enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Flatness problem - Wikipedia

    en.wikipedia.org/wiki/Flatness_problem

    The flatness problem (also known as the oldness problem) is a cosmological fine-tuning problem within the Big Bang model of the universe. Such problems arise from the observation that some of the initial conditions of the universe appear to be fine-tuned to very 'special' values, and that small deviations from these values would have extreme ...

  3. Flatness (art) - Wikipedia

    en.wikipedia.org/wiki/Flatness_(art)

    In art criticism of the 1960s and 1970s, flatness described the smoothness and absence of curvature or surface detail of a two-dimensional work of art. Views

  4. Cosmic inflation - Wikipedia

    en.wikipedia.org/wiki/Cosmic_inflation

    The flatness and horizon problems are naturally solved in the Einstein–Cartan–Sciama–Kibble theory of gravity, without needing an exotic form of matter or free parameters. [ 122 ] [ 123 ] This theory extends general relativity by removing a constraint of the symmetry of the affine connection and regarding its antisymmetric part, the ...

  5. Samuel Face - Wikipedia

    en.wikipedia.org/wiki/Samuel_Face

    The measuring instruments he co-invented ... the use of the Face flat floor technologies and processes resulted in a 100% improvement in concrete floor flatness ...

  6. Lapping - Wikipedia

    en.wikipedia.org/wiki/Lapping

    Flatness is more easily measured with a co-ordinate measuring machine. But neither of these methods can measure flatness more accurately than about 2.5 μm (9.8 × 10 −5 in). Optical flats in a wooden case. Another method that is commonly used with lapped parts is the reflection and interference of monochromatic light. [1]

  7. Optical flat - Wikipedia

    en.wikipedia.org/wiki/Optical_flat

    A flatness test of a float-glass optical window. By placing a ruler across the image, adjacent to a fringe, and counting how many fringes cross it, the flatness of the surface can be measured along any line. The window has a flatness of 4–6λ (~2100–3100 nm) per inch. An optical flat test in both green and red.

  8. Flatness (cosmology) - Wikipedia

    en.wikipedia.org/wiki/Flatness_(cosmology)

    In cosmology, flatness is a property of a space without curvature. Such a space is called a "flat space" or Euclidean space. [citation needed]

  9. Interferometry - Wikipedia

    en.wikipedia.org/wiki/Interferometry

    The Twyman–Green interferometer, invented by Twyman and Green in 1916, is a variant of the Michelson interferometer widely used to test optical components. [58] The basic characteristics distinguishing it from the Michelson configuration are the use of a monochromatic point light source and a collimator.