COREPHYSICS

• Dwarfstellides are stable stellides that peakmassed as dwarfstars.
• Dwarfstellides peakmassed between 0.8 and 9 solarmasses.
• Dwarfstars form primarily by the accretion of nucleons and nuclides..
• Dwarfstellides form by the collapse of accreted nucleons and nuclides.
• Dwarfstellides are a monocore nucleus inside a teelosphere inside a gravitysheath inside a gravitysheath interface.
• Dwarfstellides may or may not have an atmosphere.
  
• Dwarfstellides reactivate with sufficient further accretion.

• Dwarfstars are understable dwarfstellides.
• Dwarfstar primary content is nucleons and nuclides.
• Dwarfstars are a nucleus inside a substrate inside an atmosphere inside a teelosphere inside a gravitysheath inside a gravitysheath interface.
• Dwarfstars peakmass between 0.8 and 9 solarmasses.
• Dwarfstars undergo nucleon and nuclide collapse during semistabilisation.
• Dwarfstar collapses are gravitycollapse, emissioncollapse, and fusioncollapse.

• Dwarfstars semistabilise as dwarfstellides.
• Semistabilisation is achieved by ejecting more gravitymassvelocity than is absorbed.
• Gravitymassvelocity ejection is by proton emission, substrate ejection, and teel ejection.
• Gravitymassvelocity ejections are triggered by gravitycollapse, emissioncollapse, and fusioncollapse.
• Gravitycollapse is dwarfstar contraction by teelstream and solarwind ejection.
• Emissioncollapse is contraction of protons and nuclides by photon emission.
• Fusioncollapse is contraction of nuclide stratums post nuclide fusions.
• Nuclides stratify by isotopenumber as conditions dictate.
• Stratification is lowest isotopenumber outer to highest isotopenumber inner.
• Dwarfstars stratify by mechanisms and content.
• Stratums are photosphere, neutronosphere, primasphere, lithisphere.

• Dwarfstars may or may not have a solidbonded nuclide core in the nucleus.
• Dwarfstar atmospheres are stratified as conditions dictate.
• Stratification is by mechanism and primary content.
• Stratums are photosphere, neutronosphere, primasphere, and lithisphere.

• Photospheres are the outer stratum of a dwarfstar atmosphere.
• Photospheres include for simplicity coronas and chromospheres.
• Primary photosphere content is engorged protons.
• Engorged protons emit fundamides, photides, and electrons.
• A proportion of proton emissions escape from the dwarfstar.
• Emission escape is emissioncollapse for the dwarfstar.

• Neutronosphere are the stratum below the photosphere and above the primasphere.
• Primary neutronosphere content is engorged neutrons.
• Neutrons rise from neutronosphere to photosphere transmuting to protons.
• Protons fall from photosphere to neutronosphere transmuting to neutrons.
• Neutrons fall from neutronosphere to primasphere becoming stripped.
• Stripped neutrons rise from primasphere to neutronosphere becoming engorged.

• Primaspheres are the stratum below the neutronosphere and above the lithisphere.
• Primary primasphere content is engorged primalnuclides.
• Primalnuclides are the elements deuterium and helium.
• Primalnuclides are elementnumbers 2 and 3.
• Deuterium isotopes are fused from stripped neutrons.
• Isotope Deuterium-3 (tritium) transmutes to isotope Helium-3 (tralphium).
• Tralphiums directly manufacture neutrons.
• Tralphiums indirectly manufacture heliums with higher isotopenumbers.
• Indirect helium manufacture is by captive emission.
• Indirectly manufactured Helium-6 and Helium-8 are understable and transmute to lithiums.
• Neutrons rise from primasphere to neutronosphere becoming engorged.
• Stripped objects fall from primasphere to lithisphere.
• Lithiums fall from primasphere to lithisphere.

• Lithispheres are the stratum below the primasphere and are the dwarfstar core.
• Primary lithisphere content is lithicnuclides.
• Lithicnuclides are the elements lithium to manganese.
• Lithicnuclides are elementnumbers 3 to 25.
• Lithispheres are where lithicnuclides fuse with stripped objects.
• Lithicnuclide fusions result in isotopenumber increases.
• Peak isotopenumber achieved corresponds to dwarfstar peakmass achieved.

• Dwarfstar substrate content is fundamides, photides, and morphides.
• Primary content is emitted or ejected by nucleons /nuclides.
• Secondary content is stripped neutrons and stripped primalnuclides.
• Secondary content is downdrawn by dwarfstar intrinsic gravitypull.
• Substrate content moves through and between nucleon /nuclide teelospheres.
• Substrate content may or may not be carried along by teelstream systems.
• Substrate heft is increased by ejections /emissions from nucleons  /nuclides.
• Increasing substrate heft decreases nucleon /nuclide packingdensity.
• Substrate heft is decreased by absorption into nucleons /nuclides.
• Decreasing substrate heft increases nucleon /nuclide packingdensity.
• Substrate content contributes to nucleon /nuclide engorgement.
• Engorged objects attune to substrate /teelstream heft.
• Increasing substrate heft pushes substrate content toward dwarfstar surface.
• Gravitycollapse pushes substrate content toward dwarfstar surface.
• Emissioncollapse pushes substrate content toward dwarfstar surface.
• Fusioncollapse pushes substrate content toward dwarfstar surface.
• Substrate heft dominates collapse before dwarfstar peakmass.
• Collapse dominates substrate heft after dwarfstar peakmass.

• Teelospheres are teelstream systems coursing through a dwarfstar.
• Teelstream systems are primarily driven by dwarfstar spin.
• Teelstream systems can be axial, centrifugal, chaotic, or a mix.
• Teelstream systems are local and global.
• Local systems are confined to a stratum or region.
• Global systems move to and from dwarfstar centre to dwarfstar gravitysheath interface.
• Global teelstreams eject teels across the gravitysheath interface.
• Teelstreams engorge dwarfstar morphides and nuclides.
• Teelstreams cationise dwarfstar axial morphides and nuclides.
• Teelstreams may or may not carry along substrate.
• Teelstreams may or may not carry along morphides and nuclides as a plasmastream.

• Fusion continues throughout the life of a dwarfstar.
• Fusion is stripped object to stripped object.
• Fusion is stripped object to nuclide.
• Stripped objects have reduced teelosphere extent.
• Reduced teelosphere extent eases fusion with other stripped objects.
• Reduced teelosphere extent eases fusion with nuclides.
• Nuclides are cationised by teelstreams.
• Cationised nuclides are less able to resist fusion with stripped objects.

• Fusioncollapse is primarily in the lithisphere.
• Fusioncollapse is secondarily in the primasphere.
• Lithisphere /primasphere nuclides are engorged and understable.
• Nuclides attune to substrate /teelstream heft.
• Nuclides stratify by isotopenumber as conditions dictate.
• Stratification is outer lowest to inner highest isotopenumber.
• Fusion events increase nuclide isotopenumbers.
• Fusion events eject more gravitymassvelocity than is absorbed.
• Thus increasing isotopenumbers equate to decreasing nuclide understability.
• Fusion events unattune nuclide to substrate /teelstream heft.
• Thus nuclides eject /emit until attuned to substrate /teelstream heft.
• Successive fusion events eject /emit less content into the substrate.
• Reduced substrate content reduces substrate heft.
• Reduced substrate heft allows potential nuclide packing density increase.
• Dwarfstar intrinsic gravitypull draws nuclides downward.
• Dwarfstar intrinsic gravitypull transmutes packingdensity potential to packingdensity extant.
• Increasing nuclide packingdensity decreases dwarfstar atmosphere volume.
• Decreasing atmosphere volume is fusioncollapse.
• Final possible dwarfstar nuclide fusions are to manganese isotopes.
• Fusions beyond manganese result in overstable nuclides.

