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<math> g^2 \approx \hbar c </math>
 
<math> g^2 \approx \hbar c </math>
   
One way of understanding this coupling constant is as follows. When two nucleons are at a distance <math> r </math> they communicate by exchanging particle whose de Broglie wavelength is comparable to <math> r </math>, so their momentum is <math> \hbar/r </math>, and if they are relativistic their energy is <math> \hbar c / r </math>. However, the pion is not a scalar, but a rather a pseudo scalar, meaning its spin is zero but its parity is negative. This pairity precludes spherically symmetric s-wave scattering (angular momentum <math> l = 0 </math>). The next leading order in the [http://galileo.phys.virginia.edu/classes/752.mf1i.spring03/Scattering_II.htm partial wave expansion] is p-wave (with angular momentum <math> l = 1 </math>), which is suppressed by the ratio of the Compton wavelengths squared of the particles and mediators. Hence,
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One way of understanding this coupling constant is as follows. When two nucleons are at a distance <math> r </math> they communicate by exchanging particle whose de Broglie wavelength is comparable to <math> r <math>, so their momentum is <math> \hbar/r </math>, and if they are relativistic their energy is <math> \hbar c / r </math>. However, the pion is not a scalar, but a rather a pseudo scalar, meaning its spin is zero but its parity is negative. This pairity precludes spherically symmetric s-wave scattering (angular momentum <math> l = 0 </math>). The next leading order in the [http://galileo.phys.virginia.edu/classes/752.mf1i.spring03/Scattering_II.htm partial wave expansion] is p-wave (with angular momentum <math> l = 1 </math>), which is suppressed by the ratio of the Compton wavelengths squared of the particles and mediators. Hence,
   
 
<math> g^2 \approx \hbar c \left(\frac{m_{\pi}}{m_n}\right)^2 </math>
 
<math> g^2 \approx \hbar c \left(\frac{m_{\pi}}{m_n}\right)^2 </math>
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