Invertible disformal transformations with higher derivatives
Abstract
We consider a higher-derivative generalization of disformal transformations in -dimensional spacetime and clarify the conditions under which they form a group with respect to the matrix product and the functional composition. These conditions allow us to systematically construct the inverse transformation in a fully covariant manner. Applying the invertible generalized disformal transformation to known ghost-free scalar-tensor theories, we obtain a novel class of ghost-free scalar-tensor theories, whose action contains the third- or higher-order derivatives of the scalar field as well as nontrivial higher-order derivative couplings to the curvature tensor.
I Introduction
Scalar-tensor theories have been studied extensively as a model of inflation/dark energy, and there has been a growing interest in incorporating higher-derivative interactions of the scalar field into the action without introducing Ostrogradsky ghost Woodard (2015); Motohashi and Suyama (2020). It was shown that the ghost can be eliminated if the higher-derivative terms are degenerate Motohashi and Suyama (2015); Langlois and Noui (2016); Motohashi et al. (2016); Klein and Roest (2016); Motohashi et al. (2018a, b). With the knowledge of the degeneracy conditions, one can systematically construct ghost-free scalar-tensor theories, which are known as degenerate higher-order scalar-tensor (DHOST) theories Langlois and Noui (2016); Crisostomi et al. (2016); Ben Achour et al. (2016); Takahashi and Kobayashi (2017); Langlois et al. (2019).*1*1*1Relaxing the degeneracy conditions so that the higher-derivative terms are degenerate only in the unitary gauge, we obtain a broader class of scalar-tensor theories Gao (2014); De Felice et al. (2018); Gao and Yao (2019); Motohashi and Hu (2020); De Felice et al. (2021). In that case, there is an apparent extra DOF in a generic gauge, but it satisfies an elliptic differential equation and hence is an instantaneous (or “shadowy”) mode De Felice et al. (2018, 2021). The DHOST theory includes the Horndeski Horndeski (1974); Deffayet et al. (2011); Kobayashi et al. (2011) and the Gleyzes-Langlois-Piazza-Vernizzi theories Gleyzes et al. (2015) as special cases, and hence form a general class of healthy scalar-tensor theories (see Langlois (2019); Kobayashi (2019) for reviews).
To pursue more general frameworks of scalar-tensor theories, a redefinition of the metric or an invertible transformation has been playing an important role. This is because, in general, an invertible transformation maps a ghost-free theory to another ghost-free theory as it does not change the number of dynamical degrees of freedom (DOFs) Domènech et al. (2015); Takahashi et al. (2017). Let us consider a transformation between and . For a given action of scalar-tensor theories , we substitute the transformation law to obtain a new action . Hence, and are respectively referred to as the original- and new-frame metrics. So long as the transformation is invertible, the two actions are mathematically equivalent up to the redefinition of variables and boundary terms. However, when matter fields are taken into account, one has to define the metric to which the matter fields are minimally coupled. As an aside, even if the gravity sector is degenerate, introducing a matter sector could revive the Ostrogradsky ghost, and hence one needs a careful analysis Deffayet and Garcia-Saenz (2020). Therefore, the resultant action can be regarded as a new theory, rather than a mere redefinition of the original action .
