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  2. Casimir effect - Wikipedia

    en.wikipedia.org/wiki/Casimir_effect

    with the sum running over all possible values of n enumerating the standing waves. The factor of ⁠ 1 / 2 ⁠ is present because the zero-point energy of the n th mode is ⁠ 1 / 2 ⁠ E n, where E n is the energy increment for the n th mode. (It is the same ⁠ 1 / 2 ⁠ as appears in the equation E = ⁠ 1 / 2 ⁠ ħω.) Written in this way ...

  3. AP Physics 1 - Wikipedia

    en.wikipedia.org/wiki/AP_Physics_1

    AP Physics 1 is an algebra-based, introductory college-level physics course that includes mechanics topics such as motion, fluids, force, momentum, energy, harmonic motion, and rotation. The College Board published a curriculum framework that includes eight big ideas on which AP Physics 1 is based.

  4. Relative change - Wikipedia

    en.wikipedia.org/wiki/Relative_change

    A percentage change is a way to express a change in a variable. It represents the relative change between the old value and the new one. [6]For example, if a house is worth $100,000 today and the year after its value goes up to $110,000, the percentage change of its value can be expressed as = = %.

  5. List of unsolved problems in physics - Wikipedia

    en.wikipedia.org/wiki/List_of_unsolved_problems...

    The following is a list of notable unsolved problems grouped into broad areas of physics. [1]Some of the major unsolved problems in physics are theoretical, meaning that existing theories seem incapable of explaining a certain observed phenomenon or experimental result.

  6. Gravitational constant - Wikipedia

    en.wikipedia.org/wiki/Gravitational_constant

    In SI units, its value is approximately 6.6743 × 10 −11 m 3 kg −1 s −2. ‍ [1] The modern notation of Newton's law involving G was introduced in the 1890s by C. V. Boys . The first implicit measurement with an accuracy within about 1% is attributed to Henry Cavendish in a 1798 experiment .

  7. Critical mass - Wikipedia

    en.wikipedia.org/wiki/Critical_mass

    If the density is 1% more and the mass 2% less, then the volume is 3% less and the diameter 1% less. The probability for a neutron per cm travelled to hit a nucleus is proportional to the density. It follows that 1% greater density means that the distance travelled before leaving the system is 1% less.

  8. Idealized greenhouse model - Wikipedia

    en.wikipedia.org/wiki/Idealized_greenhouse_model

    [7] ε=0.78 implies 22% of the surface radiation escapes directly to space, consistent with the statement of 15% to 30% escaping in the greenhouse effect. The radiative forcing for doubling carbon dioxide is 3.71 W m −2, in a simple parameterization. This is also the value endorsed by the IPCC. From the equation for ,

  9. Margin of error - Wikipedia

    en.wikipedia.org/wiki/Margin_of_error

    For a confidence level, there is a corresponding confidence interval about the mean , that is, the interval [, +] within which values of should fall with probability . Precise values of z γ {\displaystyle z_{\gamma }} are given by the quantile function of the normal distribution (which the 68–95–99.7 rule approximates).