scholarly journals Sampling the Flow of a Bandlimited Function

Author(s):  
Akram Aldroubi ◽  
Karlheinz Gröchenig ◽  
Longxiu Huang ◽  
Philippe Jaming ◽  
Ilya Krishtal ◽  
...  

AbstractWe analyze the problem of reconstruction of a bandlimited function f from the space–time samples of its states $$f_t=\phi _t*f$$ f t = ϕ t ∗ f resulting from the convolution with a kernel $$\phi _t$$ ϕ t . It is well-known that, in natural phenomena, uniform space–time samples of f are not sufficient to reconstruct f in a stable way. To enable stable reconstruction, a space–time sampling with periodic nonuniformly spaced samples must be used as was shown by Lu and Vetterli. We show that the stability of reconstruction, as measured by a condition number, controls the maximal gap between the spacial samples. We provide a quantitative statement of this result. In addition, instead of irregular space–time samples, we show that uniform dynamical samples at sub-Nyquist spatial rate allow one to stably reconstruct the function $$\widehat{f}$$ f ^ away from certain, explicitly described blind spots. We also consider several classes of finite dimensional subsets of bandlimited functions in which the stable reconstruction is possible, even inside the blind spots. We obtain quantitative estimates for it using Remez-Turán type inequalities. En route, we obtain Remez-Turán inequality for prolate spheroidal wave functions. To illustrate our results, we present some numerics and explicit estimates for the heat flow problem.

2008 ◽  
Vol 17 (08) ◽  
pp. 1179-1196 ◽  
Author(s):  
MARTÍN G. RICHARTE ◽  
CLAUDIO SIMEONE

We study spherically symmetric thin shell wormholes in a string cloud background in (3 + 1)-dimensional space–time. The amount of exotic matter required for the construction, the traversability and the stability of such wormholes under radial perturbations are analyzed as functions of the parameters of the model. In addition, in the appendices a nonperturbative approach to the dynamics and a possible extension of the analysis to a related model are briefly discussed.


2021 ◽  
Vol 280 (9) ◽  
pp. 108962
Author(s):  
Alexander Ulanovskii ◽  
Ilya Zlotnikov

1994 ◽  
Vol 09 (17) ◽  
pp. 1589-1601 ◽  
Author(s):  
THOMAS M. GOULD ◽  
STEPHEN D.H. HSU

We examine the space-time symmetries of forward 2→2 scattering. These symmetries have non-trivial consequences for any class of configurations which might dominate the amplitude in the semiclassical approximation. We derive some dynamical results regarding the stability of configurations which arise solely from reflection symmetry and positivity of the (Euclidean) path-integral action. We consider the relative importance of initial state effects on non-O(3) symmetric configurations.


1993 ◽  
Vol 08 (10) ◽  
pp. 1787-1796 ◽  
Author(s):  
I.L. SHAPIRO ◽  
E.G. YAGUNOV

New set of one-loop finite GUT models is constructed. In particular there are some SU (N), N=5, 7, 9…models with two Higgs multiplets. The stability of finite solutions in UV and IR limits is investigated. The asymptotical behavior of the effective Yukawa and scalar couplings verify the asymptotical finiteness of the models. The renormalization group equations in curved space-time are also considered.


2016 ◽  
Vol 37 (2) ◽  
pp. 621-636 ◽  
Author(s):  
Sanaz Moghim ◽  
Shawna L. McKnight ◽  
Ke Zhang ◽  
Ardeshir M. Ebtehaj ◽  
Ryan G. Knox ◽  
...  

The stability of Kerr’s space-time with |a| < M , in the usual notation, against infinitesimal perturbations is discussed. No exponentially growing ‘normal modes’ occur. However, since (a) the exponentially decaying modes have not been shown to be complete, (b) there are normal modes with real frequencies, the stability of the Kerr space-time has not been established rigorously.


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