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Search 3,721 documents across 34 fields — every claim tier-rated by evidence
3,633 are the core, quality-scored corpus (34 lettered sections — see How We Work); the remaining 88 are cross-corpus synthesis documents (68 InterDocs, 12 Connections, 8 Theories) also indexed here.
28 results for "supernova nucleosynthesis" — page 2 of 2
Q_2_03 — Cosmic Rays and High-Energy Astrophysics
Cosmic rays — high-energy particles from space, mostly protons and atomic nuclei — were discovered by Victor Hess in 1912 via balloon flights that measured ionization increasing with altitude, earning him the Nobel Prize
Q_2_14 — Gamma-Ray Bursts
Gamma-ray bursts (GRBs) are the most energetic electromagnetic events in the universe — brief, intense flashes of gamma radiation that, when corrected for beaming, release ~10⁴⁴–10⁴⁷ joules in seconds to minutes. First d
Q_2_18 — Neutrino Astronomy: Ghostly Messengers from the Cosmos
Neutrino astronomy — the observation of astrophysical sources through their neutrino emission rather than electromagnetic radiation — opened a new window on the universe by detecting particles that can escape from region
Q_3_11 — Cosmic Reionization and First Stars
The Epoch of Reionization (EoR) refers to the period in cosmic history (~150 million to ~1 billion years after the Big Bang, redshifts z ≈ 15–6) when the first luminous sources — Population III (Pop III) stars, early gal
Q_3_16 — Cosmochemistry: Meteorite Analysis, Presolar Grains, and Solar Composition
Cosmochemistry is the study of the chemical composition of the universe and the processes that produced it, with a primary focus on the analysis of meteorites — extraterrestrial rocks that survive passage through Earth's
ZA_2_18 — Dark Energy Mechanisms: Cosmological Constant, Quintessence, and the Accelerating Universe
Dark energy — the unknown agent driving the accelerating expansion of the universe — constitutes approximately 68.3% of the total energy density of the cosmos (Planck 2018 results), making it the dominant component of th
ZA_1_18 — Dark Energy and the Cosmological Constant Problem
Dark energy — the mysterious component constituting ~68% of the total energy density of the observable universe — drives the accelerating expansion of space and represents one of the deepest unsolved problems in physics.
ZA_3_03 — Nuclear Physics: Fission, Fusion, and the Heart of Matter
Nuclear physics studies the atomic nucleus — the dense core of protons and neutrons bound by the strong nuclear force, containing 99.95% of an atom's mass in just 10⁻¹⁵ meters. The field revealed that mass can be convert
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