Two-dimensional SCFTs from matter-coupled 7D N=2 gauged supergravity
Parinya Karndumri, Patharadanai Nuchino

TL;DR
This paper constructs and analyzes supersymmetric $AdS_3$ solutions in 7D gauged supergravity, revealing new holographic duals to 2D SCFTs and RG flows from 6D theories, with some solutions upliftable to M-theory.
Contribution
It introduces a new class of supersymmetric $AdS_3$ solutions with specific internal geometries, extending the understanding of holographic duals for lower-dimensional SCFTs.
Findings
Existence of $AdS_3$ solutions with $M^4= ext{product of Riemann surfaces}$
Identification of RG flows from 6D to 2D SCFTs
Some solutions uplift to eleven-dimensional supergravity.
Abstract
We study supersymmetric solutions of gauged supergravity in seven dimensions coupled to three vector multiplets with gauge group and being a four-manifold with constant curvature. The gauged supergravity admits two supersymmetric critical points with and symmetries corresponding to superconformal field theories (SCFTs) in six dimensions. For with being a Riemann surface, we obtain a large class of supersymmetric solutions preserving four supercharges and symmetry for one of the being a hyperbolic space , and the solutions are dual to SCFTs in two dimensions. For a smaller symmetry , only solutions exist. Some of these are also solutions…
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Two-dimensional SCFTs from matter-coupled gauged supergravity
Parinya Karndumria and Patharadanai Nuchinob
String Theory and Supergravity Group, Department of Physics, Faculty of Science, Chulalongkorn University, 254 Phayathai Road, Pathumwan, Bangkok 10330, Thailand
E-mail: a[email protected]
E-mail: b[email protected]
Abstract
We study supersymmetric solutions of gauged supergravity in seven dimensions coupled to three vector multiplets with gauge group and being a four-manifold with constant curvature. The gauged supergravity admits two supersymmetric critical points with and symmetries corresponding to superconformal field theories (SCFTs) in six dimensions. For with being a Riemann surface, we obtain a large class of supersymmetric solutions preserving four supercharges and symmetry for one of the being a hyperbolic space , and the solutions are dual to SCFTs in two dimensions. For a smaller symmetry , only solutions exist. Some of these are also solutions of pure gauged supergravity with gauge group. We numerically study domain walls interpolating between the two supersymmetric vacua and these geometries. The solutions describe holographic RG flows across dimensions from SCFTs in six dimensions to two-dimensional SCFTs in the IR. Similar solutions for being a Kahler four-cycle with negative curvature are also given. In addition, unlike case, it is possible to twist by gauge fields resulting in two-dimensional SCFTs. Some of the solutions can be uplifted to eleven dimensions and provide a new class of solutions in M-theory.
1 Introduction
One of the most interesting implications of the AdS/CFT correspondence [1] is the study of holographic RG flows. These solutions take the form of a domain wall interpolating between vacua and holographically describe deformations of a conformal field theory (CFT) in the UV to another CFT in the IR or in some cases to a non-conformal field theory dual to a singular geometry, see [2, 3, 4] for example. Of particular interest are RG flows across dimensions in which a higher dimensional CFT flows to a lower dimensional CFT. This type of RG flows allows us to investigate the structure and dynamics of less known CFTs in higher, especially five and six, dimensions using the well-understood lower dimensional CFTs. In this paper, we will consider this type of RG flows in six-dimensional CFTs to two dimensions. Furthermore, the study along this direction is much more fruitful and controllable in the presence of supersymmetry. We are then mainly interested in RG flows within superconformal field theories (SCFTs).
Supersymmetric solutions of gauged supergravities play an important role in studying the aforementioned RG flows. In general, RG flows across dimensions from a -dimensional SCFT to a -dimensional SCFT are obtained by twisted compactification of the former on an -dimensional manifold . The twist is needed for the compactification to preserve some amount of supersymmetry. This is achieved by turning on some gauge fields to cancel the spin connection on . In the supergravity dual, these RG flows are described by domain walls interpolating between an vacuum to an geometry. Solutions of this type have been studied in various dimensions, see [5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26] for an incomplete list.
