✎ Axion Models [The Physics Travel Guide]

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====== The Axion ======

Axions are proposed as a solution to the [[open_problems:strong_cp_problem|strong CP problem]]. In some sense, it's the simplest solution, because the QCD vacuum energy has a minimum at $\bar{\theta}=0$ and the axion allows the vacuum to relax to this ground state. Without the axion the QCD vacuum is frozen and $\bar{\theta}$ is therefore fixed at some not-necessarily minimum value.

* A great laymen discussion of the axion mechanism is [[https://www.susanjfowler.com/blog/2016/9/17/from-the-fledgling-physicist-archives-an-introduction-to-axions|From The Fledgling Physicist Archives: An Introduction To Axions]] by Susan J Fowler.

<blockquote>
One possibility is provided by the fact that the sate with $\theta=0$ is the bottom of the zone and thus has the lowest energy. This means if $\theta$ becomes a dynamical variable, the vacuum can relax to the $\theta=0$ state (just like electrons can drop to the bottom of the conduction band by emitting phonons). This is the basis of the axion mechanism [190-192]. The axion is a hypothetical pseudo-scalar particle, which couples to $G \tilde G$. The equations of motion for the axion field automatically remove the effective $\theta$ term, which is now a combination of $\theta_{QCD}$ and the axion expectation value. Experimental limits on the axion coupling are very severe, but an "invisible axion" might still exist.

<cite>[[https://books.google.de/books?id=rbcQMK6a6ekC&lpg=PA129&ots=kb7yWQczYE&dq=%22pure%20gauge%22%20zero%20field%20strength%20vacuum%20not%20gauge%20invariant&hl=de&pg=PA135#v=onepage&q&f=false|page 138 in The QCD Vacuum, Hadrons and Superdense Matter]]
by E. V. Shuryak</cite>
</blockquote>

<blockquote>
Technically
this new global U(1) symmetry is not quite an exact symmetry. Like the strong
CP symmetry itself, it is a pseudo-symmetry, broken only by non-perturbative or
instanton (tunneling) effects. This is exactly why it works as desired. The trick is to
make the Higgs field energy depend on the θ value in such a way that, for any initial
value of θ, the Higgs field will choose a vacuum value such that the resulting physical
parameter θeffective is zero. The Higgs vacuum expectation values aquire phases such
that the phase of the quark mass matrix cancels against the initial θ.

<cite>http://www.slac.stanford.edu/cgi-wrap/getdoc/slac-pub-8964.pdf</cite>
</blockquote>
  
<tabbox Student>

<note tip>
In this section things should be explained by analogy and with pictures and, if necessary, some formulas.
</note>
 
<tabbox Researcher>

<note tip>
The motto in this section is: //the higher the level of abstraction, the better//.
</note>

--> Example1#

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For a great discussion of the history of axion models, see Axions: Past, Present, and Future by Mark Srednicki

<blockquote>
By the time the papers were written Weinberg and Wilczek both used the name “axion” for this particle. I rather liked the alternate name “higglet” which was floating around for a while.

<cite>[[http://www.slac.stanford.edu/cgi-wrap/getdoc/slac-pub-8964.pdf|Helen Quinn]]</cite>
</blockquote>

<blockquote>
An obvious question about the axion hypothesis is how natural it really is. Why introduce a global PQ “symmetry” if it is not actually a symmetry? What is the sense in constraining a theory so that the classical Lagrangian possesses a certain symmetry if the symmetry is actually anomalous? It could be argued that the best evidence that PQ “symmetries” are natural comes from string theory, which produces them without any contrivance.

<cite>Axions In String Theory  by Peter Svrcek, Edward Witten</cite>
</blockquote>

<blockquote>"My favorite solution is that the up quark mass becomes very small by evolving near to a chirally symmetric point. We know that if one of the masses is strictly zero, $\theta$ becomes invisible. The mechanism that I have in mind is that at a very high energy scale, where the weak interactions really communicate a lot with QCD, so that the $\theta$ angle at that scale would be influenced a lot by the weak interactions, one might put one of the quark masses, preferably the up quark mass, to zero. This would correspond to the $U(1)$ chiral symmetry which we know is broken by instantons. So if you scale down from that very high energy scale to low energy scales, the fact that the other quark masses (say the d quark) is unequal to zero will shift the up quark mass to the value it has in the real world. Now to me this appears to be a possible scenario, but it depends very much on numerical analysis whether this works out or not. Usually people who do more detailed calculations tend to disagree with the statement that this is a viable scenario for the $\theta$ angle problem. I am not so totally convinced yet, and I believe that, because of the uncertainties in QCD, this is a possible explanation. It could be for instance, that even if $\theta$ is large at high energies, the renormalization group would rotate it to small values just because the quark masses are so small. The renormalization group could get huge effects from instantons which align according to $\theta$. **I have some hesitation to accept the bold, daring assumptions that e.g. Peccei, Quinn made.** 
See: <cite>[[https://books.google.de/books?id=bvSxDgAAQBAJ&lpg=PA232&ots=ceJzZ6xXeG&dq=Renormalization%20Scheme%20Dependence%20beta%20function%20hooft&hl=de&pg=PA234#v=onepage&q&f=false|’t Hooft]] </cite></blockquote>

<blockquote>
By taking this standard road, one needs to implement the axion in form of a hypothetical degree of freedom from beyond the SM. This requires an introduction of a singlet scalar field with a very large VEV plus either a hypothetical heavy quark [8] or an additional Higgs doublet [9] (for a review see, e.g., [10]).

<cite>[[https://arxiv.org/pdf/1608.08969.pdf|Domestic Axion]] Gia Dvali</cite>
</blockquote>

It is possible that an additional gravitational $\theta$ term:

$$ \theta_G R \tilde R, $$
where $R$ is the Riemann tensor, exists. If this is the case, the axion solution does not work.

<blockquote>
there is an old believe
that quantum gravity effects can generate an additional
breaking of the axion shift symmetry (2) and therefore
ruin the axion solution to the strong CP problem (see,
e.g., [13]). [...] The existence of a nonvanishing topological vacuum
susceptibility in pure gravity is currently an open
question.  [...] [I]n the absence
of an axion (or a massless fermion), there exist two physically
observable theta parameters, one from QCD (1)
and one from gravity (9). Consequently, after the axion
is introduced, it can only cancel a single combination of
the two ϑ-terms, whereas the other combination remains
physically observable. Hence, the strong CP problem is
not solved.

<cite>[[https://arxiv.org/pdf/1608.08969.pdf|Domestic Axion]] Gia Dvali</cite>
</blockquote>

<blockquote>
It is well known that a phase transition with PQ symmetry
breaking can form axionic cosmic strings. These
strings later become boundaries of domain walls [26] and
decay producing axions.

<cite>[[https://arxiv.org/pdf/1608.08969.pdf|Domestic Axion]] Gia Dvali</cite>
</blockquote>

</tabbox>

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