• Dwarfstars in which fusion ceases become whitedwarfs.
• A proportion of whitedwarf nuclides are still understable and unattuned to substrate /teelstream heft.
• Emissioncollapse and gravitycollapse continues.
• Contraction continues.
• Nuclides at the centre liquidbond and solidbond.
• Liquidbonding /solidbonding extends outward.
• Liquidbonding /solidbonding ceases when emissioncollapse, substrate ejection, and teel ejection has ceased.
• The whitedwarf has semistabilised as a dwarfstellide.

• S1 stars -
•  Dwarfstars -
• Peakmass between 0.8 and 1.4 solarmasses approximately.
• Stabilise as cold blackdwarfs.
• Giantstars -
• Peakmass between 1.4 and 9.0 solarmasses approximately.
• stabilise as cold blackdwarfs.

• Nucleus -
• Isotopes stratified by increasing massdensity from surface to centre. 
• The greater the peakmass of the S1 star, the greater the mass of the isotopes that can be fused.
• Atmosphere -
• Nucleons, isotopes, and molecules stratified by massdensity from the surface inward, turbulence permitting.
• Teelosphere -
• Locally centrifugal, globally axial.

• S1 stars form by accretion.
• S1 stars simultaneously undergo -
• Accretion expansion.
• Stabilisation contraction.
  • Before peakmass -
  • Accretion expansion dominates stabilisation contraction.
  • After peakmass -
  • Stabilisation contraction dominates accretion expansion.
• Dwarfstar stabilisation is as cold blackdwarfs.
• Giantstars stabilisation is as whitedwarfs and then as cold blackdwarfs.

• S1 stars stabilise by emission and ejection -
  • Emission:
  • Photons emitted by engorged nucleons and isotopes.
  • Photons emitted by fusing nucleons and isotopes.
  • Ejection:
  • Teels ejected by stabilisation contraction.
  • Electroids, nucleons, and isotopes ejected by emission pressure.

• S1 star interiors are circulating plasmastreams.
• S1 star isotopes are stratified inwardly by increasing massdensity.
• Plasmastream circulations are vertical, horizontal, and often vortexed.
• Plasmastreams cross the interfaces between isotope stratums.
• Isotopes move with plasmastreams but their ability to move out of their stratums is limited.
• Plasmastream circulations are influenced but not dominated by the isotopes in them.
• Isotope circulations are influenced but not dominated by the plasmastreams they are within.

• S1 star fuse stratums of ferric isotopes inside their stratums of subferric isotopes.
  • Ferric isotopes are more massive than subferric isotopes.
  • Ferric isotope pairs have greater mutual gravitypull than pairs of subferric isotopes.
  • Ferric isotopes, mass for mass, emit less emission pressure than subferric isotopes.
• Consequently S1 stars undergo ferric core contraction:
  • The ferric core volume progressively decreases.
  • The packing density of the ferric core progressively increases.
  • The ferric core's contraction rate progressively increases
  • The rate at which isotopes in the ferric core fuse and/or accrete progressively increases.
• S1 star contraction rates increase with S1 star peakmass.
• Contraction reduces the space between the isotope nuclei.
• The reduced space compresses the isotope teelospheres.
• Teelosphere teels are ejected from the ferric core into the subferric stratums.
• Some or all of the subferric stratums are expelled from the S1 star.
• The proportion of the subferric stratums that are expelled rises with S1 star peakmass.

• The photosphere consists of protons.
• The protons are understable.
• The protons are emitting photons and subphotonics.
• The photons and the subphotonics are emission pressure.
• The emission pressure is such that the photosphere is chaotic.
• The emission pressure is in all directions.
• The chaotic photosphere is only regionally plasmatised and magnetised.
• The regional plasmatisation and magnetisation makes the intensity of the downward emission variable.
• Thus there are weakspots in the photosphere/neutronosphere interface.
• Neutron plasmas force through the weakspots as sunspots.