS IN CORE PHYSICS     Nothing in the globular factbase clashes with Core Physics expectations. These extrapolations from the Core Physics Taxonomic Table may provide insight.
  • A globular has a gravitysheath inside a gravitysheath interface.
  • A globular is a nucleus of stars inside a halo of stars.
  • Globulars are engorged by the galaxy teelstream system.
  • The teelstream system strips globulars of non-accretides.
  • The teelstream can be a plasmastream.
  • The teelstreams/plasmastreams engorge the globular's stars..
  • Sufficiently engorged stars are Population II stars.
  • Population II stars cannot form ferric cores and thus:.
  • Globular nuclei are mostly Population II stars.
  • Globular halos can have some  Population I stars.
  • Population I stars may form ferric cores.
  • Population I stars may form in situ but are more likely to be accreted.
  • Population I stars are more massdense than Population II stars.
  • Population I stars progressively move through the halo to the nucleus.
  • Globulars progressively converge on the galaxy nucleus.
    • Progressive convergence equates to increasing engorgement.
    • Progressive convergence equates to increasing density of adjacent stars and globulars.
    • Progressively increasing adjacent star density equates to increasing rates of star accretion.
    • Progressively increasing adjacent globular density equates to increasing rates of globular collisions.
    • Progressively increasing adjacent globular density equates to progressively decreases in globular gravitysheaths volumes.
    • Progressively decreases in globular gravitysheath volumes equates to a progressive losing globular halo stars.
  • Globulars converging on the galaxy nucleus are progressively dissipated.
GLOBULAR LIFECYCLE
  • A globular forming inside a galaxy may be unable to form a nucleus.
  • A globular forming inside a galaxy may be unable to form a contracted region inside the nucleus.
  • A globular that was a dwarf galaxy may have a nucleus before accretion.
  • A globular that was a dwarf galaxy may have a contracted region inside the nucleus before accretion.
  • A globular that was a dwarf galaxy may have a darksphere.
  • Globulars always dissipate before they can stabilise..

GALAXIES           A taxon.

GALAXIES     A taxon in the taxa Galactides. Galaxies are galactides in type adjacency.

GALACTIDES     A taxa consisting of taxons that grow by accretion and maintain a holisphere until dissipation or stabilisation. The taxa has three taxons:   globulars, galaxies, and galactars.

