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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.
192 results for "neutron star matter" — page 1 of 10
ZA_3_18 — Quark-Gluon Plasma and Exotic Matter States
Quark-gluon plasma (QGP) — a deconfined state of matter in which quarks and gluons, normally bound inside protons and neutrons by the strong nuclear force (quantum chromodynamics, QCD), roam freely over extended volumes
ZA_3_17 — Exotic Matter States: Quark-Gluon Plasma, Strange Matter, and Extreme Condensates
Exotic matter states — forms of matter that exist under conditions of extreme temperature, density, or quantum degeneracy far beyond everyday experience — reveal the fundamental structure of matter and the behavior of qu
Q_2_02 — Neutron Stars, Pulsars, and Extreme Physics
Neutron stars are the collapsed remnants of massive stars, packing 1.4 to approximately 2.1 solar masses into a sphere roughly 20 kilometers across — reaching densities of 10¹⁷ kg/m³, where a teaspoon of material would w
Q_4_16 — Chandrasekhar Limit: White Dwarf Physics and Stellar Death
The Chandrasekhar limit — approximately 1.4 solar masses ($1.4 \, M_\odot$) — is the maximum mass of a stable white dwarf star, the dense remnant left after a low- or intermediate-mass star (initial mass up to ~8 $M_\odo
ZA_2_02 — Gravity, Gravitational Waves, and Anomalous Gravitational Claims
Gravity — the weakest of the four fundamental forces yet the dominant force at cosmic scales — remains the most mysterious force in physics. Newton's law of universal gravitation (1687) described gravitational attraction
Q_2_15 — Magnetars and Fast Radio Bursts
Magnetars are neutron stars with ultra-strong magnetic fields (B ~ 10¹³–10¹⁵ gauss — a thousand times stronger than typical radio pulsars and ~10¹⁰ times the strongest laboratory magnets), powered not by rotation (as wit
Q_2_09 — Binary Star Systems and X-Ray Sources
Most stars in the Milky Way exist in binary or multiple-star systems — estimates range from ~50% for solar-type stars to >70% for massive O/B stars. Binary star interactions drive some of the most energetic phenomena in
Q_2_04 — Stellar Evolution: The Life Cycle of Stars
Stars are born in collapsing molecular clouds, live by nuclear fusion for millions to trillions of years, and die in ways determined almost entirely by their initial mass. Low-mass stars (< 8 M☉) shed their outer layers
ZH_4_18 — Indigenous Star Map Catalog
Indigenous star map systems — the astronomical knowledge embedded in the oral traditions, navigation practices, ceremonial calendars, and landscape relationships of non-Western cultures — represent a vast but systematica
ZH_3_16 — Polynesian Star Compass: Celestial Navigation of the Pacific
The Polynesian star compass represents one of humanity's most sophisticated non-instrument navigation systems — enabling deliberate, repeatable voyages across thousands of miles of open Pacific Ocean centuries before Eur
ZH_5_17 — Ancient Variable Star Observations (Algol)
Algol (Beta Persei, the "Demon Star") — a second-magnitude eclipsing binary star in the constellation Perseus that dims dramatically every 2.867 days as its fainter companion transits the primary star — may have been rec
ZH_2_03 — Islamic Golden Age Astronomy: Observatories and Star Catalogs
Islamic astronomy (c. 750–1500 CE) represents one of the most productive and sophisticated periods in the history of astronomical science — a sustained tradition of observation, mathematical innovation, and critical enga
ZH_1_15 — Star Catalogs: From Hipparchus to Hipparcos and the Tycho Catalog
A star catalog — a systematic list of stars with their positions, magnitudes, and sometimes colors, proper motions, and spectral types — is the foundational document of observational astronomy. The compilation of ever mo
ZH_1_04 — Nebra Sky Disk: Bronze Age Star Map Analysis
The Nebra sky disk (Himmelsscheibe von Nebra) is a bronze disk approximately 30 cm in diameter, decorated with gold-leaf appliqué representing the sun (or full moon), a crescent moon, stars (including a cluster interpret
ZH_1_22 — Egyptian Star Ceilings
Egyptian star ceilings — elaborate astronomical paintings and carvings on the ceilings of tombs, temples, and coffin lids spanning over 2,000 years of Egyptian civilization — constitute the largest and most continuous bo
ZH_1_02 — Egyptian Astronomy: Decans, Star Clocks, Pyramid Orientation
Ancient Egypt developed one of the most sophisticated astronomical traditions of the pre-telescopic world, integrating celestial observation into timekeeping, calendar construction, temple orientation, and funerary cosmo
C_5_30 — Star People Origins: Celestial Ancestry Myths Worldwide
Traditions of celestial ancestry — the belief that humanity, or a founding lineage, originated from or was taught by beings from specific stars or constellations — are found across dozens of cultures worldwide. The Dogon
E_1_14 — Supernovae in Human History: Crab Nebula, SN 1006, Vela
Supernovae — the catastrophic explosions of massive stars (core-collapse, Type II/Ib/Ic) or white dwarfs exceeding the Chandrasekhar mass limit (thermonuclear, Type Ia) — are among the most energetic events in the univer
Q_1_17 — Modified Gravity Theories (MOND, TeVeS, and Alternatives to Dark Matter)
Modified Newtonian Dynamics (MOND) is a hypothesis proposed by Mordehai Milgrom in 1983 that modifies Newton's second law at very low accelerations (below approximately 1.2 × 10⁻¹⁰ m/s²) to explain galaxy rotation curves
Q_4_02 — Gravitational Wave Astronomy
Gravitational waves — ripples in spacetime predicted by Einstein's general relativity (1916) and first directly detected by LIGO (Laser Interferometer Gravitational-Wave Observatory) on September 14, 2015 (event GW150914
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