13.06.2015 Views

Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Questions and answers 573<br />

frame. Just as a frame of reference may have limited validity due <strong>to</strong> global<br />

geometry, here even if spacetime is flat, its noncommutativity accumulates<br />

the uncertainty the further out one goes from the origin of that frame. Is it a<br />

problem? Only if some other observer with some other origin does not reach<br />

the same conclusion. The other observer would have transformed coordinates<br />

defined via eq. (24.17) which describes a quantum Poincaré transformation,<br />

in particular a shift is allowed. The new variables x μ ′ defined by the RHS<br />

of eq. (24.17) obey the relations eq. (24.1) but are shifted by a μ from the<br />

original. The only thing, which I explain in Section 24.5.1 is that the transformation<br />

parameters such as a μ are themselves opera<strong>to</strong>rs (its a quantum group<br />

not a classical group) so the new variables are not simply related <strong>to</strong> the old<br />

ones by a numerical matrix. In short, there is clearly no classical Poincaré<br />

invariance of eq. (24.1) but there is a quantum one. If one takes expectation<br />

values one then has real numbers but the expectation values do not then<br />

transform under a usual Poincaré transformation as the questioner perhaps<br />

assumes. Just because the uncertainty relations are not usual-Poincaré invariant<br />

does not mean an origin is being singled out in the universe. Rather <strong>to</strong><br />

actually relate a new observer’s expectations <strong>to</strong> the old one, one has <strong>to</strong> know<br />

the expectation value of the a μ and face also that they need not commute with<br />

the x μ . In short, a quantum frame transformation is itself “fuzzy” which is not<br />

surprising since the different observers’ own locations should be fuzzy. To be<br />

sure one has approximated Poincaré invariant <strong>to</strong> O(λ) but the equations such<br />

as eq. (24.1) are themselves at that level (both sides are zero if λ = 0andwe<br />

have usual commuting x μ ). My goal in Section 24.5.1 is indeed <strong>to</strong> get physicists<br />

thinking properly about quantum frame rotations as a theory of <strong>Quantum</strong><br />

<strong>Gravity</strong> has <strong>to</strong> address their expectation values <strong>to</strong>o. However, I don’t see any<br />

inconsistency.<br />

2. The x μ are opera<strong>to</strong>rs whose expectation values, we suppose, are the physically<br />

observed macroscopic spacetime coordinates at which a particle might<br />

be approximately located. A theory of <strong>Quantum</strong> <strong>Gravity</strong> has <strong>to</strong> provide the<br />

states on which these expectations are computed so the noncommutative<br />

algebra is not the whole of the observed physics. It’s a joint effort between<br />

the (proposed) noncommutative geometry and the effective quantum state in<br />

which the opera<strong>to</strong>rs are observed.<br />

3. There is no contradiction. The “first predictions” I refer <strong>to</strong> are order of magnitude<br />

computations for a time-or-arrival experiment that can be done without<br />

solving all problems of interpretation of momentum and their addition. Addition<br />

of momenta would be more relevant in the many particle theory. For a<br />

single pho<strong>to</strong>n modelled as a noncommutative plane wave, one does not need<br />

<strong>to</strong> have solved the many particle theory. One does still need some sort of

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!