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goleafsgo113
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how can i calculate the fractional abundance of HI, HII, H- and e- for hydrogen in the photosphere (T=5770K) and density 10^17?
The equation for calculating the fractional abundance of each particle in hydrogen is: f = n/(n + n0), where f is the fractional abundance, n is the number of particles and n0 is the total number of particles.
The number of particles in hydrogen can be determined using the mass of hydrogen and Avogadro's number. The number of particles is equal to the mass of hydrogen in grams divided by the molar mass of hydrogen (1.008 g/mol) multiplied by Avogadro's number (6.022 x 10^23 particles/mol).
The number of particles for each particle in hydrogen is as follows: n(HI) = 0.5 x n(H), n(HII) = 0.25 x n(H), n(H-) = 0.25 x n(H), n(e-) = n(H).
Yes, the fractional abundance of each particle in hydrogen can change depending on factors such as temperature and pressure. These factors can affect the ionization of hydrogen atoms, resulting in changes in the fractional abundance of HI, HII, H-, and e-.
The fractional abundance of each particle in hydrogen is used in various fields of science, including astrophysics, chemistry, and plasma physics. It is used to understand the physical and chemical processes occurring in hydrogen gas, such as ionization and recombination, and to make predictions about the behavior of hydrogen in different environments.