COREPHYSICS

• Stellides form by (1) the accretion of nucleons and nuclides.
• Stellides form by (2) the collapse of accreted nucleons and nuclides.
• Stellides are defined by their senior collapse mechanism.
• Stellides collapse mechanism are gravitycollapse, emissioncollapse, fusioncollapse, ferriccollapse, fissioncollapse, and stellaspherecollapse.
• Stellides are protostellides (emissioncollapse), dwarfstellides (fusioncollapse), whitestellides (ferriccollapse), blackstellides (fissioncollapse), and galastellides (stellaspherecollapse).
  
• Stellides semistabilise as a monocore nucleus and a teelosphere.

• Protostellides are stellides that peakmass as protostars.
• Protostars are grains, planets, and giantplanets.
• Protostellides peakmass up to 0.8 solarmasses.
• Protostars form by the accretion of nucleons and nuclides.
• Protostellides form by the collapse of accreted nucleons and nuclides.
• Protostellide collapse mechanisms are gravitycollapse and emissioncollapse.
  
• Protostellides semistabilise as a monocore nucleus and teelosphere.
• Protostellides reactivate with sufficient further accretion.

• Dwarfstellides are stellides that peakmass as dwarfstars.
• Dwarfstellides peakmass as stars of between 0.8 and 9 solarmasses.
• Dwarfstars form by the accretion of nucleons and nuclides..
• Dwarfstellides form by the collapse of accreted nucleons and nuclides.
• Dwarfstellide collapse mechanisms are gravitycollapse, emissioncollapse, and fusioncollapse.
  
• Dwarfstellides collapse to whitedwarfs.
• Dwarfstellides semistabilise as a monocore nucleus and a teelosphere.
• Dwarfstellides reactivate with sufficient further accretion.

• Whitestellides are stellides that peakmass as whitestars.
• Whitestellides peakmass as stars of between 9 and 25 solarmasses.
• Whitestars form by the accretion of nucleons and nuclides.
• Whitestellides form by the collapse of accreted nucleons and nuclides.
• Whitestellide collapse mechanisms are gravitycollapse, emissioncollapse, fusioncollapse, and ferriccollapse.
• Whitestellides collapse to neutronstars of 3 solarmasses or more.
  
• Whitestellides semistabilise as a monocore nucleus, teelosphere, and gravitysheath.
• Whitestellides reactivate with sufficient further accretion.

• Blackstellides are stellides that peakmass as blackstars.
• Blackstellides peakmass as stars of between 25 and 45 solarmasses.
• Blackstars form by the accretion of nucleons and nuclides.
• Blackstellides form by the collapse of accreted nucleons and nuclides.
• Blackstellide collapse mechanisms are gravitycollapse, emissioncollapse, fusioncollapse, ferriccollapse, and fissioncollapse.
  
• Blackstellides collapse to blackholes of 2 solarmasses or more.
• Blackstellides semistabilise as a monocore nucleus, eventhorizon, and teelosphere.
• Blackstellides reactivate with sufficient further accretion.

• Galastellides are stellides that peakmass as galastars.
• Galastellides peakmass as galaxies of 45 solarmasses or more.
• Galastars form by the accretion of nucleons and nuclides.
• Galastellides form by the collapse of accreted nucleons and nuclides.
• Galastellide collapse mechanisms are gravitycollapse, emissioncollapse, fusioncollapse, ferriccollapse, fissioncollapse, and stellaspherecollapse.
• Galastellides collapse to blackholes of unknown mass.
• Galastellides semistabilise as a monocore nucleus, eventhorizon, and teelosphere.
• Galastellides reactivate with sufficient further accretion.
• Semistabilised galastellides are hypothetical objects.

• All types of stellide are fundamentally different only in the quantity of energy and gravitymass they accrete. The more they absorb, the more collapse mechanisms they undergo, and the more extreme is the resulting semistable stellide.

• The factbase for stellide interiors is sparse with many Current Paradigm hypotheses and theories having high naxosnumbers. By extension, the lack of facts means stellide naxosnumber counts in Core Physics are also uncomfortably high. Thus, the stellide descriptions in Core Physics must be considered taxonomically unsound until enough new facts can be established.

• Stellides accrete nucleons and nuclides in whatever form is available. Gas clouds are a source of nucleons. Smaller stellides are a source of nuclides for larger stellides. Notably, the stellaspheres of larger galastellides are observed to contain the accreted remains of smaller galastellides.

• In the Current Paradigm there is a disconnect between the masses of stellar blackholes (blackstellides) and supermassive blackholes (galastellides) suggesting suggests the latter could not achieve their present mass within the BBSM timeline. This and other instances in Core Physics do not fit the BBSM timeline suggesting that it will benefit from reconsideration, especially given that the BBSM timeline is a logictrap with no exit facts and a high naxosnumber count.

• Fissioncollapse as undergone by blackstars and galastars is not a part of the Current Paradigm.

• Four taxons -
• Protostars -
• Objects with an accreted nucleus and a lifecycle peakmassed for intrinsic mass contraction.
• Peakmass up to 0.8 of a solarmass.
  
• S1 stars -
• Objects with an accreted nucleus and a lifecycle peakmassed for emission contraction.
• Peakmass between 0.9 and 9.0 of a solarmass.
  
• S2 stars -
• Objects with an accreted nucleus and a lifecycle peakmassed for ferriccore contraction.
• Peakmass between 9.0 and 25 solarmasses.
• S3 stars -
• Objects with an accreted nucleus and a lifecycle peakmassed for chainreaction contraction.
• Peakmass between 25.0 and 40.0 solarmasses.

• Nucleus
  • Nucleons, isotopes, and molecules bound by mutual gravitypull.
  • With increasing star mass, molecules are broken to isotopes.
  • With increasing star mass, isotopes stratify by massdensity.
  • Stratification is by increasing massdensity from surface to centre.
• Atmosphere
  • Nucleons, isotopes, and molecules bound to the nucleus by its extrinsic gravitypull.
  • With increasing star mass, atmospheric objects stratify by massdensity 
  • Stratification is by increasing massdensity from atmosphere top to atmosphere bottom.
  • Stratification is fractured by turbulence.
• Teelosphere
  • The complexity and extent of star teelospheres increases with star mass.
  • Teelospheres are teelstream systems.
  • Low mass stars have centrifugal or chaotic teelospheres.
  • With increasing star mass there are regional axialities.
  • With increasing star mass there is overall axiality with regional centrifugality.

• Stars form and grow by accretion.
• Accretion adds energy and mass.
• Per the energy/mass differential, accretion adds more energy than mass.
  • Accreting stars are understable.
  • Accreting stars simultaneously undergo accretion expansion and stabilisation contraction.
• Rule of thumb:
  • Before peakmass, accretion expansion dominates stabilisation contraction.
  • After peakmass, stabilisation contraction dominates accretion expansion.
• Stars stabilise by stabilisation contraction.
• Additionally -
  • S1 stars stabilise by fusion, emission contraction, and ejection contraction.
  • S2 stars stabilise by fusion, emission/ejection contraction and ferriccore contraction.
  • S3 stars stabilise by fusion, emission/ejection contraction, ferriccore contraction, and chainreaction contraction.
• Stars stabilise as -
• Protostar blackdwarfs.
• S1 blackdwarfs.
• S2 blackdwarfs.
• S3 blackdwarfs.
• Less massive stars may be accreted by more massive stars before they stabilise.

• Stars stabilise by ejecting or emitting energyvelocity and massvelocity.
• Stabilisation happens because, per the energy/mass differential mechanism, more energyvelocity than massvelocity is ejected/emitted.
• • Emissions:
    • Electroids, photons, and subphotonics, emitted by engorged protons.
  • Ejections:
    • Subphotonics and superphotonics ejected during stabilisation contraction.
    • Subphotonics and superphotonics ejected by emission pressure.
  • • Subferric stratums ejected by ferriccore contraction.
    • Subfissile stratums ejected by chainreaction fission contraction.

• Star teelstream systems circulate through gasbonded and liquidbonded stratums.
• Teelstreams of sufficient momentum carry plasmatoids and are plasmastreams.
• Plasmastreams cross interfaces between stratums of different isotopes.
• The ability of isotopes to leave their own stratums is limited.
  • Thus isotopes influence the track of their plasmastreams.
  • Thus plasmastreams influence the track of their isotopes.
• The speed and density of plasmastreams increases with the axiality of their isotopes.

• Stars of sufficient mass have nucleonospheres.
• Nucleonospheres consist mainly of nucleons.
• Nucleonospheres are the outer atmosphere.
• Nucleonospheres consist of a neutronosphere inside a protonosphere.
  • Neutronospheres consist of neutrons.
  • Protonospheres consist of protons.
• Nucleonospheres consist of circulating plasmastreams.
  • Neutronosphere plasmastreams consist of engorged neutrons.
  • Protonosphere plasmastreams consist of engorged protons.
• Plasmastreams circulate across the neutronosphere/protonosphere interface.
• Plasmastream momentum increases with descent and vice versa.
• Nucleon engorgement increases with descent and vice versa.
  • Protons moving from protonosphere to neutronosphere transmute to neutrons.
  • Neutrons moving from neutronosphere to protonosphere transmute to protons.
• Major plasmastream upwells are visible as sunspots/starspots.
• Protons are strongly axial and neutrons are strongly centrifugal.
• Engorged neutrons do not emit photons.
• Engorged protons emit photons continuously and are a main source of photon emission.