Thursday, 11 September 2014

Type IIB Supergravity

Type IIB supergravity represents the low energy effective field theory describing massless particles with momenta below the scale of massive modes of the superstring. This is another maximal supergravity that can be constructed in ten dimensions. The type IIB theory is chiral and cannot be obtained by dimensional reduction from eleven dimensions. Nevertheless, it is related to type IIA supergravity by T-duality. Type IIB SUGRA contains, in addition to the generic fields of the Neveu-Schwarz (NS) sector, gauge potentials characteristic of the Ramond-Ramond (RR) sector. The bosonic fields of the IIB supergravity comprise of the graviton, the antisymmetric two form with a three-form field strength and the dilaton. The fermionic content of type IIB supergravity comprises a positive chirality dilatino and a negative chirality gravitino. Spinors in IIB are complex Weyl spinors. The gravitino and the dilatino have opposite chiralities, the supersymmetry parameter has the same chirality as the gravitino. Type IIB supergravity is the low-energy limit of type IIB string theory, which contains a fundamental string and various D-branes of odd D coupling to the gauge fields, similar to the even D-branes of type IIA. The action exhibits an interesting symmetry under modular transformations. Supersymmetry is used to derive conditions on higher derivative terms in the effective action of type IIB supergravity. Superstring effective actions are dependent on the actions of supergravity theories. Thus, there is much to be learned from the old techniques used to compactify them if we translate them to string language. The field equations and the supersymmetry transformations of type IIB supergravity can be worked out in a tricky manner. With the equations of motion identified, one looks at the supergravity action that reproduces these equations of motion and complements them with the self-duality condition. The dilaton and the axion are ordinary interacting particles in the low energy theory of superstring and thus should be treated on same footing as the other low energy fields such as the graviton, the antisymmetric second rank tensor and fermoins. Second, in a type IIB superstring or supergravity it is well known that the dilaton and the axion as well as the two 2-form antisymmetric tensor fields, those are, the NS-NS 2-form and the R-R 2-form, are doublets of the SL(2,R) Mobius group whereas the graviton and the 4-form gauge field are singlets in the Einstein metric. Thus, if we wish to show that they transform covariantly under the SL(2,R) transformation these local fields must be treated as not constants but fields. In this context, notice that the vanishing or constant dilaton and axion imply the vanishing 3-form field strengths, so in order to understand the transformation rules under the SL(2,R) we are led to consider the non-constant dilaton and axion. It was conjectured that type IIB theory in ten dimensions is endowed with SL(2,Z) symmetry. The discrete subgroup of the SL(2,R) group survives as an exact symmetry of the quantum theory and has been referred to as S-duality in the literature in analogy with the corresponding symmetry in heterotic string theory. There is mounting evidence for this symmetry and it has played a very important role in providing deeper insight into the nonperturbative attributes of type IIB theory.


Type IIB Supergravity

The bosonic field content of type IIB supergravity consists of the metric, two scalars, two 2-form potentials and a chiral 4-form potential with a self-dual 5-form field strength making up a total of 128 bosonic degrees of freedom. The fermionic field content consists of two Majorana–Weyl dilatini as well as two Majorana–Weyl gravitini comprising a total of 128 fermionic degrees of freedom. These fields are organized into one 10-dimensional N = 2 supergravity multiplet. The local supersymmetry algebra for this theory has been constructed and shown to only close on-shell.

The action of type IIB supergravity in the string frame is a sum of three terms


 where


Modifed field strengths are used with


The starting point is the bosonic part of the Type IIB lagrangian density in 10D, which again involves the NS-NS fields and the Ramond-Ramond gauge potentials. The string-frame lagrangian for these fields is


To identify the on-shell action eliminate the Ricci scalar using the trace of the Einstein equations. Used in the action this yields


The on-shell action is


It is well-known that the covariant equations of motion for type IIB supergravity can not be derived from any action because of the presence of a self-dual five-form. However, after eliminating some unphysical fields, one arrives at equations of motion which are not manifestly covariant but admit a Lagrangian description. The formal covariance of the Lagrangian can then be provided by introducing auxiliary non-propagating fields. It is not possible to write a covariant action whose minimization gives the equations of motion 10-dimensional type IIB supergravity. The covariant action for type IIB supergravity can be written in the form


Decomposing  this action up to the second order and omitting full-derivative terms, one obtains the quadratic action


The covariance of the action has to be taken with a grain of salt since one cannot impose any covariant gauge conditions on the auxiliary fields. Nevertheless, the very existence of the action allows one to study in detail the properties of supergravity. The existence of a covariant action for type IIB supergravity has special interest due to the discovery of the duality between type IIB superstring theory and the four-dimensional super Yang-Mills model.

Now we proceed with the gravitino field. The action for the gravitino field leading to the covariant equations of motion has the form


Taking into account that the gravitino field is left-handed


we rewrite the previous action as follows


The type IIB effective action at second order in derivatives may be written in non-linearly realised form with respect to the SL(2,Z) symmetry of the D = 10 type IIB theory. After expanding out the Cartan forms in the type IIB effective action at second order in derivatives is


Instead, we will use an action for the type IIB supergravity theory in ten dimensions that gives the correct equations of motion after imposing the self-duality condition as an additional constraint on these equations. This action, in string frame, takes the form


The type IIB low-energy effective action, in string frame, at second order in derivatives is


The five-form field strength self duality condition that must be imposed on the equations of motion that result from varying the type IIB action. Although not manifest in this formulation, type IIB supergravity possesses an SL(2,R) symmetry that is broken to an SL(2,Z) subgroup for the full type IIB string theory. Following the evidence, these theories have a huge group of global discrete symmetries. A particularly interesting subgroup is the SL(2,Z) S-duality of type IIB superstring theory which exchanges an infinite family of solitons and bound states. It was already known that the IIB supergravity, which is the low energy effective theory of the type IIB superstring theory, possesses a discrete global symmetry, the SL(2,R) symmetry, but this symmetry was regarded as an artifact of the low energy approximation to underlying renormalizable theory and not taken seriously in those days. But nowadays the situation has radically changed since the discovery of the still rather mysterious more fundamental theory where SL(2,Z) subgroup of SL(2,R) is expected to be an exact symmetry.


Dimensional Reduction of the Effective Action

We shall also need to consider the low-energy limit of the type IIB superstring for our discussion duality. The zero-slope limit of the type IIB superstring is given by N = 2, D = 10 chiral supergravity. This theory contains a metric, a complex antisymmetric tensor, a complex scalar and a four-index antisymmetric tensor gauge field. The compactifications of type IIA and type IIB theories as we go from ten to nine dimensions have been studied by Bergshoeff, Hull and Ortin and they have explored implications of various dualities for this compactification. More recently, Andrianopoli and collaborators have studied compactification of type II theories and M-theory in various dimensions. It is well known that type IIA and type IIB theories are related by T-duality below ten dimensions. In lower dimensions the S-duality combines with the T-duality leading to U-duality. Therefore, it is of interest to obtain type IIB effective action, through dimensional reduction, in lower dimensional spacetime and explore the implications of SL(2,R) duality transformations. Let us consider the ten dimensional action for the type IIB theory



In order to express the action in a manifestly SL(2,R) invariant form, recall that the axion and the dilaton parametrize the coset. We over to the Einstein frame through the conformal transformation and the previous action takes the form


The action is invariant under following transformations



The Einstein equation can be derived by varying the action with respect to the metric and the equation of motion associated with the antisymmetric tensor fields can be obtained in a straight forward manner.

The desired equation of motion, derived from the above action, is


Note that this is a matrix equation of motion and we have suppressed the indices for notational conveniences. It is worthwhile, at this stage to point out some similarities with the the global O(d,d) symmetry that arises when one considers toroidal compactifications to lower spacetime dimension.

We consider a string effective action in D spacetime dimensions with massless fields such as graviton, antisymmetric tensor, dilaton, and Abelian gauge fields. If we compactify coordinates on a d = D − 4 dimensional torus and assume that the backgrounds are independent of these d compact coordinates, the resulting four dimensional reduced effective action takes the following form


It is more convenient for the implementation of S-duality transformation to rescale the metric to Einstein metric, and introduce the axion. Then previous action can be expressed as


where

The equations of motion derived from the action are





   
and the Bianchi identity is

  
The S-duality transformations correspond to


where the metric and moduli remain invariant.

In summarizing, we have explored the consequences of S-duality transformations on the equations of motion with nonzero cosmological constant. First, we studied a four dimensional action in a general framework. The reduced action could have been obtained from toroidal compactification of a heterotic string effective action in higher dimensions. In this context, let us briefly discuss the presence of higher order terms and the consequences of the S-duality transformations in the equations of motion. We write down the next higher order term to the low energy string effective action as


We have checked that under the S-duality transformation with the additional term also breaks S-duality invariance. The graviton equation along with the higher order correction term as mentioned above is also not invariant under the S-duality. Thus it can be argued that the presence of the higher order terms do not restore the S-duality invariance in the equations of motion. Notice that when we dimensionally reduce the terms involving quadratic in curvature, there will be additional terms in involving moduli and gauge fields arising from dimensional reduction. We have seen that the contribution of previous action to equations of motion already breaks the S-duality. Therefore, even if we explicitly take into account the contribution coming from moduli and extra gauge fields in the corresponding equations of motion, the S-duality invariance will not be restored. 


Higher Dimensional Effective Action


The purpose of this investigation is to study toroidal compactification of the type IIB theory and implications of SL(2,R) symmetry for the reduced action. It has been shown recently that the toroidally compactified type IIB string effective action possesses an SL(2,R) invariance as a consequence of the corresponding symmetry in ten dimensions when the self-dual five-form field strength is set to zero. The compactified theory on a d-dimensional torus respects the symmetry when we specify the transformation properties of the resulting scalar and vector fields.
It is well-known that the equations of motion of type IIB supergravity theory can not be obtained from a covariant action because of the presence of a four-form gauge field with the self-dual field strength in the spectrum. This gauge field couples to a self-dual three-brane which can give rise to string solution.

The type IIB equations of motion can be derived from the following covariant action


The metric, the dilaton and the antisymmetric tensor represent the massless modes in the NS-NS sector of type IIB theory. Also the scalar and the antisymmetric tensor represent the massless modes in the R-R sector. The reduced action takes the form


The reduced action have an SL(2,R) invariance which can be better understood by rewriting the action in the Einstein frame. The metric in the Einstein frame is related with the string metric as given in the second section. The action in the Einstein frame takes the following form


If we define the following SL(2,R) matrix then the previous action can be expressed in the manifestly SL(2,R) invariant form as


The action is invariant under the following global SL(2,R) transformation


Finally, the tensor field strength, defined above, can be shown to be gauge invariant by defining appropriate gauge transformations


The D-dimensional effective action takes the following form


Recalling our convention, the action for a p-forms is reduced according to


With our simplifications, toroidal compactification of a supergravity theory from D to d dimensions, containing the universal NSNS sector and a p-form, leads to the d-dimensional Poincaré invariant action


In compactifications of field theories from D to d dimensions, we require to obtain a background with a maximally symmetric d-dimensional space-time, but without any assumption on the geometry of the internal space, as long as it is compact. This allows to change the background values of the internal components of gauge invariant fields, without affecting the space-time symmetry in d dimensions. It is evident from the D-dimensional action that dilaton and axion interact with antisymmetric tensor fields, gauge fields and the scalars due to the presence of matrix in various terms and these interaction terms respect the SL(2,R) symmetry. It is important know what type of dilatonic potential is admissible in the above action which respects the S-duality symmetry. We reach a surprizing conclusion that the presence of interaction terms of the form only adds constant term which amounts to adding cosmological constant term to the reduced action. Note that the Einstein metric is SL(2,R) invariant and one can add terms involving higher powers of curvature (higher derivatives of metric) to the action and maintain the symmetry. However, we are considering the case when the gravitational part of the action has the Einstein-Hilbert term only.


The reduction to IIB is achieved when the generalised metric is taken to be the fundamental object rather than the supergravity fields themselves. These only arise upon choosing a specific parameterisation. If one had viewed the supergravity fields as fundamental, one could not have obtained a reduction to IIB. This approach allows both type II theories to appear within the same duality manifest theory. Unlike its type IIA counterpart, the type IIB supergravity can not be obtained by dimensional reduction of 11D supergravity on a circle, namely, from the low energy limit of M-Theory. Nonetheless, a strong-coupling completion of certain type IIB supergravity theories in ten dimensions is known. It is referred to as F-Theory, is formulated in twelve dimensions and makes extensive use of the nonperturbative SL(2,Z) self-duality of type IIB superstring theory. F-theory provides a realisation of IIB as a reduction from a higher-dimensional theory. The extra dimensions geometrise the S-duality of IIB supergravity so that one has a twelve-dimensional theory. There were hints that this geometrisation could be extended to the U-dualities of type IIB. F-theory is expected to give a systematic description of the IIB superstring with non-trivial dilaton and axion background to which the complex structure of a two-dimensional torus would correspond. To explain the origin of the SL(2,Z) duality of the type IIB theory has been a main motivation of F theory. In this respect it may be interesting to examine whether the theory of SL(2,Z)-covariant super D3-brane may have a 12 dimensional interpretation. Finally, a study of general dilaton and axion may shed light on F-theory, a conjectured 12-dimensional quantum field theory underlying a type IIB superstring. F-theory is expected to give a systematic description of the IIB superstring with non-trivial dilaton and axion background to which the complex structure of a two-dimensional torus would correspond. The IIB case seems to have a much richer spectrum of solutions than the IIA case. Although these new solutions are also incomplete in the sense that the sources are smeared, they constitute an important step since they change the existing paradigm that tree-level scale separation is only possible in massive IIA. Besides providing more examples of tree-level scale separation, the examples in IIB could be relevant for improving our understanding of the subtleties in such backgrounds. The IIB supergravity theory is not known to have massive deformations. One of the reasons for this is that there is no candidate vector field like in the IIA case. This type II T –duality maps the symmetries of each individual ten-dimensional type II theory into the other. This is specially useful when one symmetry is manifest in one theory but not in the other. This is the case of SL(2,R), which is manifest in the type IIB theory but it is not manifest by any means in the type IIA theory. The type IIB supergravity in ten dimensions has an explicit SL(2,R) symmetry of the equations of motion which is broken to SL(2,Z) by quantum corrections. This is the conjectured SL(2,Z) S–duality discrete gauge symmetry of the type IIB string, while SL(2,R), which we shall also refer to as an S–duality, is a solution-generating symmetry, transforming any given solution into a new one. The level of low energy effective action that this SL(2,R) invariance of the type IIB theory survives the toroidal compactification. In fact, this is not surprising since a symmetry in a higher dimensional theory should become a part of the bigger symmetry in the lower dimensional theory, although in this case, it requires quite non-trivial calculation to prove the invariance. Hence it is enough for our purposes to calculate the coefficient in type IIB string theory. The reason we want to do the calculation in the type IIB theory is because we want to impose the constraints implied by S–duality which allow us to obtain explicit expressions for these amplitudes at high genera. The main output obtained by imposing the constraints of supersymmetry and S–duality for a certain class of interactions in the type IIB effective action is that the moduli dependent coefficients of these interactions satisfy first order differential equations on moduli space. This holds to all orders in the expansion. We shall simply write very schematically the structure of these equations which is good enough for our purposes. Based on the constraints of supersymmetry and S–duality of the type IIB theory, we are able to find at least a part of the coefficients of certain higher genus amplitudes which yield the transcendental nature of the term in the M theory effective action. Our work emphasizes the important role supersymmetry and U–dualities play in constraining the effective action in general. Learning about the symmetries of the ten-dimensional theory they descend from is then essential for a proper understanding of the lower dimensional theories. As we have mentioned, there are more string-like solutions not only with electric charge but also with magnetic charge in type II theories in lower dimensions which should form multiplets of bigger symmetry group, the U-duality group. Apart from the string-like solutions, there are also other p-brane solutions in these theories which deserve a systematic study to properly identify the complete U-duality group. This will provide strong evidence for the conjecture of the U-duality symmetries in those theories.


Type IIA Supergravity

Type IIA supergravity is a ten-dimensional theory which can be obtained either by taking a certain limit in type IIA string theory, or by doing a dimensional reduction of eleven-dimensional supergravity, which is the supergravity theory with the highest possible dimensionality. The massless modes of a superstring can be described by an effective action which is the corresponding supergravity theory. Having mentioned that the type IIA supergravity action is obtained by a simple dimensional reduction from the eleven-dimensional theory would seem to indicate that this form of the theory is unique. Based on this conjecture, the 10D type IIA theory and all of its constituents should have their 11-dimensional origins. We would like to describe the interactions of the massless modes, which is constrained by supersymmetry to be described by the type IIA supergravity theory in ten dimensions. Type IIA supergravity is a ten-dimensional, non-chiral supergravity theory. A supergravity theory is a supersymmetric theory that includes gravity, the ten-dimensional metric is a bosonic field that enters the action. The fact that N = 2 means that the supersymmetry transformations of the fields are generated by two independent parameters. In ten dimensions, this means that the theory has 32 conserved supercharges. IIA supergravity is non-chiral, which means that the supersymmetry parameters have opposite chiralities. In components, type IIA supergravity describe the dynamics of the gravity supermultiplet. To make the local supersymmetry of this component formalism manifest, one proceeds as in global supersymmetry by introducing the notion of superspace and superfields. The massless bosonic field contents of type II can be divided in two sectors from its very first construction: the Neveu-Schwarz-Neveu-Schwarz sector (NSNS) and the Ramond-Ramond sector (RR). A well studied and unique example of a massive theory of gravity is the massive type IIA supergravity in ten dimensions constructed by Romans. Amongst massive theories, massive type IIA supergravities can be easily characterised solely by there field content in which the NSNS 2-rank tensor field is massive. Massive theories are continuous deformations of the regular ones in which the gauge transformations and supersymmetries get extra dependence via a mass parameter. Consequently, the equations of motion get extra terms linear and quadratic in this parameter. 



Type IIA Supergravity

The type IIA supergravity in ten dimensions describes the low energy limit of type IIA superstrings. This theory is non-chiral and therefore it has no anomalies. We start by reviewing bosonic part of the standard IIA supergravity action. The 10D NSNS fields are the dilaton, 2-form potential and string frame metric. The 10D RR fieldstrenghts are the 4-form, 2-form and 0-form. The action is 




The next step is the part of the 10D IIA supergravity action quadratic in fermions. We work in the string frame.


where the covariant derivatives act on the Majorana dilatino and gravitino are



The story for the 10D Type IIA supergravity action is similar. In the string frame this action is the sum of the Neveu-Schwarz, Ramond-Ramond and Chern-Simons sectors


where


The Einstein-frame action becomes


The action can be written as a total derivative using the form-field equations of motion



 

Massive IIA Supergravity

This section contains a review of Romans massive supergravity. Our starting point is the supersymmetric bosonic action of massive type IIA supergravity. In the language of differential forms, it is given by



For the form fields and dilaton, together with the Einstein equation


It is useful also to present the expressions for the ten-dimensional Hodge duals of the form fields. We find that they are given by


The action for massive type IIA supergravity in the Einstein frame reads


This action is a generalisation of the type IIA supergravity that is obtained from the low energy limit of type IIA string theory, although some care must be taken when taking the massless limit.

