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.
153 results for "dark matter alternative" — page 5 of 8
Q_1_01 — The Anthropic Principle & Fine-Tuning of the Universe
The universe appears to be astonishingly fine-tuned for the existence of complex life. Alter the cosmological constant by 1 part in 10¹²⁰, or the strong nuclear force by 0.5%, or the ratio of electromagnetic to gravitati
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
Q_2_13 — Interstellar Medium, Dust, and Nebulae
The space between stars is far from empty — the interstellar medium (ISM) is a complex, dynamic ecosystem of gas, dust, magnetic fields, and cosmic rays that pervades galaxies and plays a central role in stellar birth, d
Q_2_17 — Fermi Paradox Solutions Comprehensive
The Fermi Paradox — named after physicist Enrico Fermi's 1950 lunchtime remark "Where is everybody?" — captures the apparent contradiction between the high probability of extraterrestrial civilizations (given the ~200–40
Q_2_10 — Cosmic Voids and Large-Scale Structure
Cosmic voids are the most voluminous structures in the universe — vast, roughly spherical regions of space spanning 20–300 Mpc (65–1,000 million light-years) that contain far fewer galaxies than average. Together with fi
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_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
INTERDOC_18 — Volcanic Winter, the Bronze Age Collapse, and Civilizational Fragility
The Thera eruption (Santorini, ~1628 BCE or ~1530 BCE — dating remains contested) ejected an estimated 60 km³ of material — four times the volume of Krakatoa (1883). Ice core evidence from Greenland (GISP2) and tree-ring
INTERDOC_04 — Catastrophe-Migration-Civilization Cycle
The archaeological and paleoclimatic record reveals at least five major catastrophe-migration cycles in the last ~75,000 years, each following a recognizable pattern: a sudden environmental shock (volcanic eruption, cosm
INTERDOC_64 — Cross-Cultural Constellations: Independent Invention vs. Diffusion as a Knowledge-Transmission Probe
The 88 modern IAU constellations are a cultural product — 48 from Ptolemy (~150 CE, derived from Mesopotamian/Babylonian sources), 12 from Keyser and de Houtman (~1596, Dutch East Indies), and 28 filled in by 17th–18th c
ZB_5_13 — Ecological Economics: Valuing Nature's Services
Ecological economics is a transdisciplinary field that treats the human economy as a subsystem embedded within — and fundamentally dependent upon — the finite biophysical systems of the Earth, challenging the neoclassica
ZC_1_09 — Psychology of Leadership
Leadership psychology investigates the traits, behaviors, and situations that enable individuals to influence, motivate, and direct others toward collective goals — one of the most extensively studied and practically imp
ZC_4_05 — Tourism, Heritage, and the Anthropology of Sacred Sites
The anthropology of tourism and heritage examines how places, objects, and practices are designated as culturally significant, how they are consumed by visitors, and who controls the narratives, profits, and meanings at
G_4_08 — Graham Hancock — Data-Driven Evaluation of Claims
Graham Hancock (b. 1950, Edinburgh) is a British journalist and author who has become the most prominent advocate of the "lost civilization" hypothesis — the idea that an advanced civilization existed before the end of t
O_2_06 — Richat Structure — Saharan Eye and Atlantis Claims
The Richat Structure (also called the Eye of the Sahara or Guelb er Richat) is a prominent circular geological formation approximately 40–50 km in diameter located on the Adrar Plateau in west-central Mauritania (21°07′N
T_2_20 — Personality Disorders: Cluster Analysis and Dimensional Models
Personality disorders (PDs) — enduring patterns of inner experience and behavior that deviate markedly from cultural expectations, are pervasive and inflexible, and cause significant functional impairment — affect approx
T_2_22 — Psychopathy Neuroscience
Psychopathy is a personality disorder characterized by persistent antisocial behavior, impaired empathy and remorse, bold and disinhibited traits, and often superficial charm — affecting an estimated 1% of the general po
T_1_08 — Personality Psychology and the Big Five
Personality psychology seeks to understand individual differences in characteristic patterns of thinking, feeling, and behaving — and why these patterns remain relatively stable across time and situations.
T_3_10 — Psychology of Humor and Laughter
Humor and laughter are universal human behaviors found across all known cultures and appearing early in development (social smiling by 6–8 weeks, laughter by 3–4 months). Three classical theories dominate the field: Supe
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