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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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532 Chapter 14<br />

Fig. 14.3. Nucleon-nucleon bremsstrahlung emission of axions or pions.<br />

with the axion example Eq. (14.15) where only one Nambu-Goldstone<br />

boson w<strong>as</strong> present <strong>as</strong> opposed to the pion isotriplet. However, this additional<br />

term does not contribute to the bremsstrahlung process in the<br />

limit of nonrelativistic nucleons so that the above conclusion regarding<br />

the derivative coupling remains valid.<br />

In the process NN → NNa (Fig. 14.3) axions and pions appear so<br />

that again two Nambu-Goldstone bosons are attached to one fermion<br />

line. It is then necessary to use a derivative coupling <strong>for</strong> at le<strong>as</strong>t one<br />

of them (Raffelt and Seckel 1988). For other bremsstrahlung processes<br />

such <strong>as</strong> e − p → pe − a, where the particles interact through a virtual<br />

photon (a gauge boson) the pseudoscalar coupling causes no trouble.<br />

Also <strong>for</strong> the Compton process γe − → e − a one may use either the pseudoscalar<br />

or the derivative axion coupling: both yield the same result.<br />

Because it is not always a priori obvious whether the pseudoscalar and<br />

derivative couplings yield the same result it is a safe strategy to use the<br />

derivative coupling in all calculations.<br />

14.2.4 The Onslaught of Quantum Gravity<br />

A heavy critique w<strong>as</strong> levied against the PQ mechanism by quantumgravity<br />

inspired phenomenological considerations. The main idea is<br />

that generally the PQ symmetry, like any other global symmetry, will<br />

not be respected by gravity (Georgi, Hall, and Wise 1981). For example,<br />

a black hole can “swallow” any amount of PQ charge without a<br />

trace, while a swallowed electric charge remains visible by its Coulomb<br />

<strong>for</strong>ce. At energy scales exceeding the Planck m<strong>as</strong>s m Pl = 1.2×10 19 GeV<br />

quantum gravitational effects are expected and so m Pl is a phenomenological<br />

cutoff <strong>for</strong> any quantum theory which does not fundamentally<br />

include gravitation. In the “low-energy” world it should manifest itself<br />

by all sorts of effective interactions which are not <strong>for</strong>bidden by a symmetry<br />

and which likely involve inverse powers of the cutoff scale m Pl .

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