Theorems for Asymptotic Safety of Gauge Theories

We classify the weakly interacting fixed points of general gauge theories coupled to matter and explain how the competition between gauge and matter fluctuations gives rise to a rich spectrum of high- and low-energy fixed points. The pivotal role played by Yukawa couplings is emphasized. Necessary and sufficient conditions for asymptotic safety of gauge theories are also derived, in conjunction with strict no go theorems. Implications for phase diagrams of gauge theories and physics beyond the Standard Model are indicated.

1. Fixed points of the renormalisation group play an important role in quantum field theory and particle physics [1,2]. Low-energy fixed points characterise continuous phase transitions and the dynamical breaking of symmetry. High-energy fixed points are central for the fundamental definition of quantum field theory. Important examples are provided by asymptotic freedom of non-abelian gauge theories [3,4] where the high-energy fixed point is non-interacting. Gauge theories with complete asymptotic freedom, meaning asymptotic freedom for all of its couplings, are of particular interest in the search for extensions of the Standard Model [5]. Asymptotically free gauge theories can also display weakly coupled infrared (IR) fixed points [6,7]. More recently, it was discovered that gauge theories can develop interacting ultraviolet (UV) fixed points [8], a scenario known as asymptotic safety. This intriguing new phenomenon, originally conjectured in the context of quantum gravity [9], offers the prospect for consistent UV completions of particle physics beyond the paradigm of asymptotic freedom [10].
In this Letter we classify all weakly interacting fixed points of general gauge theories coupled to matter in four space-time dimensions starting from first principles. Our motivation for doing so is twofold: Firstly, we want to understand in general terms whether and how the competition between gauge and matter field fluctuations gives rise to quantum scale invariance. We expect that insights into conformal windows of gauge theories will offer new directions for particle physics above the electroweak energy scale. Secondly, we are particularly interested in the dynamical origin for asymptotic safety in gauge theories and conditions under which it may arise. We also hope that insights into the inner working of asymptotic safety at weak coupling will offer clues for mechanisms of asymptotic safety at strong coupling [11,12].
We pursue these questions in perturbation theory starting with pure gauge interactions and gradually adding in more gauge and matter couplings. We will find a rich spectrum of interacting high-and low-energy fixed points including necessary and sufficient conditions for their existence. Furthermore, we highlight the central importance of Yukawa couplings to balance gauge against matter fluctuations. We thereby also establish that the presence of scalar fields such as the Higgs are strict necessary conditions for asymptotic safety at weak coupling. Further key ingrediences for our results are bounds on quadratic Casimirs which are derived for general Lie algebras, together with structural aspects of perturbation theory which are detailed as we proceed.

2.
We begin our investigation of weakly coupled fixed points by considering (non-)abelian vector gauge theories with a simple gauge group G and gauge coupling g, interacting with spin-1 2 fermions or scalars or both. Throughout we scale loop factors into the definition of couplings and introduce α = g 2 /(4π) 2 . The renormalisation group running of the gauge coupling up to two loop order in perturbation theory reads where β ≡ dα/d(ln µ), and µ denoting the RG momentum scale. The one and two loop coefficients in (1) are known for arbitrary field content and given in [3,4,[13][14][15] and [6,16,17], respectively. In terms of the Dynkin index S R 2 and the quadratic Casimir C R 2 of quantum fields in some irreducible representation (irrep) R of the gauge group, they can be written as 1 The terms involving C G 2 -the quadratic Casimir in the adjoint representation of the gauge grouparise due to the fluctuations of the gauge fields. The fluctuations of charged fermionic (F) or scalar (S) matter fields, if present, contribute to (1) via the terms proportional to the Dynkin index of their representation.
Gauge theories with (1) will always display the free Gaussian fixed point α * = 0. If B > 0 this is the well-known ultraviolet (UV) fixed point of asymptotic freedom [3,4] such as in QCD. For B < 0, instead, the theory becomes free in the infrared (IR) such as in QED. In addition, (1) can also display an interacting fixed point which is perturbative if α * 1 and physically acceptable provided that B · C > 0. For B · C < 0 the would-be fixed point reads α * < 0 and resides in an unphysical regime where the theory is sick non-perturbatively [18]. Also, if B < 0 (B > 0), (4) corresponds to an interacting UV (IR) fixed point. We conclude that the availability and nature of interacting fixed points is encoded in the signs and magnitude of (2) and (3). From the explicit expressions, we observe that the pure gauge contributions to both the one and two loop terms are either negative (non-abelian) or vanishing (abelian). Conversely, terms originating from fermionic or scalar matter contribute positively. This means that with a sufficiently small amount of matter (including none), the gauge boson contributions dominate and we have B > 0, C < 0. On the other hand, for a sufficiently large amount of matter, the matter contributions dominate and we end up with B ≤ 0, C > 0. The latter is trivially the case for abelian gauge groups whose quadratic Casimir vanishes identically, C U (1) 2 = 0. Weakly interacting fixed points are absent in either of these cases.
The question of what may happen when the pure gauge and matter contributions are of similar size is not immediately obvious. It has long been known that it is possible for theories to have B, C > 0, which are therefore asymptotically free and which, if B C, can lead to a perturbative infrared Banks-Zaks fixed point [6,7]. However, no examples have been found for which B, C < 0 and where the analagous fixed point would be ultraviolet. To see if such a scenario is possible in principle, we must examine the relative effects of matter on the one-and two-loop contributions.
To that end, we resolve (2) for the adjoint Casimir and insert the result into the last term of (3) to find We make the following obervations. The first term in (5) due to the fermions is manifestly positivedefinite. The last term in (5) is positive-definite provided that B < 0. Hence, as has been noted by Caswell [6], fermionic matter alone cannot generate an asymptotically safe UV fixed point in perturbation theory. The middle term however, due to charged scalars, is not manifestly positive definite and it cannot be decided prima facie whether or not it may generate an interacting UV fixed point with B < 0 and C < 0.

3.
In order to progress with the analysis of (5), we must find expressions for the smallest quadratic Casimir for any simple Lie algebra G. Irreducible representations of simple Lie algebras are conveniently characterised by their highest weight Λ, which for a rank-n Lie algebra is an ndimensional vector of non-negative integers, not all of which are zero. 2 This is due to the theorem of highest weight, which states that inequivalent irreps are in one-to-one correspondence with distinct highest weights. The Racah formula offers an explicit expression for the quadratic Casimir for any irrep R with highest weight Λ. It is given by where (u, v) ≡ ij G ij u i v j denotes the inner product of two highest weights, with u = n i=1 u i Λ i . The weight metrics G ≡ (G ij ) are known explicitly for any Lie algebra G. Note that (u, v) > 0 for any two weights. The n-component vector δ in (6) denotes half the sum of the positive roots and reads δ = (1, 1, . . . , 1) in the Dynkin basis (which we use exclusively). The normalisation factor 1 2 in (6) is conventional. 3 For any Lie algebra, the highest weight of irreps with the smallest quadratic Casimir must be one of the fundamental weights Λ k (with k ∈ {1, . . . , n}), whose components are defined as This can be understood as follows. Consider two highest weights Λ and λ, which may be used to construct a new irrep with highest weight Λ + λ. The bilinearity of the inner product (6) then implies that It follows, trivially, that C 2 can be made arbitrarily large. To find the smallest C 2 , however, (8) states that we only need to consider irreps whose highest weights have a single non-vanishing component. Assuming Λ to be one such weight and taking λ = m Λ for some integer m ≥ 1, (8) also states that we only need to consider highest weights where this single non-vanishing component takes the smallest non-vanishing value, which is unity. This establishes (7). Inserting (7) into (6), and denoting by G the weight metric of the gauge group G, we find the quadratic Casimir in terms of the fixed index k as It remains to identify the minima of (9) with respect to k for the four classical and the five exceptional Lie algebras separately, following the Cartan classification, starting with the rank-n classical Lie algebras A n , B n , C n and D n [19]. For n ≥ 1, 2, 3 and 4 they correspond to the unique Lie algebras su(n + 1), so(2n + 1), sp(n) and so(2n), respectively. Explicit expressions for the weight metrics are summarised in [20]. For our purposes we write them in closed form as For illustration, we consider explicitly the case for A n , where G kk = k(n + 1 − k)/(n + 1), which, combined with leads to the desired expression for C 2 (A n ) as stated in (11) with k taking values between 1 and n. To find the global minima of the expressions (11) with respect to k, we proceed as follows. For A n and C n , the expressions are quadratic polynomials in k with negative k 2 coefficient, implying that its minima are achieved at the boundaries, meaning either k = 1 or k = n, or both. For B n and D n , additionally, the expressions are discontinuous for certain intermediate values of k (owing to the δ k,n−1 and δ kn factors). This implies that global minima may additionally be achieved for integer values of k within the interval (1, n). With this in mind, and after evaluating all possible cases, the final result for the smallest quadratic Casimir for the classical Lie algebras is found to be min C 2 (A n ) = n 2 n + 2 n + 1 , min C 2 (B n ) = 1 8 n(2n + 1) for n = 2, 3 n for n ≥ 4 , The five exceptional groups E 6,7,8 , F 4 , and G 2 have a fixed size, hence finding the smallest Casimir amounts to a simple minimisation. Using the appropriate expressions for the weight metrics [20], our results are summarised in Tab. 1 where, for convenience, we express (12) using the particle physics nomenclature for the gauge groups.
A few comments are in order: (i) For A n either boundary is minimal, corresponding to the fundamental and anti-fundamental representation. (ii) For B n the Casimir is minimal for k = n (the fundamental spinor representation) provided n = 2 or 3, and for k = 1 (the fundamental vector representation) provided n ≥ 4. (iii) For C n and D n , the Casimir is minimal for k = 1 (the fundamental vector representation). (iv) For D 4 , three smallest Casimirs are achieved for k = 1, 3 and 4. This degeneracy is due to the fact that the Dynkin diagram for D 4 possesses a three-fold symmetry, and thus there is a triality between the fundamental vector and the two inequivalent spinor representations. (v) For the exceptional groups, we find that the smallest Casimir is unique, except for E 6 . (vi) E 8 is the only group where the smallest Casimir is achieved for the adjoint representation (which is also one of the fundamental representations). (vii) While the quadratic Casimir in general is a non-monotonic function of the dimensionality of the representation, our findings establish that the smallest Casimir always corresponds to those representations with the smallest dimension, which is always one of the fundamental representations.
Since the overall normalisation of quadratic Casimirs (6) can be chosen freely, it is useful to consider the ratio between the smallest quadratic Casimir and the Casimir in the adjoint, which is independent of the normalisation. Fig. 1 shows our results for χ for all simple Lie algebras. Evidently, χ is going to be bounded from above χ ≤ 1 because the adjoint representation always exists. The upper boundary is achieved for the exceptional group E 8 . Furthermore, χ is also bounded from below, The lower bound is achieved for the fundamental two-dimensional representation of SU (2) SO(3) Sp (1), and for the two inequivalent two-dimensional representation of SO(4). We observe that χ is an increasing function with N for SU (N ) and Sp(N ), interpolating between 3 8 for small N and 1 2 in the infinte-N limit. For SO(N ), we find that χ grows from 3 8 to its maximum 7 12 at N = 8, from where it decays with increasing N towards 1 2 from above. From the exceptional groups, only G 2 has a χ value close to those of the classical groups. All other exceptional groups have larger values for χ, which furthermore increases with the rank of the group.

4.
We are now in a position to develop the central results of this work, summarised in Tab. 2 and Tab. 3. We have observed in (5) that charged scalars potentially may turn the two loop coefficient C negative even if B ≤ 0, provided that nontrivial scalar irreps are found with C S 2 < 1 11 C G 2 . However, the result (13), (14) now firmly establishes that this is out of reach for any simple Lie algebra, owing to C S 2 ≥ 3 8 C G 2 . Moreover, we find that the two loop coefficient obeys for any non-abelian gauge theory. Hence, while it is possible to have B parametrically small such as in a Veneziano limit with suitably rescaled gauge coupling [21], the result (15) also shows that it is impossible to have both B and C parametrically small. Most importantly, we conclude that for any gauge theory with a vanishing or positive one loop coefficient for its gauge coupling's β function, the two loop coefficient is necessarily positive, see (1). It is worth noting that (16) is not an equivalence: while C < 0 arises exclusively only if B > 0, the case C > 0 can arise irrespective of the sign of B [6,7]. Consequently, Banks-Zaks fixed points are invariably IR fixed points. From the viewpoint of the asymptotic safety conjecture, our result (16) has the form of a no go theorem: within perturbation theory, irrespective of the matter  (1), and for the two inequivalent two-dimensional representation of SO(4). For the exceptional groups the smallest Casimir grows with the rank of the group. The upper bound is achieved for E 8 . In all cases, the smallest quadratic Casimir is achieved for the irreducible representation of smallest dimensionality. content and in the absence of non gauge interactions, asymptotic safety cannot be realised for any four-dimensional simple non-abelian, or abelian, gauge theory. 4 The result (16) straightforwardly generalises to matter fields in generic reducible representations under the gauge symmetry. In this case it suffices to replace terms involving Dynkin indices and matter Casimirs in the one and two loop coefficients by where the sums run over the decomposition into irreducible representations of the fermionic (R = F ) and scalar (R = S) matter fields. Applying (17) to the two loop coefficient (5), we find that all fermionic contributions remain manifestly positive definite, and that each summand of the scalar contributions is positive definite owing to (13), (14). We conclude that the no go theorem (16) holds true for general matter representations, as summarised in Tab. 2 b).

5.
Turning to more general gauge interactions, we consider gauge theories with product gauge groups G ≡ ⊗ n a=1 G a and multiple gauge couplings α a , each associated with a simple or abelian factor G a . We assume the presence of scalar and/or fermionic matter fields, some or all of which are charged under some or all of the gauge symmetries. In the absence of Yukawa interactions, the β functions for the gauge couplings up to two loops in perturbation theory are of the form and a, b = 1, · · · , n. The coefficients B a and C aa (no sum) are the standard one and two loop coefficients of the gauge coupling α a as given in (2), (3). The new terms at two loop level are the off-diagonal contributions C ab (a = b) which parametrise the O(α b ) contributions to the renormalisation group flow of couplings α a . Nontrivial mixing between two gauge couplings arises through matter fields which are charged under both of these. The mixing terms can then be written as [22,23] The subscripts a, b on the Casimir or Dynkin index of the matter fields indicate the subgroup of G. From (19) it follows that the mixing terms are manifestly non-negative (C ab ≥ 0) for any semi simple quantum gauge theory with or without abelian factors. The expression (19) has a straightforward generalisation for reducible representations. Furthermore, if the theory contains more than one abelian factor, the off-diagonal contributions take a slightly different form in the presence of kinetic mixing [24,25]. In either of these cases, the mixing terms remain manifestly non-negative (C ab ≥ 0, a = b). Together with (16) for all diagonal entries, we find that meaning that for every infrared free gauge group factor G a , the corresponding column of the two loop gauge contribution matrix (C ab ) is non-negative.
The result (20) has immediate implications for interacting fixed points of quantum field theories with (18), which, to leading order in perturbation theory, are given by all solutions of the linear equations Assuming that B a ≤ 0 for at least one of the subgroups G a , it follows from (20) that for (21) to have a solution, at least one of the fixed points α * b must take negative values. However, we have already explained that such solutions are inconsistent [18], and conclude that the theory cannot have physically acceptable interacting fixed points within the perturbative regime as soon as any of the gauge factors is infrared free (B a ≤ 0). In other words, the result (20) has the form of a no go theorem: asymptotic safety cannot be achieved for any semi-simple quantum gauge theory of the type (18) with or without abelian factors and irrespective of the matter content.
Reversing the line of reasoning, our findings also establish that physically-acceptable interacting fixed points in gauge theories with (18) and without Yukawa interactions can only be achieved if all gauge group factors are asymptotically free (B a > 0), which excludes U (1) factors straightaway, see Tab. 3 b). All weakly interacting fixed point solutions of (21) are necessarily IR fixed points of the Banks-Zaks type inasmuch as they arise from balancing one and two loop gauge field flucutations.
They also display a lesser number of relevant directions than the asymptotically free Gaussian UV fixed point meaning that UV-IR connecting trajectories exist which flow from the Gaussian down to any of the interacting fixed points.
Next, we investigate scalar and Yukawa-type matter couplings, and clarify whether these may help to generate weakly interacting fixed points.
6. Scalar self-interactions arise unavoidably in settings with charged scalars owing to the fluctuations of the gauge fields or in settings with uncharged scalars as long as these couple indirectly to the gauge fields through charged fermions and Yukawa interactions. Quartic scalar self interactions or cubic ones in a phase with spontaneous symmetry breaking renormalise the gauge couplings starting at the three loop (four loop) level in perturbation theory, provided the scalars are charged (uncharged) [26].
In the light of (16), to help generate an interacting fixed point in the gauge sector once B ≤ 0, the scalar couplings would have to outweigh the one loop as well as the two loop gauge contributions. Even if the one loop term vanishes identically (B = 0), the result (14) together with (2), (5) and (15) establishes that the two loop gauge coefficient is strictly positive C(B = 0) ≥ C min and of order unity, with The absolute minimum (22) is achieved for Sp(1), SU (2), SO(3) and SO(4) gauge symmetries. The bound becomes slightly stronger with increasing N , reaching C min /(C G ) 2 = 25 for the classical Lie groups in the infinite N limit. For the exceptional groups G 2 , F 4 , E 6 , E 7 and E 8 we find the increasingly stronger bounds C min /(C G ) 2 = 25, 50 2 3 , 55 5 9 , 61 2 3 and 80, respectively. Notice also that for all gauge groups the minimum is achieved for charged fermions only. The presence of charged scalars systematically enhances C > C min . Thus, coming back to the scalar self interactions, even in the most favourable scenario where the one-loop coefficient vanishes and the gauge coupling is perturbatively small, a cancellation between the two loop gauge and the three or four loop scalar contributions requires scalar couplings of order unity owing to the lower bounds (15), (22). 5 Hence, the feasibility of such a scenario necessitates non-perturbatively large scalar couplings, outside the perturbative domain. We conclude that non-abelian gauge theories with any type of self interacting scalar matter, and with or without fermionic matter but without Yukawa interactions, cannot become asymptotically safe within perturbation theory. This result also completes the no go theorems stated in Tab. 2 b) and c) in the presence of scalar matter.

7.
Yukawa couplings are naturally present in settings with both scalar and fermionic matter fields [27], and contribute to the running of (some of) the gauge couplings provided that (some of) the fermions carry charges under (some of) the gauge groups. Scalars may or may not carry charges. Yukawa couplings are technically natural [28] and cannot be switched-on by fluctuations: the limit of vanishing Yukawa couplings constitutes an exact fixed point of the theory.
For concreteness we consider simple non-abelian or abelian gauge theories with the most general Yukawa interactions taking the form ∼ 1 2 (Y A ) JL φ A ψ J ζ ψ L with ζ = ±iσ 2 , with Weyl indices suppressed. In perturbation theory the Yukawa couplings Y A contribute to the renormalisation of the gauge coupling starting at the two loop level, and the beta function (1) is replaced by [29] The Yukawa couplings enter through the new term , with d(G) the dimension of the gauge group, Y A the (matrix of) Yukawa couplings, C F 2 the matrix of quadratic Casimirs of the fermionic irreps, and the trace summing over all fermionic indices. Notice that we have scaled the loop factor of (4π) into the definition of Y A . The coefficients B and C are as in (2) and (3). In general, the matrix C F 2 is diagonal according to the fermionic irreps, implying that Y 4 is positive as long as (some of) the Yukawa couplings are non-vanishing. Positivity of Y 4 can be made manifest by rewriting it as It follows that Yukawa couplings contribute with an overall negative sign to the running of gauge couplings, irrespective of the sign of the one loop gauge coefficient B. Assuming that the Yukawa couplings, and thus Y 4 , take a fixed point of their own, interacting fixed points of (23) take the form (4) except that the one loop coefficient is effectively shifted This Yukawa-induced shift has important implications. Most notably, in settings where the gauge sector is asymptotically non free (B ≤ 0), the Yukawa contribution Y * 4 may effectively change the sign of the one loop coefficient (B > 0), thereby enabling a viable interacting fixed point In more physical terms, for infrared free theories these findings state that the growth of the gauge coupling with energy, as dictated by the positive one and two loop gauge contributions (16), is invariably slowed down, and, as long as B > 0, eventually brought to a halt by Yukawa interactions. In particular, the occurrence of a UV Landau pole in the gauge coupling can be avoided dynamically. As we have shown earlier, neither scalar self interactions nor further gauge couplings are able to negotiate a fixed point at weak coupling once B ≤ 0. We therefore conclude that Yukawa interactions are the only type of interactions that can generate an interacting UV fixed point for any weakly coupled gauge theory.
In view of the above it is useful to investigate the Yukawa sector in more detail. To that end, we exploit the explicit flow for the Yukawa couplings β A = dY A /d ln µ. At the leading non-trivial order in perturbation theory which is one loop, it takes the form [30,31] The terms E A (Y ), which are of cubic order in the Yukawa couplings, arise from fluctuations of the fermion and scalar fields and encode vertex and propagator corrections [30]. General expressions for E A in the conventions adopted here are given in [32,33]. The terms F A (Y ) = 3{C F 2 , Y A } originate primarily from gauge field fluctuations and are (block-)diagonally proportional to Y A following the fermion irreps [31]. Scalar self couplings contribute to (27) starting at two loop and can be neglected for sufficiently small couplings.
The nullcline condition β A (Y, α) = 0 for the Yukawa couplings has two types of solutions. The Gaussian fixed point Y A * = 0 always exists, because both E A and F A vanish individually for vanishing Yukawa couplings, whence β A (Y = 0, α) = 0. In addition, and provided that the gauge coupling is non-vanishing, the two terms in (27) can balance against each other. Dimensional analysis shows that the functionsβ A (C) ≡ β A ( √ α C, α)/α 3/2 are independent of the gauge coupling α, implying that Yukawa nullclines take the form The "reduced" Yukawa couplings C A are numerical matrices independent of the gauge coupling g which solveβ A (C) = 0, meaning E A (C) = F A (C) for C A = 0. Evidently C A = 0 corresponds to the Gaussian. 6 The solutions (28) are promoted to genuine fixed points of the coupled system (23), (27) iff the gauge coupling simultaneously takes a real fixed point g * (26). At the fixed point, perturbativity in the Yukawa couplings then follows parametrically from perturbativity in the gauge coupling.
Inserting the nullcline back into (23) we find that the Yukawa-induced terms are of order α 3 owing to (28). This establishes that the shifted one loop coefficient B depends linearly on α through Y * 4 , meaning that (26) constitutes an implicit equation for α * . The implicit dependences are resolved by accounting for the Yukawa contributions as, effectively, modifications of the two loop coefficient. We find where the coefficient ≥ 0 only depends on group theoretical weights and the reduced Yukawa couplings parametrising the nullcline, but not on the gauge coupling. The projection of the flow for the gauge coupling (23) along a hypersurface with β A = 0 then takes the form (1) except that the two loop gauge coefficient C is shifted into C → C = C − 2 D. The shift term vanishes iff all Yukawa couplings vanish but is strictly negative otherwise, whence This result makes it manifest that Yukawa contributions can dynamically lower the effective two loop coefficient, possibly avoiding the no go theorem (16). Furthermore, the shift (30) implies that interacting fixed points for the gauge coupling take the form (4) with C → C , We stress that the expressions (26) and (31) for the gauge coupling fixed point are equivalent and numerically identical. For practical purposes, however, the latter representation, if available, is preferred as it provides the fully resolved version of the former. Following on from our earlier discussion, the fixed points (31) are physical as long as B · C > 0, and perturbative if |B| |C |. If B > 0 and C > 0, they constitute infrared fixed points of the theory, similar to Banks-Zaks fixed points except for the additional presence of Yukawa interactions. If B < 0 and C < 0, they constitute interacting UV fixed points and qualify as asymptotically safe UV completions for the theory, see Tab. 3 c) for a summary. No such weakly coupled UV completion can arise without Yukawa interactions.
We conclude that Yukawa couplings offer a dynamical mechanism to negotiate interacting fixed points in gauge theories. Most importantly, for asymptotically non-free gauge theories with B ≤ 0,  Table 2. Asymptotic safety in gauge theories coupled to matter with a) -c) stating strict no go theorems and d) -e) necessary and sufficient conditions. they offer a unique mechanism to generate weakly interacting fixed points. The strict no go theorem (16) may then be circumnavigated under the auxiliary condition that the Yukawa-induced shift term comes out large enough for C to turn negative. This result, summarised in Tab. 2'd), thus takes the form of a necessary condition for asymptotic safety.

8.
Our results are straightforwardly generalised to gauge-Yukawa theories with several abelian or non-abelian gauge group factors, assuming that some or all of the fermions are charged under some or all of the gauge groups, while the scalars may or may not be charged. The renormalisation of the gauge couplings then takes the form [29] where the two loop Yukawa contributions now arise through Y 4,a = Tr[C Fa 2 Y A (Y A ) † ]/d(G a ) ≥ 0. As is evident from the explicit expression, the quadratic Casimir of the fermions takes the role of a projector to identify the contributions to the running of α a . The running of the Yukawa couplings continues to be given by (27), except that further gauge field contributions turn the last term into a sum over gauge groups 32]. This modification leads to a larger variety of Yukawa nullclines, depending on which of the gauge couplings take vanishing or non-vanishing values at the fixed point. Provided that some or all of the Yukawa couplings take interacting fixed points they will contribute to the running of the gauge couplings (32) through Y * 4,a ≥ 0. Consequently, the gauge beta functions reduce to the form (18) except that the one loop coefficients are effectively shifted, B a → B a = B a + 2 Y * 4,a , due to the fixed point in the Yukawa sector. Most importantly, we observe that Equality holds true iff all Yukawa couplings take Gaussian values. The shift (33) implies that gauge coupling fixed points of the theory arise as the solutions of Once more, this structure has important implications. Following on from our earlier discussion of (21), the fixed point condition (34) can have physical solutions iff all B a are positive. Due to (33) this is naturally the case as long as each gauge group factor is asymptotically free. The theory is then asymptotically free in all gauge factors with interacting fixed points of the Banks-Zaks and the gauge-Yukawa type, and combinations and products thereof. The decisive difference with (21) comes into its own for theories where some or all B a are negative. Provided that the Yukawa-induced shift terms ensure that all B a become positive numbers even if one or several of the gauge factors are not asymptotically free, the fixed point condition (34) can have a variety of novel solutions, see Tab. 3 d). Such fixed points are genuinely of the gauge-Yukawa type, and furthermore constitute candidates for asymptotically safe UV completions of the theory. Also, no such fixed point can arise out of theories with (21), which once more highlights the pivotal role played by Yukawa interactions.
As a final remark, we note that the fixed point condition (34) still depends implicitly on the gauge couplings through B a , once Y 4 is evaluated on a nullcline. It is straightforward to resolve the implicit dependence provided that Y 4,a takes the form along Yukawa nullclines, in analogy to (29). 7 Continuity in each of the gauge couplings α b ≥ 0 together with the non-negativity of Y 4,a allows us to observe that the matrix (D ab ) is non-negative. The flow of the gauge couplings (32) is reduced to (18), except that the two loop term is shifted C ab → C ab = C ab − 2 D ab following (35). We conclude that the Yukawa contributions along nullclines effectively reduce the two loop gauge contributions to the renormalisation of gauge couplings. In this representation, the fixed point condition (34) turns into the equivalent form For non-negative C ab , as has been shown above, interacting fixed points can only be realised if all gauge group factors are asymptotically free. Here, however, the matrix (C ab ) is no longer required to be strictly non-negative, unlike the matrix (C ab ) of two loop gauge contributions, and the no go theorem (20) can be avoided owing to the Yukawa contributions. In view of the asymptotic safety conjecture, this completes our proof that charged fermions with charged or uncharged scalars and, most crucially, Yukawa interactions, constitute strictly necessary ingrediences for interacting UV fixed points in general weakly coupled gauge theories, see Tab. 2 e).
9. Gauge-Yukawa fixed points necessitate scalar fields. Consequently, two auxiliary conditions arise: Firstly, the scalar sector must achieve a fixed point of its own, interacting or otherwise. Secondly, the scalar sector must admit a stable ground state. To appreciate that both of these requirements are non-empty, we consider the renormalisation group flow β = dλ/d ln µ for the quartic scalar couplings λ = (λ ABCD ) based on the interaction Lagrangean To leading order the beta functions β = β(λ, Y, α) depend quadratically on the quartics, on the Yukawa and gauge couplings, and on group theoretical factors related to the gauge transformations of the scalars (if charged) [31]. Explicit expressions and generalisations for product gauge groups 7 The form (35) is evident if only one of the gauge couplings, say g b , is non-vanishing. The nullcline takes the form More generally, (35) holds true for any quantum field theory whose one loop Yukawa vertex corrections obey   (21) simple Yes B > 0 and C > 0 > C Banks-Zaks IR Fig. 3 c) simple Yes B > 0 and C > C > 0 BZ and GYs IR Fig. 4 simple or abelian Yes B < 0 and C < 0 gauge-Yukawas UV/IR Fig. 5 semi-simple, with BZs and GYs and d) or without U (1) factors Yes all B a > 0 products thereof UV/IR soln of (34) Table 3. Summary of weakly interacting fixed points in gauge theories, detailing the availability of Banks-Zaks (BZ) or gauge-Yukawa (GY) type fixed points, or combinations and products thereof.
can be found in [33,35]. Scalar self couplings are not technically natural [28] and can be switchedon by fluctuations of the fermions (due to the presence of Yukawa couplings) or by fluctuations of the gauge fields (if the scalars are charged), implying that β(λ = 0, Y, α) = 0 in general.
Next we turn to the scalar nullclines β = 0, subject to β A → 0. Using dimensional analysis, we observe that the functionsβ(C, C) ≡ β(αC, α C, α)/α 2 are α-independent. The implicit solutions C of the quadratic algebraic equationsβ(C(C), C) = 0 provide us with The "reduced" scalar couplingsC are numerical tensors which depend on group theoretical factors and the reduced Yukawa couplings, but not explicitly on the gauge coupling. Since the quartics do not impact on the gauge-Yukawa flow (to leading order) it is immaterial for this analysis whether the gauge coupling is slowly running or sitting on a fixed point.
