At the heart of every white dwarf star—the dense stellar object that remains after a star has burned away its fuel reserve of gases as it nears the end of its life cycle—lies a quantum conundrum: as white dwarfs add mass, they shrink in size, until they become so small and tightly compacted that they cannot sustain themselves, collapsing into a neutron star.
This puzzling relationship between a white dwarf’s mass and size, called the mass-radius relation, was first theorized by Nobel Prize-winning astrophysicist Subrahmanyan Chandrasekhar in the 1930s. Now, a team of Johns Hopkins astrophysicists has developed a method to observe the phenomenon itself using astronomical data collected by the Sloan Digital Sky Survey and a recent dataset released by the Gaia Space Observatory. The combined datasets provided more than 3,000 white dwarfs for the team to study.
(H) Om van complexe quantumfysica-materie hout te snijden is enige basiskennis vereist. Een prima plek om dit op te doen is: quantumuniverse.nl
Ik mag dan links over de materie dumpen, soms aangevuld met wat extra’s, maar weet en snap er niet veel van. Dus ben zelf ook begonnen met het spellen van een heldere serie daar, waarin de materie in vijftien stappen behandeld wordt, afgetrapt met,