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?

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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?
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?
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