A well-established example of such metric transformations is the disformal transformation Bekenstein (1993); Bruneton and Esposito-Farèse (2007); Bettoni and Liberati (2013), which is of the form,
(1) |
where Greek indices represent spacetime indices and denotes the covariant derivative with respect to the metric , with the scalar field unchanged. Note that in the present paper, for simplicity, a “disformal transformation” denotes a transformation of the form (1) with and in general (and also its generalization discussed below), which also contains the purely conformal transformation with as a special case. As we shall see in detail in §II.1, the transformation (1) is invertible (i.e., the new-frame metric can be uniquely expressed in terms of and without referring to any particular configuration) if and only if , where (). Interestingly, it was shown in Zumalacárregui and García-Bellido (2014) that the disformal transformation (1) in general maps the Horndeski class to its exterior, which is now known as the quadratic/cubic DHOST class Langlois and Noui (2016); Crisostomi et al. (2016); Ben Achour et al. (2016).*2*2*2However, in two spacetime dimensions, the Horndeski class is closed under the disformal transformation of the form (1) Takahashi and Kobayashi (2019). Also, the quadratic/cubic DHOST class itself is closed under the disformal transformation Ben Achour et al. (2016). Applications of the disformal transformation have been extensively explored in various contexts; inflation Kaloper (2004); van de Bruck et al. (2016, 2017); Karwan and Channuie (2017); Bordin et al. (2017); Sato and Maeda (2018); Qiu et al. (2020); Gialamas et al. (2020, 2021), cosmic microwave background van de Bruck et al. (2013); Brax et al. (2013); Burrage et al. (2016), dark matter and dark energy Zumalacárregui et al. (2010); Koivisto et al. (2012); Neveu et al. (2014); Sakstein (2015); van de Bruck and Morrice (2015); Hagala et al. (2016); Brax et al. (2015); Emond and Saffin (2016); Karwan and Sapa (2017); Sapa et al. (2018); Llinares et al. (2020); Teixeira et al. (2020); Trojanowski et al. (2020); Dusoye et al. (2021); Brax et al. (2021a); Gómez et al. (2021), cosmological perturbations Minamitsuji (2014); Tsujikawa (2015a); Motohashi and White (2016); Tsujikawa (2015b); Fujita et al. (2016); Chiba et al. (2020); Alinea and Kubota (2021); Minamitsuji (2021a), solar system tests and screening mechanisms Brax and Burrage (2014); Sakstein (2014, 2015); Ip et al. (2015); Brax and Davis (2018); Davis and Melville (2020); Brax et al. (2021b), relativistic stars Minamitsuji and Silva (2016); Brax et al. (2019); Silva and Minamitsuji (2019); Ramazanoğlu and Ünlütürk (2019); Minamitsuji (2021b); Ikeda et al. (2021), and black holes Koivisto and Nyrhinen (2017); Takahashi et al. (2019); Ben Achour et al. (2020a); Anson et al. (2021); Ben Achour et al. (2020b); Long et al. (2020); Minamitsuji (2020); Chen et al. (2021); Erices et al. (2021); Takahashi and Motohashi (2021); Ben Achour et al. (2021); Faraoni and Leblanc (2021); Zhou et al. (2021); Chatzifotis et al. (2021); Bakopoulos et al. (2021).
A natural question is whether there exists a more general class of invertible transformations, which would bring us new fruitful insights on scalar-tensor theories. The transformation (1) is the most general up to the first derivative of the scalar field. Recently, a higher-derivative generalization of the disformal transformation was studied in the context of cosmological perturbations Alinea and Kubota (2021); Minamitsuji (2021a). However, the invertibility of such generalized disformal transformations remains unclear. The aim of the present paper is to address this issue. The authors of Alinea and Kubota (2021) studied the generalized disformal transformation in the context of inflationary cosmology and showed that the transformation can be regarded as invertible if higher-derivative terms are suppressed by the slow-roll parameter and can be neglected. On the other hand, the authors of Babichev et al. (2019, 2021) studied a general derivative-dependent field transformation by applying the method of characteristics, and formulated a set of necessary and sufficient conditions for the local invertibility as the degeneracy condition to remove additional DOFs after the transformation. In particular, they applied the criteria to a disformal transformation of the form
(2) |
on a homogeneous and isotropic cosmological background and showed that the transformation is noninvertible unless , for which the transformation (2) reduces to (1). The point is that, in order to prove the noninvertibility of a transformation, it is sufficient to show it on a particular background. In contrast, the invertibility of a transformation on a particular background does not guarantee the invertibility on generic backgrounds. In principle, the invertibility conditions obtained in Babichev et al. (2019, 2021) would apply to the construction of invertible generalized disformal transformations without referring to a particular background. Nevertheless, in practice, the application would not be so straightforward, and so far there is no known explicit example of invertible disformal transformations with higher-order field derivatives.
