73 research outputs found
Constructing an Explicit AdS/CFT Correspondence with Cartan Geometry
An explicit AdS/CFT correspondence is shown for the Lie group . The
Lie symmetry structures allow for the construction of two physical theories
through the tools of Cartan geometry. One is a gravitational theory that has
anti-de Sitter symmetry. The other is also a gravitational theory but is
conformally symmetric and lives on 8-dimensional biconformal space. These
"extra" four dimensions have the degrees of freedom used to construct a
Yang-Mills theory. The two theories, based on AdS or conformal symmetry, have a
natural correspondence in the context of their Lie algebras alone where neither
SUSY, nor holography, is necessary.Comment: 13 pages, 1 Tabl
Time and dark matter from the conformal symmetries of Euclidean space
The quotient of the conformal group of Euclidean 4-space by its Weyl subgroup
results in a geometry possessing many of the properties of relativistic phase
space, including both a natural symplectic form and non-degenerate Killing
metric. We show that the general solution posesses orthogonal Lagrangian
submanifolds, with the induced metric and the spin connection on the
submanifolds necessarily Lorentzian, despite the Euclidean starting pont. By
examining the structure equations of the biconformal space in an orthonormal
frame adapted to its phase space properties, we also find that two new tensor
fields exist in this geometry, not present in Riemannian geometry. The first is
a combination of the Weyl vector with the scale factor on the metric, and
determines the timelike directions on the submanifolds. The second comes from
the components of the spin connection, symmetric with respect to the new
metric. Though this field comes from the spin connection it transforms
homogeneously. Finally, we show that in the absence of conformal curvature or
sources, the configuration space has geometric terms equivalent to a perfect
fluid and a cosmological constant.Comment: 26 pages, no figures. Appreciable introductory material added.
Results substantially strengthened and explained. New results concerning dark
matter and dark energy candidates added to this versio
Time and Dark Matter from the Conformal Symmetries of Euclidean Space
The quotient of the conformal group of Euclidean 4-space by its Weyl subgroup results in a geometry possessing many of the properties of relativistic phase space, including both a natural symplectic form and non-degenerate Killing metric. We show that the general solution posesses orthogonal Lagrangian submanifolds, with the induced metric and the spin connection on the submanifolds necessarily Lorentzian, despite the Euclidean starting pont. By examining the structure equations of the biconformal space in an orthonormal frame adapted to its phase space properties, we also find that two new tensor fields exist in this geometry, not present in Riemannian geometry. The first is a combination of the Weyl vector with the scale factor on the metric, and determines the timelike directions on the submanifolds. The second comes from the components of the spin connection, symmetric with respect to the new metric. Though this field comes from the spin connection it transforms homogeneously. Finally, we show that in the absence of conformal curvature or sources, the configuration space has geometric terms equivalent to a perfect fluid and a cosmological constant
Realistic sensitivity curves for pulsar timing arrays
We construct realistic sensitivity curves for pulsar timing array searches for gravitational waves, incorporating both red and white noise contributions to individual pulsar noise spectra, and the effect of fitting to a pulsar timing model. We demonstrate the method on both simulated pulsars and a realistic array consisting of a subset of NANOGrav pulsars used in recent analyses. A comparison between the results presented here and measured upper limit curves from actual analyses shows agreement to tens of percent. The resulting sensitivity curves can be used to assess the detectability of predicted gravitational-wave signals in the nanohertz frequency band in a coherent, flexible, and computationally efficient manner
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