96 research outputs found
On the Frame Fixing in Quantum Gravity
We provide a discussion about the necessity to fix the reference frame before
quantizing the gravitational field. Our presentation is based on stressing how
the 3+1-slicing of the space time becomes an ambiguous procedure as referred to
a quantum 4-metric.Comment: 3 pages, no figures, proceeding of the X Marcel Grossmann meeting,
Rio de Janeiro, Brazil, July 20-26, 200
A New Approach in Quantum Gravity and its Cosmological Implications
This work concerns a new reformulation of quantum geometrodynamics, which
allows to overcome a fundamental ambiguity contained in the canonical approach
to quantum gravity: the possibility of performing a (3+1)-slicing of
space-time, when the metric tensor is in a quantum regime. Our formulation
provides also a procedure to solve the problems connected to the so called
"frozen formalism". In particular we fix the reference frame (i.e. the lapse
function and the shift vector) by introducing the so called "kinematical
action"; as a consequence, the new hamiltonian constraints become parabolic, so
arriving to evolutive (Schroedinger-like) equations for the quantum dynamics.
The kinematical action can be interpreted as the action of a pressureless, but,
in general, non geodesic perfect fluid, so in the semi classical limit our
theory leads to the dynamics of the gravitational field coupled to a dust which
represents the material reference frame we have introduced fixing the slicing.
We also investigate the cosmological implications of the presence of the dust,
which, in the WKB limit of a cosmological problem, makes account for a "dark
matter" component and could play, at present time, a dynamical role.Comment: A synthesis of previous works, based on a talk given at the VIII
Italian-Korean meeting (Pescara, Italy), to appear on "Il Nuovo Cimento
Modifications in the Spectrum of Primordial Gravitational Waves Induced by Instantonic Fluctuations
Vacuum to vacuum instantonic transitions modify the power spectrum of
primordial gravitational waves. We evaluate the new form of the power spectrum
for ordinary gravity as well as the parity violation induced in the spectrum by
a modification of General Relativity known as Holst term and we outline the
possible experimental consequences.Comment: V1: 8 pages. V2: 8 pages, some points clarified, typos corrected,
some references added, final result unchanged. V3: 8 pages, title changed,
presentation improved, discussion of phenomenological consequences added,
comments very welcome. V4: Discussion further improved, comments very very
welcom
Dualism between Physical Frames and Time in Quantum Gravity
In this work we present a discussion of the existing links between the
procedures of endowing the quantum gravity with a real time and of including in
the theory a physical reference frame. More precisely, as first step, we
develop the canonical quantum dynamics, starting from the Einstein equations in
presence of a dust fluid and arrive to a Schroedinger evolution. Then, by
fixing the lapse function in the path integral of gravity, we get a
Schroedinger quantum dynamics, of which eigenvalues problem provides the
appearance of a dust fluid in the classical limit. The main issue of our
analysis is to claim that a theory, in which the time displacement invariance,
on a quantum level, is broken, is indistinguishable from a theory for which
this symmetry holds, but a real reference fluid is included.Comment: 9 pages, submitted to Mod. Phys. Lett. A, major replacements in
section 3 and
From the Einstein-Cartan to the Ashtekar-Barbero canonical constraints, passing through the Nieh-Yan functional
The Ashtekar-Barbero constraints for General Relativity with fermions are
derived from the Einstein-Cartan canonical theory rescaling the state
functional of the gravity-spinor coupled system by the exponential of the
Nieh-Yan functional. A one parameter quantization ambiguity naturally appears
and can be associated with the Immirzi parameter.Comment: Minor changes, two references added, accepted for publication in
Phys. Rev.
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