In the present paper, we will construct a general class of invertible disformal transformations with higher-order field derivatives in -dimensional spacetime. We first clarify that the invertibility of the conventional disformal transformation (1) originates from its closedness under the matrix product and the functional composition. We then consider a higher-derivative generalization of the disformal transformation with these properties and construct the inverse transformation in a fully covariant manner. We also clarify how known DHOST theories are transformed under the generalized disformal transformations. As a result, we obtain a novel class of healthy degenerate theories, which possesses at most three propagating DOFs. Interestingly, the resultant action contains the third- or higher-order derivatives of the scalar field as well as a novel type of higher-order derivative couplings to the curvature tensor.
The rest of this paper is organized as follows. In §II, we discuss under which conditions the generalized disformal transformations can be invertible and explicitly construct the inverse transformation. Our construction also applies to the vector disformal transformation Kimura et al. (2017), which we shall discuss in the Appendix. In §III, we provide several specific examples of invertible disformal transformations with the second or third derivatives of the scalar field. Then, in §IV, we study the generalized disformal transformation of known DHOST theories. Finally, we draw our conclusions in §V.
II Invertibility of disformal transformations
II.1 Transformations up to the first derivative
We first review the case of the conventional disformal transformation that contains up to the first derivative of the scalar field to clarify the reason why it is possible to construct the inverse transformation in this case. Let us consider a class of metric transformations of the form (1), which we recapitulate here for convenience:
(3) |
where we have introduced and then . Note that the following results hold in general -dimensional spacetime.
A remarkable feature of this class of transformations is that it is equipped with two binary operations and hence forms a group under each of the two operations. One of the two operations is the matrix product of two disformal metrics, while the other is the functional composition of two sequential disformal transformations. In what follows, we demonstrate that the class of conventional disformal transformations is indeed closed under the two operations mentioned above.
-
[A]
Closedness under the matrix product. We consider two independent transformations of the form (3),
(4) By contracting and with the unbarred metric, one can construct another disformal metric, which we call the matrix product of two disformal metrics. Written explicitly, the matrix product is computed as
(5) which is again of the form (3).
This property allows us to construct the inverse metric for as the inverse element in the group under the matrix product. Indeed, by choosing
(6) |
we can make , which means that the inverse metric is given by
(7) |
Here, we have assumed and .
-
[B]
Closedness under the functional composition. We consider two sequential transformations of the form (3),
(8) Here, denotes the kinetic term of the scalar field contracted by , which is computed by use of (7) as
(9) Then, the composition of the two transformations is given by
(10) which is again of the form (3).
The inverse for the map is nothing but the inverse element of in the group under the functional composition and hence is given by requiring , i.e.,
(11) |
where in the right-hand sides is regarded as a function of by use of (9). Note that we need
(12) |
to locally express in terms of . Hence, the explicit form of the inverse transformation is given by
(13) |
and a set of necessary and sufficient conditions for the disformal transformation (3) to be invertible is summarized as
(14) |
Although not directly related to the invertibility of the transformation, and are necessary to preserve the metric signature Bruneton and Esposito-Farèse (2007).
The above analysis demonstrates that the two properties [A] and [B] play an essential role in the systematic construction of the inverse metric and the inverse transformation. Note that for the existence of the inverse transformation, the existence of the inverse metric is necessary. As we saw above, when computing the functional composition of the two disformal transformations in (8), one needs to express in terms of the unbarred quantities, in which the inverse metric shows up. In the next subsection, we study a generalized disformal transformation with higher derivatives satisfying the above two properties and explicitly construct its inverse transformation.
II.2 Transformations with higher derivatives
Having clarified the reason why the conventional disformal transformation (3) is invertible, we now consider transformations with higher derivatives. The main difficulty here is that the higher covariant derivatives depend on the Christoffel symbol, i.e., the derivative of the metric. This generically spoils the property [B] since a functional composition of two transformations generically yields unwanted extra terms with higher derivatives that are not contained in the original transformation law. In order to make a transformation invertible, one has to tune it so that such extra terms do not show up. As a general example of transformations for which this tuning is possible, let us consider a metric transformation in -dimensional spacetime defined by
(15) |
Here, with and . Also, ’s () are functions of , where and are defined as follows:
(16) |
Note that the conventional disformal transformation (3) is included as a special case with , , and . In what follows, we explicitly construct the inverse transformation for (15) with a particular focus on the properties [A] and [B].
