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Waves on Noncommutative Spacetimes

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arxiv hep-th/0503087 v2 pith:X6A3BFAE submitted 2005-03-10 hep-th gr-qchep-phquant-ph

Waves on Noncommutative Spacetimes

classification hep-th gr-qchep-phquant-ph
keywords thetainterferencewavescommutativewhenalgebradeformedelements
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Waves on ``commutative'' spacetimes like R^d are elements of the commutative algebra C^0(R^d) of functions on R^d. When C^0(R^d) is deformed to a noncommutative algebra {\cal A}_\theta (R^d) with deformation parameter \theta ({\cal A}_0 (R^d) = C^0(R^d)), waves being its elements, are no longer complex-valued functions on R^d. Rules for their interpretation, such as measurement of their intensity, and energy, thus need to be stated. We address this task here. We then apply the rules to interference and diffraction for d \leq 4 and with time-space noncommutativity. Novel phenomena are encountered. Thus when the time of observation T is so brief that T \leq 2 \theta w, where w is the frequency of incident waves, no interference can be observed. For larger times, the interference pattern is deformed and depends on \frac{\theta w}{T}. It approaches the commutative pattern only when \frac{\theta w}{T} goes to 0. As an application, we discuss interference of star light due to cosmic strings.

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