Abstract:Recently the calculation of holographic free energy for mass-deformed ABJM model (mABJM) with N = 2 supersymmetry and SU (3) × U (1) global symmetry was tackled by Bobev et al. [1]. We solve the associated BPS equations, requiring IR regularity, using a perturbative method proposed by one of us in [2]. In particular, we provide an analytic proof of a crucial conjecture made in [1] based on numerical solutions: that the R-charge values of three chiral multiplets in mABJM should be independent of the IR values o… Show more
“…Just like our previous works [12][13][14][15], the result here lends further support to the perturbative prescription as a powerful alternative to numerical analyses of supergravity equations which are generically nonlinear. We comment that an important requirement for our prescription is an explicit, and preferably simple, unperturbed solution, like (3.2).…”
Section: Discussionsupporting
confidence: 84%
“…Let us comment that this approach is reminiscent of recent works [12][13][14][15], where supergravity solutions in various holographic contexts are constructed using a perturbative prescription. A notable difference here is that we are looking for non-supersymmetric solutions, so instead of first-order BPS relations we have second-order differential equations, and the analysis is more challenging.…”
We revisit the stringy construction of four-dimensional de-Sitter solutions using orientifolds O8±, proposed by Córdova et al. (2019) [1]. While the original analysis of the supergravity equations is largely numerical, we obtain semi-analytic solutions by treating the curvature as a perturbative parameter. At each order we verify that the (permissive) boundary conditions at the orientifolds are satisfied. To illustrate the advantage of our result, we calculate the four-dimensional Newton constant as a function of the cosmological constant. We also discuss how the discontinuities at O8− can be accounted for in terms of corrections to the worldvolume action.
“…Just like our previous works [12][13][14][15], the result here lends further support to the perturbative prescription as a powerful alternative to numerical analyses of supergravity equations which are generically nonlinear. We comment that an important requirement for our prescription is an explicit, and preferably simple, unperturbed solution, like (3.2).…”
Section: Discussionsupporting
confidence: 84%
“…Let us comment that this approach is reminiscent of recent works [12][13][14][15], where supergravity solutions in various holographic contexts are constructed using a perturbative prescription. A notable difference here is that we are looking for non-supersymmetric solutions, so instead of first-order BPS relations we have second-order differential equations, and the analysis is more challenging.…”
We revisit the stringy construction of four-dimensional de-Sitter solutions using orientifolds O8±, proposed by Córdova et al. (2019) [1]. While the original analysis of the supergravity equations is largely numerical, we obtain semi-analytic solutions by treating the curvature as a perturbative parameter. At each order we verify that the (permissive) boundary conditions at the orientifolds are satisfied. To illustrate the advantage of our result, we calculate the four-dimensional Newton constant as a function of the cosmological constant. We also discuss how the discontinuities at O8− can be accounted for in terms of corrections to the worldvolume action.
“…More recently, the present authors proposed and pursued a perturbative prescription which allows one to obtain the holographic action as a power series in UV expansion parameters. The conjectures based on numerical results are partly confirmed for N = 2 * and N = 1 * deformations of N = 4 super Yang-Mills [58,59], and for mABJM theory [60] which is obtained as a nontrivial fixed point of renormalization group after one of bifundamental chiral multiplet is given superpotential mass and integrated out. For the mass deformation of Brandhuber-Oz theory [25,[61][62][63], where numerical results did not lead to a definitive conjecture on analytic relations, we managed to obtain the holographic free energy in closed form, from the resummation of the perturbative results.…”
We study the Hamilton-Jacobi formulation of effective mechanical actions associated with holographic renormalization group flows when the field theory is put on the sphere and mass terms are turned on. Although the system is supersymmetric and it is described by a superpotential, Hamilton’s characteristic function is not readily given by the superpotential when the boundary of AdS is curved. We propose a method to construct the solution as a series expansion in scalar field degrees of freedom. The coefficients are functions of the warp factor to be determined by a differential equation one obtains when the ansatz is substituted into the Hamilton-Jacobi equation. We also show how the solution can be derived from the BPS equations without having to solve differential equations. The characteristic function readily provides information on holographic counterterms which cancel divergences of the on-shell action near the boundary of AdS.
“…More recently, the present authors proposed and pursued a perturbative prescription which allows one to obtain the holographic action as a power series in UV expansion parameters. The conjectures based on numerical results are partly confirmed for N = 2 * and N = 1 * deformations of N = 4 super Yang-Mills [57,58], and for mABJM theory [59] which is obtained as a nontrivial fixed point of renormalization group after one of bifundamental chiral multiplet is given superpotential mass and integrated out. For the mass deformation of Brandhuber-Oz theory [25,[60][61][62], where numerical results did not lead to a definitive conjecture on analytic relations, we managed to obtain the holographic free energy in closed form, from the resummation of the perturbative results.…”
We study the Hamilton-Jacobi formulation of effective mechanical actions associated with holographic renormalization group flows when the field theory is put on the sphere and mass terms are turned on. Although the system is supersymmetric and it is described by a superpotential, Hamilton's characteristic function is not readily given by the superpotential when the boundary of AdS is curved. We propose a method to construct the solution as a series expansion in scalar field degrees of freedom. The coefficients are functions of the warp factor to be determined by a differential equation one obtains when the ansatz is substituted into the Hamilton-Jacobi equation. We also show how the solution can be derived from the BPS equations without having to solve differential equations. The characteristic function readily provides information on holographic counterterms which cancel divergences of the on-shell action near the boundary of AdS.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.