Considering the BMN matrix model as a truncation of $\\mathcal{N}=4$SYM, we also compute the frequencies of the quasi-normal modes of the dualscalar fields in the AdS$_5$-Schwarzschild background. We compare the results,and we find a surprising similarity....
必应词典为您提供quasi-normal-modes的释义,网络释义: 准正则模;准简正模式;
Quasi-normal modes in random mediaCondensed matter physics Quasi-normal modes in random media CITY UNIVERSITY OF NEW YORK Azriel Z. Genack WangJingWe have analyzed spectra of localized microwave transmitted through quasi-1D random samples to obtain the central frequency, linewidth and field speckle ...
准正则模,quasi-normal modes criterion modification准则修正 3)quasi-regular ring准正则环 4)almost regular graph准正则图 5)para regular准正则 1.In this article, T 0, T 1/2 , T 1 spacws are re studied and two kinds of new space, T t space and para regular space,are defined/...
Zhidenko, A.: Linear perturbations of black holes: stability, quasi-normal modes and tails. PhD Thesis, arXiv:0903.3555v2Zhidenko, A., Linear perturbations of black holes: stability, quasi-normal modes and tails, Ph.D. Thesis, (Universidade de Sa˜o Paolo, Sa˜o Paolo, 2009). [ar...
We found that both for small and large values of ℓ, the imaginary part of the QNM modes are always negative, implying the stability of the underlying BH in the entire parameter space, namely b>0 and e∈(−3−3/1−a∗2,2] with a∗=a/M. Thus, it is not possible to ...
Field transmission coefficients for microwave radiation between arrays of points on the incident and output surfaces of random samples are analyzed to yield the underlying quasi-normal modes and transmission eigenchannels of each realization of the sample. The linewidths, central frequencies, and ...
For each subtracted geometry we obtain two branches of quasi-normal modes, given in terms of hypergeometric functions and spherical harmonics. One branch is over-damped and the other under-damped and they exhibit rotational splitting. No black hole bomb is possible because the Killing field which ...
In this work, we investigate the effects of this correction to the quasi-normal modes of a test scalar field propagating in this kind of black hole background analytically and numerically. It is found that although the quasi-period frequencies and the damping of oscillations are respectively ...
In the framework of general relativity (GR) quasi-normal modes (QNM) arise, as perturbations (electromagnetic or gravitational) of stellar or black hole spacetimes. Due to the emission of gravitational waves there are no normal mode oscillations but instead the frequencies become “quasi-normal” ...