A FLUX-FLUX CROSS-CORRELATION FUNCTION APPROACH TO SELF-DIFFUSION OF HYDROGEN ATOM ON A CU(111) SURFACE

2005 ◽  
Vol 04 (01) ◽  
pp. 209-223
Author(s):  
TOSHIAKI TANIIKE ◽  
KOICHI YAMASHITA

We have employed a flux-flux cross-correlation function approach (CCFA) to calculate quantum thermal rate constants of reactions for which an auto-correlation function approach (ACFA) is not adequate. In CCFA, two dividing surfaces partition a system into three regions, while in ACFA, two channels are defined by a dividing surface. Therefore, the CCFA method is appropriate for multi-channel reactions. In this paper, we show the efficiency of CCFA for multi-channel reactions. For example, we have examined self-diffusion of a hydrogen atom on a rigid Cu (111) surface. We introduce closed dividing surfaces that subdivide the potential energy surface for each channel. A combination of the closed dividing surfaces and CCFA allows us to calculate rate constants for both single and multi-hopping modes directly. Then, we calculate a diffusion constant without the usual uncorrelated hops approximation, using instead the calculated site-to-site hopping rates, thus showing the importance of multihops.

2015 ◽  
Vol 14 (1) ◽  
Author(s):  
I Nyoman Pramaita ◽  
I G.A.G.K. Diafari ◽  
DNKP Negara ◽  
Agus Dharma

In this paper, the authors propose the design of a new orthogonal small set Kasami code sequence generated using combination of non-orthogonal m-sequence and small set Kasami code sequence. The authors demonstrate that the proposed code sequence has comparable auto-correlation function (ACF), cross- correlation function (CCF), peak cross-correlation values with that of the existing orthogonal small set Kasami code sequence. Though the proposed code sequence has less code sequence sets than that of the existing orthogonal small set Kasami code sequence, the proposed code sequence possesses one more numbers of members in each code sequence set. The members of the same code set of the proposed code sequence are orthogonal to each other.


Author(s):  
Tuli De ◽  
Tanuka Chattopadhyay ◽  
Asis Kumar Chattopadhyay

AbstractSpatial clustering nature of galaxies has been studied previously through auto correlation function. The same type of cross-correlation function has been used in the present work to investigate parametric clustering nature of galaxies with respect to masses and sizes of galaxies. Here, formation and evolution of several components of nearby massive early type galaxies (M*≥ 1.3 × 1011M⊙have been envisaged through cross-correlations, in the mass-size parametric plane, with high redshift (0.2 ⩽z⩽ 7) ETGs. It is found that the inner most components of nearby ETGs have significant correlation (~ 0.5 ± (0.02–0.07)) with ETGs in the highest redshift range (2 ⩽z⩽ 7) called ‘red nuggets’ whereas intermediate components are highly correlated (~ 0.65 ± (0.03–0.07)) with ETGs in the redshift range 0.5 ⩽z⩽ 0.75. The outermost part has no correlation in any range, suggesting a scenario throughin situaccretion. The above formation scenario is consistent with the previous results obtained for NGC5128 and to some extent for nearby elliptical galaxies after considering a sample of ETGs at high redshift with stellar masses greater than or equal to 108.73M⊙. So the present work indicates a three phase formation instead of two as discussed in previous works.


2005 ◽  
Vol 636 (1) ◽  
pp. L9-L12 ◽  
Author(s):  
Jeff Cooke ◽  
Arthur M. Wolfe ◽  
Eric Gawiser ◽  
Jason X. Prochaska

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