Qualitatively and quantitatively different types of solutions λ * arise for all physically inequivalent Yukawa nullclines with C A = 0, and with C A → 0. In either of these cases, owing to the quadratic nature of the defining equations, solutions (37) generically come up in inequivalent pairs C ± per Yukawa nullcline with complex entries. Reality of quartic couplings is not automatically guaranteed and must be required as an auxiliary condition. Vacuum stability necessitates that λ * is a positive-definite tensor. 8 This information is not encoded in the renormalisation group flow even if the scalar couplings come out real, meaning that the stability of the effective potential V eff (φ) provides an independent constraint. We therefore conclude that (37), subject to are mandatory auxiliary conditions for gauge theories with scalar matter to display a physically acceptable scalar sector, in addition to the conditions for free or interacting fixed points in the gauge or gauge-Yukawa sectors. A few comments are in order: (i) Solutions of (38) with C A = 0 are mandatory for gauge-Yukawa fixed points and for asymptotic safety [8,37]. Those with C A = 0 are mandatory for Banks-Zaks fixed points in the presence of scalar matter. (ii) Both of (38) must be imposed irrespective of the UV or IR nature of the underlying fixed point. (iii) If two solutionsC ± are physical, one of them is UV and the other IR relevant. (iv) Solutions to (37), (38) also control trajectories in the vicinity of free or interacting fixed points [34]. Those with C A = 0 entail that gauge, Yukawa, and scalar couplings run at the same rate and govern the approach to gauge-Yukawa fixed points. Those with C A → 0 (referring to reduced Yukawa couplings which approach the Gaussian very rapidly Y A (α)/ √ α ≡ C A (α) 1) are relevant for asymptotically free theories to display complete asymptotic freedom, and for trajectories approaching Banks-Zaks fixed points. Scalar couplings then run into the Gaussian UV fixed point either alongside the gauge coupling, or faster λ * (α)/α 1. The latter follows from the α-dependence of the reduced Yukawa couplings C A (α) which entails an implicit α-dependence for the quartics [31]. (iv) A method to find solutions in the limit C A → 0 has been detailed in [38]. Physical solutions for the combined Yukawa and scalar nullclines with (38) exist and are known for a number of theories [39][40][41][42]. 9 This completes the derivation of necessary and sufficient conditions of existence for weakly interacting fixed points in general gauge theories coupled to matter. Gauge theories with B > 0 and C < 0 have no weakly coupled fixed points. At weak coupling, the phase diagram solely displays asymptotic freedom and the Gaussian UV fixed point, Fig. 2. The set of UV free trajectories emanating out of it are indicated by the red shaded area. Its upper boundary is provided by the Yukawa nullcline which also acts as an infrared attractor [44][45][46][47][48] due to the fact that the sign of (27) is always controlled by the gauge field fluctuations for small Yukawa couplings. On the scaling trajectory, the gauge, Yukawa and scalar couplings run at the same rate into the Gaussian UV fixed point [34]. UV free trajectories continue towards the domain of strong coupling where the theory is expected to display confinement and chiral symmetry breaking, or, possibly, a strongly coupled IR fixed point. On the other hand, above the Yukawa nullcline no trajectories are found which can reach the Gaussian in the UV. On such trajectories, the theory technically loses asymptotic freedom. Predictivity is then limited up to a finite UV scale, unless a strongly coupled UV fixed point materialises out of the blue. the Yukawa direction. The former follows from asymptotic freedom together with (23), while the latter follows from (27) and ∂F A /∂Y B being non-negative and proportional to the gauge coupling times the sum of the quadratic Casimirs of the fermions attached to the vertex. Moreover, at weak coupling and close to the Banks-Zaks, the flow is always parametrically faster into the Y 4 than into the gauge direction. Consequently, the Bank-Zaks fixed point together with the Yukawa nullcline act as a strong infrared-attractive funnel for all trajectories emanating from the Gaussian UV fixed point, see Fig. 3. This leads to low energy relations between the Yukawa and the gauge coupling dictated by (27) (at weak coupling), irrespective of their detailed UV origin. 10 Elsewise the same discussion as in the previous example applies.
Progressing towards gauge theories with B > 0 and C > C > 0 we now additionally observe a fully interacting gauge-Yukawa fixed point besides the Banks-Zaks, displayed in Fig. 4. The main new effect in theories with C > 0 as opposed to those with C < 0 is that the funneling of flow trajectories towards the IR attractive Yukawa nullcline comes to a halt, whereby couplings take an interacting IR fixed point (28), (31). Furthermore, the fixed point is genuinely attractive in both the gauge and the Yukawa directions. 11 The theory comes out more strongly coupled at the gauge-Yukawa than at the Banks-Zaks fixed point owing to (30). The gauge-Yukawa fixed point characterises a second order phase transition between a symmetric phase and a phase with spontaneous symmetry breaking where the scalars acquire a non-vanishing vacuum expectation value. Details of the phase transition becomes visible once mass terms are added, taking the role of temperature, with the scalar vacuum expectation values serving as order parameters. Spontaneous α Y 4 GY G Figure 5. Fixed points and phase diagrams of gauge-Yukawa theories with B < 0 and C < 0 at weak coupling showing asymptotic safety together with the Gaussian and gauge-Yukawa fixed points. Notice that the set of UV finite trajectories is confined to a hypercritical surface dictated by the Yukawa nullcline. symmetry breaking may also entail the breaking of chiral symmetry via Yukawa couplings. Away from fixed points, the theory may display a number of further phenomena such as first order phase transitions, dimensional transmutation, decoupling, and confinement in the deep IR. 12 Turning to simple or abelian gauge theories with B < 0 and C < 0 we observe that asymptotic freedom is absent and the Gaussian has become an infrared fixed point. Also, it is impossible for this type of theories to have a Banks-Zaks fixed point owing to the no go theorem (16). However, the Yukawa interactions have turned the two loop coefficient C > 0 effectively into C < 0 allowing for an interacting gauge-Yukawa fixed point (31) as displayed in Fig. 5. This fixed point genuinely displays an attractive and a repulsive direction, the former being a consequence of the IR attractive nature of Yukawa nullclines, and the latter a consequence of infrared freedom in the gauge coupling. Moreover, it qualifies as an asymptotically safe fixed point owing to the two UV finite trajectories emanating out of it [8]. The weak coupling trajectory connects the interacting fixed point with the Gaussian in the infrared whereby the theory remains unconfined at all scales. The strong coupling trajectory, as in the previous cases, is expected to lead to confinement and chiral symmetry breaking, or conformal behaviour at low energies. Away from the Yukawa nullcline (which always coincides with the hypercritical surface of the gauge-Yukawa fixed point), no trajectories are found which can reach the gauge-Yukawa fixed point in the UV. On such trajectories, the theory technically loses asymptotic safety and predictivity is limited by a maximal UV scale unless a novel UV fixed point emerges at strong coupling.
As an aside, it is worth noticing a similarity between gauge-Yukawa theories with complete asymptotic freedom and a Banks-Zaks, and gauge-Yukawa theories with asymptotic safety, see Figs. 3 and 5. In both cases, trajectories which escape from the UV fixed point region towards strong coupling in the IR are solely determined by the Yukawa nullcline. All settings predict IR relations between Yukawa and gauge couplings. In the former case this arises due to a funnel effect while in the latter it follows from the unstable direction of the interacting UV fixed point. Without Banks-Zaks, IR relations may be avoided at the expense of substantial fine-tuning in the deep UV, see Fig. 2.
The discussion of phase diagrams generalises to more complex settings. Gauge theories with several independent Yukawa couplings will lead to several parameters C , which, depending on their magnitudes, may generate several gauge-Yukawa fixed points. Phase diagrams will then display an enhanced structure owing to additional cross-over phenomena amongst the various fixed points. An even richer pattern arises for theories with product gauge groups, see Tab. 3 d).
Here, the gauge loop coefficients B a and C ab together with the Yukawa-induced coefficients B a uniquely determine the fixed point structure at weak coupling. Evidently, for each gauge coupling individually our discussion based on the "diagonal" coefficients B, C and C applies, meaning that parts of the enlarged phase diagrams materialise as "direct products" of those shown in Figs. 2-5.
As a novel addition, theories will also display "off-diagonal" Banks-Zaks and gauge-Yukawa fixed points as well as fully interacting products thereof, depending on the availability and structure of the solutions to (34). 13 Furthermore, each interacting fixed point naturally relates to a conformal window similar to those of QCD with fermionic matter. Some of the fixed points of (product) gauge theories offer UV conformal windows around fixed points with exact asymptotic safety at weak coupling. It is therefore natural to speculate that some such models may qualify as UV completions for the Standard Model of particle physics.
11. Finally, we briefly comment on interacting fixed points in 4d supersymmetric QFTs. Supersymmetry imposes relations amongst gauge, Yukawa, and scalar couplings [56]. In general, quartic scalar selfinteractions are no longer independent. For theories with N = 1 supersymmetry without superpotentials, gauge beta functions remain of the form (1) at weak coupling. The signs of B and C depend on the matter content [17]. Gauge sectors can develop Banks-Zaks fixed points (4) which are always IR (B > 0) but never UV [57], fully consistent with our findings in non-supersymmetric theories (16), (20). An important difference arises once superpotentials (i.e. Yukawa couplings) are present. Owing to supersymmetry, Yukawas can only take weakly interacting fixed points provided at least one of the gauge sectors is asymptotically free [57]. This implies that asymptotic safety at weak coupling is out of reach for simple N = 1 supersymmetric gauge theories. Overall, weakly interacting fixed points are either absent, or of the Banks-Zaks, or of the gauge-Yukawa type. Phase diagrams of simple 4d gauge theories with N = 1 supersymmetry take the form Fig. 2 or Fig. 4, while settings with Fig. 3 or Fig. 5 cannot be realised. For N = 2 supersymmetry, Yukawa couplings are no longer independent but related to the gauge coupling. Moreover, the running of the gauge coupling becomes one-loop exact with (1) and C ≡ 0 [58,59]. Hence, N = 2 theories are either asymptotically free or infrared free and interacting fixed points cannot arise. In the limit where B = 0, the gauge coupling becomes exactly marginal leading to a line of fixed points [58]. The latter continues to hold true for maximally extended supersymmetry, N = 4 SYM, where the constraints from supersymmetry are so powerful that the theory does not flow under the RG, and any value of the gauge coupling corresponds to a fixed point. 14

12.
In summary, we have identified the interacting fixed points of four-dimensional gauge theories in the regime where gauge and matter fields remain good fundamental degrees of freedom. Low-energy fixed points are either of the Banks-Zaks or gauge-Yukawa type, or combinations and products theoreof (Tab. 3), offering a rich spectrum of phenomena including phase transitions and the spontaneous breaking of symmetry. We have also derived no go theorems together with necessary and sufficient conditions to guarantee asymptotic safety of general gauge theories (Tab. 2). Interacting high-energy fixed points are invariably of the gauge-Yukawa type and require elementary scalar fields such as the Higgs. Hence, the findings of [8] were not a coincidence: rather, the dynamical mechanism to tame the notorious Landau poles of general infrared free gauge theories is unique, and, owing to the group-theoretical limitation (14), exclusively delivered through Yukawa interactions. We conclude that our findings open a window of opportunities towards perturbative UV completions of the Standard Model beyond the paradigm of asymptotic freedom.