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Hi there,
I have a problem to solve in Cosmology which says:
"Write the formulas for the quantum kinetic energy of neutrons, protons and electrons as well as the formula for the gravitational energy for a neutron star that is comprised of free neutrons, protons and electrons in a ratio of Nn : Np : Ne = 93,4 : 6,6 : 6,6 (Nν=Nn+Nn=1,8x1057)
The numerical coefficients should be these for homogeneous density."
Attempt for solution
I find in the book "From Quarks to Quasars" by E.N.Economou that the total quantum kinetic energy of neutrons is 92,14% of the total, Uk,tot=Uk,n/0,9214=(ακ/0,9214)ħ2N5/3/(mnR2). The coefficients are aκ=1,1.
This equation is derived from the total kinetic energy of N fermionic particles (s=1/2) that are similar and non relativistic.
And my question is:
How can this equation be used for neutrons (and protons) which are bosons and don't follow Fermi's exclusion principle (where this equation is derived from)?
I have a problem to solve in Cosmology which says:
"Write the formulas for the quantum kinetic energy of neutrons, protons and electrons as well as the formula for the gravitational energy for a neutron star that is comprised of free neutrons, protons and electrons in a ratio of Nn : Np : Ne = 93,4 : 6,6 : 6,6 (Nν=Nn+Nn=1,8x1057)
The numerical coefficients should be these for homogeneous density."
Attempt for solution
I find in the book "From Quarks to Quasars" by E.N.Economou that the total quantum kinetic energy of neutrons is 92,14% of the total, Uk,tot=Uk,n/0,9214=(ακ/0,9214)ħ2N5/3/(mnR2). The coefficients are aκ=1,1.
This equation is derived from the total kinetic energy of N fermionic particles (s=1/2) that are similar and non relativistic.
And my question is:
How can this equation be used for neutrons (and protons) which are bosons and don't follow Fermi's exclusion principle (where this equation is derived from)?