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Cosmic Kitchen: Nuclear Pasta in the Depths of Stars ⚡ экспресс

Original: "Nuclear Pasta and Crustal Quasi-Periodic Oscillations in Neutron Star"
· Vishal Parmar, Ignazio Bombaci
arXiv:2602.19125 · 2026-02-22 · CC BY 4.0 · ⏱ 1 min · Nuclear Theory High Energy Stellar
Deep inside neutron stars, atoms fuse into macaroni-like strands: this nuclear pasta makes the star tremble and reveals the secrets of its pulses.
Abstract

Scientists built a Bayesian ensemble of neutron star models and showed that exotic nuclear pasta (matter in the shape of spheres, rods, layers) in the crust arises mainly under certain properties of nuclear forces. The transition from spheres to rods is squeezed into a narrow density interval (0.0588 fm⁻³), and the thickness of the pasta is only 14% of the crust, but its mass is almost half. These layers influence the frequencies of starquakes (QPOs), which strongly depend on the curvature of the symmetry energy. Just as you can tell how well bread is baked by the crunch of its crust, so the star's tremors reveal the composition of its interior. This will help astrophysicists interpret observations.

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Long before that, Fritz Zwicky predicted that a supernova explosion gives birth to a tiny neutron star. Years later, Jocelyn Bell Burnell caught its pulses, discovering pulsars. Now we know that inside these stars is a true culinary spectacle: atomic nuclei stretch into spaghetti, layer up like lasagna, and clump into gnocchi. They call it nuclear pasta.

A layer of this pasta is the strongest material in the Universe: a piece as thin as paper could support the weight of an entire planet.

A recent study, combining nuclear models and data on gravitational waves, showed that the transition from round nuclei to strands happens at the exact same density, as if nature follows a recipe. The pasta layer is only 14% of the crust's thickness but packs nearly half its mass. These layers make the star tremble at specific frequencies, and astronomers see this trembling as the flickering of pulsars. For the first time, scientists matched calculated frequencies with real observations and found that the rhythm of the tremors reveals properties of nuclear forces—a sort of stellar seismology.

But the most unexpected twist: this nuclear pasta might explain the mysterious 'glitches' in pulsar flickers, when their pulse suddenly skips a beat. Perhaps the pasta's trembling triggers abrupt shifts that astronomers have been catching for half a century.

🎯 "Nuclear pasta" isn't a figure of speech—it's a precise term. The layers really do resemble spaghetti, lasagna, and gnocchi. But they're so strong that a strand as thin as a human hair could support the weight of a metropolis.

Scientists
Bernhard RiemannJoseph WeberKarl SchwarzschildKip ThorneRainer WeissEnrico Fermi
Tags
neutron star supernova gravitational waves pulsar
Laws
Einstein field equationsFermi–Dirac statisticsChandrasekhar limitFermi accelerationlaw of conservation of momentumquadrupole radiation formula
Original: arXiv:2602.19125 · CC BY 4.0 · bridge42worlds