Buoyant crystals halt the cooling of white dwarf stars

Antoine Bédard (), Simon Blouin () and Sihao Cheng
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Antoine Bédard: University of Warwick
Simon Blouin: University of Victoria
Sihao Cheng: Institute for Advanced Study

Nature, 2024, vol. 627, issue 8003, 286-288

Abstract: Abstract White dwarfs are stellar remnants devoid of a nuclear energy source, gradually cooling over billions of years1,2 and eventually freezing into a solid state from the inside out3,4. Recently, it was discovered that a population of freezing white dwarfs maintains a constant luminosity for a duration comparable with the age of the universe5, signalling the presence of a powerful, yet unknown, energy source that inhibits the cooling. For certain core compositions, the freezing process is predicted to trigger a solid–liquid distillation mechanism, owing to the solid phase being depleted in heavy impurities6–8. The crystals thus formed are buoyant and float up, thereby displacing heavier liquid downward and releasing gravitational energy. Here we show that distillation interrupts the cooling for billions of years and explains all the observational properties of the unusual delayed population. With a steady luminosity surpassing that of some main-sequence stars, these white dwarfs defy their conventional portrayal as dead stars. Our results highlight the existence of peculiar merger remnants9,10 and have profound implications for the use of white dwarfs in dating stellar populations11,12.

Date: 2024
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DOI: 10.1038/s41586-024-07102-y

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