Calculating Electron Distribution in Hydrogen Atoms

In summary, the conversation discusses the calculation of the number of electrons with a given energy in a sample of hydrogen atoms at a certain temperature. It is explained that this can be done by weighing each possible state by the Boltzmann factor and calculating the partition function. At a temperature of 3K, the probability of electrons being in the n=2 level is vanishingly small. However, this only applies to a gas, as in a liquid the interactions between atoms make for a more complicated problem. The approximate number of decimal places for this small probability is calculated using the partition function and the degeneracy of the 2nd energy level. It is found to be even smaller than expected, leading to the conclusion that there may be
  • #1
Rothiemurchus
203
1
How do I calculate the number of electrons with a given energy in
a sample of hydrogen atoms at a certain temperature?
For example how many electrons would be in the n=2 level
at 3 Kelvin? And does it matter whether or not hydrogen is gas or liquid or solid i.e is a different calculation needed for a gas in place of a liquid.
 
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  • #2
This is a classical problem; you weigh each possible state by the Boltzmann factor e^(-E/kT), write the partition function and calculate the probability of a given energy level. At 3K, the probability of electrons being in n=2 is vanishingly small.

This only applies to a gas; in a liquid the interactions between atoms cannot be ignored and make for a messier problem.
 
  • #3
When you say vanishingly small, have you got an approximate number
of decimal places for that small probability?
 
  • #4
Easy to get. The partition function is dominated by the ground state so we can approximate:

Z = exp (-E1/kT).

P(n=2) = g * exp (-E2/kT) / Z, where g is the degeneracy of the 2nd level (ie how many distinct states there are with that energy level). Ignoring fine structure, g=4.

So P(n=2) = 4 exp (-(E2 - E1) / kT) = 4 e -39 455.3202 = 4 * 10 -17135

Hmm... that's even smaller than I expected. Did I do something wrong?
 
  • #5
E1 = 10^-18 Joules.
P(n=2) = 4 exp (-(E2 - E1) / kT) = 4 exp [(4 x 10^-18 - 1 x 10^-18)/10^-23]

works out at about 10^10^-18

There must be something wrong with the equation.
 

What are energy levels of electrons?

Energy levels of electrons refer to the specific levels or states that an electron can occupy within an atom. These levels are determined by the amount of energy that the electron possesses.

How are energy levels of electrons related to the electron configuration?

The electron configuration of an atom is determined by the arrangement of electrons in its energy levels. The number and arrangement of electrons in an atom's energy levels help to determine the chemical and physical properties of the element.

What is the significance of energy levels of electrons?

The energy levels of electrons play a crucial role in the behavior of atoms and their interactions with other atoms. They determine the chemical and physical properties of elements, as well as the types of chemical bonds that can be formed between atoms.

How are energy levels of electrons quantized?

The energy levels of electrons are quantized, meaning they can only have certain discrete values. This is due to the wave-like nature of electrons and the restrictions placed on their movement by the laws of quantum mechanics.

How do electrons move between energy levels?

Electrons can move between energy levels by absorbing or emitting energy in the form of photons. This process is known as electron excitation and de-excitation. The specific energy of the photon determines which energy level the electron will transition to or from.

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