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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.
25 results for "strong lensing" — page 1 of 2
ZA_2_16 — Gravitational Lensing: Bending Light, Dark Matter Mapping, and Cosmic Magnification
Gravitational lensing — the deflection and focusing of light from distant sources by the gravitational field of intervening mass — is one of the most powerful predictions of Einstein's general relativity and has become a
Q_3_04 — Gravitational Lensing: Bending Light and Mapping the Invisible Universe
Gravitational lensing — the bending of light by massive objects predicted by Einstein's general relativity — has become one of the most powerful observational tools in modern astrophysics. First confirmed during the 1919
Q_4_27 — QCD / Strong Force: Detailed Overview
Quantum chromodynamics (QCD) is the quantum field theory of the strong nuclear force — the fundamental interaction that binds quarks into protons, neutrons, and other hadrons, and binds protons and neutrons into atomic n
ZA_1_03 — Quantum Chromodynamics: The Strong Nuclear Force
Quantum chromodynamics (QCD) is the theory of the strong nuclear force — the interaction that binds quarks into protons and neutrons and holds atomic nuclei together. Unlike electromagnetism, the strong force is mediated
ZA_3_15 — Color Confinement: Why Quarks Are Never Found Alone
Color confinement — one of the most profound and still incompletely understood phenomena in theoretical physics — is the empirical fact and theoretical expectation that quarks and gluons, the fundamental carriers of colo
U_1_15 — Jazz: Improvisation, African Roots, and Cultural Revolution
Jazz — America's most original and influential art form — emerged in the early 20th century from the convergence of African rhythmic and improvisational traditions, African American blues and work songs, European harmony
Q_1_06 — Dark Matter and Dark Energy
Approximately 95% of the universe's total mass-energy content is invisible: ~27% dark matter and ~68% dark energy. Dark matter was first inferred by Fritz Zwicky (1933) from galaxy cluster dynamics and confirmed by Vera
Q_1_13 — Cosmic Strings and Topological Defects
Cosmic strings are one-dimensional topological defects that may have formed during symmetry-breaking phase transitions in the early universe, analogous to cracks in ice or vortex lines in superfluids. Predicted by Kibble
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_03 — General Relativity Tests and Confirmations
Albert Einstein's general theory of relativity (GR, 1915) has survived over a century of increasingly precise experimental tests, ranging from Solar System measurements to strong-field astrophysical observations. The cla
Q_4_01 — Primordial Gravitational Waves and B-Mode Polarization
Primordial gravitational waves — ripples in spacetime generated during cosmic inflation — represent one of the most sought-after signals in cosmology. Their detection would provide direct evidence that inflation occurred
Q_4_32 — The Fundamental Constants: Physics, Life, and Mathematics
The universe runs on numbers — and not arbitrary ones. A small set of fundamental constants, mostly dimensionless, determines every property of matter, energy, space, and time. Change any of them by a fraction and atoms
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_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
G_3_05 — Self-Organization and Emergence
Self-organization is the process by which global order arises from local interactions among components of an initially disordered system, without external direction or centralized control. Emergence is the closely relate
T_4_15 — The Psychology of Cooperation and Trust: Game Theory, Reciprocity, and Institutions
Cooperation — acting in ways that benefit others at a cost to oneself — is both theoretically puzzling (why would natural selection favor organisms that sacrifice fitness for others?) and practically essential (every hum
R_3_06 — Altruism and Cooperation in Nature
Altruism — behavior that reduces the actor's fitness while increasing the recipient's — presents a fundamental puzzle for evolutionary theory: how can natural selection favor genes that reduce their bearer's reproduction
ZA_2_08 — Modified Gravity Theories: MOND, f(R), and Alternatives to Dark Matter
Modified gravity theories attempt to explain the "missing mass" problem — the discrepancy between observed gravitational effects and visible matter — without invoking dark matter particles. The most empirically successfu
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
ZA_4_15 — Condensed Matter Physics: Emergent Phenomena in Many-Body Systems
Condensed matter physics — the largest subfield of physics by number of active researchers — studies the collective behavior of vast numbers of interacting particles (electrons, atoms, ions, spins) in solid, liquid, and
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