- qc / 0 10 90 01 v 1 1 S ep 2 00 1 The metric in the superspace of Riemannian metrics and its relation to gravity ∗
نویسنده
چکیده
The space of all Riemannian metrics is infinite-dimensional. Nevertheless a great deal of usual Riemannian geometry can be carried over. The superspace of all Riemannian metrics shall be endowed with a class of Riemannian metrics; their curvature and invariance properties are discussed. Just one of this class has the property to bring the lagrangian of General Relativity into the form of a classical particle’s motion. The signature of the superspace metric depends in a non-trivial manner on the signature of the original metric, we derive the corresponding formula. Our approach is a local one: the essence is a metric in the space of all symmetric rank-two tensors, and then the space becomes a warped product of the real line with an Einstein space.
منابع مشابه
ar X iv : g r - qc / 0 10 90 05 v 1 4 S ep 2 00 1 The Newtonian limit of fourth and higher order gravity ∗
We consider the Newtonian limit of the theory based on the La-grangian L = R + p k=0 a k R2 k R √ −g. The gravitational potential of a point mass turns out to be a combination of Newtonian and Yukawa terms. For sixth-order gravity (p = 1) the coefficients are calculated explicitly. For general p one gets Φ = m/r
متن کاملON THE LIFTS OF SEMI-RIEMANNIAN METRICS
In this paper, we extend Sasaki metric for tangent bundle of a Riemannian manifold and Sasaki-Mok metric for the frame bundle of a Riemannian manifold [I] to the case of a semi-Riemannian vector bundle over a semi- Riemannian manifold. In fact, if E is a semi-Riemannian vector bundle over a semi-Riemannian manifold M, then by using an arbitrary (linear) connection on E, we can make E, as a...
متن کاملar X iv : g r - qc / 0 10 10 90 v 1 2 3 Ja n 20 01 ASYMPTOTIC FREEDOM IN CURVATURE - SATURATED GRAVITY
For a spatially flat Friedmann model with line element ds 2 = a 2 [da 2 /B(a) − dx 2 − dy 2 − dz 2 ], the 00-component of the Einstein field equation reads 8πGT 00 = 3/a 2 containing no derivative. For a nonlinear Lagrangian L(R), we obtain a second– order differential equation for B instead of the expected fourth-order equation. We discuss this equation for the curvature-saturated model propos...
متن کاملar X iv : g r - qc / 0 60 60 39 v 1 9 J un 2 00 6 The Vector - Tensor nature of Bekenstein ’ s relativistic theory of Modified Gravity
Bekenstein’s theory of relativistic gravity is conventionally written as a bi-metric theory. The two metrics are related by a disformal transformation defined by a dynamical vector field and a scalar field. In this comment we show that the theory can be re-written as Vector-Tensor theory akin to Einstein-Aether theories with non-canonical kinetic terms. We discuss some of the implications of th...
متن کاملar X iv : g r - qc / 0 10 90 12 v 1 4 S ep 2 00 1 Spacetime metric from linear electrodynamics . III
We extend our previous results on the wave propagation in a spacetime with a linear electromagnetic spacetime relation to the most general case in which the corresponding constitutive tensor is asymmetric. We find the corresponding Fresnel equation governing the geometry of light rays and show that it is always quartic in the wave covectors. The conditions for the wave covectors to define a sin...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 1989