We first examine the property [A], i.e., the closedness under the matrix product. To this end, we consider two independent transformations of the form (15),
(17) |
The matrix product of and is calculated as follows:
(18) |
which is again of the form (15), and hence the property [A] is satisfied.*3*3*3Precisely speaking, the right-hand side of (18) is not of the form (15) as it is not symmetric in and in general. Therefore, for the closedness under the matrix product, the underlying set of transformations should be enlarged to include such asymmetric terms. Nevertheless, as mentioned in the main text, the inverse element of (15) can be found in the symmetric subset. This is reminiscent of the fact that a product of two symmetric matrices is not necessarily symmetric, while the inverse of a symmetric matrix is symmetric. The inverse matrix for is obtained by putting in (18). While this requirement apparently yields five equations for four unknown functions , only four of them are independent, and hence the system is not overdetermined. Thus, the coefficient functions in are fixed as
(19) |
Here, we assumed and defined the following quantity:
(20) |
which was also assumed to be nonvanishing. As a result, the inverse metric is given by
(21) |
Next, let us study under which conditions the transformation (15) can satisfy the property [B], i.e., the closedness under the functional composition. We consider sequential transformations with
(22) |
with ’s () being functions of . In the case of the first-order disformal transformations studied in §II.1, the invertibility is guaranteed if can be locally expressed in terms of . In the present case with higher derivatives, we have
(23) |
which is a function of in general. Let us consider to express as a functional of and . If depends on or in a nontrivial manner, then the derivatives of in yield derivatives of or , which do not appear in the transformation law (15). On the other hand, so long as has no dependence on either or , then the composition of the two transformations is again of the form (15), meaning that the property [B] is satisfied. Therefore, we require
(24) |
where and , so that . We also assume so that we can solve the relation for to have . Then, we have with , and hence
(25) |
Here, we require that these two equations can be solved for and to obtain and , which is guaranteed if the Jacobian determinant is nonvanishing.
We are now ready to write down the expression for the inverse transformation for . With the requirement , we can express in terms of the unbarred quantities as
(26) |
where the functions of in the right-hand side are regarded as functions of by (23) and (25). The inverse transformation can be obtained by putting , which fixes the coefficient functions in as
(27) |
Thus, we have obtained the inverse transformation in the following form:
(28) |
where the functions of in the right-hand side can be translated back into functions of by use of (23) and (25).*4*4*4The above analysis shows that the transformation defined by (28) is the left inverse of the transformation defined by (15), i.e., . Since the left inverse of a group element is also its right inverse, it follows that .
To summarize, we have obtained a set of sufficient conditions for the generalized disformal transformation (15) to be invertible. The conditions are summarized as
(29) |
This set of conditions can be used not only as a simple criterion for the invertibility of a given transformation of the form (15) but also as a useful tool to construct invertible generalized disformal transformations as we shall see below. In order for the condition and to be satisfied, let us take as an input, with being an arbitrary function of such that . Then, by use of (23), e.g., the function is written in terms of , , , and as
(30) |
Therefore, we obtain invertible transformations by choosing the functions , , , and so that they satisfy the remaining conditions in (29), i.e., , , and . In particular, for the above , the condition yields
(31) |
We shall use this strategy to construct a nontrivial example of invertible transformations of the form (15) in §III.1.
A caveat here is that the transformation law could be ill defined for some particular configuration of . Nevertheless, it is still possible to perform the invertible disformal transformation on some seed action of scalar-tensor theories to generate a new action . For instance, provided that , , and are regular functions, the denominator of (30) vanishes for configurations with , which happens when . This means that, even if the new action admits a solution with , one cannot map the solution via the disformal transformation to generate a solution in the original frame. On the other hand, so long as we consider configurations for which the transformation law is well defined, there is one-to-one correspondence between the configuration space in the new frame and the one in the original frame.
