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  2. Quantum field theory in curved spacetime - Wikipedia

    en.wikipedia.org/wiki/Quantum_field_theory_in...

    In theoretical physics, quantum field theory in curved spacetime (QFTCS) [1] is an extension of quantum field theory from Minkowski spacetime to a general curved spacetime. This theory uses a semi-classical approach; it treats spacetime as a fixed, classical background, while giving a quantum-mechanical description of the matter and energy ...

  3. Synge's world function - Wikipedia

    en.wikipedia.org/wiki/Synge's_world_function

    In general relativity, Synge's world function is a smooth locally defined function of pairs of points in a smooth spacetime with smooth Lorentzian metric.Let , ′ be two points in spacetime, and suppose belongs to a convex normal neighborhood of , ′ (referred to the Levi-Civita connection associated to ) so that there exists a unique geodesic from to ′ included in , up to the affine ...

  4. Mikheyev–Smirnov–Wolfenstein effect - Wikipedia

    en.wikipedia.org/wiki/Mikheyev–Smirnov...

    The Mikheyev–Smirnov–Wolfenstein effect (often referred to as the matter effect) is a particle physics process which modifies neutrino oscillations in matter of varying density. The MSW effect is broadly analogous to the differential retardation of sound waves in density-variable media, however it also involves the propagation dynamics of ...

  5. List of particles - Wikipedia

    en.wikipedia.org/wiki/List_of_particles

    The field equations of condensed matter physics are remarkably similar to those of high energy particle physics. As a result, much of the theory of particle physics applies to condensed matter physics as well; in particular, there are a selection of field excitations, called quasi-particles, that can be created and explored. These include:

  6. List of physical quantities - Wikipedia

    en.wikipedia.org/wiki/List_of_physical_quantities

    D: Absorbed dose received per unit of time Gy/s L 2 T −3: Action: S: Momentum of particle multiplied by distance travelled J/Hz L 2 M T −1: scalar Angular acceleration: ω a: Change in angular velocity per unit time rad/s 2: T −2: Area: A: Extent of a surface m 2: L 2: extensive, bivector or scalar Area density: ρ A: Mass per unit area ...

  7. Meanings of minor-planet names: 34001–35000 - Wikipedia

    en.wikipedia.org/wiki/Meanings_of_minor-planet...

    Until his death in 2016, German astronomer Lutz D. Schmadel compiled these citations into the Dictionary of Minor Planet Names (DMP) and regularly updated the collection. [4] [5] Based on Paul Herget's The Names of the Minor Planets, [6] Schmadel also researched the unclear origin of numerous asteroids, most of which had been named prior to ...

  8. Today's Wordle Hint, Answer for #1316 on Saturday, January 25 ...

    www.aol.com/todays-wordle-hint-answer-1316...

    Today's Wordle Answer for #1316 on Saturday, January 25, 2025. Today's Wordle answer on Saturday, January 25, 2025, is CRISP. How'd you do? Up Next:

  9. Maxwell's equations - Wikipedia

    en.wikipedia.org/wiki/Maxwell's_equations

    In general D and H depend on both E and B, on location and time, and possibly other physical quantities. In applications one also has to describe how the free currents and charge density behave in terms of E and B possibly coupled to other physical quantities like pressure, and the mass, number density, and velocity of charge-carrying particles.