2) An atomic nucleus can be crudely modeled as a gas of nucleons with a number density of 0.09 fm-3 (where 1 fm = 10-15m). a) Calculate the Fermi energy ɛp of this system. b) Also, calculate the Fermi temperature TF. Is it reasonable to treat the nucleus as a degenerate Fermi gas at room temperature? c) Calculate the degeneracy pressure of the nucleus. What keeps the nucleus from blowing apart due to this degeneracy pressure?
2) An atomic nucleus can be crudely modeled as a gas of nucleons with a number density of 0.09 fm-3 (where 1 fm = 10-15m). a) Calculate the Fermi energy ɛp of this system. b) Also, calculate the Fermi temperature TF. Is it reasonable to treat the nucleus as a degenerate Fermi gas at room temperature? c) Calculate the degeneracy pressure of the nucleus. What keeps the nucleus from blowing apart due to this degeneracy pressure?
Related questions
Question

Transcribed Image Text:2) An atomic nucleus can be crudely modeled as a gas of nucleons with a number density of
0.09 fm-3 (where 1 fm = 10-15m).
a)
Calculate the Fermi energy ɛp of this system.
b)
Also, calculate the Fermi temperature TF. Is it reasonable to treat the nucleus as a
degenerate Fermi gas at room temperature?
c)
Calculate the degeneracy pressure of the nucleus. What keeps the nucleus from
blowing apart due to this degeneracy pressure?
Expert Solution

This question has been solved!
Explore an expertly crafted, step-by-step solution for a thorough understanding of key concepts.
This is a popular solution!
Trending now
This is a popular solution!
Step by step
Solved in 3 steps with 3 images
