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  • God OH, an abbreviation for the Orphic Hymns 0H (disambiguation) (zero H) H0 (disambiguation) This disambiguation page lists articles associated with...
    3 KB (386 words) - 23:26, 13 April 2024
  • Thumbnail for Bean's critical state model
    At low fields (H < H0), the vortices do not reach the inner surface of the hollow cylinder and the interior stays field-free. For H > H0, the vortices...
    5 KB (529 words) - 23:56, 18 September 2023
  • Calculated from Ωbh2 and h = H0 / (100 km s−1 Mpc−1). Calculated from Ωch2 and h = H0 / (100 km s−1 Mpc−1). Calculated from h = H0 / (100 km s−1 Mpc−1) per...
    95 KB (11,053 words) - 20:04, 12 May 2024
  • the Hamiltonian H be split into the free part H0 and the interaction V, H = H0 + V. In this picture, the operators behave as free field operators and the...
    50 KB (9,185 words) - 15:55, 26 February 2024
  • '2dt LG31 = G30 OR G20 '2dt '--- Step 2, Ling PsevdoCarry (H) --------------------------- H0 = LG01 '1dt H1 = LG11 '2dt H2 = LG21 OR (LP11 AND LG11) '4dt...
    5 KB (654 words) - 09:34, 13 May 2024
  • Thumbnail for Abell catalogue
    dimensionless scale parameter which usually takes value between 0.5 and 1. h = H0/100. The precise value of the Abell radius depends on the value taken for...
    12 KB (1,601 words) - 09:05, 14 August 2023
  • time like the operators in the Heisenberg picture with the Hamiltonian H' = H0. The evolution of the density matrix in the interaction picture is i ℏ...
    16 KB (2,261 words) - 20:49, 19 March 2024
  • Thumbnail for Friedmann equations
    {m}}^{-3}=2.7754\times 10^{11}h^{2}M_{\odot }\,{\rm {Mpc}}^{-3},} (where h = H0/(100 km/s/Mpc). For Ho = 67.4 km/s/Mpc, i.e. h = 0.674, ρc = 8.5×10−27 kg/m3)...
    23 KB (3,680 words) - 13:35, 29 April 2024
  • which we split into a free part H0 and an interacting part VS(t), i.e. H = H0 + VS(t). We will work in the interaction picture here, that is, V I ( t...
    8 KB (1,948 words) - 15:42, 26 April 2024
  • m[S15]) end for Mix the upper and lower halves of V into ongoing state vector h h0..7 ← h0..7 xor V0..7 h0..7 ← h0..7 xor V8..15 Result ← h End Function Compress...
    30 KB (2,814 words) - 09:48, 25 April 2024
  • List of dialling codes in the United Kingdom Search for "hh0" , "hh-0", "h-h0", or "h-h-0" on Wikipedia. All pages with titles containing HH-0 All pages...
    820 bytes (115 words) - 03:00, 4 December 2023
  • G by Si(1) = {j ∈ V | (i,j)∈ E}. Let us also consider a scalar field, h = {h0, .., hN−1} defined on the set of nodes V, so that every node i has a scalar...
    12 KB (1,512 words) - 05:19, 10 January 2024
  • Thumbnail for Observable universe
    _{\text{c}}={\frac {3H^{2}}{8\pi G}},} where G is the gravitational constant and H = H0 is the present value of the Hubble constant. The value for H0, as given...
    65 KB (6,725 words) - 22:35, 15 May 2024
  • in the Schrödinger picture the Hamiltonian does not depend on time, e.g. H = H0 + V, in the interaction picture it does, at least, if V does not commute...
    58 KB (8,102 words) - 00:38, 4 April 2024
  • exchange of W1, W2, W3, and B vector bosons (electroweak interactions) and H+, H−, H0, H0⁎ scalar bosons (Higgs interaction). In this picture, the vacuum expectation...
    137 KB (13,917 words) - 08:42, 30 April 2024
  • Lorentz violation can be introduced as a perturbative effect in the form h=h0+δh,{\displaystyle h=h_{0}+\delta h,} where h0 is the standard massive-neutrino...
    41 KB (5,479 words) - 12:33, 13 April 2023
  • in the Schrödinger picture the Hamiltonian does not depend on time, e.g. H = H0 + V, in the interaction picture it does, at least, if V does not commute...
    22 KB (3,911 words) - 21:31, 14 November 2023
  • H⊥ 1 ∩ {\displaystyle \cap } H⊥ 2. Theorem (Hodge−Weyl decomposition). H = H0 ⊕ {\displaystyle \oplus } H1 ⊕ {\displaystyle \oplus } H2. The subspace...
    78 KB (11,053 words) - 22:20, 25 March 2024