In this paper, we are interested in supersymmetric solutions of gauged supergravity in seven dimensions with gauge group. This gauged supergravity is obtained by coupling three vector multiplets to pure gauged supergravity with gauge group constructed in [27, 28]. The matter-coupled gauged supergravity has been constructed in [29, 30, 31] with an extension to include a topological mass term for the three-form field, dual to the two-form in the supergravity multiplet, given in [32]. This massive gauged supergravity admits supersymmetric vacua which has been extensively studied in [33, 34, 35]. These vacua are dual to SCFTs in six dimensions, and a number of RG flows of various types have already been studied [18, 33, 36]. However, holographic RG flows from six-dimensional SCFTs to two-dimensional SCFTs in the framework of matter-coupled gauged supergravity have not appeared so far. To fill this gap, we will give a large class of fixed points and the corresponding RG flows across dimensions within six-dimensional SCFTs.
We will consider a four-manifold with constant curvature of two types, a product of two Riemann surfaces and a Kahler four-cycle . In the first case, the twists can be performed by using with being the R-symmetry. We will look for solutions with , and symmetries. In the second case, has a spin connection. Therefore, we can perform the twists by turning on either or the full to cancel the or the parts of the spin connection, respectively. It should also be noted that a twist by cancelling the full spin connection is not possible since the R-symmetry of gauged supergravity is not large enough.
In general, the two factors in the gauge group can have different coupling constants. However, for a particular case of equal coupling constants, the resulting gauged supergravity can be embedded in eleven-dimensional supergravity via a truncation on [37]. The seven-dimensional solutions can accordingly be uplifted to eleven dimensions giving rise to new solutions of eleven-dimensional supergravity. Therefore, these solutions provide a number of new two-dimensional SCFTs with known M-theory dual. We also consider the uplifted solutions in this case.
The paper is organized as follow. In section 2, we give a short review of the matter coupled seven-dimensional gauged supergravity and supersymmetric vacua. In sections 3 and 4, we look for supersymmetric and solutions and numerically study interpolating solutions between these geometries and the fixed points. We finally give some conclusions and comments in section 5. Relevant formulae for the truncation of eleven-dimensional supergravity on giving rise to gauged supergravity with gauge group are reviewed in the appendix.
2 Seven-dimensional gauged supergravity and supersymmetric vacua
We firstly review gauged supergravity in seven dimensions coupled to three vector multiplets with gauge group. Only relevant formulae involving bosonic Lagrangian and supersymmetry transformations of fermions will be presented. The detailed construction of general seven-dimensional gauged supergravity can be found in [32], see also [38] for gaugings in the embedding tensor formalism.
2.1 Seven-dimensional gauged supergravity
The seven-dimensional gauged supergravity is obtained by coupling the minimal supergravity to three vector multiplets. The supergravity multiplet consists of the graviton , two gravitini , three vectors , two spin- fields , a two-form field and the dilaton . Each vector multiplet contains a vector field , two gaugini , and three scalars . We will use the convention that curved and flat space-time indices are denoted by , and , respectively. Indices and label triplet and doublet of R-symmetry with the latter being suppressed throughout this work. The three vector multiplets will be labeled by indices which in turn describe the triplet of the matter symmetry under which the three vector multiplets transform.
From both supergravity and vector multiplets, there are in total six vector fields denoted collectively by . Indices describe fundamental representation of the global symmetry and are lowered and raised by the invariant tensor and its inverse . The two-form field will be dualized to a three-form , which admits a topological mass term required by the existence of vacua.
The nine scalar fields parametrize coset manifold. They can be described by the coset representative
[TABLE]
with an index corresponding to representations of the compact local symmetry. The inverse of will be denoted by
[TABLE]
with the relation
[TABLE]
Being an element of , the coset representative also satisfies the relation
[TABLE]
The bosonic Lagrangian of the gauged supergravity in form language can be written as
[TABLE]
The constant describes the topological mass term for the three-form with the field strength . The gauge field strength is defined by
[TABLE]
The definition of the structure constants includes the gauge coupling constants
[TABLE]
where and are coupling constants of and , respectively.
The scalar matrix appearing in the kinetic term of vector fields is given in term of the coset representative as follow
[TABLE]
The Chern-Simons three-form satisfying is defined by
[TABLE]
The scalar potential is given by
[TABLE]
where -functions, or fermion-shift matrices, are defined as
[TABLE]
It should also be noted that indices and are raised and lowered by and , respectively. Finally, the scalar kinetic term is defined in term of the vielbein on the coset as
[TABLE]
To find supersymmetric solutions, we need supersymmetry transformations of fermionic fields , and . With all fermionic fields vanishing, these transformations read
[TABLE]
where are the usual Pauli matrices.
The dressed field strengths and are defined by the relations
[TABLE]
The covariant derivative of the supersymmetry parameter is given by
[TABLE]
where is defined in term of the composite connection as
[TABLE]
with
[TABLE]
For convenience, we also give the full bosonic field equations derived from the Lagrangian given in (5)
[TABLE]
2.2 Supersymmetric critical points
We now give a brief review of supersymmetric vacua found in [33]. There are two supersymmetric critical points with and symmetries. To compute the scalar potential, we need an explicit parametrization of coset. By defining the following matrices
[TABLE]
we can write non-compact generators of as
[TABLE]
Among the nine scalars from , there is one singlet corresponding to the non-compact generator
[TABLE]
The coset representative is then given by
[TABLE]
The scalar potential for the dilaton and the singlet scalar is readily computed to be
[TABLE]
This potential admits two supersymmetric critical points
[TABLE]
Critical points I and II have and symmetries, respectively. We have also chosen to bring the critical point to the value . The cosmological constant is denoted by . According to the AdS/CFT correspondence, these critical points correspond to SCFTs in six dimensions with and symmetries, respectively. A holographic RG flow interpolating between these two critical points has already been studied in [33], see also [39] for more general solutions. In subsequent sections, we will find supersymmetric solutions to this gauged supergravity and RG flow solutions from the above vacua to these geometries in the IR.
3 Supersymmetric solutions and RG flows
In this section, we look for supersymmetric solutions of the form with for being two-dimensional Riemann surfaces. Constants describe the curvature of with values corresponding to a two-dimensional sphere , a flat space or a hyperbolic space , respectively.
We will choose the ansatz for the seven-dimensional metric of the form
[TABLE]
in which , is the flat metric on the two-dimensional spacetime. The explicit form of the metric on can be written as
[TABLE]
The functions are defined as
[TABLE]
By using an obvious choice of vielbein
[TABLE]
we can compute the following non-vanishing components of the spin connection
[TABLE]
Throughout the paper, we will use primes to denote derivatives of a function with respect to its argument for example and .
To find supersymmetric solutions which admit non-vanishing Killing spinors, we perform a twist by turning on gauge fields along . In the following discussions, we will consider various possible twists with different unbroken symmetries.
3.1 vacua with symmetry
We first consider solutions with symmetry. To perform the twist, we turn on the following gauge fields on
[TABLE]
where are constants magnetic charges.
There is one singlet scalar from coset corresponding to the non-compact generator . We then parametrize the coset representative by
[TABLE]
with depending only on the radial coordinate . By computing the composite connection along , we can cancel the spin connections by imposing the following twist conditions
[TABLE]
together with the projection conditions
[TABLE]
Note that only the gauge field enters the twist procedure since is the gauge field of under which the gravitini and supersymmetry parameters are charged.
From the gauge fields given in (39) and (40), we can straightforwardly compute the corresponding two-form field strengths
[TABLE]
It should also be noted that these field strengths give non-vanishing term. This term is present in the field equation of the three-form fied as can be seen from equation (22). Therefore, we need to turn on the three-form field with the corresponding four-form field strength given by
[TABLE]
This is very similar to the solutions of maximal gauged supergravity considered in [8].
By imposing an additional projector
[TABLE]
required by and conditions, we find the following BPS equations
[TABLE]
It can be verified that these BPS equations satisfy all the field equations. At large , we have and with the radius given by , and the terms involving gauge fields and the three-form field are highly suppressed. We find the fixed point from these BPS equations in this limit. The solutions are then asymptotically locally as .
We now look for supersymmetric solutions satisfying and in the limit . We find a class of fixed point solutions
[TABLE]
where
[TABLE]
Note that the coupling constant does not appear in the above equations, so the solutions can be uplifted to eleven dimensions by setting .
To obtain real solutions, we require that , , , and . It turns out that solutions are possible only for one of the two is equal to with the seven-dimensional spacetime given by , and . Since the charges and are fixed by the twist conditions (42), there are only two parameters and characterizing the solutions. For and , regions in the parameter space (, ) for good AdS3 vacua to exist are shown in figure 1. Note that these regions are precisely the same as supersymmetric solutions of maximal seven-dimensional gauged supergravity in [8].
These fixed points preserve four supercharges due to the two projectors in (43) and correspond to SCFTs in two dimensions with symmetry. On the other hand, the entire RG flow solutions interpolating between the fixed point and these geometries preserve only two supercharges due to an extra projector in (47). Examples of these RG flows from the fixed point to , and with and different values of and are shown in figures 2, 3 and 4, respectively.
These solutions can be uplifted to eleven dimensions using the truncation ansatz given in [37]. By using the formulae reviewed in the appendix together with the coordinates
[TABLE]
and the matrix
[TABLE]
we find the eleven-dimensional metric
[TABLE]
with , and
[TABLE]
From the metric, we see that the symmetry corresponds to the isometry along the and directions.
3.2 vacua with symmetry
We now consider solutions with symmetry. In this case, there are three singlets from the nine scalars in coset. These correspond to non-compact generators
[TABLE]
The coset representative takes the form of
[TABLE]
The ansatz for gauge fields is obtained from that of given in (39) and (40) by setting or, equivalently,
[TABLE]
We will also simplify the notation by redefining the charges and . In this case, the four-form field strength is given by
[TABLE]
and the twist conditions read
[TABLE]
Using the projection conditions (43) and (47), we obtain the corresponding BPS equations. It turns out that compatibility between these BPS equations and field equations requires either or . Furthermore, setting gives the same BPS equations as setting with and interchanged. We will then consider only the case with the following BPS equations
[TABLE]
In this case, solutions to the BPS equations are asymptotic to the two supersymmetric vacua with and symmetries at large . Furthermore, unlike the previous case, all charge parameters are fixed by the twist conditions, and there exist only solutions.
We now look for fixed points. The solutions also preserve four supercharges and correspond to SCFTs in two dimensions as in the previous case. We begin with a class of fixed points for
[TABLE]
with or for vacua to exist. An example of RG flows from the critical point to this fixed point for and is shown in figure 5 with set to zero along the flow.
Another class of solutions with is given by
[TABLE]
with the condition . Examples of RG flow solutions from the and vacua to these fixed points are respectively shown in figures 6 and 7 for and . Note that and have the same value at both the and fixed points.
Moreover, with a suitable set of boundary conditions, there exists an RG flow from to fixed points and then to critical point as shown in figure 8. All vacua and RG flows in this case cannot be uplifted to eleven dimensions since the existence of these solutions require . Therefore, the corresponding holographic interpretation is rather limited.
3.3 vacua with symmetry
We now move on to solutions with symmetry. There are three singlet scalars from coset. These correspond to non-compact generators , and . Therefore, the coset representative can be written as
[TABLE]
To perform the twist, we take the following ansatz for the gauge field
[TABLE]
The four-form field strength in this case is given by
[TABLE]
We can now repeat the same procedure as in the previous two cases to find the corresponding BPS equations. In this case, it turns out that compatibility between the BPS equations and second-order field equations allows only one of the , , to be non-vanishing. We have verified that any of the leads to the same set of BPS equations. We will choose and for definiteness. With this choice, the BPS equations are given by
[TABLE]
For these equations, there exist fixed points only for . The resulting solution is given by
[TABLE]
This solution again preserves four supercharges and corresponds to SCFT in two dimensions. An example of RG flow solutions from six-dimensional SCFT to this fixed point for and is shown in figure 9. Note that the fixed point and the RG flow are also solutions of pure gauged supergravity with gauge group.
As in the case of solutions with symmetry, the above solutions can be uplifted to eleven dimensions by setting . The eleven-dimensional metric can be obtained from (61) by setting and , or equivalently . The result is given by
[TABLE]
with
[TABLE]
It should also be pointed out that the seven-dimensional solution in this case has recently been discussed in the context of massive type IIA theory in [40].
4 Supersymmetric solutions and RG flows
In this section, we repeat the same analysis for being a Kahler four-cycle and look for solutions of the form . For the constant , the Kahler four-cycle is given by a two-dimensional complex space , a four-dimensional flat space , or a two-dimensional complex hyperbolic space , respectively. The Kahler four-cycle has spin connection. We can perform a twist by using either or gauge fields to cancel the or parts of the spin connection.
