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The Physics of Core-Collapse Supernovae

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arxiv astro-ph/0601261 v1 pith:GCI4DHUF submitted 2006-01-12 astro-ph

classification astro-ph
keywords explosionssupernovaeachievablearguedastrophysicalbeencarbonclear
verification ladder T0 review T1 audit T2 compute T3 formal
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Supernovae are nature's grandest explosions and an astrophysical laboratory in which unique conditions exist that are not achievable on Earth. They are also the furnaces in which most of the elements heavier than carbon have been forged. Scientists have argued for decades about the physical mechanism responsible for these explosions. It is clear that the ultimate energy source is gravity, but the relative roles of neutrinos, fluid instabilities, rotation and magnetic fields continue to be debated.

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Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Wild behaviour near the finish line: the Type Ibn SN 2020able and its stratified environment

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    The Type Ibn supernova SN 2020able exploded inside a stratified, three-component helium-rich envelope, with an inner dense shell from a pre-explosion eruption and an outer shell consistent with a Wolf-Rayet wind.

  2. Implications of the UV/optical Plateau of AT2018cow

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    A wind-and-irradiation disk model fits the AT2018cow UV plateau with accretor masses from 1.4 to ~100 solar masses, removing the need for a >200 solar-mass black hole.

  3. OCCAM X. Neutron Capture Abundances with Keck/HIRES & Magellan/MIKE

    astro-ph.GA 2026-07 unverdicted novelty 5.0 of 10

    New high-resolution spectra yield abundances for 7 neutron-capture elements in open cluster stars, revealing flat Milky Way gradients for second-peak s- and r-process species and shallower slopes for first-peak s-process.

  4. SN 2025aico: Early observations of a faint Type IIb supernova with a low-mass envelope

    astro-ph.SR 2026-07 accept novelty 4.0 of 10

    SN 2025aico is a low-luminosity Type IIb from a compact He star (M_env≈0.01 M⊙, R_env≈6–10 R⊙) with M_Ni≈0.033 M⊙, M_ej≈2.8 M⊙ and weak-to-moderate 56Ni mixing.

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