It is generally believed that coupling the graviton (a classical Fierz-Pauli
massless spin-2 field) to its own energy-momentum tensor successfully recreates
the dynamics of the Einstein field equations order by order; however the
validity of this idea has recently been brought into serious doubt 1. To
remedy this confusion, we present a graviton action for which energy-momentum
self-coupling is indeed consistent with the Einstein field equations. The
Hilbert energy-momentum tensor for this graviton is calculated explicitly and
shown to supply the correct second-order term in the field equations. A
formalism for perturbative expansions of metric-based gravitational theories is
then developed, and these techniques employed to demonstrate that our graviton
action is a starting point for a straightforward energy-momentum self-coupling
procedure that, order by order, generates the Einstein-Hilbert action (up to a
classically irrelevant surface term). The perturbative formalism is extended to
include matter and a cosmological constant, and interactions between
perturbations of a free matter field and the gravitational field are studied in
a vacuum background. Finally, the effect of a non-vacuum background is
examined, and the graviton is found to develop a non-vanishing "mass-term" in
the action.
Description
Bootstrapping gravity: a consistent approach to energy-momentum
self-coupling
%0 Generic
%1 Butcher2009
%A Butcher, Luke M.
%A Hobson, Michael
%A Lasenby, Anthony
%D 2009
%K SG gravity
%T Bootstrapping gravity: a consistent approach to energy-momentum
self-coupling
%U http://arxiv.org/abs/0906.0926
%X It is generally believed that coupling the graviton (a classical Fierz-Pauli
massless spin-2 field) to its own energy-momentum tensor successfully recreates
the dynamics of the Einstein field equations order by order; however the
validity of this idea has recently been brought into serious doubt 1. To
remedy this confusion, we present a graviton action for which energy-momentum
self-coupling is indeed consistent with the Einstein field equations. The
Hilbert energy-momentum tensor for this graviton is calculated explicitly and
shown to supply the correct second-order term in the field equations. A
formalism for perturbative expansions of metric-based gravitational theories is
then developed, and these techniques employed to demonstrate that our graviton
action is a starting point for a straightforward energy-momentum self-coupling
procedure that, order by order, generates the Einstein-Hilbert action (up to a
classically irrelevant surface term). The perturbative formalism is extended to
include matter and a cosmological constant, and interactions between
perturbations of a free matter field and the gravitational field are studied in
a vacuum background. Finally, the effect of a non-vacuum background is
examined, and the graviton is found to develop a non-vanishing "mass-term" in
the action.
@misc{Butcher2009,
abstract = { It is generally believed that coupling the graviton (a classical Fierz-Pauli
massless spin-2 field) to its own energy-momentum tensor successfully recreates
the dynamics of the Einstein field equations order by order; however the
validity of this idea has recently been brought into serious doubt [1]. To
remedy this confusion, we present a graviton action for which energy-momentum
self-coupling is indeed consistent with the Einstein field equations. The
Hilbert energy-momentum tensor for this graviton is calculated explicitly and
shown to supply the correct second-order term in the field equations. A
formalism for perturbative expansions of metric-based gravitational theories is
then developed, and these techniques employed to demonstrate that our graviton
action is a starting point for a straightforward energy-momentum self-coupling
procedure that, order by order, generates the Einstein-Hilbert action (up to a
classically irrelevant surface term). The perturbative formalism is extended to
include matter and a cosmological constant, and interactions between
perturbations of a free matter field and the gravitational field are studied in
a vacuum background. Finally, the effect of a non-vacuum background is
examined, and the graviton is found to develop a non-vanishing "mass-term" in
the action.
},
added-at = {2009-06-12T11:30:48.000+0200},
author = {Butcher, Luke M. and Hobson, Michael and Lasenby, Anthony},
biburl = {https://www.bibsonomy.org/bibtex/2275bda977e21a7fd8f38be940d98cf73/tomasortin},
description = {Bootstrapping gravity: a consistent approach to energy-momentum
self-coupling},
interhash = {25e39d601d598de46e5562a5308764a9},
intrahash = {275bda977e21a7fd8f38be940d98cf73},
keywords = {SG gravity},
note = {cite arxiv:0906.0926
Comment: 18 pages},
timestamp = {2009-06-12T11:30:48.000+0200},
title = {Bootstrapping gravity: a consistent approach to energy-momentum
self-coupling},
url = {http://arxiv.org/abs/0906.0926},
year = 2009
}