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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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<strong>Quantum</strong> <strong>Gravity</strong> phenomenology 443ways in which a modified dispersion relation could manifest itself, we do have atleast some hope of experimental study.22.5.1 On the test theories with modified dispersion relationThe majority (see, e.g., Refs. [5; 6; 7; 8; 10; 11; 12; 29]) of studies concerningPlanck-scale modifications of the dispersion relation adopt the phenomenologicalformula( ) ( )m 2 ≃ E 2 −⃗p 2 + η ⃗p 2 E n E n+3+ O , (22.2)E n pE n+1QGwith real η (assumed <strong>to</strong> be of order |η| ∼1) and integer n.There is at this point a very large literature on the associated phenomenology, butI want <strong>to</strong> stress that actually some of the different phenomenological studies thatcompose this literature introduce this type of dispersion relation within differenttest theories. The limits obtained within different test theories are of course not <strong>to</strong>be compared. The same parametrization of the dispersion relation, if introducedwithin different test theories, actually gives rise <strong>to</strong> independent sets of parameters.The potential richness of this phenomenology, for what concerns the developmen<strong>to</strong>f test theories, mainly originates from the need <strong>to</strong> specify, in addition <strong>to</strong> theform of the dispersion relation, several other structural properties of the test theory.It is necessary <strong>to</strong> state whether the theory is still “Hamil<strong>to</strong>nian”, in the sensethat the velocity along the x axis is obtained from the commuta<strong>to</strong>r with a Hamil<strong>to</strong>nian(v ∼[x, H]) and whether the Heisenberg commuta<strong>to</strong>r preserves its standardform ([x, p] ∼). This second concern is significant since some of the heuristicarguments that are used <strong>to</strong> motivate the presence of a modified dispersion relationat the Planck scale also suggest that the Heisenberg commuta<strong>to</strong>r should becorrespondingly modified.Then the test theory should formulate a law of energy-momentum conservation.For example, some types of spacetime noncommutativity which contributed<strong>to</strong> interest in modified dispersion relations appear <strong>to</strong> be such <strong>to</strong> require an accompanyingmodification of the law of energy-momentum conservation. And in particulara link between modification of the dispersion relation and associated modificationof the law of energy-momentum conservation is required by the DSR principles(see below).And one should keep clearly separate the test theories that intend <strong>to</strong> describeonly kinematics and the ones that also adopt a scheme for Planck-scale dynamics.For example, in loop quantum gravity and some noncommutative spacetimes whichprovided motivation for considering modifications of the dispersion relation, while

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