One may think that arbitrary tensors of the form (e.g., and ) and/or scalar quantities constructed from , , and (e.g., and ) can be included in the transformation law (15). For instance, one could consider transformations of the form (2), in which a term with is present. In this case, one can make use of the Cayley-Hamilton theorem, which allows us to write any with in terms of . Therefore, considering a transformation composed of , the property [A] may be satisfied, which allows us to systematically construct the inverse metric. However, as mentioned earlier, a composition of such transformations generates various terms with the third-order derivative of the scalar field as well as the second-order derivative of the metric through the Christoffel symbol [see (51) and (54)], which are not contained in the original transformation law. Hence, it is practically difficult to remove all such terms, implying that the property [B] cannot be satisfied in general. This explains why transformations of the form (2) are noninvertible, as shown in Babichev et al. (2021). The reason why we could obtain a concise invertibility condition for the transformation (15) is that there is only a single function that controls whether or not the class of transformations is closed under the functional composition. The point is that, so long as the conditions in (29) are satisfied, the Christoffel symbols are encapsulated in two sets of scalar quantities and , between which the invertibility is manifest.
As a final remark, the above discussion can be extended to more general transformations containing the third derivative of ,
(32) |
where , , and here
(33) |
Likewise, it is straightforward to include arbitrarily higher-order derivatives of in the transformation. Rather than presenting a general discussion, we shall provide an example of invertible disformal transformations with the third derivative of in §III.2.
III Examples
III.1 Example with the second derivative of the scalar field
As an example of invertible disformal transformations of the form (15), let us consider the case with , , and , i.e.,
(34) |
In this case, we have
(35) |
which we require to be a function only of . Assuming that with and , from (30) we have
(36) |
for which the transformation law of the metric is explicitly written as
(37) |
Then, the inverse metric is given by
(38) |
We also have
(39) |
which can be inverted as
(40) |
The inverse disformal transformation takes the form,
(41) |
where in the arguments of and is regarded as a function of by solving for . Note that, while the transformation (37) does not contain either or , in general these terms show up in the inverse transformation (41). If , such terms vanish in (41). The simplest case would be with being a nonvanishing constant, for which the disformal transformation (37) and its inverse (41) are explicitly written as
(42) |
III.2 Example with the third derivative of the scalar field
Let us now consider another example of invertible transformations of the following form:
(43) |
where is a nonvanishing constant and we have defined
(44) |
This transformation is of the form (32) and the third derivative of appears in . The inverse metric takes the form
(45) |
Then, the relevant scalar quantities transform as follows:
(46) |
Note that the property [B] is guaranteed by , which is a natural generalization of the condition in (29).*5*5*5It should also be noted that takes the form, and hence has a nontrivial dependence on and , but this does not spoil the invertibility as the transformation (43) is independent of . On the other hand, if the transformation law had a nontrivial dependence, then should satisfy . The relations in (46) can be solved for the unbarred quantities as
(47) |
Hence, the inverse transformation is obtained as follows:
(48) |
IV Generalized disformal transformation of scalar-tensor theories
As mentioned earlier, substituting the transformation law of a disformal transformation into some seed action of scalar-tensor theories , we obtain a new action as a functional of and . In this section, we use DHOST theories known so far as a seed and discuss what action is obtained as a result of the generalized disformal transformation.
The known classes of DHOST theories in four dimensions are described by the action of the following form Langlois and Noui (2016); Crisostomi et al. (2016); Ben Achour et al. (2016); Takahashi and Kobayashi (2017); Langlois et al. (2019):
(49) |
with and being respectively the Ricci scalar and the Einstein tensor in the original frame. Here, is a scalar quantity constructed from , , , and . We discuss how the action (49) is transformed under the generalized disformal transformation (15). Note that the first covariant derivative of the scalar field remains unchanged (namely, ) and that the transformation law for is given by (23). Hence, in what follows, we derive the transformation law for the other building blocks of the action (49), i.e., the square root of the metric determinant , the Ricci tensor , and the second covariant derivative of the scalar field .
By repeated use of the matrix determinant lemma, we obtain*6*6*6In -dimensional spacetime, we have .
