2012
DOI: 10.1007/jhep08(2012)157
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The perturbative partition function of supersymmetric 5D Yang-Mills theory with matter on the five-sphere

Abstract: Based on the construction by Hosomichi, Seong and Terashima we consider N = 1 supersymmetric 5D Yang-Mills theory with matter on a five-sphere with radius r. This theory can be thought of as a deformation of the theory in flat space with deformation parameter r and this deformation preserves 8 supercharges. We calculate the full perturbative partition function as a function of r/g 2 Y M , where g Y M is the Yang-Mills coupling, and the answer is given in terms of a matrix model. We perform the calculation usin… Show more

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Cited by 154 publications
(252 citation statements)
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“…The present discussion is very similar to the 5D case [4,5] and we refer the reader there for some basic definitions from contact geometry. Using the projectors κ ∧ i v and (1 − κ ∧ i v ) we can decompose the differential form into vertical and horizontal parts…”
Section: Calculation Of Determinantsmentioning
confidence: 92%
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“…The present discussion is very similar to the 5D case [4,5] and we refer the reader there for some basic definitions from contact geometry. Using the projectors κ ∧ i v and (1 − κ ∧ i v ) we can decompose the differential form into vertical and horizontal parts…”
Section: Calculation Of Determinantsmentioning
confidence: 92%
“…In other dimensions the theory is not conformal, but we still include a similar term for the scalar fields 5) where the index I is summed over and ∆ I is the analog of the dimension for φ I . We will see that we need further terms to preserve the supersymmetry.…”
Section: Jhep03(2015)155mentioning
confidence: 99%
“…3 The low-energy theory at a generic point of this 5(K − 1)-dimensional moduli space contains (K − 1) free tensor multiplets of the six-dimensional N = (2, 0) supersymmetry. At the origin of the moduli space, the theory is at an interacting fixed point.…”
Section: Jhep03(2015)121mentioning
confidence: 99%
“…Each boundary condition describes a different theory, and the relation between them is much weaker than between families of supersymmetric vacua in flat space or in compact space. 5 Nevertheless, we will refer to the space of 3 There are some subtleties with taking this quotient and decoupling the 'center-of-mass', but they will not be relevant for the purposes of this paper. 4 From the viewpoint of the construction of this theory using type IIB string theory on an orbifold which is locally C 2 /ZK , the modes parameterizing the space (1.3) are a subset of the modes which parameterize the moduli space (1.2) for the theory defined on R 4,1 × S 1 .…”
Section: Adsmentioning
confidence: 99%
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