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  2. Parity (physics) - Wikipedia

    en.wikipedia.org/wiki/Parity_(physics)

    For example, the isotopes of oxygen include 17 O(5/2+), meaning that the spin is 5/2 and the parity is even. The shell model explains this because the first 16 nucleons are paired so that each pair has spin zero and even parity, and the last nucleon is in the 1d 5/2 shell, which has even parity since ℓ = 2 for a d orbital. [10]

  3. Numeric precision in Microsoft Excel - Wikipedia

    en.wikipedia.org/wiki/Numeric_precision_in...

    Excel's storage of numbers in binary format also affects its accuracy. [3] To illustrate, the lower figure tabulates the simple addition 1 + x − 1 for several values of x. All the values of x begin at the 15 th decimal, so Excel must take them into account. Before calculating the sum 1 + x, Excel first approximates x as a binary number

  4. Sports rating system - Wikipedia

    en.wikipedia.org/wiki/Sports_rating_system

    Rating a team is often about rating a specific collection of players. Some systems assume parity among all members of the league, such as each team being built from an equitable pool of players via a draft or free agency system as is done in many major league sports such as the NFL, MLB, NBA, and NHL. This is certainly not the case in ...

  5. Correlation function (statistical mechanics) - Wikipedia

    en.wikipedia.org/wiki/Correlation_function...

    In all cases, correlations are strongest nearest to the origin, indicating that a spin has the strongest influence on its nearest neighbors. All correlations gradually decay as the distance from the spin at the origin increases. Above the Curie temperature, the correlation between spins tends to zero as the distance between the spins gets very ...

  6. Solomon equations - Wikipedia

    en.wikipedia.org/wiki/Solomon_equations

    The latter is the important term which is responsible for transferring magnetization from one spin to the other and gives rise to the nuclear Overhauser effect. In an NOE experiment, the magnetization on one of the spins, say spin 2, is reversed by applying a selective pulse sequence. At short times then, the resulting magnetization on spin 1 ...

  7. Classical XY model - Wikipedia

    en.wikipedia.org/wiki/Classical_XY_model

    The existence of the thermodynamic limit for the free energy and spin correlations were proved by Ginibre, extending to this case the Griffiths inequality. [3]Using the Griffiths inequality in the formulation of Ginibre, Aizenman and Simon [4] proved that the two point spin correlation of the ferromagnetics XY model in dimension D, coupling J > 0 and inverse temperature β is dominated by (i.e ...

  8. Coriolis frequency - Wikipedia

    en.wikipedia.org/wiki/Coriolis_frequency

    Replacing =, where is the magnitude of the spin rate of the Earth, to obtain f = ω = 2 Ω sin ⁡ φ . {\displaystyle f=\omega =2\Omega \sin \varphi .} Thus the Coriolis parameter, f {\displaystyle f} , is the angular velocity or frequency required to maintain a body at a fixed circle of latitude or zonal region.

  9. Weyl equation - Wikipedia

    en.wikipedia.org/wiki/Weyl_equation

    The Dirac equation was published in 1928 by Paul Dirac, and was first used to model spin-1/2 particles in the framework of relativistic quantum mechanics. [2] Hermann Weyl published his equation in 1929 as a simplified version of the Dirac equation. [2] [3] Wolfgang Pauli wrote in 1933 against Weyl's equation because it violated parity. [4]

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