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l1a,b=0. q2ab Ka Kb, ν = u = v = 1l. ... l1m=0. q2 m2. ) l1n,a=0. (q q1)n. [n; q2]!q(l1)(na1). 2/2 En Ka F n ,. where RK is defined in (5). It is also known

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In the second half of this text we study bounded linear op-erators on the generalised sequence space p(ZN , U ), where p [1, ] and U issome complex Banach space. ... Collective Compactness. In the mid 1960’s Anselone and co-workers (see[3] and the

In spinors, if Ka = ιAoA. ′. then an α-plane distribution is defined by oA′. ,

1.4). 1.3. The analytic branches of eigenvalues and eigenvectors of A(t).According to the general analytic perturbation theory (see [Ka]), for |t| 6 t0there exist real-analytic functions

JOURNAL OF MATHEMATICAL STUDYJ. Math. Study, Vol. x, No. x (201x), pp. 1-74. Astrophysical Dynamics and Cosmology. Tian Ma1, Shouhong Wang2,. 1 Department of Mathematics, Sichuan University, Chengdu, P. R. China.2 Department of Mathematics, Indiana

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