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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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154 Chapter 4<br />

If the triangle condition is not satisfied the URCA processes require<br />

bystander particles to absorb momentum, leading to the “modified<br />

URCA process” shown in Fig. 4.11 (Chiu and Salpeter 1964). Of<br />

course, <strong>as</strong> below in Sect. 4.9.1, the missing momentum can be provided<br />

by pions or a pion condensate (Bahcall and Wolf 1965a,b).<br />

An explicit result <strong>for</strong> the modified URCA rate in the OPE model<br />

<strong>for</strong> the nucleon interactions is (Friman and Maxwell 1979)<br />

Q mod. URCA = 11513π<br />

120960 α2 π G 2 F cos 2 θ C C 2 A p F,e T 8 , (4.77)<br />

ignoring factors of order unity to account <strong>for</strong> a nonzero m π and nucleon<br />

correlations. As in the νν processes, only the axial-vector coupling<br />

contributes. Some details of the ph<strong>as</strong>e-space integration can be found<br />

in Shapiro and Teukolsky (1983). 24<br />

The modified URCA reactions (Fig. 4.11) are closely related to νν<br />

bremsstrahlung and the inel<strong>as</strong>tic scattering process νNN → NNν discussed<br />

earlier. It is interesting that the rate <strong>for</strong> the e p n → n n ν e process<br />

does not diverge, in contr<strong>as</strong>t with νNN → NNν where multiplescattering<br />

effects had to be invoked to obtain a sensible result. The<br />

divergence w<strong>as</strong> due to the intermediate nucleon going on-shell <strong>for</strong> a<br />

vanishing energy transfer. In e p n → n n ν e the electron h<strong>as</strong> the energy<br />

E F,e , the neutrino T , and because E F,e ≫ T (degenerate electrons!), the<br />

minimum energy transfer to the leptons is E F,e and thus never zero. Of<br />

course, this is the re<strong>as</strong>on why the modified URCA reaction w<strong>as</strong> invoked<br />

in the first place: if the intermediate nucleon line is cut, the two<br />

sub-processes are suppressed by energy-momentum constraints.<br />

The direct and modified URCA process should be expressed in terms<br />

of a common structure function applicable to charged-current processes.<br />

One may expect that at high density, spin and isospin fluctuations may<br />

suppress these reactions in analogy to the neutral-current processes<br />

discussed in the previous section. However, the URCA processes have<br />

not been discussed in the literature from this particular perspective.<br />

The equivalent of the modified URCA process <strong>for</strong> quark matter w<strong>as</strong><br />

calculated by Iwamoto (1980, 1982), more recently by Goyal and Anand<br />

(1990), and numerically by Ghosh, Phatak, and Sahu (1994) who claim<br />

that Iwamoto’s ph<strong>as</strong>e-space approximations can lead to substantial errors<br />

in the emission rate.<br />

24 Shapiro and Teukolsky’s ph<strong>as</strong>e-space volume involves a factor p 3 F,e because in<br />

their treatment of the nuclear matrix element there is no cancellation of p 2 F,e with<br />

1/ω 2 from the nucleon propagator which occurs in a bremsstrahlung calculation.

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