On the Flavor Problem in Strongly Coupled Theories - THEP Mainz
On the Flavor Problem in Strongly Coupled Theories - THEP Mainz
On the Flavor Problem in Strongly Coupled Theories - THEP Mainz
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2 Chapter 1. Introduction: <strong>Problem</strong>s beyond <strong>the</strong> Standard Model<br />
as described by <strong>the</strong> SM, <strong>the</strong> coefficient of <strong>the</strong> Higgs mass operator has to be of <strong>the</strong><br />
order of <strong>the</strong> electroweak scale, i.e. ΛEW ≈ 1 TeV. This <strong>in</strong>troduces a large unexpla<strong>in</strong>ed<br />
hierarchy <strong>in</strong> scales, unless <strong>the</strong>re is new physics at ΛEW or <strong>the</strong> dimensionless coefficient<br />
c2 is tuned to be of <strong>the</strong> order c2 ≈ Λ2 EW /Λ2 UV . Even more severe is <strong>the</strong> problem of <strong>the</strong><br />
cosmological constant, which is <strong>in</strong>directly measured at c0 ≈ � 10−12 GeV �4 /Λ4 UV [2],<br />
and ei<strong>the</strong>r calls for a UV completion at <strong>the</strong> millielectronvolt scale or a f<strong>in</strong>e-tun<strong>in</strong>g of<br />
hundreds of orders of magnitude if one assumes that ΛUV is of <strong>the</strong> order of <strong>the</strong> Planck<br />
scale MPl = 1019 GeV.<br />
Both hierarchies become a problem if one expects <strong>the</strong> <strong>the</strong>ory to be natural, for which<br />
we will adopt <strong>the</strong> def<strong>in</strong>ition of ’t Hooft,<br />
The naturalness criterion states that one such [dimensionless and<br />
measured <strong>in</strong> units of <strong>the</strong> cut-off] parameter is allowed to be much<br />
smaller than unity only if sett<strong>in</strong>g it to zero <strong>in</strong>creases <strong>the</strong> symmetry<br />
of <strong>the</strong> <strong>the</strong>ory. If this does not happen, <strong>the</strong> <strong>the</strong>ory is unnatural.[3]<br />
A good measure to judge <strong>the</strong> attractiveness of a physical <strong>the</strong>ory is <strong>the</strong>refore <strong>the</strong> absence<br />
of <strong>the</strong>se small parameters, or equivalently <strong>the</strong> absence of large hierarchies between<br />
scales. However, s<strong>in</strong>ce <strong>the</strong> cosmological constant is not directly relevant for<br />
<strong>the</strong> physics of <strong>the</strong> SM , we will ignore this problem and concentrate on <strong>the</strong> hierarchy<br />
problem of <strong>the</strong> SM <strong>in</strong> Part 1.1 of this chapter.<br />
This hierarchy problem becomes even more puzzl<strong>in</strong>g if one considers higher dimensional<br />
operators. If it can be expla<strong>in</strong>ed by new physics at <strong>the</strong> electroweak scale, one<br />
would expect from <strong>the</strong> EFT ansatz (1.1), that also <strong>the</strong> suppression scale of <strong>the</strong> irrelevant<br />
operators are of <strong>the</strong> order ΛUV = ΛEW. However, if not prevented by some<br />
mechanism <strong>in</strong> <strong>the</strong> new physics sector, bounds from measurements on flavor chang<strong>in</strong>g<br />
processes <strong>in</strong>volv<strong>in</strong>g quarks will enforce at least<br />
ΛUV � 10 3 TeV . (1.2)<br />
A UV completion of <strong>the</strong> SM should <strong>the</strong>refore not only be able to expla<strong>in</strong> why <strong>the</strong><br />
electroweak scale is stabilized aga<strong>in</strong>st radiative corrections, but also why higher dimensional<br />
operators are absent or suppressed by orders of magnitude compared to<br />
ΛEW.<br />
The question of how both of <strong>the</strong>se requirements can be brought <strong>in</strong> agreement is one<br />
of <strong>the</strong> most press<strong>in</strong>g issues for models of physics beyond <strong>the</strong> SM. Fur<strong>the</strong>r, while <strong>the</strong><br />
marg<strong>in</strong>al operators <strong>in</strong> LGauge all have natural coefficients , 3 <strong>the</strong> Yukawa coupl<strong>in</strong>gs <strong>in</strong><br />
LYukawa exhibit hierarchical structures which are not expla<strong>in</strong>ed by SM physics ei<strong>the</strong>r,<br />
and although <strong>the</strong>se parameters are not radiatively unstable, <strong>the</strong> question what sets<br />
<strong>the</strong> masses and mix<strong>in</strong>gs of quarks and leptons is also to be answered by physics beyond<br />
<strong>the</strong> SM. Part 1.2 of this chapter will describe models which aim to expla<strong>in</strong> <strong>the</strong><br />
hierarchies of <strong>the</strong> Yukawa sector and mechanisms which generate a hierarchy between<br />
<strong>the</strong> coefficients of higher dimensional operators relevant for flavor chang<strong>in</strong>g processes<br />
3 With <strong>the</strong> exception of operators allow<strong>in</strong>g for strong CP violation.