The terms in the ten-dimensional action which will contribute to the gravitino masses are



The equations of motion that follow from Lagrangian are


The gravitino and dilatino supersymmetry variations read


and


where the supercovariant derivative is given by

 

Duality–symmetric Type IIA D=10 Supergravity

We present different but classically equivalent forms of the action, give the analysis of symmetry and dynamical properties of the model, and establish the connection with the standard formulation of type IIA supergravity. We will focus on the subsector of ten–dimensional type IIA supergravity which does not involve the quartic fermion terms.

By use of the standard dimensional reduction procedure we get the following conventional part of the type IIA supergravity action



The complete action is


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The reduction of this part of the action results in



To this end, as in the case of duality–symmetric D = 11 supergravity, it is convenient to rewrite the action as follows



with



The variation of this Lagrangian is



The dual field strengths are incorporated into the action



This action is the complete duality–symmetric action for type IIA supergravity up to the four–fermion terms and has the characteristic structure of duality–symmetric supergravities. To extend the action to the Romans’s massive supergravity let us continue with its bosonic sector in the form



The complete massive type IIA supergravity Lagrangian has the following form


This action is invariant under modified gauge transformations and local supersymmetry transformations


The duality-symmetric action for the massive type IIA supergravity has the following form
  

One can, modulo a total derivative, rewrite the Chern–Simons term such that
 
                                   

After that we arrive at the following action for N = 1, D = 10 supergravity


To summarize, we have constructed the duality–symmetric version of type IIA D = 10 supergravity which in its final form contains in addition to the standard type IIA supergravity bosonic fields also their duals. The coupling of this duality–symmetric type IIA supergravity to the Dp–branes and to the NS5–brane can be carried out in a conventional way.


We discussed earlier the massless contents of Type II supergravity theories. They naturally include graviton and at low energies they give supergravities as effective theories. In string theory, supergravities have their role as effective theories for describing the massless sector of the field theory limit to lowest order. As effective theories, the supergravity actions are expected to receive higher order derivative corrections. In the M-theory context in particular, there is very active research aimed at finding the correct modification of supergravity. The associated actions of type IIA strings are obtained by using the metrics and other background fields of the type IIA supergravities. The resulting actions agree with those of type IIA strings obtained in the study of the supergravities. Supersymmetry ensures that this theory is unique. Furthermore the IIA ten-dimensional supergravity has to be the dimensional reduction of the 11D higher-dimensional theory, since the two theories have the same supersymmetry algebras. The superfields which describe IIA D = 10 supergravity are subject to the constraints which are obtained from the D = 11 supergravity constraints using the ansatz and solving for Bianchi identities. One approach to deriving the exact supergravity solutions would be to work in the context of D = 11 supergravity. Since type IIA supergravity is related to eleven-dimensional supergravity by dimensional reduction, any exact solution of type IIA supergravity is related to a solution of D = 11 supergravity with translational invariance along one of the spatial directions. An interesting problem for future study is to construct the Lagrangian description of the consistent coupling of a type IIA supergravity action to an NS5-brane source. The latter requires the construction of a duality-symmetric version of type IIA supergravity by the dimensional reduction of the duality-symmetric D = 11 supergravity. The truncation of such a IIA supergravity action shall produce the duality-symmetric version of the N = 1, D = 10 supergravity, which should naturally couple to a heterotic fivebrane. Note that recent investigations of interacting brane actions may provide one with a possibility of making this coupling supersymmetric. Historically, eleven-dimensional supergravity theory is interesting because eleven is the highest dimension and supersymmetry invariance is possible. But one should keep in mind that, just as type IIA supergravity should only be seen as an effective theory at low energy but not a complete theory, the eleven-dimensional supergravity can only at best be a low-energy description of a consistent theory. It would be interesting to find other solutions of type IIA supergravity and to study their possible 11-dimensional origin. There are many potentially fruitful directions for future research.