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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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594 Appendix D<br />

of antifermions is given by the same expression with µ → −µ. Then µ<br />

is implicitly given by the ph<strong>as</strong>e-space integral<br />

∫<br />

n f =<br />

2 d 3 (<br />

)<br />

p 1<br />

(2π) 3 e (E p−µ)/T<br />

+ 1 − 1<br />

, (D.5)<br />

e (E p+µ)/T<br />

+ 1<br />

where the second term represents antifermions and the factor 2 is <strong>for</strong> the<br />

two spin degrees of freedom. Again, the fermion density is understood<br />

to mean the density of fermions minus that of antifermions.<br />

At vanishing temperature, f p becomes a step function Θ(µ − E p ).<br />

If µ > 0 so that n f > 0, i.e. an excess of fermions over antifermions,<br />

there are no antifermions at all at T = 0. The fermion integral yields<br />

n f = p 3 F/3π 2 ,<br />

(D.6)<br />

where the Fermi momentum is defined by µ 2 0 = p 2 F + m 2 with µ 0 the<br />

zero-temperature chemical potential. The Fermi energy is defined by<br />

E 2 F = p 2 F + m 2 e, i.e. E F = µ 0 .<br />

Equation D.6 is taken <strong>as</strong> the definition of the Fermi momentum even<br />

at T > 0; it is a useful parameter to characterize the fermion density,<br />

whether or not they are degenerate. Numerically it is<br />

p F = 5.15 keV (Y e ρ) 1/3<br />

(D.7)<br />

<strong>for</strong> electrons with the m<strong>as</strong>s density ρ in units of g cm −3 .<br />

In general, Eq. (D.5) cannot be made explicit <strong>for</strong> µ; it h<strong>as</strong> to be<br />

solved numerically or by an approximation method. In the ρ-T -plane,<br />

contours <strong>for</strong> the electron chemical potential are shown in Fig. D.3.<br />

Above the main plot, the electron density is characterized by p F . On<br />

the right side, the temperature is shown in units of keV. Recall that<br />

10 7 K = 0.8621 keV (Appendix A).<br />

For nonrelativistic electrons the contours in Fig. D.3 are very sensitive<br />

to the exact value of µ. There<strong>for</strong>e, in this regime the nonrelativistic<br />

chemical potential<br />

ˆµ ≡ µ − m (D.8)<br />

is a more appropriate parameter. Often ˆµ is referred to <strong>as</strong> the chemical<br />

potential. This can be very confusing when relativistic effects are<br />

important. In terms of ˆµ, the relativistic Fermi-Dirac distribution is<br />

f p =<br />

1<br />

e (E kin−ˆµ)/T<br />

+ 1 ,<br />

(D.9)<br />

with the kinetic energy E kin = E p −m → p 2 /2m (nonrelativistic limit).

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