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

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

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_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

Q_4_04 — Neutrino Astronomy and Neutrino Mass

Neutrinos — nearly massless, electrically neutral leptons that interact only via the weak nuclear force and gravity — are among the most abundant particles in the universe (~330/cm³ relic neutrinos from the Big Bang) yet

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_00 — Physics Methods: Subfolder Summary

Q_2_19 — Modified Gravity Theories: MOND, TeVeS & Alternatives to Dark Matter

Modified gravity theories propose that the observed discrepancies between predicted and measured gravitational effects in galaxies and galaxy clusters — conventionally attributed to dark matter — instead result from modi

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_14 — Gamma-Ray Bursts

Gamma-ray bursts (GRBs) are the most energetic electromagnetic events in the universe — brief, intense flashes of gamma radiation that, when corrected for beaming, release ~10⁴⁴–10⁴⁷ joules in seconds to minutes. First d

Q_2_18 — Neutrino Astronomy: Ghostly Messengers from the Cosmos

Neutrino astronomy — the observation of astrophysical sources through their neutrino emission rather than electromagnetic radiation — opened a new window on the universe by detecting particles that can escape from region

Q_3_20 — Exoplanet Atmospheres: Spectroscopy, Biosignatures & Habitability

The characterization of exoplanet atmospheres represents one of the most rapidly advancing frontiers in astrophysics, driven by the James Webb Space Telescope (JWST, launched December 25, 2021) and ground-based high-reso

Q_3_10 — Tidal Forces, Roche Limits, and Orbital Mechanics

Tidal forces — differential gravitational pulls across an extended body — and orbital mechanics — the motion of objects under gravitational influence — are fundamental physical phenomena governing everything from Earth's

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_07 — Plasma Cosmology and the Electric Universe Hypothesis

Plasma cosmology and its populist extension, the Electric Universe (EU) hypothesis, propose that electromagnetic forces — rather than gravity — are the dominant organizing force in the cosmos, and that plasma (ionized ga

Q_3_08 — Planetary Formation and Protoplanetary Disks

Planets form within protoplanetary disks — rotationally supported structures of gas and dust orbiting newly formed stars, with typical masses of 0.1–10% of the stellar mass, radii of 10–1000 AU, and lifetimes of ~1–10 mi

Q_3_00 — Planetary Solar Astrobiology: Subfolder Summary

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

ZA_2_20 — Dark Matter & Dark Energy

Approximately 95% of the universe's total energy content consists of two components that have never been directly detected: dark matter (~26.4%) and dark energy (~68.7%), with ordinary baryonic matter comprising only ~4.

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