In 2007, Terence Tao wrote on his blog an essay about soft analysis, hard analysis and the finitization of soft analysis statements into hard analysis statements. One of his main examples was a quasi-finitization of the infinite pigeonhole principle IPP, arriving at the “finitary” infinite pigeonhole principle FIPP1. That turned out to not be the proper formulation and so we proposed an alterna...

We study a d−dimensional FRW universe, containing a perfect fluid with p = wρ and 1 d−1 ≤ w ≤ 1, and find a correspondence principle similar to that of Horowitz and Polchinski in the black hole case. This principle follows quite generally from thermodynamics and the conservation of energy momentum tensor, and can be stated along similar lines as in the black hole case: “When the temperature T o...

In the general context of complex data processing, this paper reviews a recent practical approach to the continuous wavelet formalism on the sphere. This formalism notably yields a correspondence principle which relates wavelets on the plane and on the sphere. Two fast algorithms are also presented for the analysis of signals on the sphere with steerable wavelets.

A model that is capable of maintaining the identities of individuated elements as they move is described. It solves a particular problem of underdetermination, the motion correspondence problem, by simultaneously applying 3 constraints: the nearest neighbor principle, the relative velocity principle, and the element integrity principle. The model generates the same correspondence solutions as d...

100 ~4tttij:±fjI1B1:.~~~~~ CD Based on the abridged paper below, please answer the following questions: 1. Please detailed explain the difference between user satisfaction and technology acceptance by this paper and your opinions. (20%) 2. From you have learned research method, please tell me the main meaning of Table 2. (10%) 3. After reading the paper, please practically point out two future ...

We determine the quasinormal frequencies for all gravitational perturbations of the ddimensional Schwarzschild black hole, in the infinite damping limit. Using the potentials for gravitational perturbations derived recently by Ishibashi and Kodama, we show that in all cases the asymptotic real part of the frequency is proportional to the Hawking temperature with a coefficient of log 3. Via the ...

We study a d−dimensional FRW universe, containing a perfect fluid with p = wρ and 1 d−1 ≤ w ≤ 1, and find a correspondence principle similar to that of Horowitz and Polchinski in the black hole case. This principle follows quite generally from thermodynamics and the conservation of energy momentum tensor, and can be stated along similar lines as in the black hole case: “When the temperature T o...

nowadays, the status of regulations of securities exchange section in accordance with its huge transactions and its increasing role in countries’ economies has gained particular significance. on the other hand, taking into account that iran is presently an observer member of wto and the necessity of its becoming a permanent one in the near future, it is essential to revise and amend its rules a...