(50) |
with defined in (20). Here, we have assumed and , which are necessary to preserve the metric signature. The change of the Christoffel symbol is a tensor, which is written as follows:
(51) |
In terms of this , the Ricci tensor in the original frame can be expressed as
(52) |
where . The Ricci scalar in the original frame can be written in the form,
(53) |
where the last term is the covariant divergence associated with . Also, the tensor shows up in the transformation law for the second derivative of as
(54) |
The above relations allow us to systematically compute the transformation of the action (49). Since contains the derivative of in which there are second derivatives of , the resultant action contains the third or higher derivatives of in general. It should be noted that so long as the transformation (15) is invertible, the number of DOFs does not change under the transformation Domènech et al. (2015); Takahashi et al. (2017). Hence, the generalized disformal transformation (15) can generate a new class of higher-derivative ghost-free theories, which itself is closed under the same class of transformations. Also, performing the generalized disformal transformation on the known minimally modified gravity theories Lin and Mukohyama (2017); Chagoya and Tasinato (2019); Aoki et al. (2018); Afshordi et al. (2007); Iyonaga et al. (2018, 2020); Gao and Yao (2020) (i.e., those without a propagating scalar DOF) yields a novel class of minimally modified gravity.
Given the above transformation rules for the building blocks, it is straightforward to write down the transformation of the action (49). Since the full expression is quite involved, here we demonstrate the transformation of the following subclass of the action:
(55) |
which reduces to the Einstein-Hilbert action with a canonical scalar field when and with being the reduced Planck mass. Note that, if has a nontrivial dependence on , this action itself does not yield a degenerate theory. When , one has to take into account quadratic terms of to render the theory degenerate. Applying the above transformation rules, we obtain
(56) |
with . In particular, for transformations of the form (37), we have
(57) |
with and
(58) |
Thus, as mentioned earlier, the resultant action contains the third derivative of . Moreover, there is a new type of higher-order derivative coupling to the curvature tensor of the form . Clearly, one would obtain even higher-order derivatives of and other new types of coupling such as or if one considers the more general transformation (32). Nevertheless, since it is generated from the ghost-free action via the invertible transformation, this higher-derivative action describes a healthy degenerate theory, i.e., there are at most three propagating DOFs without the Ostrogradsky ghosts.
V Conclusions
In the present paper, we studied a higher-derivative generalization of the disformal transformation, with a special focus on transformations of the form (15), which we recapitulate here:
(59) |
with ’s () being functions of , , , and . For this type of transformation, we derived the invertibility conditions (29) focusing on the group structure and explicitly constructed its inverse transformation (28). Our construction of the inverse transformation is based on the following two properties: [A] the closedness under the matrix product and [B] the closedness under the functional composition. With these two properties, the generalized disformal transformations form a group with respect to the matrix product and the functional composition, which allows us to systematically construct the inverse metric and the inverse transformation in a fully covariant manner. This strategy can be straightforwardly extended to even more general disformal transformations, e.g., of the form (32). Our results hold in general -dimensional spacetime. Moreover, it also applies to the vector disformal transformation Kimura et al. (2017) and the multidisformal transformation Watanabe et al. (2015); Firouzjahi et al. (2018), the former of which is discussed in the Appendix. We also investigated the generalized disformal transformation of known DHOST theories which contain up to the second derivative of the scalar field. As a consequence, we obtained a new class of ghost-free theories containing the third or higher derivatives of the scalar field as well as novel derivative couplings to the curvature tensor, e.g., .
