RESEARCH BASE
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.
1,812 results for "Friday the 13th" — page 17 of 91
J_1_11 — Antikythera Mechanism and Ancient Computing Devices
The Antikythera Mechanism — recovered in 1901 from a Roman-era shipwreck off the Greek island of Antikythera (dated to c. 70–60 BCE by ceramic and coin evidence; the device itself likely constructed c. 150–100 BCE) — is
J_5_13 — Mesopotamian Technology Survey: Innovations of the Fertile Crescent
Mesopotamia — the land between the Tigris and Euphrates rivers (modern Iraq, northeastern Syria, southeastern Turkey, southwestern Iran) — is often called the "Cradle of Civilization," and the claim is justified not mere
TH_04 — The Suppression Convergence Pattern
That powerful groups burn books and bury inconvenient ideas is old news. What this theory notices is stranger: across civilizations that never met — imperial China, the medieval Church, the Maya, modern states — they rea
TH_03 — The Fibonacci Inevitability Principle
You've probably seen the claim that one special number — the "golden ratio," about 1.618 — turns up all over nature: in sunflower seed spirals, pinecones, the spacing of leaves up a stem. It's usually sold as a mystical
TH_02 — The Metabolic Consciousness Threshold
Here's a question that sounds purely philosophical but might actually have a number for an answer: how much energy does it take to be conscious? This theory says there's a floor — a minimum amount of power a system must
TH_06 — The Dislocated Consciousness Hypothesis
Almost nobody seriously doubts that people experience ghosts — the felt presence, the figure on the stair, the certainty of being watched. The real question is what produces those experiences, and the honest answer is th
Q_4_09 — Statistical Mechanics: Boltzmann, Ensembles, and Thermodynamic Emergence
Statistical mechanics is the bridge between the microscopic world of atoms and molecules (governed by classical or quantum mechanics) and the macroscopic world of thermodynamics (governed by temperature, pressure, entrop
Q_4_20 — Catalysis: From Haber-Bosch to Asymmetric Synthesis
Catalysis — the acceleration of a chemical reaction by a substance (the catalyst) that is not consumed in the process — accounts for over 90% of all industrial chemical processes and has earned more Nobel Prizes than any
Q_4_13 — Classical Mechanics: Newton, Lagrange, Hamilton, and the Action Principle
Classical mechanics — the study of the motion of bodies under the action of forces — is the oldest and most mature branch of physics, tracing from Galileo's kinematics (1638) and Newton's three laws and universal gravita
Q_2_12 — Cosmic Nucleosynthesis and Primordial Helium Abundance
Big Bang nucleosynthesis (BBN) — the formation of the lightest elements during the first ~20 minutes after the Big Bang — stands as one of the most remarkable quantitative successes of modern cosmology. With only one fre
Q_2_06 — Nucleosynthesis: How the Elements Were Forged
Every element in the periodic table has a specific cosmic origin story. Big Bang nucleosynthesis (BBN) produced hydrogen, helium, and traces of lithium in the first 20 minutes after the Big Bang. Stellar nucleosynthesis
Q_2_07 — Cosmic Distance Ladder: Measuring the Universe
The cosmic distance ladder is a succession of techniques by which astronomers measure distances from nearby stars to the edge of the observable universe — each rung calibrates the next. Trigonometric parallax (reliable t
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
Q_3_05 — Olbers' Paradox and the Dark Night Sky
Olbers' paradox — named after German astronomer Heinrich Olbers (1826), though discussed earlier by Kepler (1610), Halley (1720), and de Chéseaux (1744) — asks: if the universe is infinite, static, and uniformly filled w
Q_3_01 — The Fermi Paradox & Drake Equation
Enrico Fermi's 1950 lunch question — "Where is everybody?" — remains one of the deepest unanswered questions in science. The galaxy is ~13.6 billion years old, contains ~100–400 billion stars, and (as we now know from Ke
Q_3_19 — The Fermi Paradox: A Catalog of Proposed Solutions
The Fermi Paradox — the apparent contradiction between the high probability of extraterrestrial civilizations (given ~200–400 billion stars in the Milky Way, with ~20% harboring Earth-like planets in habitable zones) and
Q_3_02 — Ancient-Modern Scientific Parallels Synthesis
Every major ancient cosmological tradition contains concepts that map remarkably onto modern scientific discoveries. From the Hindu kalpa aligning within 5% of Earth's actual age, to the universal "cosmic egg" motif mirr
ZB_2_14 — Photosynthesis Evolution and Diversity
Photosynthesis — the conversion of light energy into chemical energy — is arguably the most important biochemical process on Earth, responsible for virtually all atmospheric oxygen and the primary energy input for nearly
ZB_2_18 — Phage-Bacteria Coevolution: Arms Races in the Microbial World
Bacteriophages (phages) — viruses that infect and replicate within bacteria — are the most abundant biological entities on Earth (~10³¹ total particles, outnumbering bacteria ~10:1 in most environments), and their coevol
ZB_5_28 — Photosynthesis: Light Harvesting, Carbon Fixation, and the Bioenergetic Foundation of Life
Photosynthesis — the conversion of light energy into chemical energy by living organisms — is the bioenergetic foundation of virtually all life on Earth, fixing approximately 120 billion tonnes of carbon annually and pro
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