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Discover how to simplify complex physics problems from chapters III to VI using just six key constants. By memorizing these essential numbers, you can enhance your problem-solving speed and accuracy while working on a variety of physics concepts. This guide covers vital constants such as the speed of light, elementary charge, mass of the electron, and fundamental physical relationships essential for transitioning to the SI system. Simplifying your equation-solving process has never been easier or more efficient!
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All problems fromPhysics III to VI can be solved 'by heart' by memorizing six simple numbers (correct to a few percent): c = 3·108 m/s α= 1/137 ≡ e2/(4πε0ħc) m = 511 keV ≈ ½ MeV/c2 mN = 1836 m ≈ 1 GeV/c2 k = 25 meV/300K + for transition to SI-system: e = 1.6·10−19 C → 1eV = 1.6·10−19 J ε0 = 107/4πc2 C/Vm μ0 = 1/ε0c2 = 4π·10−7 T/(A/m) (T = Tesla) NA = 6·1023 molecules/mole and: ħc = hc/2π ≈ 200 eV·nm (← AP) = 200 MeV·fm (← NP) = 0.2 GeV·fm (← PP) Natural constants