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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Processes in a Nuclear Medium 137<br />

In addition, one frequently uses the static structure functions which<br />

are functions of the momentum transfer alone. For example,<br />

S µν<br />

V (k) =<br />

∫ +∞<br />

−∞<br />

dω<br />

2π Sµν V (ω, k) = 1<br />

n B<br />

⟨<br />

V µ (k)V ν (−k) ⟩ . (4.39)<br />

It w<strong>as</strong> used that ∫ +∞<br />

−∞ dω eiωt = 2πδ(t) so that ∫ dt in Eq. (4.38) is<br />

trivially done and yields the operators at equal times. In Eq. (4.39)<br />

V (k) is V (t, k) at an arbitrary time, <strong>for</strong> example t = 0. It only matters<br />

that both V (k) and V (−k) are taken at equal times.<br />

In an isotropic medium the tensorial composition of the dynamical<br />

structure function can be obtained only from the energy-momentum<br />

transfer K and the four-velocity U of the medium; U = (1, 0, 0, 0) in its<br />

rest frame. The general <strong>for</strong>m of the vector term is (Kirzhnits, Losyakov,<br />

and Chechin 1990)<br />

S µν<br />

V = S 1,V U µ U ν + S 2,V (U µ U ν − g µν )<br />

+ S 3,V K µ K ν + S 4,V (K µ U ν + U µ K ν ). (4.40)<br />

An analogous expression pertains to S µν<br />

A<br />

while the mixed term is<br />

S µν<br />

V A = i S V A ϵ µναβ U α K β (4.41)<br />

because of its trans<strong>for</strong>mation properties under parity. The functions<br />

S l,V and S l,A (l = 1, . . . , 4), and S V A depend on medium properties<br />

and on the Lorentz scalars K 2 and U · K that can be constructed from<br />

U and K; the third possibility U 2 = 1 is a constant. Instead of K 2 and<br />

U · K one may use the energy and momentum transfer ω and k = |k|<br />

me<strong>as</strong>ured in the medium rest frame.<br />

The structure functions are defined <strong>for</strong> both positive and negative<br />

energy transfers because the medium can both give or take energy from<br />

a probe. Taking axion emission and absorption <strong>as</strong> an example, the rate<br />

of change of the occupation number of an axion field mode k is given by<br />

( ) 2<br />

CA n [ B<br />

∂ t f k =<br />

(fk + 1) S µν<br />

A (−ω, k) − f k S µν<br />

A (ω, k) ] K µ K ν .<br />

2f a 2ω<br />

(4.42)<br />

If axions are trapped and reach thermal equilibrium, ∂ t f k = 0 and f k =<br />

(e ω/T − 1) −1 , a Bose-Einstein distribution. This implies the detailedbalance<br />

condition<br />

S µν<br />

A (ω, k) = S µν<br />

A (−ω, k) e ω/T . (4.43)<br />

Recall that a positive energy transfer is energy given to the medium.

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