There are several interesting directions for further studies. One of them is to study cosmology in the novel class of theories obtained via the generalized disformal transformation. In particular, it would be important to study which subclass accommodates models where the speed of gravitational waves coincides with that of light, in accordance with the almost simultaneous detection of the gravitational waves GW170817 and the -ray burst 170817A emitted from a binary neutron star merger Abbott et al. (2017a, b, c). Applied to the early universe, especially cosmological inflation, it would be important to clarify the frame invariance of cosmological perturbations by extending the analysis in Alinea and Kubota (2021); Minamitsuji (2021a). Investigating how the generalized disformal coupling affects the screening mechanism would also be intriguing. Another direction of interest is to see how the known solutions in scalar-tensor theories are transformed under (15), following the works Anson et al. (2021); Ben Achour et al. (2020b). Note that the new terms in the transformation law (15) depend on the derivative of the scalar kinetic term , meaning that they become trivial for solutions with being constant Babichev and Charmousis (2014); Kobayashi and Tanahashi (2014); Babichev and Esposito-Farèse (2017); Babichev et al. (2017, 2018); Ben Achour and Liu (2019); Motohashi and Minamitsuji (2019); Minamitsuji and Edholm (2019); Khoury et al. (2020); Babichev et al. (2017); Charmousis et al. (2019); Takahashi and Motohashi (2020), while there would be a nontrivial contribution for solutions with a nonconstant Babichev et al. (2017); Minamitsuji and Edholm (2020); Ben Achour et al. (2020a). We leave these issues for future work.
Acknowledgements.
K.T. was supported by JSPS (Japan Society for the Promotion of Science) KAKENHI Grant No. JP21J00695. H.M. was supported by JSPS KAKENHI Grant No. JP18K13565. M.M. was supported by the Portuguese national fund through the Fundação para a Ciência e a Tecnologia in the scope of the framework of the Decree-Law 57/2016 of August 29, changed by Law 57/2017 of July 19, and the Centro de Astrofísica e Gravitação through the Project No. UIDB/00099/2020. M.M. also would like to thank Yukawa Institute for Theoretical Physics for the hospitality under the Visitors Program of FY2021. *Appendix A Vector disformal transformations with derivatives
In the main text, we constructed an invertible disformal transformation with higher derivatives (15) as a generalization of the conventional disformal transformation (1) in the context of scalar-tensor theories. A similar transformation was also studied in the context of vector-tensor theories Kimura et al. (2017), which is explicitly written as
(60) |
with the vector field unchanged. Here, and are functions of . In this appendix, we construct invertible disformal transformations with the derivative of . Note that the following results reduce to those in §II under the replacement , while the dependence on without derivative is not reproduced. We shall adopt a notation similar to the one used in the main text to make the correspondence clear. Namely, in this appendix are the vector counterparts corresponding to the ones defined for the case of scalar field.
Let us consider a metric transformation in dimensions defined by
(61) |
where . Here, ’s () are functions of , in which and are defined as follows:
(62) |
It is straightforward to verify that the transformation (61) satisfies the property [A], i.e., the closedness under the matrix product. Therefore, one can systematically construct the inverse metric , and the result is given by
(63) |
with defined by
(64) |
Hence, we have
(65) |
which is a function of in general. As we did in §II, we require [i.e., ] so that the transformation satisfies the property [B], i.e., the closedness under the functional composition. We also assume so that we can solve the relation for to have . Then, we have
(66) |
Here, we require that these two equations can be solved for and to obtain and . The inverse transformation is written as
(67) |
where the functions of in the right-hand side can be translated into functions of by use of (65) and (66).
For vector-tensor theories, further generalization including the field strength tensor would also be possible. Note that vanishes in the scalar limit , and hence such an extension is peculiar to the vector disformal transformation. The disformal transformation with in four dimensions was first studied in Gümrükçüoğlu and Namba (2019), which has the form
(68) |
with and (). For instance, we have and . Interestingly, this was shown to be the most general metric transformation in four dimensions that consists of and its dual De Felice and Naruko (2020). Note that the transformation (68) does not contain the derivative of the metric, and hence the invertibility condition can be obtained by simply requiring that the Jacobian determinant is nonvanishing Gümrükçüoğlu and Namba (2019). It should be noted that the Cayley-Hamilton theorem yields
(69) |
in four dimensions, which allows us to express any with as a linear combination of and . Thanks to this relation, the transformation (68) can satisfy both the properties [A] and [B]. Likewise, it could in principle be possible to incorporate into the transformation law (61) to obtain a more nontrivial class of invertible vector disformal transformations. However, it should be noted that the matrix identity following from the Cayley-Hamilton theorem is dimension dependent, and hence a dimension-independent expression for the inverse transformation would no longer be available in this case.
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