6 research outputs found
Renormalization Group Flow in Scalar-Tensor Theories. II
We study the UV behaviour of actions including integer powers of scalar
curvature and even powers of scalar fields with Functional Renormalization
Group techniques. We find UV fixed points where the gravitational couplings
have non-trivial values while the matter ones are Gaussian. We prove several
properties of the linearized flow at such a fixed point in arbitrary dimensions
in the one-loop approximation and find recursive relations among the critical
exponents. We illustrate these results in explicit calculations in for
actions including up to four powers of scalar curvature and two powers of the
scalar field. In this setting we notice that the same recursive properties
among the critical exponents, which were proven at one-loop order, still hold,
in such a way that the UV critical surface is found to be five dimensional. We
then search for the same type of fixed point in a scalar theory with minimal
coupling to gravity in including up to eight powers of scalar curvature.
Assuming that the recursive properties of the critical exponents still hold,
one would conclude that the UV critical surface of these theories is five
dimensional.Comment: 14 pages. v.2: Minor changes, some references adde
Asymptotic Safety, Emergence and Minimal Length
There seems to be a common prejudice that asymptotic safety is either
incompatible with, or at best unrelated to, the other topics in the title. This
is not the case. In fact, we show that 1) the existence of a fixed point with
suitable properties is a promising way of deriving emergent properties of
gravity, and 2) there is a sense in which asymptotic safety implies a minimal
length. In so doing we also discuss possible signatures of asymptotic safety in
scattering experiments.Comment: LaTEX, 20 pages, 2 figures; v.2: minor changes, reflecting published
versio
Renormalization group flow of Horava-Lifshitz gravity at low energies
Contains fulltext :
126237.pdf (preprint version ) (Open Access
Inflationary solutions in asymptotically safe f(R) theories
We discuss the existence of inflationary solutions in a class of renormalization group improved polynomial f(R) theories, which have been studied recently in the context of the asymptotic safety scenario for quantum gravity. These theories seem to possess a nontrivial ultraviolet fixed point, where the dimensionful couplings scale according to their canonical dimensionality. Assuming that the cutoff is proportional to the Hubble parameter, we obtain modified Friedmann equations which admit both power-law and exponential solutions. We establish that for sufficiently high-order polynomial the solutions are reliable in the sense that considering still higher-order polynomials is very unlikely to change the solution