GALAXY FACTBASE     The galaxy factbase is not extensive. It is limited by observing distances and equipment inadequacy. Factbase expansions and revisions are expected.
  • A galaxy is a holisphere around a masscentre.
  • Galaxies are in type adjacency to adjacent galaxies.
  • Galaxies with enough mass are a nucleus of tightly bound stars and a halo of diffuse stars.
  • Stars can be solo or in globulars.
  • Galaxies vary widely in mass and, commensurately, in the number of stars they contain.
    • Dwarf galaxies     Galaxies without enough mass to form a spiral disk of stars in the halo. Such a galaxy, subject to circumstance, can be a type adjacent dwarf galaxy or a dominance adjacent globular. It may be that all dwarfs unable to accrete enough mass to become spirals are doomed to become globulars eventually.
    • Spiral galaxies     Galaxies with enough mass to form a spiral disk of stars in the halo. Spirals are common in the outer reaches of galactars and less common toward the centre.
    • Elliptical galaxies     Galaxies with enough mass to become a spheroid of of stars. Nuclei cannot be seen. Disks (if any) cannot be seen. Elliptical galaxies are common toward the centre of galactars and less common in the outer reaches.
  • Galaxies with enough mass have a darksphere.
GALAXIES IN CORE PHYSICS     Nothing in the galaxy factbase clashes with Core Physics expectations. These extrapolations from the Core Physics Taxonomic Table may provide insight.
  • A star in a galaxy has its own gravitysheath.
  • A star in a galaxy is in dominance adjacency.
  • A globular in a galaxy has its own gravitysheath.
  • A globular in a galaxy is in dominance adjacency.
  • A galaxy observed by photon emission was understable at the time of emission.
  • A galaxy unobservable by photon emission may, or may not, be understable.
  • A galaxy with enough mass has a galactic darksphere.
  • A galaxy with enough mass has a galactic darksphere with a galactic blackhole inside.
    • A galactic blackhole in an understable galaxy is itself understable.
    • Understable galactic blackholes stabilise per the energy/mass differential.
    • Understable galactic blackholes stabilise by ejecting teels.
    • Understable galactic blackholes cannot stabilise before its nucleus and  halo.
  • A galaxy has a teelstream system.
  • Galaxy teelstreams may contain plasmatoids and be plasmastreams.
  • Galaxy teelstreams have significant momentum in the nucleus.
  • Teelstream momentum in the nucleus engorges the nucleus stars.
  • Engorged star photospheres emit photons prodigiously.
  • Engorgement in nucleus stars is reinforced by photon emission pressure.
  • Engorgement inhibits all but the simplest fusions in nucleus stars.
  • Engorgement in stars near, or inside,  the darksphere is such that all fusion is inhibited.
  • Photon emission from stars near, or inside, the darksphere is from understable protons in the photosphere and is intense.
  • Galactic blackholes with enough mass overengorge stars near, or inside, the darksphere, dissipating and then accreting them.
  • Halo stars undergo the fusion cycle commensurate with their peakmass and subject to the degree of their engorgement.
  • Halo star "nurseries" accelerate the fusion cycle in stars by seeding each other with pre-fused isotopes.
  • Over time, halo stars move toward the nucleus.
  • Over time, nucleus stars move toward the darksphere and the blackhole.
  • Over time, the galactic blackhole accretes all it can before stabilising as a cold blackhole.
CAVEAT     Concern is being expressed by some researchers that the mass of some galactic blackholes is such that it cannot have been accreted inside the currently estimated time elapsed since the beginning of the Universe.@@@@@
  • Time elapsed     The age of the Universe needs to be reconsidered in the light of the Core Physics Taxonomic Table.
  • Accretion rate     The Current Paradigm (with suspicion) recognises the existence of darkmatter. It does not recognise it, however, as a significant percentage of the "feedstock" of galactic blackholes. In Core Physics, galactic blackholes do eat their own stars but they first dissipate them into digestibles. Thus the feedstock is morphides, photides, and fundamides. Yet much of the feedstock is not dissipation material at all. It is photides and fundamides: that is, photons and darkmatter. Given that darkmatter in some galaxies is estimated to be over 80% of the matter content, there is a lot of it there to be eaten.   
CAVEAT     In the Current Paradigm, the metal-rare condition of stars in galactic nuclei is taken as meaning the stars are old. They can be old, of course, but the cause of their metal-rarity is because they are engorged. Indeed, when galaxies have very massive galactic blackholes, their lifespan can be short through being overengorged and dissipated.

CAVEAT
     The endpoint in the lifecycle of a galaxy is being accreted or becoming stable - stable being without any ejections, emissions, or expulsions. It may be that no galaxies in the visible universe have yet stabilised. 

CAVEAT
     Galaxies are observed in a wide range of sizes and masses. However, there is a size/mass beyond which no galaxies are observed. Whether this is a limitation of some kind is currently unknown. However, Core Physics currently suggests no reason for such a limitation.

CAVEAT     The nucleus of a galaxy consists of strongforced stars engorged inside an energetic teelstream system. The teelstream system inhibits the ability of the stars to fuse the more massive isotopes. If the eventhorizon is sufficiently massive, a limited number of stars are subforced to its surface.



GALACTARS          A taxon.

This is a holding entry

GALACTIDES
     A taxa consisting of taxons with a peakmass high enough to maintain a holisphere. The taxa has three taxons:     globulars, galaxies, and galactars.

GALACTARS     Clusters of type adjacent galaxies bound by mutual gravitypull.

GALACTAR FACTBASE      The galactar factbase is thin. It is limited by great observing distances and equipment inadequacy. Factbase expansions and revisions can be expected.
  • Galactars are holispheres bound to a masscentre and inside a gravitysheath.
  • Galactar holispheres consist of all types of object from galaxies downward.
  • Galactars contain up to around a thousand galaxies.
  • Galactar masses are up to around 1015 solarmasses.
  • Galactar mass is 90% subphotonic darkmatter.
  • Galactar diameters are up to around 5mpc.
GALACTARS IN CORE PHYSICS     Nothing in the galactar factbase clashes with Core Physics expectations. These extrapolations from the Core Physics Taxonomic Table may provide insight.
  • Each galaxy in a galactar has its own gravitysheath.
  • Each galaxy in a galactar is in dominance adjacency inside the galactar gravitysheath.
  • Each galaxy in a galactar is in type adjacency to adjacent galaxies.
  • Each galactar is inside its own gravitysheath.
  • Galactars inside the gravitysheath of another galactar are in dominance adjacency.
  • Galactars in dominance adjacency and below escape velocity are dissipated and absorbed over time.
  • Galactar holispheres consist of all types of object from stars downward.
  • Galactars observed by photon emission are understable at the time of emission.
  • Galactars unobservable by photon emission may, or may not, be understable.
    • Understable galactars undergo accretion expansion.
    • Understable galactars undergo stabilisation contraction.
    • Understable galactars stabilise per the energy/mass differential.
  • The mass of a galactar is such that it has a central event horizon.
CAVEAT     The endpoint in the lifecycle of a galactar is either being accreted or becoming stable - stable being without any ejections, emissions, or expulsions. It may be that no galactar in the visible universe has yet stabilised.