4.1 vacua with symmetry
We begin with vacua with symmetry and take the following ansatz for the seven-dimensional metric
[TABLE]
The metric on the Kahler four-cycle is given by
[TABLE]
with and the function defined by
[TABLE]
, , are left-invariant one-forms satisfying . Their explicit form is given by
[TABLE]
The ranges of the coordinates are , , and .
By choosing the following choice of vielbein
[TABLE]
we find non-vanishing components of the spin connection
[TABLE]
We can now perform the twist by turning on gauge fields with the following ansatz
[TABLE]
The associated two-form field strengths are given by
[TABLE]
where is the Kahler structure defined by
[TABLE]
To implement the twist, we impose the following projectors on the Killing spinors
[TABLE]
together with the twist condition
[TABLE]
As in the previous cases, we need to turn on the three-form field with the field strength
[TABLE]
With all these and the projector (47), we can derive the following BPS equations
[TABLE]
with being the singlet scalar in (41).
The BPS equations admit an fixed point given by
[TABLE]
The solution preserves four supercharges and exists for
[TABLE]
with , , and . The fixed point is dual to an two-dimensional SCFT.
Examples of RG flows interpolating between this fixed point and the critical point for and different values of are shown in figure 10.
As in the case, the fixed point and the associated RG flows can be uplifted to eleven dimensions by setting . The eleven-dimensional metric can be obtained from (61) by replacing by and using the gauge fields in (96). We will not repeat it here.
4.2 vacua with symmetry
We next consider solutions with smaller residual symmetry by imposing the condition . There are three singlet scalars with the coset representative given by (64). As in the previous section, compatibility between BPS equations and field equations requires or , and these two cases are equivalent. We will consider the case of with the following BPS equations
[TABLE]
There exist two classes of fixed points preserving four supercharges and corresponding to SCFTs in two dimensions with symmetry. With , the first class of fixed points is given by
[TABLE]
with or for vacua to exist. An RG flow solution from the critical point to fixed point for , and is shown in figure 11.
Another class of fixed points is given by
[TABLE]
To obtain good vacua, we require that . Various RG flows from six-dimensional SCFTs with and symmetries to these fixed points for and are shown in figures 12, 13 and 14.
As in the case of , all of these fixed points and RG flows cannot be uplifted to eleven dimensions using the truncation given in [37], so we do not have a clear holographic interpretation in this case.
4.3 vacua with symmetry
By setting in the case, we obtain solutions with symmetry. As in the previous case, the three singlet scalars need to vanish in order for fixed points to exist. We will accordingly set all vector multiplet scalars to zero for brevity. The resulting BPS equations are given by
[TABLE]
After imposing the twist condition (100), we obtain an solution for given by
[TABLE]
An RG flow from to this fixed point for is shown in figure 15.
4.4 vacua with symmetry
For Kahler four-cycles with spin connection, we can also perform the twist by identifying with the gauge symmetry . In this case, we will use the metric on in the form
[TABLE]
with being the left-invariant one-forms given in (93) and defined in (36).
With the seven-dimensional vielbein
[TABLE]
we can compute the following non-vanishing components of the spin connection
[TABLE]
We then turn on the gauge fields as follow
[TABLE]
with the two-form field strengths given by
[TABLE]
As in the previous cases, we also need a non-vanishing four-form field strength
[TABLE]
together with the twist condition
[TABLE]
and the following projectors
[TABLE]
It should be noted that the second condition in (128) consists of only two independent projectors since projector can be obtained from the product of those coming from and . Therefore, the resulting fixed points preserve two supercharges corresponding to superconformal symmetry in two dimensions.
With all these and the coset representative for the singlet scalar in (30), we find the following BPS equations
[TABLE]
We now look for fixed points for the case of that can be embedded in eleven dimensions. Setting in the above equations, we find the following fixed point
[TABLE]
An RG flow interpolating between the vacuum and this fixed point is shown in figure 16.
We can also uplift this solution to eleven dimensions by first choosing the coordinates
[TABLE]
with being coordinates on satisfying . After using the matrix
[TABLE]
we find the eleven-dimensional metric
[TABLE]
with given by
[TABLE]
and . The gauge fields are given by
[TABLE]
For , we find the following fixed points
[TABLE]
These are solutions with the condition . Finally, we can numerically find RG flow solutions connecting these fixed points to vacua with and symmetries. Examples of these solutions for and are given in figures 17, 18 and 19.
