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pH scale


  • WordNet 3.6
    • n pH scale (from potential of Hydrogen) the logarithm of the reciprocal of hydrogen-ion concentration in gram atoms per liter; provides a measure on a scale from 0 to 14 of the acidity or alkalinity of a solution (where 7 is neutral and greater than 7 is more basic and less than 7 is more acidic);
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In news:

Articles Tagged with " pH scale ".
Items Tagged with ' pH scale '.
Your soil 's pH, which stands for potential of hydrogen, is the measure of acidity or alkalinity, on a scale of 0 to 14.

In science:

Then, under the scaling relation µhα = ν rβ, the solution of the (scaled) coupled CTRW master (integral) equation, eq. (3), ph,r (x, t), weakly converges to the Green function of the fractional diffusion equation, u(x, t), for h → 0 and r → 0.
Five Years of Continuous-time Random Walks in Econophysics
Moffat, Large scale cosmological inhomogeneities, inflation and acceleration without dark energy, arXiv:astro-ph/0504004. R. H.
One-loop corrections to the curvature perturbation from inflation
Hass, “Scaling Behavior of Entanglement in Twoand Three-Dimensional Free Fermions,” [arXiv:quant-ph/0602094].
Holographic Entanglement Entropy: An Overview
Amenomori et al., Large-scale Sideral Anisotropy of Galactic Cosmic-Ray Intensity Observed by the Tibet Air Shower Array, arXiv:0505114 [astro-ph] E.
Skymap for atmospheric muons at TeV energies measured in deep-sea neutrino telescope ANTARES
Verde, “Non-Gaussianity from Large-Scale Structure Surveys,” arXiv:1001.5217 [astro-ph.
Primordial Non-Gaussianities from Inflation Models
Hor´ak, J., “Parametric resonance as a model for QPO sources – I. A general approach to multiple scales”, arXiv, e-print, (2004). [ADS], [arXiv:astro-ph/0408092].
Foundations of Black Hole Accretion Disk Theory
Uraltsev, “Charm CP violation and the electric dipole moments from the charm scale,” arXiv:1205.0233 [hep-ph]. 105. B.
Brief Review of Charm Physics
Yuan, “Detecting a Light Gravitino at Linear Collider to Probe the SUSY Breaking Scale, hep-ph/9601362. 50. D.
Supersymmetry Phenomenology With a Broad Brush
Ser., in press, astro-ph/9707144 Madore, B.F., Freedman, W.L., & Sakai, S. 1997, in The Extragalactic Distance Scale, eds.
The Distances of the Magellanic Clouds
Equations (2) and (5) imply that distances are scaled by αx = p¯h/M ωx, time by 1/ωx and energies, including Vb above, by ¯hωx, where M is the atomic mass, and ωx/2π is the harmonic frequency.
The Gross-Pitaevskii Equation for Bose Particles in a Double Well Potential: Two Mode Models and Beyond
Techniques for scale setting appropriate to this problem are outlined in Horbostel, et. al., Ph Rev. D67, 034023.
Heavy quark masses from Fermilab Fermions
Ciucu, “Scaling properties in the stochastic network calculus,” Ph.D. dissertation, Univ. of Virginia, Aug. 2007. A.
Statistical End-to-end Performance Bounds for Networks under Long Memory FBM Cross Traffic
I (0)) ˆ̺b,ph is the correlation function; τcorr is its typical scale.
Should recombinations of radical pairs be considered as accompanied by measurements?
Mellier, “Gravitational Lensing by Large Scale Structures: A Review,” in Proceedings of the Gravitational Lensing Winter School, Aussois, France, 2003, arXiv:astro-ph/0305089.
Constraining the expansion history of the universe from the red shift evolution of cosmic shear
Shellard, “Rapid Separable Analysis of Higher Order Correlators in Large Scale Structure,” ArXiv e-prints (2010), arXiv:1008.1730 [astro-ph.
Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity