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.
103 results for "SPECT prayer" — page 3 of 6
Q_1_15 — Dark Energy Models and Quintessence
The accelerating expansion of the universe, discovered in 1998 via Type Ia supernovae, demands an explanation. The simplest model — Einstein's cosmological constant Λ with equation of state $w = p/\rho = -1$ exactly — fi
Q_1_24 — Cosmic Microwave Background Deep Analysis
The Cosmic Microwave Background (CMB) is the oldest observable electromagnetic radiation in the universe — thermal radiation released approximately 380,000 years after the Big Bang (redshift z ≈ 1,100) when the universe
Q_1_20 — Fractal Cosmology: Is the Universe Self-Similar Across Scales?
The observable universe organises matter into a staggering fractal-like web of galaxy filaments, walls, voids, and clusters — structures visible at scales from 1 Mpc (galaxy groups) to 600 Mpc (the Hercules-Corona Boreal
Q_4_21 — Chromatography: Separation Science from Tswett to Modern Proteomics
Chromatography — the separation of mixtures by differential partitioning between a stationary phase and a mobile phase — is the most widely used analytical technique in chemistry, biology, and medicine. Mikhail Tswett (U
Q_2_11 — Stellar Populations, Metallicity, and Generations
Stars preserve the chemical fingerprint of the gas from which they formed, making them archaeological records of the universe's chemical history. Walter Baade (1944) recognized two distinct stellar populations: Populatio
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_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_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_12 — Telescope Technology and Observational Cosmology
The history of astronomy is inseparable from the history of telescope technology, and each major advance in instrumentation has triggered transformative discoveries. Galileo (1609) turned a simple refracting telescope to
Q_3_03 — Exoplanets, Habitable Zones, and the Search for Life
The discovery of exoplanets — worlds orbiting stars other than the Sun — has transformed astronomy from a field where planets were known only in our solar system to one cataloging over 5,700 confirmed exoplanets as of 20
ZC_1_10 — Environmental Psychology
Environmental psychology examines the transactions between individuals and their physical surroundings — how built and natural environments influence human behavior, cognition, emotion, and well-being, and reciprocally,
ZC_1_05 — Psychology of Religion & Spiritual Experience
The psychology of religion — the empirical study of religious and spiritual experience, belief, and behavior — was inaugurated by William James's The Varieties of Religious Experience (1902), which established that relig
ZC_1_07 — Behavioral Economics — Nudge Theory & Decision-Making
Behavioral economics integrates psychological insights into economic models of human decision-making, challenging the neoclassical assumption of perfectly rational "Homo economicus" and documenting systematic deviations
ZC_1_11 — Psychology of Time
The psychology of time encompasses how humans perceive duration, orient themselves across past-present-future, and how temporal cognition influences decision-making, memory, motivation, and well-being.
G_1_04 — Isotope Analysis and Provenance Studies
Isotope analysis — the measurement of ratios of stable or radiogenic isotopes preserved in human bone, tooth enamel, animal remains, ceramics, metals, and organic residues — has become one of the most powerful tools in m
G_1_03 — Remote Sensing Satellite Archaeology and Geophysics
Remote sensing and geophysical survey — the use of satellite imagery, airborne sensors, and ground-based electromagnetic instruments to detect buried or hidden archaeological features without excavation — has become one
G_1_02 — Digital Archaeology: LiDAR, Remote Sensing, GIS, and AI in Discovery
Digital archaeology encompasses a suite of non-invasive and computational technologies that have revolutionised how sites are discovered, documented, and interpreted. Airborne LiDAR has revealed entire cities beneath tro
G_1_06 — Paleoproteomics — Ancient Proteins Beyond DNA
Paleoproteomics is the extraction, identification, and analysis of ancient proteins from archaeological and paleontological materials — an emerging molecular method that extends biological identification far beyond the t
G_1_09 — Provenance Analysis: Strontium, Lead, and Oxygen Isotope Sourcing
Isotopic provenance analysis has revolutionized archaeology by enabling researchers to determine where an artifact was made, where a person grew up, what they ate, and how far they traveled — all from the chemical signat
G_3_10 — David Bohm's Implicate Order and Holographic Universe
David Bohm (1917–1992) was one of the most original and philosophically minded physicists of the 20th century, contributing both rigorous quantum mechanics and sweeping metaphysical visions. His pilot wave theory (1952)
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