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By adding WZ terms to the superstring actions, we find actions with kappa symmetry. Similarly, for super-p-branes, we can describe actions, and find a brane scan, related to the existence of a kappa symmetry. In curved superspace, the supergravity equations of motion in 11 dimensions are obtained from the condition of kappa symmetry. The superembedding formalism starts with the superembedding conditions. For the case of the particle, we describe it and give example. For the superstring, we sketch how it is done.
We define the Maldacena–Núñez no-go theorem for supergravity compactifications and show that it implies that there are no de Sitter or Minkowski compactifications, both in massless and in massive supergravity. The case of no Randall–Sundrum solutions in d = 5 gauged supergravity is treated separately. The swampland conjecture for string theory compactifications is based on some “sporadic” results, and there is a more general no-go theorem, but there are loopholes.
Supersymmetry is defined as a Bose–Fermi symmetry. Spinors are defined in general dimensions. The Wess–Zumino model is defined first in two dimensions on-shell, where the invariance of the action is proven using Majorana spinor identities. The susy algebra is defined, and using Fierz identities, one proves the closure of the algebra and resulting off-shell susy. Then, the four-dimensional free off-shell Wess–Zumino model is defined as a simple generalization.
N = 2 supergravity in four dimensions is defined, and the related special geometry is defined. First one starts with the rigid susy case, then special geometry is defined, and then the subset of very-special geometry and associated duality symmetries are defined. The general properties of other, more general supergravity theories (with more susy or in higher dimensions) are described. The unique N = 1 11-dimensional supergravity theory is described. We end with some comments on off-shell and superspace models in the more general cases.
We first define the notion of Kaluza–Klein (KK) compactification, the three types of KK metrics one can define, and then we consider fields with (Lorentz) spin in the KK theory. The original KK theory, for compactification on S1 from five dimensions to four dimensions, is described, and we end with general properties of KK reductions.
The N = 1 four-dimensional supergravity is described in superspace, in the super-geometric approach. We discuss the invariances, gauge choices, and the fields, then the superspace constraints, and then solve the constraints and the Bianchi identities.
We consider Minimal Supergravity, starting with the masses and parameters of MSSM, followed by the supergravity extension. Then, susy breaking is treated, in particular in the mechanisms for the MSSM and MinSugra cases. The MinSugra case, with its gravity mediation mechanism, is described in detail, and the Polonyi model is given as an example.
The three-dimensional N = 1 off-shell supergravity action is described, with its symmetries explained, and the susy transformation rules and invariance of the action. The closure of the susy algebra is discussed.
We describe the AdS/CFT correspondence, obtained from string theory in certain backgrounds, in a decoupling limit. We also consider the M theory cases of gravity duals and then the gravity duals of N extremal Dp-branes. In the Penrose limit of supergravity solutions, we obtain pp waves. The Penrose limit can also be taken on the isometry group and algebra.
We define U-duality as being generated by T-dualities and S-dualities together. We show how this leads to the unification of string theory states (and their corresponding supergravity solutions) under M theory. The string duality web is then defined. Finally, we show how U-duality is obtained from M theory.
We start by reviewing the Standard Model, its spectrum, symmetries, representations, and Lagrangian. Then, we consider the Grand Unified Theories extensions, in particular the SU(5) GUT, the SO(10) GUT, and other (bigger) groups. Then, we consider the Minimal Supersymmetric Standard Model (MSSM) and Minimal Supergravity, and new low-energy string (supergravity) constructions.
This graduate textbook covers the basic formalism of supergravity, as well as its modern applications, suitable for a focused first course. Assuming a working knowledge of quantum field theory, Part I gives basic formalism, including on- and off-shell supergravity, the covariant formulation, superspace and coset formulations, coupling to matter, higher dimensions, and extended supersymmetry. A wide range of modern applications are introduced in Part II, including string theoretical (T- and U-duality, anti-de Sitter/conformal field theory (Ads/CFT), susy and sugra on the worldsheet, and superembeddings), gravitational (p-brane solutions and their susy, attractor mechanism, and Witten’s positive energy theorem), and phenomenological (inflation in supergravity, supergravity no-go theorems, string theory constructions at low energies, and minimal supergravity and its susy breaking). The broader emphasis on applications than competing texts gives Ph.D. students the tools they need to do research that uses supergravity and benefits researchers already working in areas related to supergravity.
To define irreducible representations, spinors with dotted and undotted indices are defined. Irreducible representations of susy are defined, first in the massless case, then in the massive case, with and without central charges. The R-symmetry of the algebras is defined. The Lagrangians for the d = 4 multiplets, N = 1 chiral, N = 1 vector, their coupling and the N = 2 models, and finally the unique N = 4 model, are described.
From the unique N = 1 11-dimensional supergravity, all the other supergravities in lower dimensions are thought to be obtained. To obtain the seven-dimensional gauged supergravity, we first describe a first-order formulation of 11-dimensional supergravity. Then, we describe a nonlinear ansatz, leading to a consistent truncation. The concepts of consistent truncation and nonlinear ansatze are described, and the linearized ansatz on S4 and the spherical harmonics on S4 are reviewed. Relatedly, we describe the Lagrangians and transformation rules for the (maximal) N = 8 d = 4, N = 8 d = 5, and N = 4 d = 7 gauged supergravities, the massive type IIA 10-dimensional supergravity, type IIB 10-dimensional supergravity, and some general properties of gaugings, in particular the non-compact ISO(7) gauging. We end with modified supergravities: the one with SO(1, 3) × SU(8) local Lorentz covariance in 11 dimensions, the generalization known as exceptional field theory, and the geometric approach to supergravity, in particular d'Auria and Fré’s 11-dimensional supergravity with OSp(1|32) invariance.