Black holes, bandwidths and Beethoven

被引:67
作者
Kempf, A [1 ]
机构
[1] Univ Florida, Dept Phys, Inst Fundamental Theory, Gainesville, FL 32611 USA
关键词
D O I
10.1063/1.533244
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It is usually believed that a function phi(t) whose Fourier spectrum is bounded can vary at most as fast as its highest frequency component omega(max). This is, in fact, not the case, as Aharonov, Berry, and others drastically demonstrated with explicit counterexamples, so-called superoscillations. It has been claimed that even the recording of an entire Beethoven symphony can occur as part of a signal with a 1 Hz bandwidth. Bandlimited functions also occur as ultraviolet regularized fields. Their superoscillations have been suggested, for example, to resolve the trans-Planckian frequencies problem of black hole radiation. Here, we give an exact proof for generic superoscillations. Namely, we show that for every fixed bandwidth there exist functions that pass through any finite number of arbitrarily prespecified points. Further, we show that, in spite of the presence of superoscillations, the behavior of bandlimited functions can be characterized reliably, namely through an uncertainty relation: The standard deviation Delta T of samples phi(t(n)) taken at the Nyquist rate obeys Delta T greater than or equal to 1/4 omega(max). This uncertainty relation generalizes to variable bandwidths. For ultraviolet regularized fields we identify the bandwidth as the in general spatially variable finite local density of degrees of freedom. (C) 2000 American Institute of Physics. [S0022-2488(00)03904-9].
引用
收藏
页码:2360 / 2374
页数:15
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