5 Conclusions
We have studied supersymmetric solutions of seven-dimensional gauged supergravity with gauge group. For being a product of two Riemann surfaces, we have found a large class of solutions with symmetry for similar to the corresponding solutions in maximal gauged supergravity studied in [8]. Furthermore, there exist a number of solutions with and symmetries. In the latter case, all scalars from vector multiplets vanish, so the solution can be interpreted as a solution of pure gauged supergravity with gauge group. We have also numerically given various holographic RG flows from supersymmetric vacua with and symmetries to these fixed points. The solutions decribe RG flows across dimensions from SCFTs in six dimensions to two-dimensional SCFTs in the IR.
For being a Kahler four-cycle, the solutions only exist for the Kahler four-cycles with negative curvature. In this case, the spin connection on is a connection. There are two possibilities for performing the twists, along the and parts. For a twist by , we have found fixed points with , and symmetries. The solutions preserve four supercharges and correspond to two-dimensional SCFTs. For a twist along the part, we have performed the twist by turning on the gauge fields. Unlike the previous cases, the fixed points in this case preserve only two supercharges. The solutions are accordingly dual to two-dimensional SCFTs. We have studied RG flows from supersymmetric vacua to these geometries as well.
All of these solutions provide a large class of solutions and RG flows across dimensions from six-dimensional SCFTs to two-dimensional SCFTs. The solutions might be useful in the holographic study of supersymmetric deformations of SCFTs in six dimensions to two dimensions. For equal gauge coupling constants, the gauged supergravity can be embedded in eleven-dimensional supergravity. We have also given the uplifted eleven-dimensional metric. These solutions with a clear M-theory origin should be of particular interest in the study of wrapped M5-branes on four-manifolds.
For solutions with different coupling constants, there is no known embedding in string/M theory. Therefore, in this case, the holographic interpretation as RG flows in the dual SCFTs should be done with some caveats. It would be interesting to look for the embedding of these solutions in ten or eleven dimensions. This could give rise to the full holographic duals of the effective theories on -branes wrapped on four-manifolds. Similar solutions in gauged supergravity with other gauge groups also deserve further study. Finally, it should be noted that the RG flows across dimensions given here can be interpreted as supersymmetric black strings in asymptotically space. Our solutions should be useful in the study of black string entropy using twisted indices of SCFTs along the line of [41].
Acknowledgement
This work is supported by The Thailand Research Fund (TRF) under grant RSA6280022.
Appendix A Truncation ansatz of eleven-dimensional supergravity on
In this appendix, we review relevant formulae for embedding solutions of seven-dimensional gauged supergravity in eleven-dimensional supergravity. Since the solutions involve all types of seven-dimensional fields namely scalar, vector and three-form fields, the eleven-dimensional four-form field strength is very complicated. Accordingly, we omit an explicit form of the four-form in each case for brevity. It can however be computed by using the formula given in [37] and the mapping between seven- and eleven-dimensional fields given here.
The truncation of eleven-dimensional supergravity on leading to seven-dimensional gauged supergravity is described by the metric ansatz
[TABLE]
with the following definitions
[TABLE]
, , are coordinates on satisfying .
Together with the four-form ansatz given in [37], the Lagrangian for the resulting gauged supergravity, after multiplied by , reads
[TABLE]
with the scalar potential given by
[TABLE]
A symmetric scalar matrix , with unit determinant describes nine scalars in coset. This is equivalent to coset due to the isomorphisms and .
In term of the coset representative with indices , we have the relation
[TABLE]
The coset representative is related to that of by the relation
[TABLE]
in which and are chirally projected gamma matrices of satisfying the relations
[TABLE]
and , , see more detail in [32]. Note also that also satisfy similar relations which we will not repeat them here. We use the following choice of
[TABLE]
All these ingredients lead to the following identification of the fields and parameters in seven and eleven dimensions
[TABLE]
With this identification, it can also be easily verified that the scalar matrix for the gauge kinetic terms also match
[TABLE]
For convenience, we explicitly give the coset representative and gauge fields as follow.
- •
singlet scalar:
[TABLE]
We have used the relation with .
- •
singlet scalar:
[TABLE]
- •
singlet scalars:
[TABLE]
In all cases, it can be verified using the relation (146) that the above give precisely in the main text.
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