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Scalar field

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In mathematics and physics, a scalar field associates a scalar value to every point in a space. The scalar may either be a mathematical number, or a physical quantity. Scalar fields are often used in physics, for instance to indicate the temperature distribution throughout space, or the air pressure.

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[edit] Definition

Mathematically, a scalar field on a region U is a real or complex-valued function on U. The region U may be a set in some Euclidean space, or more generally a subset of a manifold, and it is typical to impose further conditions on the field, such that it be continuous or often continuously differentiable to some order. In a mathematical context, the term "scalar field" may be used to distinguish a function of this kind with a more general tensor field, density, or differential form.

Physically, a scalar field is additionally distinguished by having units of measurement associated with it. In this context, a scalar field should also be independent of the coordinate system used to describe the physical system — that is, any two observers using the same units must agree on the numerical value of a scalar field at any given point of physical space. Scalar fields are contrasted with other physical quantities such as vector fields, which associate a vector to every point of a region, and tensor fields. More subtly, scalar fields are often contrasted with pseudoscalar fields.

[edit] Uses in physics

In physics, scalar fields often describe the potential energy associated with a particular force. The force is a vector field, which can be obtained as the gradient of the potential energy scalar field. Examples include:

[edit] Examples in quantum theory and relativity

  • Scalar fields like the Higgs field can be found within scalar-tensor theories, using as scalar field the Higgs field of the Standard Model [4], [5]. This field interacts gravitatively and Yukawa-like (short-ranged) with the particles that get mass through it [6].
  • Scalar fields are found within superstring theories as dilaton fields, breaking the conformal symmetry of the string, though balancing the quantum anomalies of this tensor [7].
  • Scalar fields are supposed to cause the accelerated expansion of the universe (inflation [8]), helping to solve the horizon problem and giving an hypothetical reason for the non-vanishing cosmological constant of cosmology. Massless (i.e. long-ranged) scalar fields in this context are known as inflatons. Massive (i.e. short-ranged) scalar fields are proposed, too, using for example Higgs-like fields (e.g. [9]).

[edit] Other kinds of fields

[edit] See also

[edit] References

  1. ^ P.W. Higgs; Phys. Rev. Lett. 13(16): 508, Oct. 1964.
  2. ^ P. Jordanm Schwerkraft und Weltall, Vieweg (Braunschweig) 1955.
  3. ^ C. Brans and R. Dicke; Phis. Rev. 124(3): 925, 1961.
  4. ^ A. Zee; Phys. Rev. Lett. 42(7): 417, 1979.
  5. ^ H. Dehnen et al.; Int. J. of Theor. Phys. 31(1): 109, 1992.
  6. ^ H. Dehnen and H. Frommmert, Int. J. of theor. Phys. 30(7): 987, 1991.
  7. ^ C.H. Brans; "The Roots of scalar-tensor theory", arXiv:gr-qc/0506063v1, June 2005.
  8. ^ A. Guth; Pys. Rev. D23: 346, 1981.
  9. ^ J.L. Cervantes-Cota and H. Dehnen; Phys. Rev. D51, 395, 1995.

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