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  2. Equivalence principle - Wikipedia

    en.wikipedia.org/wiki/Equivalence_principle

    The equivalence principle is the hypothesis that the observed equivalence of gravitational and inertial mass is a consequence of nature. The weak form, known for centuries, relates to masses of any composition in free fall taking the same trajectories and landing at identical times.

  3. Weak equivalence - Wikipedia

    en.wikipedia.org/wiki/Weak_equivalence

    Weak equivalence principle This page was last edited on 27 May 2024, at 02:43 (UTC). Text is available under the Creative Commons Attribution ...

  4. Tests of special relativity - Wikipedia

    en.wikipedia.org/wiki/Tests_of_special_relativity

    Because "local Lorentz invariance" (LLI) also holds in freely falling frames, experiments concerning the weak Equivalence principle belong to this class of tests as well. The outcomes are analyzed by test theories (as mentioned above) like RMS or, more importantly, by SME. [3]

  5. Tests of general relativity - Wikipedia

    en.wikipedia.org/wiki/Tests_of_general_relativity

    Constraints on this, and on the existence of a composition-dependent fifth force or gravitational Yukawa interaction are very strong, and are discussed under fifth force and weak equivalence principle. A version of the equivalence principle, called the strong equivalence principle, asserts that self-gravitation falling bodies, such as stars ...

  6. Weak equivalence (homotopy theory) - Wikipedia

    en.wikipedia.org/wiki/Weak_equivalence_(homotopy...

    In mathematics, a weak equivalence is a notion from homotopy theory that in some sense identifies objects that have the same "shape". This notion is formalized in the axiomatic definition of a model category. A model category is a category with classes of morphisms called weak equivalences, fibrations, and cofibrations, satisfying several axioms.

  7. Weak interaction - Wikipedia

    en.wikipedia.org/wiki/Weak_interaction

    where Y W is the weak hypercharge of a particle with electrical charge Q (in elementary charge units) and weak isospin T 3. Weak hypercharge is the generator of the U(1) component of the electroweak gauge group; whereas some particles have a weak isospin of zero, all known spin-⁠ 1 / 2 ⁠ particles have a non-zero weak hypercharge. [f]

  8. Robert H. Dicke - Wikipedia

    en.wikipedia.org/wiki/Robert_H._Dicke

    In 1961, this led to the Brans–Dicke theory of gravitation, [7] developed with Carl H. Brans, an equivalence-principle violating modification of general relativity. A highlight experiment was the test of the equivalence principle by Roll, Krotkov and Dicke, which was a factor of 100 more accurate than previous work. [8]

  9. Shapiro time delay - Wikipedia

    en.wikipedia.org/wiki/Shapiro_time_delay

    The Shapiro time delay effect, or gravitational time delay effect, is one of the four classic Solar System tests of general relativity. Radar signals passing near a massive object take slightly longer to travel to a target and longer to return than they would if the mass of the object were not present.