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  2. Improper integral - Wikipedia

    en.wikipedia.org/wiki/Improper_integral

    In mathematical analysis, an improper integral is an extension of the notion of a definite integral to cases that violate the usual assumptions for that kind of integral. [ 1] In the context of Riemann integrals (or, equivalently, Darboux integrals ), this typically involves unboundedness, either of the set over which the integral is taken or ...

  3. Proper time - Wikipedia

    en.wikipedia.org/wiki/Proper_time

    Proper time. In relativity, proper time (from Latin, meaning own time) along a timelike world line is defined as the time as measured by a clock following that line. The proper time interval between two events on a world line is the change in proper time, which is independent of coordinates, and is a Lorentz scalar. [ 1]

  4. Symmetry operation - Wikipedia

    en.wikipedia.org/wiki/Symmetry_operation

    The improper rotation is represented by the symbol S n where n is the order. Since the improper rotation is the combination of a proper rotation and a reflection, S n will always exist whenever C n and a perpendicular plane exist separately. [3] S 1 is usually denoted as σ, a reflection operation about a mirror plane.

  5. Integral - Wikipedia

    en.wikipedia.org/wiki/Integral

    e. In mathematics, an integral is the continuous analog of a sum, which is used to calculate areas, volumes, and their generalizations. Integration, the process of computing an integral, is one of the two fundamental operations of calculus, [ a] the other being differentiation. Integration was initially used to solve problems in mathematics and ...

  6. Proper motion - Wikipedia

    en.wikipedia.org/wiki/Proper_motion

    Proper motion may alternatively be defined by the angular changes per year in the star's right ascension ( μα) and declination ( μδ) with respect to a constant epoch . The components of proper motion by convention are arrived at as follows. Suppose an object moves from coordinates (α 1, δ 1) to coordinates (α 2, δ 2) in a time Δ t.

  7. Comoving and proper distances - Wikipedia

    en.wikipedia.org/wiki/Comoving_and_proper_distances

    Comoving distance and proper distance. Comoving distance is the distance between two points measured along a path defined at the present cosmological time. For objects moving with the Hubble flow, it is deemed to remain constant in time. The comoving distance from an observer to a distant object (e.g. galaxy) can be computed by the following ...

  8. Cauchy principal value - Wikipedia

    en.wikipedia.org/wiki/Cauchy_principal_value

    Cauchy principal value. In mathematics, the Cauchy principal value, named after Augustin-Louis Cauchy, is a method for assigning values to certain improper integrals which would otherwise be undefined. In this method, a singularity on an integral interval is avoided by limiting the integral interval to the non singular domain.

  9. Proper convex function - Wikipedia

    en.wikipedia.org/wiki/Proper_convex_function

    Proper convex function. In mathematical analysis, in particular the subfields of convex analysis and optimization, a proper convex function is an extended real -valued convex function with a non-empty domain, that never takes on the value and also is not identically equal to. In convex analysis and variational analysis, a point (in the domain ...

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