Statistical Quantum good question

In summary, the conversation discusses the topic of a 2-D electron gas and its properties, such as the single particle energy states with momentum p, the Fermi energy, and the average electron energy at T=0. The expression for the average number of particles and the total energy is mentioned, as well as the differences in calculations between 2D and 3D. The topic is considered to have interesting implications in 2D physics, particularly with the Fermi energy.
  • #1
adelveis
2
0
So here is my question. Have a 2-D electron gas where:

E = P(x)^2/(2m) + P(y)^2/(2m)

Where p^2= p(y)^2 + p(x)^2

1. How many single particle energy states are there with momentum p?

( this may be a really simple question but I need a refresher.)

2. If there are N electrons is the metal, and T=0 , find the fermi energy of the 2-D electron gas

3. Find the ave electron energy of the gas in the 2-D Fermi energy at T=0.

this last one i think I have a better idea since with the 3-D there is a factor of 1/8, the 2-D it would most likely have a factor of 1/4.

Any other help with the first 2 would be awesome!
 
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  • #2
Just start from the beginning. What's the expression of the average number of particles? From this, what's the expression for the total energy? How does that change from 3D to 2D?

You'll uncover some pretty interesting physics in 2D if you work it out, particularly with the Fermi energy.
 
  • #3


I would be happy to provide a response to your questions.

1. The number of single particle energy states with momentum p can be calculated using the formula:

N(p) = A/(2πħ)^2 * p^2

Where A is the area of the 2-D system. This formula is derived from the fact that in 2-D systems, the density of states is proportional to the square of the momentum.

2. At T=0, the Fermi energy (EF) can be calculated by using the formula:

EF = (ħ^2/2m)(πN/A)^2

Where N is the number of electrons and A is the area of the 2-D system.

3. The average electron energy at EF can be calculated by using the formula:

<E> = (3/5)EF

This formula is derived from the fact that at T=0, the average electron energy is equal to the Fermi energy multiplied by a factor of (3/5) due to the Pauli exclusion principle.

I hope this helps with your understanding of the 2-D electron gas and its properties. If you have any further questions, please don't hesitate to ask. Best of luck with your studies!
 

Related to Statistical Quantum good question

What is statistical quantum?

Statistical quantum is a branch of quantum mechanics that uses statistical methods to study the behavior of quantum systems. It is based on the principles of probability and statistics to describe the behavior of particles at the quantum level.

How is statistical quantum different from traditional quantum mechanics?

Traditional quantum mechanics focuses on the behavior of individual particles, while statistical quantum looks at the behavior of groups of particles. It uses statistical methods to describe the probability of a particle's behavior, rather than predicting its exact behavior.

What are some real-world applications of statistical quantum?

Statistical quantum has many applications in fields such as physics, chemistry, and materials science. It is used to study the behavior of atoms and molecules, as well as in the development of new technologies such as quantum computing and quantum cryptography.

What are some challenges in studying statistical quantum?

One of the main challenges in studying statistical quantum is the complexity of the mathematical models used to describe quantum systems. These models can be difficult to understand and solve, even for experienced scientists. Additionally, quantum systems are often unpredictable and can behave in unexpected ways, making it challenging to accurately predict their behavior.

Why is statistical quantum important in understanding the universe?

Statistical quantum is essential in understanding the behavior of particles at the quantum level, which is crucial in understanding the fundamental laws of the universe. It allows scientists to study and make predictions about the behavior of particles, which can help us understand the behavior of larger systems and the universe as a whole.

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