1,400 research outputs found
Complete Solution for M(atrix) Theory at Two Loops
The complete result for the effective potential for two graviton exchange at
two loops in M(atrix) theory can be expressed in terms of a generalized
hypergeometric function.Comment: 4 pages, TeX, no figure
Compactifying M-Theory to Four Dimensions
We consider compactifications of -theory to four-dimensional
Minkowski space on seven-dimensional non-compact manifolds. These
compactifications include a warp factor which is non-constant due to the
presence of sources coming from fivebranes wrapping two-dimensional
submanifolds of the internal seven-dimensional space. We derive the expression
for the field strengths and consider an explicit example of this general class
of solutions.Comment: 15 pages, TeX, no figures, references adde
Graviton scattering amplitudes in M theory
We compute graviton scattering amplitudes in M theory using Feynman rules for a scalar particle coupled to gravity in eleven dimensions. The processes that we consider describe the single graviton exchange and the double graviton exchange, that in M(atrix) theory correspond to the v^4/r^7 and v^6/r^14 term, respectively. We argue that the v^6/r^14 term appearing in M(atrix) theory at two loops can be obtained from the covariant eleven-dimensional four-graviton amplitude. Finally, we calculate the v^8/r^18 term appearing at two loops in M(atrix) theory. It has been previously conjectured that this term is related to a four graviton scattering amplitude involving the R^4 vertex of M theory
Kaluza-Klein Theories Without Truncation
In this note we present a closed expression for the space-time effective
action for all bosonic fields (massless and massive) obtained from the
compactification of gravity or supergravity theories (such as type II or
eleven-dimensional supergravities) from to space-time dimensions.Comment: 20 page
Supersymmetry Breaking and alpha'-Corrections to Flux Induced Potentials
We obtain the vacuum solutions for M-theory compactified on eight-manifolds
with non-vanishing four-form flux by analyzing the scalar potential appearing
in the three-dimensional theory. Many of these vacua are not supersymmetric and
yet have a vanishing three-dimensional cosmological constant. We show that in
the context of Type IIB compactifications on Calabi-Yau threefolds with fluxes
and external brane sources alpha'-corrections generate a correction to the
supergravity potential proportional to the Euler number of the internal
manifold which spoils the no-scale structure appearing in the classical
potential. This indicates that alpha'-corrections may indeed lead to a
stabilization of the radial modulus appearing in these compactifications.Comment: 28 pages, no figures, reference adde
Supersymmetry Breaking, M-Theory and Fluxes
We consider warped compactifications of -theory to
three-dimensional Minkowski space on compact eight-manifolds. Taking all the
leading quantum gravity corrections of eleven-dimensional supergravity into
account we obtain the solution to the equations of motion and Bianchi
identities. Generically these vacua are not supersymmetric and yet have a
vanishing three-dimensional cosmological constant.Comment: 17 pages, TEX, no figures. References adde
Runaway in the Landscape
We consider flux compactifications of type IIB string theory on the mirror of
a rigid Calabi-Yau. In special cases, these models are dual to the type IIA
flux vacua with runaway direction in flux space. We show that new weak coupling
AdS solutions can be found for large complex structure, while Minkowski
solutions with all moduli stabilized are confined to be at strong coupling. The
existence of these solutions, as found in a previous work, is nevertheless
guaranteed by a non-renormalization theorem of the type IIB flux
superpotential. Based on our results, we are led to the conjecture that
supersymmetric runaway directions in flux space are always accompanied by a
spectrum of moduli masses reaching down to the AdS scale. This could be
violated in a non-supersymmetric situation.Comment: 26 page
Finite-temperature three-point function in 2D CFT
We calculate the finite temperature three-point correlation function for
primary fields in a 2D conformal field theory in momentum space. This result
has applications to any strongly coupled field theory with a 2D CFT dual, as
well as to Kerr/CFT.Comment: 6 page
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