Question: In Fig. 43-10, the equation for n(K), the number density per unit energy for particles, is Where n is the total particle number density. At
Where n is the total particle number density. At the center of the Sun, the temperature is 1.50 ( 107 K and the average proton energy Kavg is 1.94 keV. Find the ratio of the proton number density at 5.00 keV to the number density at the average proton energy.
K12 n(K ) = 1.13n-
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