CAVEAT
     Large aggregations of galaxies are observed that exceed what is currently considered to be a galactar. Whether these are larger galactars or clusters of galactars is unclear. Just as there seems to be an upper limit to the mass and/or size of understable hypergiantstars, there may be a limit to the mass and/or size of understable galactars. However, there is currently nothing (in Core Physics) that prevents galactars coming together as galactar clusters. That is: as a cluster of type adjacent galactars bound by their mutual gravitypull inside is own gravitysheath. The mass of a galactar cluster would be such that there would be an event horizon at its centre.

CAVEAT     Everything known in the Universe stabilises if conditions allow. For a galactar, stabilisation requires the ejection of a significant proportion of its energy and mass after peakmass. This creates a vicious circle.
  • Ejections from understable galactars are into the gravitysheaths of adjacent galactars.
  • Thus understable galactars are absorbing the ejections of adjacent galactars.
  • Thus stabilising galaxies are simultaneously absorbing and ejecting.
  • Thus galactars cannot stabilise.
The vicious circle is only broken if the Universe is seen as a spheroidal galactar cluster beyond which there is a region of space. The galactars on the outside of the Universe would eject their excess of energy and mass into that space and thus be the exhaust allowing all the galactars to stabilise eventually.

Notably, the ejected mass would become a holisphere for the spheroid which would grow in mass as the the galactars stabilised. The gravitypull of the holisphere would have exactly the effect on the spheroid that is currently attributed to darkenergy.

So is the Universe a spheroid of galactars. Possibly. But probably not. See the next caveat.


CAVEAT     An important lesson to be taken from the current Core Physics taxonomy is that, just as the notion that the Earth is the centre of the Universe was abandoned, the notion that humans occupy the centre point in the taxonomic table should be abandoned also.

The mechanics of gravitypull and repellence are not explained by positing a teel universe. It is therefore reasonable to suppose the explanations for gravitypull and repellence will be found in pre-teel cumulations. This may mean there is just one taxon below that of teels but that cannot be assumed.

Similarly, the current description of the larger universe is effectively bounded by what can be seen. However, the Core Physics taxonomy is constructed out of a very small set of rules. There is no good reason to suppose that the universe that cannot be seen is not subject to exactly the same rules.

The previous caveat hypothesised the universe as a spheroid of galactars. That is a possibility although not the only possibility. What is also a possibility, actually more a likelihood, is that the Universe is part of a uberuniverse operating under the same fundamental rules already empirically verified.

As to what that the structure of the uberuniverse might be, as of now, an open question.  Answers may be forthcoming if it can be determined what the Universe will be when it has stabilised. Will it be an independent object like a molecule in an atmosphere. Or will it be a subsidiary unit in a larger object like a quark in a nucleon. Time will tell us. Or it will not. 


BLACKHOLE          An object with a massdensity so high it is always inside a darksphere.

There are two forms of blackhole:  stellar blackholes and galactic blackholes.
  • Stellar blackholes     These result from the collapse of hypergiantstars.
  • Galactic blackholes     These form inside the darkspheres that form around the gravitycentres of galaxies with enough mass.
* * * * *
Hypergianstars have enough mass to fuse stratums of transuranic isotopes inside stratums of fissile isotopes. When the fissile stratums reach critical mass they implode. The transuranic stratums are simultaneously overengorged and crushed together. The transuranic isotopes are broken into lesser isotopes. Much of the isotope teelospheres are expelled out to reinforce the fission explosion.

What remains is a compact sphere of stripped isotopes surrounding a core of stripped nucleons. The exact mix depends on the peakmass of the hypergiantstar. The higher the peakmass the higher the proportion of nucleons over isotopes. It is possible that the higher peakmass hypergiantstars collapse to have a central core of solidbonded teels. It may even be possible that the highest peakmass hypergiantstars collapse to an object that is entirely solidbonded teels.


It is possible that hypergiantstars precollapse already have a darksphere surrounding their gravitycentre. Certainly, the postcollapse blackhole has one surrounding its gravitycentre. At their least massive, the surface of the darksphere and the surface of the blackhole coincide. With increases in blackhole mass, the volume of the darksphere increases more than does the volume of the blacksphere.

Stellar blackholes are not inert. Notably, they have teelospheres formed into substantial and active teelstream systems. The systems extend beyond the darkspheres.

The extrinsic gravitypull of stellar blackholes is such that they accrete anything that comes within range that is not so big that it will accrete them. That said, most of the feedstock of any blackhole is subphotonic. The subphotonic mass of many galaxies is believed to be upwards over 70% of the total mass so there is plenty of that feedstock available.

The act of accretion makes a blackhole understable or more understable. Thereafter they undergo stabilisation by ejecting teels. A blackhole that is continually accreting and thus in continuous stabilisation is a blackhole that is increasing its mass.  A stable blackhole is a cold blackhole, one which is neither accreting nor ejection. Whether there are yet any cold blackholes in the Universe is unknown.

* * * * *

Galaxies are accumulations of stars bound together by their mutual gravitypull. At their centre galaxies have
  • Masscentre     The point around which the stars move and to which they are ultimately attracted.
  • Gravitycentre.     Where the intrinsic gravitypull of the galaxy cancels out. The gravitycentre can be a point and the cancellation total. However, more likely it is a sphere and the cancellation to a degree.
If a galaxy has enough mass, the gravitycentre becomes a darksheath, a region from within which an object can only escape if it can exceed the escapevelocity at the darksheath surface. Galaxy mass increases commensurately increase the darksheath volume and the darksheath surface escapevelocity. A sufficient increase raises the surface escapevelocity to lightspeed.
  • Objects in a darksheath decelerate moving toward the gravitycentre.
  • Objects in a darksheath accelerate moving away from the gravitycentre.
  • Objects with a sufficiently low entry speed can be held in trojan adjacency.
  • Objects that lose speed in collisions can be held in trojan adjacency.
  • Trojan objects aggregate, begin to spin, and have an extrinsic gravitypull.
  • The trojan aggregate is now the blackhole at the centre of the darksheath.
  • The blackhole extrinsic gravitypull actively accretes objects into the darksheath.
  • Accreted objects are dissipated and absorbed into the blackhole.
  • The mass of the blackhole grows.
  • At the surface of the darksheath, a massvelocity of zero relative to the masscentre supplants the escapevelocity of lightspeed relative to the gravitycentre.
The primary "feedstock" of blackholes is subphotonics (darkmatter). The above description reflects this. However, process is accelerated if one or more stars becomes trojan adjacent at an early stage.

Blackholes of sufficient mass have a substantial high-mementum teelocean. Objects drawn into the teeloceon are broken down and assimilated.

Blackholes have teelospheres formed into high-momentum teelstream systems. As the mass of blackholes increase, the teelospheres extend further and further out into the gravitysheath. The very dense inner break down more  that extend beyond the darksheath. These break down more substantial objects by overengorgement and gravitational spaghettification.

Accretion understabilises a blackhole, triggering stabilisation by ejection, emission, and expulsion. However, as the mass of the blackhole increases it can first no longer expel and then no longer emit. However, undestable blackholes all eject. The surrounding teelstream systems are the means by which blackholes eject their excess massvelocity and energyvelocity out of their gravitysheaths.

Per the energy/mass differential, understable blackholes are increasing their measures of energy and mass. Blackholes only stop growing when there is nothing to be accreted. By default, understable blackholes increase  and its escape velocity rises, it firstly can no longer expel and then, as the escapevelocity exceeds lightspeed, it can no longer emit. From hereon stabilisation is by the ejection of teels.

The energy/mass differential means that as long as the blackhole can keep on accreting it can keep on growing. , then it cannot emit,@@@@@
 

The extrinsic gravitypull of galactiv












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Copyright 2022 - Sian Luise Winchester









Comments and suggestions:  peter.ed.winchester@gmail.comCopyright 2021 - Sian Luise Winchester