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  2. Duhamel's integral - Wikipedia

    en.wikipedia.org/wiki/Duhamel's_integral

    The response of a linear, viscously damped single-degree of freedom (SDOF) system to a time-varying mechanical excitation p(t) is given by the following second-order ordinary differential equation

  3. Viscous damping - Wikipedia

    en.wikipedia.org/wiki/Viscous_damping

    In a single-degree-of-freedom system, viscous damping model relates force to velocity as shown below: = ˙ Where is the viscous damping coefficient with SI units of /.This model adequately describes the damping force on a body that is moving at a moderate speed through a fluid. [3]

  4. Vacuum energy - Wikipedia

    en.wikipedia.org/wiki/Vacuum_energy

    Thus, according to the theory, even the vacuum has a vastly complex structure and all calculations of quantum field theory must be made in relation to this model of the vacuum. The theory considers vacuum to implicitly have the same properties as a particle, such as spin or polarization in the case of light, energy, and so on. According to the ...

  5. Edward Tryon - Wikipedia

    en.wikipedia.org/wiki/Edward_Tryon

    In 1973, he proposed that the universe is a large-scale quantum fluctuation in vacuum energy. This is called vacuum genesis or the zero-energy universe hypothesis. He has been quoted as saying, "the universe is simply one of those things that happens from time to time." [14] In 1967, he began working at Columbia University as a research assistant.

  6. Diffusion damping - Wikipedia

    en.wikipedia.org/wiki/Diffusion_damping

    Diffusion damping thus damps temperature and density anisotropies in the early universe. With baryonic matter (protons and electrons) escaping the dense areas along with the photons; the temperature and density inequalities were adiabatically damped. That is to say the ratios of photons to baryons remained constant during the damping process.

  7. Friedmann equations - Wikipedia

    en.wikipedia.org/wiki/Friedmann_equations

    This term originally was used as a means to determine the spatial geometry of the universe, where ρ c is the critical density for which the spatial geometry is flat (or Euclidean). Assuming a zero vacuum energy density, if Ω is larger than unity, the space sections of the universe are closed; the universe will eventually stop expanding, then ...

  8. Theory of everything - Wikipedia

    en.wikipedia.org/wiki/Theory_of_everything

    A theory of everything (TOE), final theory, ultimate theory, unified field theory, or master theory is a hypothetical singular, all-encompassing, coherent theoretical framework of physics that fully explains and links together all aspects of the universe. [1]: 6 Finding a theory of everything is one of the major unsolved problems in physics. [2 ...

  9. Borde–Guth–Vilenkin theorem - Wikipedia

    en.wikipedia.org/wiki/Borde–Guth–Vilenkin...

    Sean M. Carroll argues that the theorem only applies to classical spacetime, and may not hold under consideration of a complete theory of quantum gravity. He added that Alan Guth, one of the co-authors of the theorem, disagrees with Vilenkin and believes that the universe had no beginning.